Sample records for hosts mindi farber-deanda

  1. Ethanol production by recombinant hosts

    DOE Patents [OSTI]

    Ingram, Lonnie O. (Gainesville, FL); Beall, David S. (Gainesville, FL); Burchhardt, Gerhard F. H. (Gainesville, FL); Guimaraes, Walter V. (Vicosa, BR); Ohta, Kazuyoshi (Miyazaki, JP); Wood, Brent E. (Gainesville, FL); Shanmugam, Keelnatham T. (Gainesville, FL)

    1995-01-01T23:59:59.000Z

    Novel plasmids comprising genes which code for the alcohol dehydrogenase and pyruvate decarboxylase are described. Also described are recombinant hosts which have been transformed with genes coding for alcohol dehydrogenase and pyruvate. By virtue of their transformation with these genes, the recombinant hosts are capable of producing significant amounts of ethanol as a fermentation product. Also disclosed are methods for increasing the growth of recombinant hosts and methods for reducing the accumulation of undesirable metabolic products in the growth medium of these hosts. Also disclosed are recombinant host capable of producing significant amounts of ethanol as a fermentation product of oligosaccharides and plasmids comprising genes encoding polysaccharases, in addition to the genes described above which code for the alcohol dehydrogenase and pyruvate decarboxylase. Further, methods are described for producing ethanol from oligomeric feedstock using the recombinant hosts described above. Also provided is a method for enhancing the production of functional proteins in a recombinant host comprising overexpressing an adhB gene in the host. Further provided are process designs for fermenting oligosaccharide-containing biomass to ethanol.

  2. Ethanol production by recombinant hosts

    DOE Patents [OSTI]

    Fowler, David E. (Gainesville, FL); Horton, Philip G. (Gainesville, FL); Ben-Bassat, Arie (Gainesville, FL)

    1996-01-01T23:59:59.000Z

    Novel plasmids comprising genes which code for the alcohol dehydrogenase and pyruvate decarboxylase are described. Also described are recombinant hosts which have been transformed with genes coding for alcohol dehydrogenase and pyruvate. By virtue of their transformation with these genes, the recombinant hosts are capable of producing significant amounts of ethanol as a fermentation product. Also disclosed are methods for increasing the growth of recombinant hosts and methods for reducing the accumulation of undesirable metabolic products in the growth medium of these hosts. Also disclosed are recombinant host capable of producing significant amounts of ethanol as a fermentation product of oligosaccharides and plasmids comprising genes encoding polysaccharases, in addition to the genes described above which code for the alcohol dehydrogenase and pyruvate decarboxylase. Further, methods are described for producing ethanol from oligomeric feedstock using the recombinant hosts described above. Also provided is a method for enhancing the production of functional proteins in a recombinant host comprising overexpressing an adhB gene in the host. Further provided are process designs for fermenting oligosaccharide-containing biomass to ethanol.

  3. Molecular Gas in Quasar Hosts

    E-Print Network [OSTI]

    Richard Barvainis

    1997-01-29T23:59:59.000Z

    The study of molecular gas in quasar host galaxies addresses a number of interesting questions pertaining to the hosts' ISM, to unified schemes relating quasars and IR galaxies, and to the processes fueling nuclear activity. In this contribution I review observations of molecular gas in quasar hosts from z=0.06 to z=4.7. The Cloverleaf quasar at z=2.5 is featured as a case where there are now enough detected transitions (four in CO, and one each in CI and HCN) to allow detailed modeling of physical conditions in the molecular ISM. We find that the CO-emitting gas is warmer, denser, and less optically thick than that found in typical Galactic molecular clouds. These differences are probably due to the presence of the luminous quasar in the nucleus of the Cloverleaf's host galaxy.

  4. Host a Meeting | Argonne National Laboratory

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Host a meeting Blue Jeans is a cloud-based video, web, and audio collaboration solution available to Argonne employees for hosting meetings. Blue Jeans works for both...

  5. Host Event Based Network Monitoring

    SciTech Connect (OSTI)

    Jonathan Chugg

    2013-01-01T23:59:59.000Z

    The purpose of INL抯 research on this project is to demonstrate the feasibility of a host event based network monitoring tool and the effects on host performance. Current host based network monitoring tools work on polling which can miss activity if it occurs between polls. Instead of polling, a tool could be developed that makes use of event APIs in the operating system to receive asynchronous notifications of network activity. Analysis and logging of these events will allow the tool to construct the complete real-time and historical network configuration of the host while the tool is running. This research focused on three major operating systems commonly used by SCADA systems: Linux, WindowsXP, and Windows7. Windows 7 offers two paths that have minimal impact on the system and should be seriously considered. First is the new Windows Event Logging API, and, second, Windows 7 offers the ALE API within WFP. Any future work should focus on these methods.

  6. Winds of Planet Hosting Stars

    E-Print Network [OSTI]

    Nicholson, B A; Brookshaw, L; Vidotto, A A; Carter, B D; Marsden, S C; Soutter, J; Waite, I A; Horner, J

    2015-01-01T23:59:59.000Z

    The field of exoplanetary science is one of the most rapidly growing areas of astrophysical research. As more planets are discovered around other stars, new techniques have been developed that have allowed astronomers to begin to characterise them. Two of the most important factors in understanding the evolution of these planets, and potentially determining whether they are habitable, are the behaviour of the winds of the host star and the way in which they interact with the planet. The purpose of this project is to reconstruct the magnetic fields of planet hosting stars from spectropolarimetric observations, and to use these magnetic field maps to inform simulations of the stellar winds in those systems using the Block Adaptive Tree Solar-wind Roe Upwind Scheme (BATS-R-US) code. The BATS-R-US code was originally written to investigate the behaviour of the Solar wind, and so has been altered to be used in the context of other stellar systems. These simulations will give information about the velocity, pressur...

  7. Avian Roosting Behavior and Vector-Host Contact Rates for West Nile Virus Hosts

    E-Print Network [OSTI]

    Janousek, William M.

    2012-01-01T23:59:59.000Z

    roosting height. Figure 2. Mean number of host-seeking Cx.pipiens and Cx. restuans mosquitoes collected per trap night5. Mean number of host-seeking Cx. pipiens and Cx. restuans

  8. Host conservatism, host shifts and diversification across three trophic levels in two Neotropical forests

    E-Print Network [OSTI]

    Feldman, Chris R

    adaptive radiations (Ehrlich & Raven, 1964; Sch- luter, 2000). Evidence for the importance of major host are characterized by small radiations of moths associated with unique host plants in the same geographic area (i

  9. Solid hosts for dye laser rods: Part 1, Criteria for choosing a host material

    SciTech Connect (OSTI)

    Erickson, G.F.

    1987-01-01T23:59:59.000Z

    This paper will attempt to provide selection criteria for polymers as hosts for flashlamp-pumped dye laser rods. The properties of transparent polymer materials are compared with typical inorganic crystal and glass hosts. 2 figs., 1 tab.

  10. Behavioral Interactions between Parasites and Hosts: Host Suicide and the Evolution of Complex Life Cycles

    E-Print Network [OSTI]

    Smith, Deborah R.

    1980-07-01T23:59:59.000Z

    by predation, thus preventing the maturation of its parasite and lowering the risk of parasitic infection for other members of the host specie^. If the mature parasite would have been more likely to infect the host's kin than nonkin, the host's suicidal... in reproductive success. Threatened with parasitic attack, the host梠r potential host梒an attempt to increase its reproductive fitness in two ways, which are not mutually exclusive. It can protect itself or it can protect its kin. Certain actions on the part...

  11. Sustainability transformations in Olympic host cities

    E-Print Network [OSTI]

    Mokrushina, Ksenia

    2012-01-01T23:59:59.000Z

    The Olympic Games represent an unparalleled fast-track urban development opportunity for Olympic host cities. Taking the premise that the transformational effect of the Olympics has a potential to drive long-term urban ...

  12. Secretary Chu Hosts FY 2012 Budget Briefing

    Broader source: Energy.gov [DOE]

    Secretary Chu hosted a media briefing on the Department's Fiscal Year 2012 Budget Request. You can watch video of the event and check out his PowerPoint presentation, or see the budget documents themselves.

  13. Secretary of Energy Advisory Board Hosts Conference Call on Shale...

    Energy Savers [EERE]

    of Energy Advisory Board Hosts Conference Call on Shale Gas Draft Report Secretary of Energy Advisory Board Hosts Conference Call on Shale Gas Draft Report November 10, 2011 -...

  14. Phosphine oxide derivatives as hosts for blue phosphors: A joint...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    oxide derivatives as hosts for blue phosphors: A joint theoretical and experimental study of their electronic Phosphine oxide derivatives as hosts for blue phosphors: A joint...

  15. Volvo Truck Headquarters in North Carolina to Host Event With...

    Energy Savers [EERE]

    Volvo Truck Headquarters in North Carolina to Host Event With Acting Under Secretary of Energy Majumdar Volvo Truck Headquarters in North Carolina to Host Event With Acting Under...

  16. Energy Secretary Ernest Moniz to Host First Schlesinger Medal...

    Energy Savers [EERE]

    Ernest Moniz to Host First Schlesinger Medal Ceremony and Energy Security Symposium Energy Secretary Ernest Moniz to Host First Schlesinger Medal Ceremony and Energy Security...

  17. MEDIA BRIEFING CONFERENCE CALL: Secretary Chu to Host Solar Energy...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    BRIEFING CONFERENCE CALL: Secretary Chu to Host Solar Energy Conference Call MEDIA BRIEFING CONFERENCE CALL: Secretary Chu to Host Solar Energy Conference Call February 4, 2011 -...

  18. Regional Geology: GIS Database for Alternative Host Rocks and...

    Energy Savers [EERE]

    Regional Geology: GIS Database for Alternative Host Rocks and Potential Siting Guidelines Regional Geology: GIS Database for Alternative Host Rocks and Potential Siting Guidelines...

  19. Secretary Chu to Host Conference Call Announcing the Winners...

    Energy Savers [EERE]

    to Host Conference Call Announcing the Winners of the America's Next Top Energy Innovator Challenge Secretary Chu to Host Conference Call Announcing the Winners of the America's...

  20. Senior Adviser Richard Kauffman to Host Live Chat on Renewable...

    Office of Environmental Management (EM)

    Senior Adviser Richard Kauffman to Host Live Chat on Renewable Energy Innovation and Deployment Senior Adviser Richard Kauffman to Host Live Chat on Renewable Energy Innovation and...

  1. Secretary Moniz Hosts Energy Security Symposium, Honors Dr. Daniel...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Hosts Energy Security Symposium, Honors Dr. Daniel Yergin with First James R. Schlesinger Medal for Energy Security Secretary Moniz Hosts Energy Security Symposium, Honors Dr....

  2. Sandia National Laboratories: Sandia to host PV Bankability workshop...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    ClimateECNews & EventsConferencesSandia to host PV Bankability workshop at Solar Power International (SPI) 2013 Sandia to host PV Bankability workshop at Solar Power International...

  3. A model for coupling within-host and between-host dynamics in an ...

    E-Print Network [OSTI]

    2011-12-20T23:59:59.000Z

    Abstract Studies on the modeling of the coupled dy- namics of infectious diseases at both the population level (the epidemic process or between-host dynamics).

  4. (New hosts and vectors for genome cloning)

    SciTech Connect (OSTI)

    Not Available

    1991-01-01T23:59:59.000Z

    The main goal of our project remains the development of new bacterial hosts and vectors for the stable propagation of human DNA clones in E. coli. During the past six months of our current budget period, we have (1) continued to develop new hosts that permit the stable maintenance of unstable features of human DNA, and (2) developed a series of vectors for (a) cloning large DNA inserts, (b) assessing the frequency of human sequences that are lethal to the growth of E. coli, and (c) assessing the stability of human sequences cloned in M13 for large-scale sequencing projects.

  5. DMBC: Domain Names & Web Hosting Domain Names

    E-Print Network [OSTI]

    Stowell, Michael

    DMBC: Domain Names & Web Hosting Domain Names Top Level Domains 路 .com 路 .net 路 .org 路 .edu 路 .gov.9% of the web-viewing audience is used to typing in. Chances are, a visitor will type in ".com" even if you tell and simple 路 Try to avoid dashes or underscores in the domain name unless there is no other option Web

  6. Beryllium abundances in stars hosting giant planets

    E-Print Network [OSTI]

    N. C. Santos; R. J. Garcia Lopez; G. Israelian; M. Mayor; R. Rebolo; A. Garcia-Gil; M. R. Perez de Taoro; S. Randich

    2002-02-25T23:59:59.000Z

    We have derived beryllium abundances in a wide sample of stars hosting planets, with spectral types in the range F7V-K0V, aimed at studying in detail the effects of the presence of planets on the structure and evolution of the associated stars. Predictions from current models are compared with the derived abundances and suggestions are provided to explain the observed inconsistencies. We show that while still not clear, the results suggest that theoretical models may have to be revised for stars with Teff<5500K. On the other hand, a comparison between planet host and non-planet host stars shows no clear difference between both populations. Although preliminary, this result favors a ``primordial'' origin for the metallicity ``excess'' observed for the planetary host stars. Under this assumption, i.e. that there would be no differences between stars with and without giant planets, the light element depletion pattern of our sample of stars may also be used to further investigate and constraint Li and Be depletion mechanisms.

  7. Host conservatism, host shifts and diversification across three trophic levels in two Neotropical forests

    E-Print Network [OSTI]

    Papaj, Daniel

    adaptive radiations (Ehrlich & Raven, 1964; Sch- luter, 2000). Evidence for the importance of major host. The moth璸lant associations in particular are characterized by small radiations of moths associated

  8. Host Plants of Xylosandrus mutilatus in Mississippi

    SciTech Connect (OSTI)

    Stone, W.D.; Nebeker, T.E. [Department of Entomology and Plant Pathology, Mississippi State University, Box 9775, Mississippi State, MS 39762 (United States); Gerard, P.D. [Experimental Statistics Unit, Mississippi State University, Box 9731, Mississippi State, MS 39762 (United States)

    2007-03-15T23:59:59.000Z

    Host range of Xylosandrus mutilatus (Blandford) in North America is reported here for the first time. Descriptive data such as number of attacks per host, size of stems at point of attacks, and height of attacks above ground are presented. Hosts observed in Mississippi were Acer rubrum L., Acer saccharum Marsh., Acer palmatum Thunb., Ostrya virginiana (Mill.) K. Koch., Cornus florida L., Fagus grandifolia Ehrh., Liquidamber styraciflua L., Carya spp., Liriodendron tulipifera L., Melia azedarach L., Pinus taeda L., Prunus serotina Ehrh., Prunus americana Marsh., Ulmus alata Michaux, and Vitus rotundifolia Michaux. Liquidamber styraciflua had significantly more successful attacks, significantly higher probability of attacks, and significantly higher number of adult beetles per host tree than did Carya spp., A. rubrum, and L. tulipifera. This information is relevant in determining the impact this exotic beetle may have in nurseries, urban areas, and other forestry systems where this beetle becomes established. (author) [Spanish] El rango de hospederos de Xylosandrus mutilatus (Blandford) en America del Norte esta reportado aqui por la primera vez. Se presentan datos descriptivos como el numero de ataques por hospederos, el tamano de los tallos en el punto de ataque y la altura por encima del nivel de tierra de los ataques. Los hospederos observados en el estado de Mississippi fueron Acer rubrum L., Acer saccharum Marsh., Acer palmatum Thunb., Ostrya virginiana (Mill.) K. Koch., Cornus florida L., Fagus grandifolia Ehrh., Liquidamber styraciflua L., Carya spp., Liriodendron tulipifera L., Melia azedarach L., Pinus taeda L., Prunus serotina Ehrh., Prunus americana Marsh., Ulmus alata Michaux y Vitus rotundifolia Michaux. Liquidamber styraciflua tuvo ataques significativamente mas exitosos, una probabilidad significativamente mas alta de ataques y un numero significativamente mayor de adultos de escarabajos por arbol hospedero que Carya spp., A. rubrum y L. tulipifera. Esta informacion es pertinente en determinar el impacto que pueda tener este escarabajo exotico en invernaderos, areas urbanas y otros sistemas forestales donde el escarabajo se establece. (author)

  9. Identification of host response signatures of infection.

    SciTech Connect (OSTI)

    Branda, Steven S.; Sinha, Anupama; Bent, Zachary

    2013-02-01T23:59:59.000Z

    Biological weapons of mass destruction and emerging infectious diseases represent a serious and growing threat to our national security. Effective response to a bioattack or disease outbreak critically depends upon efficient and reliable distinguishing between infected vs healthy individuals, to enable rational use of scarce, invasive, and/or costly countermeasures (diagnostics, therapies, quarantine). Screening based on direct detection of the causative pathogen can be problematic, because culture- and probe-based assays are confounded by unanticipated pathogens (e.g., deeply diverged, engineered), and readily-accessible specimens (e.g., blood) often contain little or no pathogen, particularly at pre-symptomatic stages of disease. Thus, in addition to the pathogen itself, one would like to detect infection-specific host response signatures in the specimen, preferably ones comprised of nucleic acids (NA), which can be recovered and amplified from tiny specimens (e.g., fingerstick draws). Proof-of-concept studies have not been definitive, however, largely due to use of sub-optimal sample preparation and detection technologies. For purposes of pathogen detection, Sandia has developed novel molecular biology methods that enable selective isolation of NA unique to, or shared between, complex samples, followed by identification and quantitation via Second Generation Sequencing (SGS). The central hypothesis of the current study is that variations on this approach will support efficient identification and verification of NA-based host response signatures of infectious disease. To test this hypothesis, we re-engineered Sandia's sophisticated sample preparation pipelines, and developed new SGS data analysis tools and strategies, in order to pioneer use of SGS for identification of host NA correlating with infection. Proof-of-concept studies were carried out using specimens drawn from pathogen-infected non-human primates (NHP). This work provides a strong foundation for large-scale, highly-efficient efforts to identify and verify infection-specific host NA signatures in human populations.

  10. THE MASS DISTRIBUTION OF SUBGIANT PLANET HOSTS

    SciTech Connect (OSTI)

    Lloyd, James P. [Department of Astronomy, Cornell University, Ithaca, NY (United States)

    2013-09-01T23:59:59.000Z

    High mass stars are hostile to Doppler measurements due to rotation and activity on the main-sequence, so RV searches for planets around massive stars have relied on evolved stars. A large number of planets have been found around evolved stars with M > 1.5 M{sub Sun }. To test the robustness of mass determinations, Lloyd compared mass distributions of planet hosting subgiants with distributions from integrating isochrones and concluded that it is unlikely the subgiant planet hosts are this massive, but rather that the mass inferences are systematically in error. The conclusions of Lloyd have been called in to question by Johnson et al., who show TRILEGAL-based mass distributions that disagree with the mass distributions in Lloyd, which they attribute to Malmquist bias. Johnson et al. argue that the very small spectroscopic observational uncertainties favor high masses, and there are a large number of high mass sub giants in RV surveys. However, in this Letter, it is shown that Malmquist bias does not impact the mass distributions, but the mass distribution is sensitive to Galaxy model. The relationship needed to reconcile the subgiant planet host masses with any model of the Galactic stellar population is implausible, and the conclusion of Lloyd that spectroscopic mass determinations of subgiants are likely to have been overestimated is robust.

  11. On Quasar Masses and Quasar Host Galaxies

    E-Print Network [OSTI]

    Ari Laor

    1998-07-27T23:59:59.000Z

    The mass of massive black holes in quasar cores can be deduced using the typical velocities of Hb-emitting clouds in the Broad Line Region (BLR) and the size of this region. However, this estimate depends on various assumptions and is susceptible to large systematic errors. The Hb-deduced black hole mass in a sample of 14 bright quasars is found here to correlate with the quasar host galaxy luminosity, as determined with the Hubble Space Telescope (HST). This correlation is similar to the black hole mass vs. bulge luminosity correlation found by Magorrian et al. in a sample of 32 nearby normal galaxies. The similarity of the two correlations is remarkable since the two samples involve apparently different types of objects and since the black hole mass estimates in quasars and in nearby galaxies are based on very different methods. This similarity provides a ``calibration'' of the Hb-deduced black hole mass estimate, suggesting it is accurate to +-0.5 on log scale. The similarity of the two correlations also suggests that quasars reside in otherwise normal galaxies, and that the luminosity of quasar hosts can be estimated to +-0.5 mag based on the quasar continuum luminosity and the Hb line width. Future imaging observations of additional broad-line active galaxies with the HST are required in order to explore the extent, slope, and scatter of the black hole mass vs. host bulge luminosity correlation in active galaxies.

  12. Resource Overbooking and Application Profiling in Shared Hosting Platforms *

    E-Print Network [OSTI]

    Urgaonkar, Bhuvan

    Resource Overbooking and Application Profiling in Shared Hosting Platforms * Bhuvan Urgaonkar for provisioning CPU and network resources in shared hosting platforms running potentially antagonistic third of overbooking resources in shared platforms, to maximize the platform yield: the revenue generated

  13. High power laser having a trivalent liquid host

    DOE Patents [OSTI]

    Ault, Earl R.

    2005-08-16T23:59:59.000Z

    A laser having a lasing chamber and a semiconductor pumping device with trivalent titanium ions dissolved in a liquid host within the lasing chamber. Since the host is a liquid, it can be removed from the optical cavity when it becomes heated avoiding the inevitable optical distortion and birefringence common to glass and crystal hosts.

  14. Lithium abundances in exoplanet-hosts stars

    E-Print Network [OSTI]

    M. Castro; S. Vauclair; O. Richard; N. C. Santos

    2008-03-20T23:59:59.000Z

    Exoplanet-host stars (EHS) are known to present surface chemical abundances different from those of stars without any detected planet (NEHS). EHS are, on the average, overmetallic compared to the Sun. The observations also show that, for cool stars, lithium is more depleted in EHS than in NEHS. The overmetallicity of EHS may be studied in the framework of two different scenarii. We have computed main sequence stellar models with various masses, metallicities and accretion rates. The results show different profiles for the lithium destruction according to the scenario. We compare these results to the spectroscopic observations of lithium.

  15. Spectral decomposition of broad-line agns and host galaxies

    SciTech Connect (OSTI)

    Vanden Berk, Daniel E.; Shen, Jiajian; /Penn State U., Astron. Astrophys.; Yip, Ching-Wa; /Pittsburgh U.; Schneider, Donald P.; /Penn State U., Astron. Astrophys.; Connolly,; /Pittsburgh U.; Burton, Ross E.; /Pittsburgh U. /Case Western Reserve U.; Jester, Sebastian; /Fermilab; Hall, Patrick B.; /York U., Canada; Szalay, Alex S.; /Johns Hopkins; Brinkmann, John; /Apache Point Observ.

    2005-09-01T23:59:59.000Z

    Using an eigenspectrum decomposition technique, we separate the host galaxy from the broad line active galactic nucleus (AGN) in a set of 4666 spectra from the Sloan Digital Sky Survey (SDSS), from redshifts near zero up to about 0.75. The decomposition technique uses separate sets of galaxy and quasar eigenspectra to efficiently and reliably separate the AGN and host spectroscopic components. The technique accurately reproduces the host galaxy spectrum, its contributing fraction, and its classification. We show how the accuracy of the decomposition depends upon S/N, host galaxy fraction, and the galaxy class. Based on the eigencoefficients, the sample of SDSS broad-line AGN host galaxies spans a wide range of spectral types, but the distribution differs significantly from inactive galaxies. In particular, post-starburst activity appears to be much more common among AGN host galaxies. The luminosities of the hosts are much higher than expected for normal early-type galaxies, and their colors become increasingly bluer than early-type galaxies with increasing host luminosity. Most of the AGNs with detected hosts are emitting at between 1% and 10% of their estimated Eddington luminosities, but the sensitivity of the technique usually does not extend to the Eddington limit. There are mild correlations among the AGN and host galaxy eigencoefficients, possibly indicating a link between recent star formation and the onset of AGN activity. The catalog of spectral reconstruction parameters is available as an electronic table.

  16. Fastbus host interface for VAX/VMS

    SciTech Connect (OSTI)

    Siskind, E.J.

    1983-02-01T23:59:59.000Z

    A list processing microprocessor controlled host interface for FASTBUS has been constructed by connection of a FASTBUS cable segment to the VAX DR-32 Device Interconnect (DDI) implemented via the DEC DR-780 channel on a VAX-11/780 system. Block transfer rates of 5.7 megabytes/second (700 ns per 32 bit longword) are achieved on VAX-11/780 systems equipped with a single MS-780 memory controller, while interleaved dual memory controller systems reach 8.0 megabytes/second (500 ns per longword) performance. The hardware and software interface should work equally well on DR-750 equipped VAX-11/750 systems (with appropriate reductions in achievable bandwidth) as well as on any future VAX systems equipped with a DDI adapter.

  17. ISO Observations of Quasars and Quasar Hosts

    E-Print Network [OSTI]

    Belinda J. Wilkes

    1997-01-23T23:59:59.000Z

    The Infrared Space Observatory (ISO), launched in November 1995, allows us to measure the far-infrared (far-IR) emission of quasars in greater detail and over a wider energy range than previously possible. In this paper, preliminary results in a study of the 5--200 $\\mu m$ continuum of quasars and active galaxies are presented. Comparison of the spectral energy distributions show that, if the far-IR emission from quasars is thermal emission from galaxian dust, the host galaxies of quasars must contain dust in quantities comparable to IR luminous galaxies rather than normal spiral galaxies. In the near-IR, the ISO data confirm an excess due to a warm `AGN-related' dust component, possibly from the putative molecular torus. We report detection of the high-redshift quasar, 1202-0727, in the near-IR indicating that it is unusually IR-bright compared with low-redshift quasars.

  18. Properties of SN-host galaxies

    E-Print Network [OSTI]

    F. Combes

    2003-08-08T23:59:59.000Z

    It is of prime importance to recognize evolution and extinction effects in supernovae results as a function of redshift, for SN Ia to be considered as distance indicators. This review surveys all observational data searching for an evolution and/or extinction, according to host morphology. For instance, it has been observed that high-z SNe Ia have bluer colours than the local ones: although this goes against extinction to explain why SN are dimmer with redshift until z ~ 1, supporting a decelerating universe, it also demonstrates intrinsic evolution effects. -- SNe Ia could evolve because the age and metallicity of their progenitors evolve. The main parameter is carbon abundance. Smaller C leads to a dimmer SN Ia and also less scatter on peak brightness, as it is the case in elliptical galaxy today. Age of the progenitor is an important factor: young populations lead to brighter SNe Ia, as in spiral galaxies, and a spread in ages lead to a larger scatter, explaining the observed lower scatter at high z. -- Selection biases also play a role, like the Malmquist bias; high-z SNe Ia are found at larger distance from their host center: there is more obscuration in the center, and also detection is easier with no contamination from the center. This might be one of the reason why less obscuration has been found for SNe Ia at high z. -- There is clearly a sample evolution with z: currently only the less bright SNe Ia are detected at high z, with less scatter. The brightest objects have a slowly declining light-curve, and at high z, no slow decline has been observed. This may be interpreted as an age effect, high-z SN having younger progenitors.

  19. Department of Energy Hosts Inaugural Energy Frontier Research...

    Office of Science (SC) Website

    News & Events DOE Announcements Department of Energy Hosts Inaugural Energy Frontier Research Center Summit Energy Frontier Research Centers (EFRCs) EFRCs Home Centers...

  20. Energy Department Hosts FORGE Webinar and Resource Reporting...

    Office of Environmental Management (EM)

    FORGE Webinar and Resource Reporting Methodology Workshop at the Upcoming National Geothermal Summit, August 4-5 Energy Department Hosts FORGE Webinar and Resource Reporting...

  1. NNSA hosts Illinois emergency responders during technical exchange...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Press Releases Video Gallery Photo Gallery Jobs Apply for Our Jobs Our Jobs Working at NNSA Blog Home NNSA Blog NNSA hosts Illinois emergency responders during technical ......

  2. Energy Secretary Moniz Will Host North American Energy Ministers...

    Energy Savers [EERE]

    Energy Secretary Ernest Moniz will host a trilateral meeting with Natural Resources Canada Minister Greg Rickford and Mexican Secretary of Energy Pedro Joaquin Coldwell. The...

  3. Department of Energy to Host Secretary of Energy Advisory Board...

    Energy Savers [EERE]

    of Energy will host a public meeting of the Secretary of Energy Advisory Board (SEAB) Natural Gas Subcommittee. The meeting will allow subcommittee members to hear...

  4. Sandia Energy - Sandia Will Host PV Bankability Workshop at Solar...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Will Host PV Bankability Workshop at Solar Power International (SPI) 2013 Home Renewable Energy Energy Facilities Grid Integration Partnership News Distribution Grid Integration...

  5. Importance-Scanning Worm Using Vulnerable-Host Distribution

    E-Print Network [OSTI]

    Ji, Chuanyi

    Importance-Scanning Worm Using Vulnerable-Host Distribution Zesheng Chen School of Electrical scanning. The distribution of vulnerable hosts on the Internet, however, is highly non- uniform over the IP-address space. This implies that random scanning wastes many scans on invulnerable addresses, and more virulent

  6. Methods for production of proteins in host cells

    DOE Patents [OSTI]

    Donnelly, Mark; Joachimiak, Andrzej

    2004-01-13T23:59:59.000Z

    The present invention provides methods for the production of proteins, particularly toxic proteins, in host cells. The invention provides methods which use a fusion protein comprising a chaperonin binding domain in host cells induced or regulated to have increased levels of chaperonin which binds the chaperonin binding domain.

  7. An Approach to the Automated Determination of Host Information Value

    SciTech Connect (OSTI)

    Beaver, Justin M [ORNL; Patton, Robert M [ORNL

    2011-01-01T23:59:59.000Z

    Enterprise networks are comprised of thousands of interconnected computer hosts, each of which is capable of creating, removing, and exchanging data according to the needs of their users. Thus, the distribution of high-value, sensitive, and proprietary information across enterprise networks is poorly managed and understood. A significant technology gap in information security is the inability to automatically quantify the value of the information contained on each host in a network. Such insight would allow an enterprise to scale its defenses, react intelligently to an intrusion, manage its configuration audits, and understand the leak potential in the event that a host is compromised. This paper outlines a novel approach to the automated determination of the value of the information contained on a host computer. It involves the classification of each text document on the host machine using the frequency of the document s terms and phrases. A host information value is computed using an enterprise-defined weighting schema and applying it to a host s document distribution. The method is adaptable to specific organizational information needs, requires manual intervention only during schema creation, and is repeatable and consistent regardless of changes in information on the host machines.

  8. Managing Server Energy and Operational Costs in Hosting Centers

    E-Print Network [OSTI]

    Lu, Jiaheng

    is the growing importance of energy/power consumption of these servers at the hosting centers, in termsManaging Server Energy and Operational Costs in Hosting Centers Yiyu Chen Dept. of IE Penn State.00. General Terms: Design, Performance Keywords: Energy Management, Performance Modeling, Feed- back Control

  9. Host galaxies and environment of BL Lac objects

    E-Print Network [OSTI]

    J. Heidt

    1998-12-14T23:59:59.000Z

    Since the last meeting on BL Lac objects 10 years ago, BL Lac host galaxies and their cluster environment have gained much attention. Hence, our current knowledge of the properties of BL Lac host galaxies and their cluster environment has improved considerably, which will be reviewed. The importance of future observing programs using (very) large telescopes is briefly outlined.

  10. Host virtualization: a taxonomy of management challenges Vitalian A. Danciu

    E-Print Network [OSTI]

    according to established conceptual management frameworks and juxtapose the result to a survey of currentHost virtualization: a taxonomy of management challenges Vitalian A. Danciu Munich Network Management Team Ludwig颅Maximilians颅Universit? at, Munich, Germany danciu@mnm颅team.org Abstract: Host

  11. Host virtualization: a taxonomy of management challenges Vitalian A. Danciu

    E-Print Network [OSTI]

    according to established conceptual management frameworks and juxtapose the result to a survey of currentHost virtualization: a taxonomy of management challenges Vitalian A. Danciu Munich Network Management Team Ludwig-Maximilians-Universit篓at, Munich, Germany danciu@mnm-team.org Abstract: Host

  12. Resource Overbooking and Application Profiling in Shared Hosting Platforms

    E-Print Network [OSTI]

    Massachusetts at Amherst, University of

    Resource Overbooking and Application Profiling in Shared Hosting Platforms #3; Bhuvan Urgaonkar resources in shared hosting platforms running potentially antagonistic third璸arty applications. The primary platforms, to maximize the platform yield: the revenue generated by the available resources. We do

  13. Improving Type Ia Supernova Standard Candle Cosmology Measurements Using Observations of Early-Type Host Galaxies

    E-Print Network [OSTI]

    Meyers, Joshua Evan

    2012-01-01T23:59:59.000Z

    Host Galaxies of Type Ia Supernovae Introduction SN Ia Hosts109 C HAPTER 1 Cosmology, Type Ia Supernovae and HostGalaxies Observations of supernovae have played a role in

  14. Cabbage : a new host of Sclerotinia sclerotiorum for Pakistan

    E-Print Network [OSTI]

    Paris-Sud XI, Universit de

    NOTE Cabbage : a new host of Sclerotinia sclerotiorum for Pakistan M. Siddique MIRZA Yasmin AHMAD National Agricultural Research Centre PARC, Islamabad, Pakistan. SUMMARY Sclerotinia rot of cabbage, Sclerotinia, identification, pathogenicity, Pakistan. R蒘UM Le chou, un nouvel h魌e de Sclerotinia

  15. Jefferson Lab hosts 19 schools for Virginia Regional High School...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    hosts 19 schools for Virginia Regional High School Science Bowl on Feb. 10 January 30, 2007 Some of the brightest young minds in the Commonwealth will meet at the Department of...

  16. Jefferson Lab hosts 22 teams for Virginia High School Science...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    of the Jefferson Lab Science Bowl logo. Jefferson Lab hosts 22 teams for Virginia High School Science Bowl on Feb. 12 February 1, 2005 Some of the brightest young minds in the...

  17. DOE Hosts Solid-State Lighting Commercial Product Testing Program...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Department of Energy (DOE) hosted a workshop on October 27, 2006, to introduce the DOE SSL Commercial Product Testing Program. The workshop, held in Washington, D.C., drew over...

  18. Host/virus interactions in the marine cyanobacterium prochlorococcus

    E-Print Network [OSTI]

    Frois-Moniz, Katya

    2014-01-01T23:59:59.000Z

    Bacterial viruses shape the diversity, metabolic function, and community dynamics of their microbial hosts. As microbes drive many major biogeochemical cycles, viral infection is therefore a phenomenon of global significance. ...

  19. Host nation security force development : a new roadmap

    E-Print Network [OSTI]

    Fitzgerald, Shawn (Shawn Michael)

    2013-01-01T23:59:59.000Z

    A new model concerning the concepts of host nation security force development, or security sector reform (SSR), is proposed. This model is rooted in scholarly literature and seeks to fill current gaps in United States Army ...

  20. Controls on Fault-Hosted Fluid Flow: Preliminary Results from...

    Open Energy Info (EERE)

    Geothermal Field, CA Jump to: navigation, search OpenEI Reference LibraryAdd to library Conference Proceedings: Controls on Fault-Hosted Fluid Flow: Preliminary Results from the...

  1. Interfacial assembly of dendritic microcapsules with host-guest chemistry

    E-Print Network [OSTI]

    Zheng, Yu; Yu, Ziyi; Parker, Richard M.; Wu, Yuchao; Abell, Chris; Scherman, Oren A.

    2014-12-16T23:59:59.000Z

    with functional groups at a water朿hloroform interface using microfluidic technology. Two polymeric layers can be assembled and disassembled at the droplet interface using the efficiency of cucurbit[8]uril (CB[8]) host杇uest supramolecular chemistry...

  2. Evolution of parasite virulence when host responses cause disease

    E-Print Network [OSTI]

    Day, Troy; Graham, Andrea; Read, Andrew F

    The trade-off hypothesis of virulence evolution rests on the assumption that infection-induced mortality is a consequence of host exploitation by parasites. This hypothesis lies at the heart of many empirical and theoretical ...

  3. Acting Biomass Program Manager Dr. Valerie Reed to Host Live...

    Broader source: Energy.gov (indexed) [DOE]

    December 16th, the Energy Department (@energy) will be hosting a live Twitter Q&A on biofuels with Dr. Valerie Reed, Acting Manager of the Biomass Program. Dr. Reed holds a Ph. D....

  4. Energy and Interior Departments Host Offshore Energy Knowledge...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Related Articles DOE to Host a Booth at Offshore WINDPOWER Wind Program Newsletter: Second Quarter 2012 DOE-DOI Strategy Seeks to Harness U.S. Offshore Wind Energy Potential...

  5. Host nutrition and infectious disease: an ecological view

    E-Print Network [OSTI]

    Smith, Val H.; Jones II, Tyrees P.; Smith, Marilyn S.

    2005-06-01T23:59:59.000Z

    Nutrition is typically discussed in terms of maintaining a proper diet and avoiding nutrient deficiency diseases. However, nutrition can also be viewed from an ecological standpoint: mammalian hosts and their pathogens ...

  6. Radio Afterglows and Host Galaxies of Gamma-Ray Bursts

    E-Print Network [OSTI]

    Li, Long-Biao; Huang, Yong-Feng; Wu, Xue-Feng; Kong, Si-Wei; Li, Di; Chang, Heon-Young; Choi, Chul-Sung

    2015-01-01T23:59:59.000Z

    Considering the contribution of the emission from the host galaxies of gamma-ray bursts (GRBs) to the radio afterglows, we investigate the effect of host galaxies on observations statistically. For the three types of events, e.g. low-luminosity, standard and high-luminosity GRBs, it is found that a tight correlation exists between the ratio of the radio flux (RRF) of host galaxy to the total radio peak emission and the observational frequency. Especially, toward lower frequencies, the contribution from the host increases significantly. The correlation can be used to get a useful estimate for the radio brightness of those host galaxies which only have very limited radio afterglow data. Using this prediction, we re-considered the theoretical radio afterglow light curves for four kinds of events, i.e. high-luminosity, low-luminosity, standard and failed GRBs, taking into account the contribution from the host galaxies and aiming at exploring the detectability of these events by the Five-hundred-meter Aperture Sp...

  7. Emerging disease dynamics in a model coupling within-host and ...

    E-Print Network [OSTI]

    Xiuli Cen

    2014-08-27T23:59:59.000Z

    Aug 2, 2014 ... Immunological models consider the within-host dynamics independent of the interactions between hosts (e.g., De Leenheer and Smith, 2003;.

  8. Expression profile of host restriction factors in HIV-1 elite controllers

    E-Print Network [OSTI]

    2013-01-01T23:59:59.000Z

    et al. : Expression profile of host restriction factors inOpen Access Expression profile of host restriction factorsthat a transcriptional profile signature of CD4+ T cells is

  9. Molecular Comparison and DNA Fingerprinting of Sporisorium reilianum and Peronosclerospora sorghi Relating to Host Specificity and Host Resistance

    E-Print Network [OSTI]

    Radwan, Ghada Lotfy Hassan Elhefny

    2013-02-28T23:59:59.000Z

    on host and race specificity. MATERIALS AND METHODS Head smut isolates A total of 44 isolates of S. reilianum sorghum isolates, collected in 2004, 2006, 2009 and 2011 from different locations in Texas (Corpus Christi, Weslaco, and College Station...

  10. The Mass Dependence Between Protoplanetary Disks and their Stellar Hosts

    E-Print Network [OSTI]

    Andrews, Sean M; Kraus, Adam L; Wilner, David J

    2013-01-01T23:59:59.000Z

    We present a substantial extension of the mm-wave continuum photometry catalog for Taurus circumstellar dust disks. Combining new Submillimeter Array data with measurements in the literature, we construct a mm-wave luminosity distribution for Class II disks that is statistically complete for stellar hosts with spectral types earlier than M8.5 and has a (3-sigma) depth of ~3 mJy. The resulting census eliminates a longstanding bias against disks with late-type hosts, and thereby reveals a strong correlation between L_mm and the host spectral type. We confirm that this corresponds to a statistically robust relationship between the masses of dust disks and the stars that host them. A Bayesian regression technique is used to characterize these relationships: the results indicate a typical 1.3 mm flux density of 25 mJy for solar mass hosts and a power-law scaling L_mm \\propto M_star^1.5-2.0. We suggest that a reasonable treatment of dust temperature in the conversion from L_mm to M_disk favors an inherently linear ...

  11. Effects of internal mineral structures on the magnetic remanence of silicate-hosted titanomagnetite inclusions

    E-Print Network [OSTI]

    Dunin-Borkowski, Rafal E.

    Effects of internal mineral structures on the magnetic remanence of silicate-hosted titanomagnetite epitaxially by exsolution from their host silicate. Close examination of clinopyroxene- hosted inclusions of silicate-hosted titanomagnetite inclusions: An electron holography study, J. Geophys. Res., 111, B12S15

  12. Understanding host-acceptance behavior and larval feeding of the parasitic wasp Melittobia digitata (Hymenoptera: Eulophidae) to facilitate rearing on an artificial host

    E-Print Network [OSTI]

    Cooperband, Miriam Faith

    1998-01-01T23:59:59.000Z

    , M digitata was found to oviposit on artificial hosts, Parafilm(& domes containing artificial diet. It was determined that females preferred artificial hosts containing the agar-based diet to those containing only agar. Further testing ruled out...

  13. QSO HOST GALAXIES AT Z=2.3

    E-Print Network [OSTI]

    J. B. Hutchings

    1995-06-02T23:59:59.000Z

    Images are discussed of six QSOs at z=2.3, one QSO-like IRAS source at z=2.3, and one QSO at z=1.1, taken with resolution 0.6 to 0.9 arcsec. Five of the QSOs are radio-quiet. All QSOs except one are just resolved, while the IRAS source has definite structure. In some cases, part of the QSO fuzz appears to be a close companion rather than a concentric host galaxy. The luminosities implied for the hosts or companions are typical of bright galaxies with young hot star populations. Radio-quiet QSOs appear to have host galaxies less luminous by ~2 magnitudes than radio-loud QSOs.

  14. Host galaxies of z ~ 4.7 QSOs

    E-Print Network [OSTI]

    J. B. Hutchings

    2002-12-20T23:59:59.000Z

    2 micron broad- and narrow-band imaging with the Gemini-N telescope of five z~4.7 QSOs, has resolved both the host galaxies and [O II] emission-line gas. The resolved fluxes of the host galaxies fall within the extrapolated spread of the K-z relationship for radio galaxies at lower redshifts, and their resolved morphology is irregular. The [O II] images indicate knots coincident with many continuum features and also some bright jet-like features near the nucleus. The line emission total fluxes indicate overall equivalent widths of 5 to 10 A at rest wavelengths. Two of the QSOs are in a local environment of faint galaxies of similar magnitude to the hosts, and three have nearby galaxies with excess narrow-band flux, which would be [O II] if they are at the QSO redshift.

  15. [New hosts and vectors for genome cloning]. Progress report

    SciTech Connect (OSTI)

    Not Available

    1991-12-31T23:59:59.000Z

    The main goal of our project remains the development of new bacterial hosts and vectors for the stable propagation of human DNA clones in E. coli. During the past six months of our current budget period, we have (1) continued to develop new hosts that permit the stable maintenance of unstable features of human DNA, and (2) developed a series of vectors for (a) cloning large DNA inserts, (b) assessing the frequency of human sequences that are lethal to the growth of E. coli, and (c) assessing the stability of human sequences cloned in M13 for large-scale sequencing projects.

  16. Cell Host & Microbe Durable Protection from Herpes Simplex Virus-2

    E-Print Network [OSTI]

    Lieberman, Judy

    Cell Host & Microbe Article Durable Protection from Herpes Simplex Virus-2 Transmission Following is a problem. Intravaginal administration of small interfering RNA (siRNA) lipoplexes targeting Herpes Simplex protection against viral transmission. INTRODUCTION Genital Herpes Simplex Virus 2 (HSV-2) infection causes

  17. Engineering Challenge Camp Hosted by the West Virginia University

    E-Print Network [OSTI]

    Mohaghegh, Shahab

    4th and 5th Grade Engineering Challenge Camp Hosted by the West Virginia University Benjamin M. Statler College of Engineering and Mineral Resources and sponsored in part by Halliburton, AEP and Axiall Industries. July 28-August 1, 2014 Monday, July 28, 2014-- Up, Up and Away Day (Aerospace Engineering) Time

  18. Engineering Challenge Camp Hosted by the West Virginia University

    E-Print Network [OSTI]

    Mohaghegh, Shahab

    1st , 2nd , and 3rd Grade Engineering Challenge Camp Hosted by the West Virginia University Benjamin M. Statler College of Engineering & Mineral Resources and sponsored in part by Halliburton, Axiall, July 28, 2014-- Up, Up and Away Day (Aerospace Engineering) Time Activity Place Led By 8:30-8:45 a

  19. Cell Host & Microbe Actin and Intermediate Filaments Stabilize

    E-Print Network [OSTI]

    Valdivia, Raphael

    Cell Host & Microbe Article Actin and Intermediate Filaments Stabilize the Chlamydia trachomatis inclusions within a cell leading to the highest yield of EBs (Wilson et al., 2006). The expansion of inclu- sions is likely fueled by the acquisition of membrane lipids from Golgi-derived vesicles (Carabeo et al

  20. Scleral Reinforcement Through Host Tissue Integration with Biomimetic Enzymatically Degradable

    E-Print Network [OSTI]

    Healy, Kevin Edward

    . Wildsoet, O.D., Ph.D.1 Enzymatically degradable semi-interpenetrating polymer networks (edsIPNs) were Polymer Network James Su, M.Eng.,1 Samuel T. Wall, Ph.D.,2 Kevin E. Healy, Ph.D.,2,3 and Christine FScleral Reinforcement Through Host Tissue Integration with Biomimetic Enzymatically Degradable Semi-Interpenetrating

  1. and Co-Host Riverside Electric Vehicle Day

    E-Print Network [OSTI]

    Mills, Allen P.

    and Co-Host Riverside Electric Vehicle Day Where: UC Riverside | CE-CERT, 1084 Columbia Ave, 92507 renewable sourc- es, efficiently use electric transporta- tion through advanced vehicles and im- prove our million electric vehi- cles on California's roads by 2023 and to ensure that low-income communities, which

  2. Continuous Time Bayesian Networks for Host Level Network Intrusion Detection

    E-Print Network [OSTI]

    Shelton, Christian R.

    R. Shelton Department of Computer Science and Engineering University of California, Riverside continuous time Bayesian networks learned from historic non-attack data and flag future event sequences whose. In this paper, we look at the problem of detecting such attacks at the host level. Instead of constructing

  3. page 1 11 June 2008 Hosted by World Robotics 2008

    E-Print Network [OSTI]

    De Luca, Alessandro

    June 2008 Hosted by Industrial robots are meeting the changing demands of their customers Total world supply of industrial robots up to 2007 Distribution in the main regions (Americas, Asia, Europe robots operating Estimated worldwide operational stock of industrial robots 3 66 454 605 750 923 951 994

  4. Intracellular invasion of green algae in a salamander host

    E-Print Network [OSTI]

    Intracellular invasion of green algae in a salamander host Ryan Kerneya,1 , Eunsoo Kimb , Roger P) and green algae ("Oophila amblystomatis" Lamber ex Printz) has been considered an ectosymbiotic mutu- alism tracts, consistent with oviductal transmission of algae from one salamander generation to the next

  5. Research Focus Delicious poison: genetics of Drosophila host plant

    E-Print Network [OSTI]

    Pierce, Naomi E.

    perception could be a tar- get of natural selection during host specialization. Five papers using data from in the generalist sister species. Both studies also report higher rates of amino acid changing substitutions observes more gene losses and elevated rates of amino acid substitutions in specialist species. However

  6. Community Police Academy Hosted By: University of Delaware Police

    E-Print Network [OSTI]

    Firestone, Jeremy

    Community Police Academy Hosted By: University of Delaware Police When: Wednesdays, 6:00 p.m. - 9:00 p.m. (March 4th through April 29th , 2015) Where: 413 Academy Street Newark DE 19716 - University should I expect to learn: The Community Police Academy (CPA) is an informative learning process

  7. Host life history responses to parasitism Philip Agnewa

    E-Print Network [OSTI]

    -specific growth, reproduction and survival [1, 2]. Life history theory aims to understand how these traits, reproduction and survival. These effects are often not immediate, but increase with time since infection and survival. This review illustrates this argument with several empirical studies showing hosts behaving

  8. Japan Denies Report It Dropped Proposal to Host Fusion Reactor

    E-Print Network [OSTI]

    Print Japan Denies Report It Dropped Proposal to Host Fusion Reactor June 22 (Bloomberg) -- Japan fusion reactor, a decision that would end a standoff with France to site the 4.6 billion-euro ($5 the International Thermonuclear Experimental Reactor in return for assurances it will manage the project in France

  9. ISO Observations of Quasars and Quasar Hosts Belinda J. Wilkes

    E-Print Network [OSTI]

    Wilkes, Belinda

    ISO Observations of Quasars and Quasar Hosts Belinda J. Wilkes Smithsonian Astrophysical Observatory, 60 Garden St., Cambridge, MA 02138, USA Abstract. The Infrared Space Observatory (ISO), launched spiral galaxies. In the near璉R, the ISO data confirm an excess due to a warm `AGN璻elated' dust

  10. Integrated Detection of Pathogens and Host Biomarkers for Wounds

    SciTech Connect (OSTI)

    Jaing, C

    2012-03-19T23:59:59.000Z

    The increasing incidence and complications arising from combat wounds has necessitated a reassessment of methods for effective treatment. Infection, excessive inflammation, and incidence of drug-resistant organisms all contribute toward negative outcomes for afflicted individuals. The organisms and host processes involved in wound progression, however, are incompletely understood. We therefore set out, using our unique technical resources, to construct a profile of combat wounds which did or did not successfully resolve. We employed the Lawrence Livermore Microbial Detection Array and identified a number of nosocomial pathogens present in wound samples. Some of these identities corresponded with bacterial isolates previously cultured, while others were not obtained via standard microbiology. Further, we optimized proteomics protocols for the identification of host biomarkers indicative of various stages in wound progression. In combination with our pathogen data, our biomarker discovery efforts will provide a profile corresponding to wound complications, and will assist significantly in treatment of these complex cases.

  11. Metal binding proteins, recombinant host cells and methods

    DOE Patents [OSTI]

    Summers, Anne O.; Caguiat, Jonathan J.

    2004-06-15T23:59:59.000Z

    The present disclosure provides artificial heavy metal binding proteins termed chelons by the inventors. These chelons bind cadmium and/or mercuric ions with relatively high affinity. Also disclosed are coding sequences, recombinant DNA molecules and recombinant host cells comprising those recombinant DNA molecules for expression of the chelon proteins. In the recombinant host cells or transgenic plants, the chelons can be used to bind heavy metals taken up from contaminated soil, groundwater or irrigation water and to concentrate and sequester those ions. Recombinant enteric bacteria can be used within the gastrointestinal tracts of animals or humans exposed to toxic metal ions such as mercury and/or cadmium, where the chelon recombinantly expressed in chosen in accordance with the ion to be rededicated. Alternatively, the chelons can be immobilized to solid supports to bind and concentrate heavy metals from a contaminated aqueous medium including biological fluids.

  12. Linking Short Gamma Ray Bursts and their Host Galaxies

    E-Print Network [OSTI]

    James E. Rhoads

    2008-07-16T23:59:59.000Z

    The luminosities of short gamma ray burst host galaxies are anticorrelated with both the isotropic equivalent gamma ray energy and the gamma ray luminosity of the explosions. Observational selection effects only strengthen the significance of this correlation. The correlation may indicate that there are two physically distinct groups of SGRBs. If so, it requires that the more luminous class of explosions be associated with the younger class of progenitors. Alternatively, it could be due to a continuous distribution of burst and host properties. As one possible explanation, we find that the effect of binary neutron star masses on inspiral time and energy reservoir produces a correlation of the appropriate sign, but does not automatically reproduce the correlation slope or the full range of SGRB energy scales. Any future model of SGRB progenitors needs to reproduce this correlation.

  13. Supplement 20, Part 7, Parasite-Subject Catalogue: Hosts

    E-Print Network [OSTI]

    Shaw, Judith H.; Edwards, Shirley J.; Rayburn, Jane D.; Tolson, Deborah A.; Hood, Martha W.

    1976-01-01T23:59:59.000Z

    . In other words, when using the Parasite-Subject Catalogues, it wTill be necessary to consult the Author Catalogue for complete bibliographical information. The following are the parts of each supplement : Part 1, Authors: A-Z Part 2, Parasite... SUPPLEMENT 20, PART 7 PARASITE-SUBJECT CATALOGUE : HOSTS By DEBORAH A. TOLSON, Biological Laboratory Technician MARTHA W. HOOD, Zoologist JUDITH H. SHAW, Zoologist JANE D. RAYBURN, Technical Information Specialist SHIRLEY J. EDWARDS, Supervisory...

  14. Recombinant host cells and media for ethanol production

    DOE Patents [OSTI]

    Wood, Brent E; Ingram, Lonnie O; Yomano, Lorraine P; York, Sean W

    2014-02-18T23:59:59.000Z

    Disclosed are recombinant host cells suitable for degrading an oligosaccharide that have been optimized for growth and production of high yields of ethanol, and methods of making and using these cells. The invention further provides minimal media comprising urea-like compounds for economical production of ethanol by recombinant microorganisms. Recombinant host cells in accordance with the invention are modified by gene mutation to eliminate genes responsible for the production of unwanted products other than ethanol, thereby increasing the yield of ethanol produced from the oligosaccharides, relative to unmutated parent strains. The new and improved strains of recombinant bacteria are capable of superior ethanol productivity and yield when grown under conditions suitable for fermentation in minimal growth media containing inexpensive reagents. Systems optimized for ethanol production combine a selected optimized minimal medium with a recombinant host cell optimized for use in the selected medium. Preferred systems are suitable for efficient ethanol production by simultaneous saccharification and fermentation (SSF) using lignocellulose as an oligosaccharide source. The invention also provides novel isolated polynucleotide sequences, polypeptide sequences, vectors and antibodies.

  15. Lithium depletion and the rotational history of exoplanet host stars

    E-Print Network [OSTI]

    Jerome Bouvier

    2008-09-03T23:59:59.000Z

    Israelian et al. (2004) reported that exoplanet host stars are lithium depleted compared to solar-type stars without detected massive planets, a result recently confirmed by Gonzalez (2008). We investigate whether enhanced lithium depletion in exoplanet host stars may result from their rotational history. We have developed rotational evolution models for slow and fast solar-type rotators from the pre-main sequence (PMS) to the age of the Sun and compare them to the distribution of rotational periods observed for solar-type stars between 1 Myr and 5 Gyr. We show that slow rotators develop a high degree of differential rotation between the radiative core and the convective envelope, while fast rotators evolve with little core-envelope decoupling. We suggest that strong differential rotation at the base of the convective envelope is responsible for enhanced lithium depletion in slow rotators. We conclude that lithium-depleted exoplanet host stars were slow rotators on the zero-age main sequence (ZAMS) and argue that slow rotation results from a long lasting star-disk interaction during the PMS. Altogether, this suggests that long-lived disks (> 5 Myr) may be a necessary condition for massive planet formation/migration.

  16. Crystallizing Membrane Proteins in Lipidic Mesophases. A Host Lipid Screen

    SciTech Connect (OSTI)

    Li, Dianfan; Lee, Jean; Caffrey, Martin (Trinity); (Limerick)

    2011-11-30T23:59:59.000Z

    The default lipid for the bulk of the crystallogenesis studies performed to date using the cubic mesophase method is monoolein. There is no good reason, however, why this 18-carbon, cis-monounsaturated monoacylglycerol should be the preferred lipid for all target membrane proteins. The latter come from an array of biomembrane types with varying properties that include hydrophobic thickness, intrinsic curvature, lateral pressure profile, lipid and protein makeup, and compositional asymmetry. Thus, it seems reasonable that screening for crystallizability based on the identity of the lipid creating the hosting mesophase would be worthwhile. For this, monoacylglycerols with differing acyl chain characteristics, such as length and olefinic bond position, must be available. A lipid synthesis and purification program is in place in the author's laboratory to serve this need. In the current study with the outer membrane sugar transporter, OprB, we demonstrate the utility of host lipid screening as a means for generating diffraction-quality crystals. Host lipid screening is likely to prove a generally useful strategy for mesophase-based crystallization of membrane proteins.

  17. DOE and Chinese Ministry of Science and Technology Co-Host First...

    Energy Savers [EERE]

    DOE and Chinese Ministry of Science and Technology Co-Host First Ever Electric Vehicle Forum DOE and Chinese Ministry of Science and Technology Co-Host First Ever Electric Vehicle...

  18. Chytrid fungus Batrachochytrium dendrobatidis has nonamphibian hosts and releases chemicals that cause

    E-Print Network [OSTI]

    Johnson, Pieter

    for a pathogen, some can serve as res- ervoir hosts. Reservoir hosts can sustain the parasite when par- ticular abandoned after Rowley et al. (17) retracted their initial report of the de- tection of B. dendrobatidis

  19. TODAY: ARPA-E Director Arun Majumdar to Host Live Chat on Reducing...

    Office of Environmental Management (EM)

    TODAY: ARPA-E Director Arun Majumdar to Host Live Chat on Reducing America's Oil Dependence Through Innovation TODAY: ARPA-E Director Arun Majumdar to Host Live Chat on Reducing...

  20. Arkansas Natural Gas Company Hosts Tour With U.S. Deputy Secretary...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Arkansas Natural Gas Company Hosts Tour With U.S. Deputy Secretary of Energy Poneman Arkansas Natural Gas Company Hosts Tour With U.S. Deputy Secretary of Energy Poneman February...

  1. April 16, 2012 GEOSHARE: Geospatial Open Source Hosting of Agriculture, Resource &

    E-Print Network [OSTI]

    Ginzel, Matthew

    April 16, 2012 GEOSHARE: Geospatial Open Source Hosting of the key recommendations in its recently launched report. The geospatial data

  2. Differential introgression causes genealogical discordance in host races of Acrocercops transecta (Insecta: Lepidoptera)

    E-Print Network [OSTI]

    Yoshizawa, Kazunori

    1 Differential introgression causes genealogical discordance in host races of Acrocercops transecta@nibb.ac.jp KY: psocid@res.agr.hokudai.ac.jp Running title: Genealogical discordance in host races #12;2 Abstract the Lyonia race from the Juglnas race, whereas the Tpi, Per and Ldh genealogies did not reflect the two host

  3. Comparison of Field Galaxy and Supernovae Host Galaxy Properties Rachael Merritt

    E-Print Network [OSTI]

    Cinabro, David

    of the thermonuclear and core collapse hosts, this project confirms that field properties fall between supernova host properties. #12;2 Introduction: In 2011, Joel Williams compared properties of thermonuclear (type I) and core Smith and Matthew Taylor, Williams' sample consisted of 34 thermonuclear and 75 core collapse hosts

  4. THE MASS DEPENDENCE BETWEEN PROTOPLANETARY DISKS AND THEIR STELLAR HOSTS

    SciTech Connect (OSTI)

    Andrews, Sean M.; Rosenfeld, Katherine A.; Kraus, Adam L.; Wilner, David J., E-mail: sandrews@cfa.harvard.edu [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States)

    2013-07-10T23:59:59.000Z

    We present a substantial extension of the millimeter (mm) wave continuum photometry catalog for circumstellar dust disks in the Taurus star-forming region, based on a new ''snapshot'' {lambda} = 1.3 mm survey with the Submillimeter Array. Combining these new data with measurements in the literature, we construct a mm-wave luminosity distribution, f(L{sub mm}), for Class II disks that is statistically complete for stellar hosts with spectral types earlier than M8.5 and has a 3{sigma} depth of roughly 3 mJy. The resulting census eliminates a longstanding selection bias against disks with late-type hosts, and thereby demonstrates that there is a strong correlation between L{sub mm} and the host spectral type. By translating the locations of individual stars in the Hertzsprung-Russell diagram into masses and ages, and adopting a simple conversion between L{sub mm} and the disk mass, M{sub d} , we confirm that this correlation corresponds to a statistically robust relationship between the masses of dust disks and the stars that host them. A Bayesian regression technique is used to characterize these relationships in the presence of measurement errors, data censoring, and significant intrinsic scatter: the best-fit results indicate a typical 1.3 mm flux density of {approx}25 mJy for 1 M{sub Sun} hosts and a power-law scaling L{sub mm}{proportional_to}M{sub *}{sup 1.5-2.0}. We suggest that a reasonable treatment of dust temperature in the conversion from L{sub mm} to M{sub d} favors an inherently linear M{sub d} {proportional_to}M{sub *} scaling, with a typical disk-to-star mass ratio of {approx}0.2%-0.6%. The measured rms dispersion around this regression curve is {+-}0.7 dex, suggesting that the combined effects of diverse evolutionary states, dust opacities, and temperatures in these disks imprint a full width at half-maximum range of a factor of {approx}40 on the inferred M{sub d} (or L{sub mm}) at any given host mass. We argue that this relationship between M{sub d} and M{sub *} likely represents the origin of the inferred correlation between giant planet frequency and host star mass in the exoplanet population, and provides some basic support for the core accretion model for planet formation. Moreover, we caution that the effects of incompleteness and selection bias must be considered in comparative studies of disk evolution, and illustrate that fact with statistical comparisons of f(L{sub mm}) between the Taurus catalog presented here and incomplete subsamples in the Ophiuchus, IC 348, and Upper Sco young clusters.

  5. Limits to the potential distribution of light brown apple moth in Arizona朇alifornia based on climate suitability and host plant availability

    E-Print Network [OSTI]

    Gutierrez, Andrew Paul; Mills, Nicholas J.; Ponti, Luigi

    2010-01-01T23:59:59.000Z

    and host plant availability Andrew Paul Gutierrez Nicholasthrough host plant availability. Outside of irrigated crops,non limiting host plant availability. A regional analysis of

  6. Monitoring and Modeling Non-Point Source Contributions of Host-Specific Fecal Contamination in San Pablo Bay

    E-Print Network [OSTI]

    Wuertz, Stefan; Bombardelli, Fabian A; Sirikanchana, Kwanrawee; Wang, Dan

    2009-01-01T23:59:59.000Z

    Host-Specific Fecal Contamination in San Pablo Bay Principlelivestock sources of fecal contamination in Kenya with host-Huang. Abstract Fecal contamination from non-point sources

  7. Type Ia supernova Hubble residuals and host-galaxy properties

    SciTech Connect (OSTI)

    Kim, A. G.; Aldering, G.; Aragon, C.; Bailey, S.; Fakhouri, H. K. [Physics Division, Lawrence Berkeley National Laboratory, 1 Cyclotron Road, Berkeley, CA 94720 (United States); Antilogus, P.; Bongard, S.; Canto, A.; Cellier-Holzem, F.; Fleury, M.; Guy, J. [Laboratoire de Physique Nucl閍ire et des Hautes 蒼ergies, Universit Pierre et Marie Curie Paris 6, Universit Paris Diderot Paris 7, CNRS-IN2P3, 4 place Jussieu, F-75252 Paris Cedex 05 (France); Baltay, C. [Department of Physics, Yale University, New Haven, CT 06250-8121 (United States); Buton, C.; Feindt, U.; Greskovic, P.; Kowalski, M. [Physikalisches Institut, Universit鋞 Bonn, Nu遖llee 12, D-53115 Bonn (Germany); Childress, M. [Research School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611 (Australia); Chotard, N.; Copin, Y.; Gangler, E. [Universit de Lyon, F-69622 Lyon (France); Universit de Lyon 1, Villeurbanne (France); CNRS/IN2P3, Institut de Physique Nucl閍ire de Lyon (France); and others

    2014-03-20T23:59:59.000Z

    Kim et al. introduced a new methodology for determining peak-brightness absolute magnitudes of type Ia supernovae from multi-band light curves. We examine the relation between their parameterization of light curves and Hubble residuals, based on photometry synthesized from the Nearby Supernova Factory spectrophotometric time series, with global host-galaxy properties. The K13 Hubble residual step with host mass is 0.013 0.031 mag for a supernova subsample with data coverage corresponding to the K13 training; at <<1?, the step is not significant and lower than previous measurements. Relaxing the data coverage requirement of the Hubble residual step with the host mass is 0.045 0.026 mag for the larger sample; a calculation using the modes of the distributions, less sensitive to outliers, yields a step of 0.019 mag. The analysis of this article uses K13 inferred luminosities, as distinguished from previous works that use magnitude corrections as a function of SALT2 color and stretch parameters: steps at >2? significance are found in SALT2 Hubble residuals in samples split by the values of their K13 x(1) and x(2) light-curve parameters. x(1) affects the light-curve width and color around peak (similar to the ?m {sub 15} and stretch parameters), and x(2) affects colors, the near-UV light-curve width, and the light-curve decline 20-30 days after peak brightness. The novel light-curve analysis, increased parameter set, and magnitude corrections of K13 may be capturing features of SN Ia diversity arising from progenitor stellar evolution.

  8. HOST GALAXY PROPERTIES AND HUBBLE RESIDUALS OF TYPE Ia SUPERNOVAE FROM THE NEARBY SUPERNOVA FACTORY

    SciTech Connect (OSTI)

    Childress, M.; Aldering, G.; Aragon, C.; Bailey, S.; Fakhouri, H. K.; Hsiao, E. Y.; Kim, A. G.; Loken, S. [Physics Division, Lawrence Berkeley National Laboratory, 1 Cyclotron Road, Berkeley, CA 94720 (United States); Antilogus, P.; Bongard, S.; Canto, A.; Cellier-Holzem, F.; Guy, J. [Laboratoire de Physique Nucleaire et des Hautes Energies, Universite Pierre et Marie Curie Paris 6, Universite Paris Diderot Paris 7, CNRS-IN2P3, 4 place Jussieu, F-75252 Paris Cedex 05 (France); Baltay, C. [Department of Physics, Yale University, New Haven, CT 06250-8121 (United States); Buton, C.; Kerschhaggl, M.; Kowalski, M. [Physikalisches Institut, Universitaet Bonn, Nussallee 12, D-53115 Bonn (Germany); Chotard, N.; Copin, Y.; Gangler, E. [Universite de Lyon, F-69622, Lyon (France); Universite de Lyon 1, Villeurbanne (France); CNRS/IN2P3, Institut de Physique Nucleaire de Lyon (France); and others

    2013-06-20T23:59:59.000Z

    We examine the relationship between Type Ia supernova (SN Ia) Hubble residuals and the properties of their host galaxies using a sample of 115 SNe Ia from the Nearby Supernova Factory. We use host galaxy stellar masses and specific star formation rates fitted from photometry for all hosts, as well as gas-phase metallicities for a subset of 69 star-forming (non-active galactic nucleus) hosts, to show that the SN Ia Hubble residuals correlate with each of these host properties. With these data we find new evidence for a correlation between SN Ia intrinsic color and host metallicity. When we combine our data with those of other published SN Ia surveys, we find the difference between mean SN Ia brightnesses in low- and high-mass hosts is 0.077 {+-} 0.014 mag. When viewed in narrow (0.2 dex) bins of host stellar mass, the data reveal apparent plateaus of Hubble residuals at high and low host masses with a rapid transition over a short mass range (9.8 {<=} log (M{sub *}/M{sub Sun }) {<=} 10.4). Although metallicity has been a favored interpretation for the origin of the Hubble residual trend with host mass, we illustrate how dust in star-forming galaxies and mean SN Ia progenitor age both evolve along the galaxy mass sequence, thereby presenting equally viable explanations for some or all of the observed SN Ia host bias.

  9. Guest-host crosslinked polyimides for integrated optics

    SciTech Connect (OSTI)

    Kowalczyk, T.C.; Kosc, T.Z.; Singer, K.D. [Case Western Reserve Univ., Cleveland, OH (United States). Dept. of Physics; Beuhler, A.J.; Wargowski, D.A. [Amoco Chemical Co., Naperville, IL (United States). Amoco Research Center; Cahill, P.A.; Seager, C.H.; Meinhardt, M.B. [Sandia National Labs., Albuquerque, NM (United States)

    1995-07-01T23:59:59.000Z

    We report on the optical and electrical characterization of aromatic, fluorinated, fully imidized, organic soluble, thermally and photochemically, crosslinkable, guest-host polyimides for integrated optics. Refractive indices and optical losses were measured to evaluate the performance of these materials for passive applications. Materials were doped with two high temperature nonlinear optical chromophores, and poled during crosslinking to produce nonlinear optical materials. Measurements of electro-optic coefficient, macroscopic second order susceptibility, and conductivity were performed to assess these materials as potential candidates for active devices.

  10. Compilation of network activity logs on a DECnet host

    SciTech Connect (OSTI)

    George, M.

    1987-07-01T23:59:59.000Z

    Log files are created for all incoming connection requests on a DECnet host. These log files contain connection data such as the requesting source, destination, and throughput. The procedures (referred to as collect software) outlined in this report, were written to collect these log files, to extract the essential information, and to condense the data into one-line records. The two VAX/VMS systems at SNLA that currently run these procedures compile network transaction logs on a weekly basis. This document is intended for VAX/VMS system managers who wish to install, and possibly modify, this software.

  11. EM Hosts Business Opportunity Forum | Department of Energy

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels DataDepartment of Energy Your Density Isn't Your Destiny:RevisedAdvisory Board Contributions EM Highlights Advisory BoardEM Hosts Business

  12. EM Hosts Successful Visit from Canadian Nuclear Laboratories at Hanford

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels DataDepartment of Energy Your Density Isn't Your Destiny:RevisedAdvisory Board Contributions EM Highlights Advisory BoardEM Hosts

  13. Hosting foreign educators | Y-12 National Security Complex

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office of Science (SC) EnvironmentalGyroSol茅(tm) HarmonicbetandEnergy 2010 A FileHosting foreign

  14. KCP Field Office hosts leadership meeting | National Nuclear Security

    National Nuclear Security Administration (NNSA)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742EnergyOn AprilA groupTubahq.na.gov OfficeAdministration Field Office hosts leadership meeting

  15. KCP hosts top STEM educators to develop curriculum | National Nuclear

    National Nuclear Security Administration (NNSA)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742EnergyOn AprilA groupTubahq.na.gov OfficeAdministration Field Office hostsSecurity

  16. LANL hosts annual Hazmat Challenge | National Nuclear Security

    National Nuclear Security Administration (NNSA)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742EnergyOn AprilA groupTubahq.na.gov OfficeAdministration FieldSecurityAdministration hosts

  17. OREM hosts annual community budget workshop | Department of Energy

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level:Energy: Grid Integration Redefining What's Possible for Renewable Energy:Nanowire3627 FederalTransformers |OJT!LSU/CAMDOREM hosts annual

  18. Lab hosts multi-lab cyber security games

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office of Science (SC)Integrated Codes |Is Your Home asLCLS ExperimentalFive R&D awards formuonLab hosts

  19. Los Alamos National Laboratory to host Robot Rodeo

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office of Science (SC)Integrated Codes |Is YourAwards PollutionPollutionenvironmentalLosLANL to host

  20. The host immunological response to cancer therapy: An emerging concept in tumor biology

    SciTech Connect (OSTI)

    Voloshin, Tali [Department of Molecular Pharmacology, Rappaport Faculty of Medicine and the Rappaport Institute, Technion桰srael Institute of Technology, 1 Efron Street, Bat Galim, Haifa 31096 (Israel); Voest, Emile E. [Department of Medical Oncology, University Medical Center Utrecht, Utrecht (Netherlands); Shaked, Yuval, E-mail: yshaked@tx.technion.ac.il [Department of Molecular Pharmacology, Rappaport Faculty of Medicine and the Rappaport Institute, Technion桰srael Institute of Technology, 1 Efron Street, Bat Galim, Haifa 31096 (Israel)

    2013-07-01T23:59:59.000Z

    Almost any type of anti-cancer treatment including chemotherapy, radiation, surgery and targeted drugs can induce host molecular and cellular immunological effects which, in turn, can lead to tumor outgrowth and relapse despite an initial successful therapy outcome. Tumor relapse due to host immunological effects is attributed to angiogenesis, tumor cell dissemination from the primary tumors and seeding at metastatic sites. This short review will describe the types of host cells that participate in this process, the types of factors secreted from the host following therapy that can promote tumor re-growth, and the possible implications of this unique and yet only partially-known process. It is postulated that blocking these specific immunological effects in the reactive host in response to cancer therapy may aid in identifying new host-dependent targets for cancer, which in combination with conventional treatments can prolong therapy efficacy and extend survival. Additional studies investigating this specific research direction梑oth in preclinical models and in the clinical setting are essential in order to advance our understanding of how tumors relapse and evade therapy. -- Highlights: Cancer therapy induces host molecular and cellular pro-tumorigenic effects. Host effects in response to therapy may promote tumor relapse and metastasis. The reactive host consists of immunological mediators promoting tumor re-growth. Blocking therapy-induced host mediators may improve outcome.

  1. Lithophysal Rock Mass Mechanical Properties of the Repository Host Horizon

    SciTech Connect (OSTI)

    D. Rigby

    2004-11-10T23:59:59.000Z

    The purpose of this calculation is to develop estimates of key mechanical properties for the lithophysal rock masses of the Topopah Spring Tuff (Tpt) within the repository host horizon, including their uncertainties and spatial variability. The mechanical properties to be characterized include an elastic parameter, Young's modulus, and a strength parameter, uniaxial compressive strength. Since lithophysal porosity is used as a surrogate property to develop the distributions of the mechanical properties, an estimate of the distribution of lithophysal porosity is also developed. The resulting characterizations of rock parameters are important for supporting the subsurface design, developing the preclosure safety analysis, and assessing the postclosure performance of the repository (e.g., drift degradation and modeling of rockfall impacts on engineered barrier system components).

  2. An endosymbiont positively modulates ornithine decarboxylase in host trypanosomatids

    SciTech Connect (OSTI)

    Frossard, Mariana Lins [Laboratorio de Ultraestrutura Celular Hertha Meyer, Instituto de Biofisica Carlos Chagas Filho, Universidade Federal do Rio de Janeiro, 21941-590 Rio de Janeiro, RJ (Brazil); Seabra, Sergio Henrique [Laboratorio de Ultraestrutura Celular Hertha Meyer, Instituto de Biofisica Carlos Chagas Filho, Universidade Federal do Rio de Janeiro, 21941-590 Rio de Janeiro, RJ (Brazil); Matta, Renato Augusto da [Laboratorio de Biologia Celular e Tecidual, Centro de Biociencias e Biotecnologia, Universidade Estadual do Norte Fluminense, Avenida Alberto Lamego, 2000, 28013-600 Campos dos Goytacazes, RJ (Brazil); Souza, Wanderley de [Laboratorio de Ultraestrutura Celular Hertha Meyer, Instituto de Biofisica Carlos Chagas Filho, Universidade Federal do Rio de Janeiro, 21941-590 Rio de Janeiro, RJ (Brazil); Garcia de Mello, Fernando [Laboratorio de Neuroquimica, Instituto de Biofisica Carlos Chagas Filho, Universidade Federal do Rio de Janeiro, 21941-590 Rio de Janeiro, RJ (Brazil); Motta, Maria Cristina Machado [Laboratorio de Ultraestrutura Celular Hertha Meyer, Instituto de Biofisica Carlos Chagas Filho, Universidade Federal do Rio de Janeiro, 21941-590 Rio de Janeiro, RJ (Brazil)]. E-mail: motta@biof.ufrj.br

    2006-05-05T23:59:59.000Z

    Summary: Some trypanosomatids, such as Crithidia deanei, are endosymbiont-containing species. Aposymbiotic strains are obtained after antibiotic treatment, revealing interesting aspects of this symbiotic association. Ornithine decarboxylase (ODC) promotes polyamine biosynthesis and contributes to cell proliferation. Here, we show that ODC activity is higher in endosymbiont-bearing trypanosomatids than in aposymbiotic cells, but isolated endosymbionts did not display this enzyme activity. Intriguingly, expressed levels of ODC were similar in both strains, suggesting that ODC is positively modulated in endosymbiont-bearing cells. When the aposymbiotic strain was grown in conditioned medium, obtained after cultivation of the endosymbiont-bearing strain, cellular proliferation as well as ODC activity and localization were similar to that observed in the endosymbiont-containing trypanosomatids. Furthermore, dialyzed-heated medium and trypsin treatment reduced ODC activity of the aposymbiont strain. Taken together, these data indicate that the endosymbiont can enhance the protozoan ODC activity by providing factors of protein nature, which increase the host polyamine metabolism.

  3. Three regimes of extrasolar planets inferred from host star metallicities

    E-Print Network [OSTI]

    Buchhave, Lars A; Latham, David W; Sasselov, Dimitar; Cochran, William D; Endl, Michael; Isaacson, Howard; Juncher, Diana; Marcy, Geoffrey W

    2014-01-01T23:59:59.000Z

    Approximately half of the extrasolar planets (exoplanets) with radii less than four Earth radii are in orbits with short periods. Despite their sheer abundance, the compositions of such planets are largely unknown. The available evidence suggests that they range in composition from small, high-density rocky planets to low-density planets consisting of rocky cores surrounded by thick hydrogen and helium gas envelopes. Understanding the transition from the gaseous planets to Earth-like rocky worlds is important to estimate the number of potentially habitable planets in our Galaxy and provide constraints on planet formation theories. Here we report the abundances of heavy elements (that is, the metallicities) of more than 400 stars hosting 600 exoplanet candidates, and find that the exoplanets can be categorized into three populations defined by statistically distinct (~ 4.5{\\sigma}) metallicity regions. We interpret these regions as reflecting the formation regimes of terrestrial-like planets (radii less than 1...

  4. Host Plant Influences on Performance and Haplotype Diversity of Dalbulus maidis, a Specialist Herbivore of Zea

    E-Print Network [OSTI]

    Davila-Flores, Amanda

    2012-12-06T23:59:59.000Z

    host plants, followed by planned, a priori contrasts (with Sidak?s correction; Abdi and Williams 2010) to evaluate whether corn leafhopper overall performance was affected by transitions in Zea: (i) life history, i.e. perennial teosinte vs. Balsas... preference for any of the host plants if denied a choice of host plant (Bellota-Villafuerte 2012). When warranted by the ANOVA (P Abdi and Williams 2010) to evaluate whether individual...

  5. MEDIA ADVISORY: REAC/TS hosts 5th International Symposium on...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    REACTS hosts 5th International Symposium on the Medical Basis for Radiation Accident Preparedness FOR IMMEDIATE RELEASE June 27, 2011 FY11-35 Who: Radiation Emergency...

  6. TITLE: Cornell's Urban Sustainability Initiatives HOST: Marianne Krasny, Helene Dillard and Marvin Pritts

    E-Print Network [OSTI]

    Angenent, Lars T.

    TITLE: Cornell's Urban Sustainability Initiatives HOST: Marianne Krasny, Helene Dillard and Marvin by Marianne Krasny (Natural Resources), Helene Dillard (CCE), and Marvin Pritts (Horticulture). #12;

  7. Radiofrequency field absorption by carbon nanotubes embedded in a conductive host

    E-Print Network [OSTI]

    Hanson, George

    Radiofrequency field absorption by carbon nanotubes embedded in a conductive host Mikhail V. Shuba centimeters depth penetration of visible and infrared radiation in tissue. Thermoacoustic imaging refers

  8. Plug-In Electric Vehicle Handbook for Public Charging Station Hosts (Brochure)

    SciTech Connect (OSTI)

    Not Available

    2012-04-01T23:59:59.000Z

    This handbook answers basic questions about plug-in electric vehicles, charging stations, charging equipment, and considerations for station owners, property owners, and station hosts.

  9. Host galaxy spectra and consequences for supernova typing from the SDSS SN survey

    SciTech Connect (OSTI)

    Olmstead, Matthew D.; Brown, Peter J.; Brownstein, Joel R.; Dawson, Kyle S. [Department of Physics and Astronomy, University of Utah, Salt Lake City, UT 84112 (United States); Sako, Masao; Gupta, Ravi R. [Department of Physics and Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104 (United States); Bassett, Bruce; Kunz, Martin [African Institute for Mathematical Sciences, 6 Melrose Road, Muizenberg, 7945 (South Africa); Bizyaev, Dmitry; Brinkmann, J.; Brewington, Howard; Ebelke, Garrett L. [Apache Point Observatory, P.O. Box 59, Sunspot, NM 88349 (United States); Campbell, Heather [Institute of Astronomy, Madingley Road, Cambridge CB4 0HA (United Kingdom); D'Andrea, Chris B.; Lampeitl, Hubert [Institute of Cosmology and Gravitation, Dennis Sciama Building, University of Portsmouth, Portsmouth, PO1 3FX (United Kingdom); Frieman, Joshua A. [Center for Particle Astrophysics, Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, IL 60510 (United States); Galbany, Llu韘 [Institut de F韘ica d'Altes Energies, Universitat Aut騨oma de Barcelona, E-08193 Bellaterra (Barcelona) (Spain); Garnavich, Peter [Department of Physics, University of Notre Dame, Notre Dame, IN 46556 (United States); Hlozek, Renee [Department of Astrophysics, Peyton Hall, 4 Ivy Lane, Princeton, NJ 08544 (United States); Jha, Saurabh W., E-mail: olmstead@physics.utah.edu [Department of Physics and Astronomy, Rutgers, the State University of New Jersey, 136 Frelinghuysen Road, Piscataway, NJ 08854 (United States); and others

    2014-04-01T23:59:59.000Z

    We present the spectroscopy from 5254 galaxies that hosted supernovae (SNe) or other transient events in the Sloan Digital Sky Survey II (SDSS-II). Obtained during SDSS-I, SDSS-II, and the Baryon Oscillation Spectroscopic Survey, this sample represents the largest systematic, unbiased, magnitude limited spectroscopic survey of SN host galaxies. Using the host galaxy redshifts, we test the impact of photometric SN classification based on SDSS imaging data with and without using spectroscopic redshifts of the host galaxies. Following our suggested scheme, there are a total of 1166 photometrically classified SNe Ia when using a flat redshift prior and 1126 SNe Ia when the host spectroscopic redshift is assumed. For 1024 (87.8%) candidates classified as likely SNe Ia without redshift information, we find that the classification is unchanged when adding the host galaxy redshift. Using photometry from SDSS imaging data and the host galaxy spectra, we also report host galaxy properties for use in future analysis of SN astrophysics. Finally, we investigate the differences in the interpretation of the light curve properties with and without knowledge of the redshift. Without host galaxy redshifts, we find that SALT2 light curve fits are systematically biased toward lower photometric redshift estimates and redder colors in the limit of low signal-to-noise data. The general improvements in performance of the light curve fitter and the increased diversity of the host galaxy sample highlights the importance of host galaxy spectroscopy for current photometric SN surveys such as the Dark Energy Survey and future surveys such as the Large Synoptic Survey Telescope.

  10. Dynamical Study of Guest-Host Orientational Interaction in LiquidCrystalline Materials

    SciTech Connect (OSTI)

    Truong, Thai Viet

    2005-12-20T23:59:59.000Z

    Guest-host interaction has long been a subject of interest in many disciplines. Emphasis is often on how a small amount of guest substance could significantly affect the properties of a host material. This thesis describe our work in studying a guest-host effect where dye-doping of liquid crystalline materials greatly enhances the optical Kerr nonlinearity of the material. The dye molecules, upon excitation and via intermolecular interaction, provides an extra torque to reorient the host molecules, leading to the enhanced optical Kerr nonlinearity. We carried out a comprehensive study on the dynamics of the photoexcited dye-doped liquid crystalline medium. Using various experimental techniques, we separately characterized the dynamical responses of the relevant molecular species present in the medium following photo-excitation, and thus were able to follow the transient process in which photo-excitation of the dye molecules exert through guest-host interaction a net torque on the host LC material, leading to the observed enhanced molecular reorientation. We also observed for the first time the enhanced reorientation in a pure liquid crystal system, where the guest population is created through photoexcitation of the host molecules themselves. Experimental results agree quantitatively with the time-dependent theory based on a mean-field model of the guest-host interaction.

  11. Mineral paragenesis and textures associated with sandstone-hosted roll-front uranium deposits, NW China

    E-Print Network [OSTI]

    Fayek, Mostafa

    Mineral paragenesis and textures associated with sandstone-hosted roll-front uranium deposits, NW Sciences, State Key Laboratory of Mineral Deposit Research, Nanjing University, Nanjing 210093, People, Wuyiyi and Shihongtan sandstone-hosted roll-front uranium deposits, northwest China. The mineralization

  12. Isotope systematics of ore-bearing granites and host rocks of the Orlovka-Spokoinoe mining

    E-Print Network [OSTI]

    Siebel, Wolfgang

    Isotope systematics of ore-bearing granites and host rocks of the Orlovka-Spokoinoe mining district and Spokoinoe granite massifs and their host rocks in the Orlovka- Spokoinoe mining district, Eastern Transbaikalia, Russia. Pb isotope analyses indicate one common Pb source for all three granite massifs

  13. GUEST-HOST ENCOUNTERS IN DIASPORA-HERITAGE TOURISM: THE TAGLIT-BIRTHRIGHT ISRAEL MIFGASH

    E-Print Network [OSTI]

    Fraden, Seth

    understanding. A specialized form of educational travel, heritage tourism entails visits to places of historical1 GUEST-HOST ENCOUNTERS IN DIASPORA-HERITAGE TOURISM: THE TAGLIT-BIRTHRIGHT ISRAEL MIFGASH Sasson, Philadelphia PA. #12;2 GUEST-HOST ENCOUNTERS IN DIASPORA-HERITAGE TOURISM: THE TAGLIT-BIRTHRIGHT ISRAEL MIFGASH

  14. ECOLOGY AND POPULATION BIOLOGY Effects of Aggregation Size and Host Plant on the Survival of an

    E-Print Network [OSTI]

    Campbell, Diane

    -Tended Membracid (Hemiptera: Membracidae): Potential Roles in Selecting for Generalized Host Plant Use JENNIFER S membracid Publilia modesta (Uhler) (Hemiptera: Membracidae) that feeds on host species Chry- sothamnus, Billick and Tonkel 2003) and other Hemiptera (Addicott 1979, Offenberg 2001). In these associations

  15. INVESTIGATION OF THE THERMOCHROMIC PROPERTIES OF POLYTHIOPHENES DISPERSED IN HOST POLYMERS

    E-Print Network [OSTI]

    Euler, William B.

    INVESTIGATION OF THE THERMOCHROMIC PROPERTIES OF POLYTHIOPHENES DISPERSED IN HOST POLYMERS Brett L films or in solution. However, the utilization of conjugated polymers in many electronic applications requires them to be dispersed in a host polymer matrix.2 There have been few investigations

  16. HoBIDS: A Data Mining Approach to Host Based Intrusion Detection

    E-Print Network [OSTI]

    Hershkop, Shlomo

    HoBIDS: A Data Mining Approach to Host Based Intrusion Detection Department of Computer Science of a host based IDS built on a data mining framework. This framework allows the system to detect both known and lightweight sensor system with the capabilities of sophisticated data-mining techniques to build a powerful

  17. Metallicities of M Dwarf Planet Hosts from Spectral Synthesis

    E-Print Network [OSTI]

    Jacob L. Bean; G. Fritz Benedict; Michael Endl

    2006-11-02T23:59:59.000Z

    We present the first spectroscopic metallicities of three M dwarfs with known or candidate planetary mass companions. We have analyzed high resolution, high signal-to-noise spectra of these stars which we obtained at McDonald Observatory. Our analysis technique is based on spectral synthesis of atomic and molecular features using recently revised cool-star model atmospheres and spectrum synthesis code. The technique has been shown to yield results consistent with the analyses of solar-type stars and allows measurements of M dwarf [M/H] values to 0.12 dex precision. From our analysis, we find [M/H] = -0.12, -0.32, and -0.33 for GJ 876, GJ 436, and GJ 581 respectively. These three M dwarf planet hosts have sub-solar metallicities, a surprising departure from the trend observed in FGK-type stars. This study is the first part of our ongoing work to determine the metallicities of the M dwarfs included in the McDonald Observatory planet search program.

  18. MAGNETIC ACTIVITY CYCLES IN THE EXOPLANET HOST STAR {epsilon} ERIDANI

    SciTech Connect (OSTI)

    Metcalfe, T. S.; Mathur, S. [Space Science Institute, 4750 Walnut Street, Suite 205, Boulder, CO 80301 (United States); Buccino, A. P.; Mauas, P. J. D.; Petrucci, R. [Instituto de Astronomia y Fisica del Espacio (CONICET), C.C. 67 Sucursal 28, C1428EHA-Buenos Aires (Argentina); Brown, B. P. [Department of Astronomy and Center for Magnetic Self-Organization, University of Wisconsin, Madison, WI 53706-1582 (United States); Soderblom, D. R. [Space Telescope Science Institute, 3700 San Martin Dr., Baltimore, MD 21218 (United States); Henry, T. J. [Department of Physics and Astronomy, Georgia State University, Atlanta, GA 30302 (United States); Hall, J. C. [Lowell Observatory, 1400 West Mars Hill Road, Flagstaff, AZ 86001 (United States); Basu, S. [Department of Astronomy, Yale University, P.O. Box 208101, New Haven, CT 06520 (United States)

    2013-02-01T23:59:59.000Z

    The active K2 dwarf {epsilon} Eri has been extensively characterized both as a young solar analog and more recently as an exoplanet host star. As one of the nearest and brightest stars in the sky, it provides an unparalleled opportunity to constrain stellar dynamo theory beyond the Sun. We confirm and document the 3-year magnetic activity cycle in {epsilon} Eri originally reported by Hatzes and coworkers, and we examine the archival data from previous observations spanning 45 years. The data show coexisting 3-year and 13-year periods leading into a broad activity minimum that resembles a Maunder minimum-like state, followed by the resurgence of a coherent 3-year cycle. The nearly continuous activity record suggests the simultaneous operation of two stellar dynamos with cycle periods of 2.95 {+-} 0.03 years and 12.7 {+-} 0.3 years, which, by analogy with the solar case, suggests a revised identification of the dynamo mechanisms that are responsible for the so-called 'active' and 'inactive' sequences as proposed by Boehm-Vitense. Finally, based on the observed properties of {epsilon} Eri, we argue that the rotational history of the Sun is what makes it an outlier in the context of magnetic cycles observed in other stars (as also suggested by its Li depletion), and that a Jovian-mass companion cannot be the universal explanation for the solar peculiarities.

  19. Lithium abundances in exoplanet-host stars : modelling

    E-Print Network [OSTI]

    M. Castro; S. Vauclair; O. Richard; N. C. Santos

    2008-11-18T23:59:59.000Z

    Aims. Exoplanet-host stars (EHS) are known to present superficial chemical abundances different from those of stars without any detected planet (NEHS). EHS are, on the average, overmetallic compared to the Sun. The observations also show that, for cool stars, lithium is more depleted in EHS than in NEHS. The aim of this paper is to obtain constraints on possible models able to explain this difference, in the framework of overmetallic models compared to models with solar abundances. Methods. We have computed main sequence stellar models with various masses and metallicities. The results show different behaviour for the lithium destruction according to those parameters. We compare these results to the spectroscopic observations of lithium. Results. Our models show that the observed lithium differences between EHS and NEHS are not directly due to the overmetallicity of the EHS: some extra mixing is needed below the convective zones. We discuss possible explanations for the needed extra mixing, in particular an increase of the mixing efficiency associated with the development of shear instabilities below the convective zone, triggered by angular momentum transfer due to the planetary migration.

  20. Kuiper belt structure around nearby super-Earth host stars

    E-Print Network [OSTI]

    Kennedy, Grant M; Marmier, Maxime; Greaves, Jane S; Wyatt, Mark C; Bryden, Geoffrey; Holland, Wayne; Lovis, Christophe; Matthews, Brenda C; Pepe, Francesco; Sibthorpe, Bruce; Udry, St閜hane

    2015-01-01T23:59:59.000Z

    We present new observations of the Kuiper belt analogues around HD 38858 and HD 20794, hosts of super-Earth mass planets within 1 au. As two of the four nearby G-type stars (with HD 69830 and 61 Vir) that form the basis of a possible correlation between low-mass planets and debris disc brightness, these systems are of particular interest. The disc around HD 38858 is well resolved with Herschel and we constrain the disc geometry and radial structure. We also present a probable JCMT sub-mm continuum detection of the disc and a CO J=2-1 upper limit. The disc around HD 20794 is much fainter and appears marginally resolved with Herschel, and is constrained to be less extended than the discs around 61 Vir and HD 38858. We also set limits on the radial location of hot dust recently detected around HD 20794 with near-IR interferometry. We present HARPS upper limits on unseen planets in these four systems, ruling out additional super-Earths within a few au, and Saturn-mass planets within 10 au. We consider the disc st...

  1. Effect of pretreating of host oil on coprocessing. Quarterly progress report, January 1--March 31, 1994

    SciTech Connect (OSTI)

    Wender, I.; Tierney, J.W.

    1994-04-30T23:59:59.000Z

    The principal objective of this research is to gain information on the role that host petroleum-derived oils (1000{degrees} F+), as well as that of catalytically treated host oils, play when used as liquefaction solvents in coprocessing with coal. The host oil will be extensively characterized and then pretreated in a number of ways which involve catalytic reactions such as hydrogenation, hydrocracking, and isomerization. The pretreated oils will then be characterized by elemental analysis, catalytic dehydrogenation, distillation, GC-MS, and NMR. The effect of the host oil on coprocessing with coal will be compared to that obtained using catalytically modified host oils. When appropriate, model compounds will be used to study specific reactions brought about by the pretreatments.

  2. The Effect of Host Galaxies on Type Ia Supernovae in the SDSS-II Supernova Survey

    SciTech Connect (OSTI)

    Lampeitl, Hubert; /Portsmouth U., ICG; Smith, Mathew; /Cape Town U. /Portsmouth U., ICG; Nichol, Robert C.; /Portsmouth U., ICG; Bassett, Bruce; /South African Astron. Observ. /Cape Town U.; Cinabro, David; /Wayne State U.; Dilday, Benjamin; /Rutgers U., Piscataway; Foley, Ryan J.; /Harvard-Smithsonian Ctr. Astrophys.; Frieman, Joshua A.; /Chicago U. /Fermilab; Garnavich, Peter M.; /Notre Dame U.; Goobar, Ariel; /Stockholm U., OKC; Im, Myungshin; /Seoul Natl. U. /Rutgers U., Piscataway

    2010-05-01T23:59:59.000Z

    We present an analysis of the host galaxy dependencies of Type Ia Supernovae (SNe Ia) from the full three year sample of the SDSS-II Supernova Survey. We re-discover, to high significance, the strong correlation between host galaxy type and the width of the observed SN light curve, i.e., fainter, quickly declining SNe Ia favor passive host galaxies, while brighter, slowly declining Ia's favor star-forming galaxies. We also find evidence (at between 2 to 3{sigma}) that SNe Ia are {approx_equal} 0.1 magnitudes brighter in passive host galaxies, than in star-forming hosts, after the SN Ia light curves have been standardized using the light curve shape and color variations: This difference in brightness is present in both the SALT2 and MCLS2k2 light curve fitting methodologies. We see evidence for differences in the SN Ia color relationship between passive and star-forming host galaxies, e.g., for the MLCS2k2 technique, we see that SNe Ia in passive hosts favor a dust law of R{sub V} {approx_equal} 1, while SNe Ia in star-forming hosts require R{sub V} {approx} 2. The significance of these trends depends on the range of SN colors considered. We demonstrate that these effects can be parameterized using the stellar mass of the host galaxy (with a confidence of > 4{sigma}) and including this extra parameter provides a better statistical fit to our data. Our results suggest that future cosmological analyses of SN Ia samples should include host galaxy information.

  3. Hubble Residuals of Nearby SN Ia Are Correlated with Host Galaxy Masses

    SciTech Connect (OSTI)

    Kelly, Patrick L.; /KIPAC, Menlo Park /SLAC; Hicken, Malcolm; /Harvard-Smithsonian Ctr. Astrophys.; Burke, David L.; /KIPAC, Menlo Park /SLAC; Mandel, Kaisey S.; Kirshner, Robert P.; /Harvard-Smithsonian Ctr. Astrophys.

    2010-05-03T23:59:59.000Z

    From Sloan Digital Sky Survey u{prime} g{prime} r{prime} i{prime} z{prime} imaging, we estimate the stellar masses of the host galaxies of 70 low redshift SN Ia (0.015 < z < 0.08) from the hosts absolute luminosities and mass-to-light ratios. These nearby SN were discovered largely by searches targeting luminous galaxies, and we find that their host galaxies are substantially more massive than the hosts of SN discovered by the flux-limited Supernova Legacy Survey. Testing four separate light curve fitters, we detect {approx}2.5{sigma} correlations of Hubble residuals with both host galaxy size and stellar mass, such that SN Ia occurring in physically larger, more massive hosts are {approx}10% brighter after light curve correction. The Hubble residual is the deviation of the inferred distance modulus to the SN, calculated from its apparent luminosity and light curve properties, away from the expected value at the SN redshift. Marginalizing over linear trends in Hubble residuals with light curve parameters shows that the correlations cannot be attributed to a light curve-dependent calibration error. Combining 180 higher-redshift ESSENCE, SNLS, and HigherZ SN with 30 nearby SN whose host masses are less than 10{sup 10.8} M{circle_dot} n a cosmology fit yields 1 + w = 0.22{sub -0.108}{sup +0.152}, while a combination where the 30 nearby SN instead have host masses greater than 10{sup 10.8} M{circle_dot} yields 1 + w = ?0.03{sub -0.143}{sup +0.217}. Progenitor metallicity, stellar population age, and dust extinction correlate with galaxy mass and may be responsible for these systematic effects. Host galaxy measurements will yield improved distances to SN Ia.

  4. Evaluation of Potato Psyllid, Bactericera Cockerelli (Sulc) (Hemiptera: Triozidae), Host Preferences, Adaptation, Behavior, and Transmission of 'Candidatus Liberibacter Solanacearum' among Wild and Cultivated Solanaceous Hosts in the Lower Rio Grande Valley of Texas

    E-Print Network [OSTI]

    Thinakaran, Jenita

    2014-04-30T23:59:59.000Z

    EVALUATION OF POTATO PSYLLID, BACTERICERA COCKERELLI (奤LC) (HEMIPTERA: TRIOZIDAE), HOST PREFERENCES, ADAPTATION, BEHAVIOR, AND TRANSMISSION OF 慍ANDIDATUS LIBERIBACTER SOLANACEARUM AMONG WILD AND CULTIVATED SOLANACEOUS HOSTS IN THE LOWER..., BACTERICERA COCKERELLI (SULC) (HEMIPTERA: TRIOZIDAE), ON SOLANACEOUS HOSTS UNDER FIELD CONDITIONS .................................... 19 Introduction...

  5. A VIBRATIONAL SPECTROSCOPIC STUDY OF AQUEOUS HYDROGEN HALIDE SOLUTIONS: APPLICATION TO ATMOSPHERIC AEROSOL CHEMISTRY

    E-Print Network [OSTI]

    to thank Carri, Misty, Kelly, and Mindy, who provided the comic relief and road trips that helped me keep

  6. Infection outcomes under genetic and environmental variation in a host-parasite system: Implications for maintenance of polymorphism and the evolution of virulence

    E-Print Network [OSTI]

    Ferreira do Vale, Pedro Filipe

    2009-01-01T23:59:59.000Z

    Virulence (the harm to the host during infection) is the outcome of continuous coevolution between hosts and parasites. This thesis adds to a growing body of work on host-parasite interactions, and describes experiments ...

  7. Sandia/New Mexico's host, the City of Albuquerque, has a long...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    SandiaNew Mexico's host, the City of Albuquerque, has a long-term goal of Zero Waste to the Landfill by 2030. Zero Waste is generally accepted to mean greater than 90% of waste...

  8. NERSC Hosts HS Students on Job Shadow Day- NERSC Center News...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Cardo, Richard Gerber, Jason Hick and Jim Mellander of NERSC hosted Aaron Allen, Edward Gong, Dan Li, Darshan Parajuli and Patrick Xu at the Oakland Scientific Facility. John Bell...

  9. MODELING THE GRB HOST GALAXY MASS DISTRIBUTION: ARE GRBs UNBIASED TRACERS OF STAR FORMATION?

    E-Print Network [OSTI]

    Kocevski, Daniel

    We model the mass distribution of long gamma-ray burst (GRB) host galaxies given recent results suggesting that GRBs occur in low-metallicity environments. By utilizing measurements of the redshift evolution of the ...

  10. Characterization of host lymphoid cells in antibody-facilitated bone marrow chimeras

    SciTech Connect (OSTI)

    McCarthy, S.A.; Griffith, I.J.; Gambel, P.; Francescutti, L.H.; Wegmann, T.G.

    1985-07-01T23:59:59.000Z

    The authors have produced stable murine antibody-facilitated (AF) chimeras by the simultaneous injection of P1 bone marrow cells and anti-P2 monoclonal antibody into normal (unirradiated) adult (P1 X P2)F1 recipients. These AF chimeras are healthy, long-lived, and exhibit no overt signs of graft-versus-host disease. They are immunocompetent and tolerant of host, P2-encoded alloantigens. Donor cell engraftment and takeover, monitored by glucosephosphate isomerase isozyme patterns, is usually complete (greater than 95%) in the peripheral blood, bone marrow, and hemopoietic stem cell compartments of long-term (greater than 3 months posttransplantation) AF chimeras. The authors report here, however, that splenic, lymph node, and thymic leukocytes of AF chimeras represent donor/host chimeric populations. Spleen cell populations of AF chimeras exhibit substantial chimera-to-chimera variation in the preponderant residual host cell type(s) present. Interpretations of the implications of these findings are discussed.

  11. Platforms for exploring host-pathogen interactions in hepatitis C virus infection

    E-Print Network [OSTI]

    Trehan, Kartik

    2012-01-01T23:59:59.000Z

    Afflicting almost 200 million worldwide, hepatitis C virus (HCV) mounts a chronic infection of liver hepatocytes that causes substantial morbidity and mortality. An understanding of host-virus interactions will drive the ...

  12. U.S. Department of Energy to Host Press Call on Transition of...

    Broader source: Energy.gov (indexed) [DOE]

    586 4940 U.S. Department of Energy to Host Press Call on Transition of Legacy Cleanup Work at Los Alamos National Laboratory WASHINGTON- On Wednesday, December 3, 2014, the Office...

  13. BMB Dept Seminar Schedule (Fall 2012) _v8 Dates Speakers (& their homepages), Seminar Title, and Hosts

    E-Print Network [OSTI]

    Cinabro, David

    Rudenko, PhD, Assistant Professor, Department of Pharmacology, University of Michigan. (http://www.lsi.umich.edu/facultyresearch/labs/rudenko) (http://www.chembio.umich.edu/people/rudenko.html) Title: Host: Ladislau Kovari Dec 4, 2012 Speaker

  14. RESEARCH ARTICLES Evolutionary Origins of a Novel Host Plant Detoxification Gene in Butterflies

    E-Print Network [OSTI]

    Wheat, Christopher

    RESEARCH ARTICLES Evolutionary Origins of a Novel Host Plant Detoxification Gene in Butterflies of Biological Sciences, Pennsylvania State University Chemical interactions between plants and their insect as a coevolutionary key innovation. By generating and sequencing expressed sequence tags, genomic libraries

  15. Influenza type C virus biology, interaction with the host, and epidemiology

    E-Print Network [OSTI]

    Reeves, William Wyatt

    1995-01-01T23:59:59.000Z

    glycoprotein, HEF, which is responsible for attachment to the sialic acid host cell receptor, receptor destruction, and viral-cell fusion (similar to the HN glycoprotein of Paramyxoviruses). RNA segment 5 codes for the nucleoprotein (NP) which is the backbone...

  16. Genome analysis of Bifidobacterium bifidum PRL2010 reveals metabolic pathways for host-derived

    E-Print Network [OSTI]

    Gleeson, Joseph G.

    Genome analysis of Bifidobacterium bifidum PRL2010 reveals metabolic pathways for host,214,650-bp genome of Bifidobacterium bifidum PRL2010, a strain isolated from infant stool, revealed

  17. Cyanobacterium sp. host cell and vector for production of chemical compounds in cyanobacterial cultures

    SciTech Connect (OSTI)

    Piven, Irina; Friedrich, Alexandra; Duhring, Ulf; Uliczka, Frank; Baier, Kerstin; Inaba, Masami; Shi, Tuo; Wang, Kui; Enke, Heike; Kramer, Dan

    2014-09-30T23:59:59.000Z

    A cyanobacterial host cell, Cyanobacterium sp., that harbors at least one recombinant gene for the production of a chemical compounds is provided, as well as vectors derived from an endogenous plasmid isolated from the cell.

  18. Host identity impacts rhizosphere fungal communities associated with three alpine plant species

    E-Print Network [OSTI]

    Becklin, Katie M.; Hertweck, Kate L.; Jumpponen, Ari

    2012-01-01T23:59:59.000Z

    Fungal diversity and composition are still relatively unknown in many ecosystems; however, host identity and environmental conditions are hypothesized to influence fungal community assembly. To test these hypotheses we ...

  19. Emplacing Displacement: Cultural Landscapes of Refugee-hosting in Ukwimi, Zambia

    E-Print Network [OSTI]

    Gray, Angela M.

    2009-09-15T23:59:59.000Z

    In response to calls for increased understanding of and solutions to the issue of protracted refugee situations, this dissertation examines the social and spatial implications of a long history of refugee-hosting in Eastern ...

  20. Caught in the Crossfire: Strategies of Multinationals in Host Countries at War

    E-Print Network [OSTI]

    Dai, Li

    2012-02-14T23:59:59.000Z

    This dissertation examines the strategic choices of multinational enterprises (MNEs) in host countries that become engaged in war. By combining the resource-based view and resource management theory, and drawing additional insights from research...

  1. Anti-inflammatory drugs for modulation of host response to biomaterials and application in diabetes therapy

    E-Print Network [OSTI]

    Dang, Thuy Tram, Ph. D. Massachusetts Institute of Technology

    2012-01-01T23:59:59.000Z

    Host response to implanted biomaterials and medical devices poses tremendous challenges to their clinical applications. Today, the quest to mitigate this immunological attack for improved longevity of these devices remains ...

  2. DOE Hosts Solid-State Lighting Commercial Product Testing Program Workshop

    Broader source: Energy.gov [DOE]

    The U.S. Department of Energy (DOE) hosted a workshop on October 27, 2006, to introduce the DOE SSL Commercial Product Testing Program. The workshop, held in Washington, D.C., drew over 40...

  3. Biological and biomedical implications of the co-evolution of pathogens and their hosts

    E-Print Network [OSTI]

    Woolhouse, Mark EJ; Webster, Joanne P; Domingo, Esteban; Charlesworth, Brian; Levin, Bruce R

    Co-evolution between host and pathogen is, in principle, a powerful determinant of the biology and genetics of infection and disease. Yet co-evolution has proven difficult to demonstrate rigorously in practice, and ...

  4. Effect of the hepatoma growth period on host plasma and liver lipid concentrations

    E-Print Network [OSTI]

    Matocha, Martha Frances

    1979-01-01T23:59:59.000Z

    EFFECT OF THE HEPATOMA GROWTH PERIOD ON HOST PLASMA AND LIVER LIPID CONCENTRATIONS A Thesis by MARTHA FRANCES MATOCHA Submitted to the Graduate College of Texas A&M University in partial fulfillment of the requirement for the degree... of MASTER OF SCIENCE August 1979 Niajor Sub ect: Biochem. 'stry EFFECT OF THE HEPATOMA GROWTH PERIOD ON HOST PLASMA AND LIVER LIPID CONCENTRATIONS A Thesis MARTHA FRANCES MATOCHA Approved as to style and content by: (Chairman of Committee) (Mern...

  5. HOST GALAXIES OF TYPE Ia SUPERNOVAE FROM THE NEARBY SUPERNOVA FACTORY

    SciTech Connect (OSTI)

    Childress, M.; Aldering, G.; Aragon, C.; Bailey, S.; Fakhouri, H. K.; Hsiao, E. Y.; Kim, A. G.; Loken, S. [Physics Division, Lawrence Berkeley National Laboratory, 1 Cyclotron Road, Berkeley, CA 94720 (United States); Antilogus, P.; Bongard, S.; Canto, A.; Cellier-Holzem, F.; Guy, J. [Laboratoire de Physique Nucleaire et des Hautes Energies, Universite Pierre et Marie Curie Paris 6, Universite Paris Diderot Paris 7, CNRS-IN2P3, 4 place Jussieu, F-75252 Paris Cedex 05 (France); Baltay, C. [Department of Physics, Yale University, New Haven, CT 06250-8121 (United States); Buton, C.; Kerschhaggl, M.; Kowalski, M. [Physikalisches Institut, Universitaet Bonn, Nussallee 12, D-53115 Bonn (Germany); Chotard, N.; Copin, Y.; Gangler, E. [Universite de Lyon, F-69622, Lyon (France); Universite de Lyon 1, Villeurbanne (France); CNRS/IN2P3, Institut de Physique Nucleaire de Lyon (France); and others

    2013-06-20T23:59:59.000Z

    We present photometric and spectroscopic observations of galaxies hosting Type Ia supernovae (SNe Ia) observed by the Nearby Supernova Factory. Combining Galaxy Evolution Explorer (GALEX) UV data with optical and near-infrared photometry, we employ stellar population synthesis techniques to measure SN Ia host galaxy stellar masses, star formation rates (SFRs), and reddening due to dust. We reinforce the key role of GALEX UV data in deriving accurate estimates of galaxy SFRs and dust extinction. Optical spectra of SN Ia host galaxies are fitted simultaneously for their stellar continua and emission lines fluxes, from which we derive high-precision redshifts, gas-phase metallicities, and H{alpha}-based SFRs. With these data we show that SN Ia host galaxies present tight agreement with the fiducial galaxy mass-metallicity relation from Sloan Digital Sky Survey (SDSS) for stellar masses log(M{sub *}/M{sub Sun }) > 8.5 where the relation is well defined. The star formation activity of SN Ia host galaxies is consistent with a sample of comparable SDSS field galaxies, though this comparison is limited by systematic uncertainties in SFR measurements. Our analysis indicates that SN Ia host galaxies are, on average, typical representatives of normal field galaxies.

  6. The Optically Unbiased Gamma-Ray Burst Host (TOUGH) Survey. VII. The Host Galaxy Luminosity Function: Probing the Relationship Between GRBs and Star Formation to Redshift $\\sim6$

    E-Print Network [OSTI]

    Schulze, S; Hjorth, J; Levan, A J; Jakobsson, P; Bj鰎nsson, G; Perley, D A; Kr黨ler, T; Gorosabel, J; Tanvir, N R; Postigo, A de Ugarte; Fynbo, J P U; Milvang-Jensen, B; M鴏ler, P; Watson, D J

    2015-01-01T23:59:59.000Z

    Gamma-ray bursts (GRBs) offer a route to characterizing star-forming galaxies and quantifying high-$z$ star-formation that is distinct from the approach of traditional galaxy surveys: GRB selection is independent of dust and probes even the faintest galaxies that can evade detection in flux-limited surveys. However, the exact relation between GRB rate and Star Formation Rate (SFR) throughout all redshifts is controversial. The TOUGH survey includes observations of all GRB hosts (69) in an optically unbiased sample and we utilize these to constrain the evolution of the UV GRB-host-galaxy Luminosity Function (LF) between $z=0$ and $z=4.5$, and compare this with LFs derived from both Lyman-break galaxy (LBG) surveys and simulation modeling. At all redshifts we find the GRB hosts to be most consistent with a Luminosity Function derived from SFR weighted models incorporating GRB production via both metallicity-dependent and independent channels with a relatively high level of bias towards low metallicity hosts. In...

  7. A HOST PHASE FOR THE DISPOSAL OF WEAPONS PLUTONIUM

    SciTech Connect (OSTI)

    WERNER LUTZE; K. B. HELEAN; W. L. GONG - UNIVERSITY OF NEW MEXICO RODNEY C. EWING - UNIVERSITY OF MICHIGAN

    1999-01-01T23:59:59.000Z

    Research was conducted into the possible use of zircon (ZrSiO{sub 4}) as a host phase for storage or disposal of excess weapons plutonium. Zircon is one of the most chemically durable minerals. Its structure can accommodate a variety of elements, including plutonium and uranium. Natural zircon contains uranium and thorium together in different quantities, usually in the range of less than one weight percent up to several weight percent. Zircon occurs in nature as a crystalline or a partially to fully metamict mineral, depending on age and actinide element concentration, i.e., on radiation damage. These zircon samples have been studied extensively and the results are documented in the literature in terms of radiation damage to the crystal structure and related property changes, e.g., density, hardness, loss of uranium and lead, etc. Thus, a unique suite of natural analogues are available to describe the effect of decay of {sup 239}Pu on zircon's structure and how zircon's physical and chemical properties will be affected over very long periods of time. Actually, the oldest zircon samples known are over 3 billion years old. This period covers the time for decay of {sup 239}Pu (half-life 24,300 yr.) and most of its daughter {sup 235}U (half-life 700 million yr.). Because of its chemical durability, even under extreme geological conditions, zircon is the most widely used mineral for geochronological dating (7,000 publications). It is the oldest dated mineral on earth and in the universe. Zircon has already been doped with about 10 weight percent of plutonium. Pure PuSiO{sub 4} has also been synthesized and has the same crystal structure as zircon. However, use of zircon as a storage medium or waste form for plutonium requires further materials characterization. Experiments can either be conducted in laboratories where plutonium can be handled or plutonium can be simulated by other elements, and experiments can be done under less restricted conditions. The authors conducted work with zircon doped with thorium, uranium and cerium, respectively. They synthesized various zircon compositions and studied the solid solution properties of mixed (Zr,X)SiO{sub 4} [X represents Th, U, Ce, respectively]. They measured the dissolution rate of pure crystalline zircon at elevated temperatures and of an amorphous hydrated zircon. This final report together with two previous annual reports summarize the accomplishments made in two areas: (1) synthesis of zircon solid solutions with Th, U, and Ce; and (2) measurement of the chemical durability of zircon. The focus of the final report is on the measurement of zircon's dissolution rate in water and on the determination of volubility limits of Th, U, and Ce in zircon.

  8. The Evolution of Host Specialization in the Vertebrate Gut Symbiont Lactobacillus reuteri

    SciTech Connect (OSTI)

    Frese, Steven A. [University of Nebraska, Lincoln; Benson, Andrew K. [University of Nebraska, Lincoln; Tannock, Gerald W. [University of Otago, Dunedin, New Zealand; Loach, Diane M. [University of Otago, Dunedin, New Zealand; Kim, Jaehyoung [University of Nebraska, Lincoln; Zhang, Min [University of Nebraska, Lincoln; Oh, Phaik Lyn [University of Nebraska, Lincoln; Heng, Nicholas C. K. [University of Otago, Dunedin, New Zealand; Patil, Prabhu [University of Nebraska, Lincoln; Juge, Nathalie [Institute of Food Research, Norwich Research Park, Norwich, United Kingdom; MacKenzie, Donald A. [Institute of Food Research, Norwich Research Park, Norwich, United Kingdom; Pearson, Bruce M. [Institute of Food Research, Norwich Research Park, Norwich, United Kingdom; Lapidus, Alla L. [U.S. Department of Energy, Joint Genome Institute; Dalin, Eileen [U.S. Department of Energy, Joint Genome Institute; Tice, Hope [U.S. Department of Energy, Joint Genome Institute; Goltsman, Eugene [U.S. Department of Energy, Joint Genome Institute; Land, Miriam L [ORNL; Hauser, Loren John [ORNL; Ivanova, N [U.S. Department of Energy, Joint Genome Institute; Kyrpides, Nikos C [U.S. Department of Energy, Joint Genome Institute; Walter, Jens [University of Nebraska, Lincoln

    2011-01-01T23:59:59.000Z

    Recent research has provided mechanistic insight into the important contributions of the gut microbiota to vertebrate biology, but questions remain about the evolutionary processes that have shaped this symbiosis. In the present study, we showed in experiments with gnotobiotic mice that the evolution of Lactobacillus reuteri with rodents resulted in the emergence of host specialization. To identify genomic events marking adaptations to the murine host, we compared the genome of the rodent isolate L. reuteri 100-23 with that of the human isolate L. reuteri F275, and we identified hundreds of genes that were specific to each strain. In order to differentiate true host-specific genome content from strain-level differences, comparative genome hybridizations were performed to query 57 L. reuteri strains originating from six different vertebrate hosts in combination with genome sequence comparisons of nine strains encompassing five phylogenetic lineages of the species. This approach revealed that rodent strains, although showing a high degree of genomic plasticity, possessed a specific genome inventory that was rare or absent in strains from other vertebrate hosts. The distinct genome content of L. reuteri lineages reflected the niche characteristics in the gastrointestinal tracts of their respective hosts, and inactivation of seven out of eight representative rodent-specific genes in L. reuteri 100-23 resulted in impaired ecological performance in the gut of mice. The comparative genomic analyses suggested fundamentally different trends of genome evolution in rodent and human L. reuteri populations, with the former possessing a large and adaptable pan-genome while the latter being subjected to a process of reductive evolution. In conclusion, this study provided experimental evidence and a molecular basis for the evolution of host specificity in a vertebrate gut symbiont, and it identified genomic events that have shaped this process.

  9. Spectroscopic Properties of Star-Forming Host Galaxies and Type Ia Supernova Hubble Residuals in a Nearly Unbiased Sample

    SciTech Connect (OSTI)

    D'Andrea, Chris B. [Univ. of Pennsylvania, Philadelphia, PA (United States); et al.

    2011-12-20T23:59:59.000Z

    We examine the correlation between supernova host galaxy properties and their residuals on the Hubble diagram. We use supernovae discovered during the Sloan Digital Sky Survey II - Supernova Survey, and focus on objects at a redshift of z < 0.15, where the selection effects of the survey are known to yield a complete Type Ia supernova sample. To minimize the bias in our analysis with respect to measured host-galaxy properties, spectra were obtained for nearly all hosts, spanning a range in magnitude of -23 < M_r < -17. In contrast to previous works that use photometric estimates of host mass as a proxy for global metallicity, we analyze host-galaxy spectra to obtain gas-phase metallicities and star-formation rates from host galaxies with active star formation. From a final sample of ~ 40 emission-line galaxies, we find that light-curve corrected Type Ia supernovae are ~ 0.1 magnitudes brighter in high-metallicity hosts than in low-metallicity hosts. We also find a significant (> 3{\\sigma}) correlation between the Hubble residuals of Type Ia supernovae and the specific star-formation rate of the host galaxy. We comment on the importance of supernova/host-galaxy correlations as a source of systematic bias in future deep supernova surveys.

  10. Detection of the host galaxy of S5 0716+714

    E-Print Network [OSTI]

    K. Nilsson; T. Pursimo; A. Sillanp滗; L. O. Takalo; E. Lindfors

    2008-07-01T23:59:59.000Z

    We have acquired a deep i-band image of the BL Lacertae object S5 0716+714 while the target was in an low optical state. Due to the faintness of the nucleus, we were able to detect the underlying host galaxy. The host galaxy is measured to have an I-band magnitude of 17.5 +- 0.5 and an effective radius of (2.7 +- 0.8) arcsec. Using the host galaxy as a ``standard candle'', we derive z = 0.31 +- 0.08 (1 sigma error) for the host galaxy of S5 0716+714. This redshift is consistent with the redshift z = 0.26 determined by spectroscopy for 3 galaxies close to S5 0716+714. The effective radius at z = 0.31 would be 12 +- 4 kpc, which is consistent with values obtained for BL Lac host galaxies. An optical spectrum acquired during the same epoch shows no identifiable spectral lines.

  11. Design of a Host Traffic Management system for Hard Real Time networks

    E-Print Network [OSTI]

    Krishna Moorthy, Jayasankar

    1997-01-01T23:59:59.000Z

    MODEL A. What Is NetEx? . B. NetEx Block Schematic . . C. The Host Traffic Manager D. The Network Traffic Manager (NTM) III DESIGN OF THE HOST TRAFFIC MANAGER A. Design Requirements B. Design Methodology C. HTM ? System Layout D. Design... of Future Work REFERENCES . 7 7 9 10 12 12 13 16 17 22 25 27 29 32 32 32 36 37 39 39 41 43 45 CHAPTER Page VITA 47 LIST OF FIGURES FIGURE Page Decomposition of Connection into Servers ISO OSI Model NetEx Block Schematic I...

  12. The Host Galaxies of Radio-Loud and Radio-Quiet Quasars

    E-Print Network [OSTI]

    James S. Dunlop

    2001-03-15T23:59:59.000Z

    I review our knowledge of the properties of the host galaxies of radio-loud and radio-quiet quasars, both in comparison to each other and in the context of the general galaxy population. It is now clear that the hosts of radio-loud and radio-quiet quasars with M_V 10^9 solar masses appears to be a necessary (although perhaps not sufficient) condition for the production of radio jets of sufficient power to produce an FRII radio source within a massive galaxy halo.

  13. Lawrence Livermore National Laboratory Workshop Characterization of Pathogenicity, Virulence and Host-Pathogen Interactions

    SciTech Connect (OSTI)

    Krishnan, A

    2006-08-30T23:59:59.000Z

    The threats of bio-terrorism and newly emerging infectious diseases pose serious challenges to the national security infrastructure. Rapid detection and diagnosis of infectious disease in human populations, as well as characterizing pathogen biology, are critical for reducing the morbidity and mortality associated with such threats. One of the key challenges in managing an infectious disease outbreak, whether through natural causes or acts of overt terrorism, is detection early enough to initiate effective countermeasures. Much recent attention has been directed towards the utility of biomarkers or molecular signatures that result from the interaction of the pathogen with the host for improving our ability to diagnose and mitigate the impact of a developing infection during the time window when effective countermeasures can be instituted. Host responses may provide early signals in blood even from localized infections. Multiple innate and adaptive immune molecules, in combination with other biochemical markers, may provide disease-specific information and new targets for countermeasures. The presence of pathogen specific markers and an understanding of the molecular capabilities and adaptations of the pathogen when it interacts with its host may likewise assist in early detection and provide opportunities for targeting countermeasures. An important question that needs to be addressed is whether these molecular-based approaches will prove useful for early diagnosis, complement current methods of direct agent detection, and aid development and use of countermeasures. Lawrence Livermore National Laboratory (LLNL) will host a workshop to explore the utility of host- and pathogen-based molecular diagnostics, prioritize key research issues, and determine the critical steps needed to transition host-pathogen research to tools that can be applied towards a more effective national bio-defense strategy. The workshop will bring together leading researchers/scientists in the area of host-pathogen interactions as well as policy makers from federal agencies. The main objectives of the workshop are: (1) to assess the current national needs, capabilities, near-term technologies, and future challenges in applying various diagnostics tools to public health and bio-defense; (2) to evaluate the utility and feasibility of host-response and pathogen biomarker profiling in the diagnosis and management of infectious diseases; and (3) to create a comprehensive developmental strategy from proof-of-concept, through validation, to deployment of appropriate advanced technology for the clinical/public health and bio-defense environments.

  14. DOE and Northeast Energy Efficiency Partnerships Host Two-Day Market Introduction Workshop in Boston

    Broader source: Energy.gov [DOE]

    Over 100 attendees gathered in Boston, MA to participate in the "Voices for SSL Efficiency" Solid-State Lighting Workshop on July 16-17, 2007. The workshop, hosted by DOE and Northeast Energy Efficiency Partnerships (NEEP), was the second DOE meeting to explore how Federal, State, and private-sector organizations can work together to guide market introduction of high-performance SSL products. The first workshop, hosted by DOE and Southern California Edison, was held in Pasadena in April 2007. In both workshops, a diverse gathering of participants energy efficiency organizations, utilities, government, and industry shared insights, ideas, and updates on the rapidly evolving SSL market.

  15. Seasonal Abundance and Dispersal of the Cotton Fleahopper as Related to Host Plant Phenology.

    E-Print Network [OSTI]

    Almand, Lyndon K.; Sterling, W.L.; Green, C.L.

    1976-01-01T23:59:59.000Z

    occurred. Croton served as a host plant both for overwintering eggs and throughout the growing season. Seasonal Abundance and Dispersal of the Cotton Fleahopper as Related to Host Plant Phenology *L. K. Almand W. L. Sterling C. L. Green... to various wind speeds also was de rmined in a wind tunnel with a testing area of about 3 lhic feet. Nymphs ;less than 24 hours old which had ltched from overwintering eggs (procedure developed I Sterling and Plapp, 1972) were collected for testing Id...

  16. [New hosts and vectors for genome cloning]. Progress report, 1990--1991

    SciTech Connect (OSTI)

    Not Available

    1991-12-31T23:59:59.000Z

    The main goal of our project remains the development of new bacterial hosts and vectors for the stable propagation of human DNA clones in E. coli. During the past six months of our current budget period, we have (1) continued to develop new hosts that permit the stable maintenance of unstable features of human DNA, and (2) developed a series of vectors for (a) cloning large DNA inserts, (b) assessing the frequency of human sequences that are lethal to the growth of E. coli, and (c) assessing the stability of human sequences cloned in M13 for large-scale sequencing projects.

  17. The Investigation on Fibrous Veins and Their Host from Mt. Ida, Ouachita Mountains, Arkansas

    E-Print Network [OSTI]

    Chung, Jae Won

    2004-09-30T23:59:59.000Z

    of the host is given by: ?* = 3b/(16kBV0B) (2) where b is the radius of rock sphere containing one vein or spherical crystal, ?* is the critical value of surrounding host rock viscosity, k is a constant in kinetic law for precipitation/dissolution... goal to test some of these implications. 7 2. GEOLOGY Samples of fibrous veins were collected from Paleozoic Womble Shale around Mt. Ida, Arkansas (Fig. 2). The study area lies within the Benton Uplift of eastern Arkansas. The Benton Uplift...

  18. Relationship between microstructures and grain-scale trace element distribution in komatiite-hosted magmatic sulphide ores

    E-Print Network [OSTI]

    2013 Available online 6 November 2013 Keywords: Komatiite hosted Ni sulphides EBSD Laser ablation ICP) have been studied by electron backscatter diffraction and laser ablation inductively coupled plasma

  19. Improved Catalysts for Heavy Oil Upgrading Based on Zeolite Y Nanoparticles Encapsulated Stable Nanoporous Host

    SciTech Connect (OSTI)

    Conrad Ingram; Mark Mitchell

    2007-09-30T23:59:59.000Z

    The objective of this project is to synthesize nanocrystals of highly acidic zeolite Y nanoclusters, encapsulate them within the channels of mesoporous (nanoporous) silicates or nanoporous organosilicates, and evaluate the 'zeolite Y/Nanoporous host' composites as catalysts for the upgrading of heavy petroleum feedstocks. In comparison to conventionally-used zeolite Y catalysts of micron size particles, the nanocrystals (< 100 nm particle size) which contain shorter path lengths, are expected to allow faster diffusion of large hydrocarbon substrates and the catalysis products within and out of the zeolite's channels and cages (<1 nm size). This is expected to significantly reduce deactivation of the catalyst and to prolong their period of reactivity. Encapsulating zeolite Y nanocrystals within the nanoporous materials is expected to protect its external surfaces and pore entrances from being blocked by large hydrocarbon substrates, since these substrates will initially be converted to small molecules by the nanoporous host (a catalyst in its own right). The project consisted of four major tasks as follows: (1) synthesis of the nanoparticles of zeolite Y (of various chemical compositions) using various techniques such as the addition of organic additives to conventional zeolite Y synthesis mixtures to suppress zeolite Y crystal growth; (2) synthesis of nanoporous silicate host materials of up to 30 nm pore diameter, using poly (alkylene oxide) copolymers which when removed will yield a mesoporous material; (3) synthesis of zeolite Y/Nanoporous Host composite materials as potential catalysts; and (4) evaluation of the catalyst for the upgrading of heavy petroleum feedstocks.

  20. A Summary Report Keeping pace with changing global markets, meeting world demand for a host

    E-Print Network [OSTI]

    Minnesota, University of

    in an uncertain world. Robert Johns (CTS director), Rebecca Jasper (Council of Supply Chain ManagementA Summary Report Keeping pace with changing global markets, meeting world demand for a host, transportation infrastructure, ports, railroads, biofuels and agricultural byproducts, and transportation

  1. Plant Disease / October 2001 1113 Effect of Host Plant Resistance and Reduced Rates and Frequencies

    E-Print Network [OSTI]

    Douches, David S.

    Plant Disease / October 2001 1113 Effect of Host Plant Resistance and Reduced Rates and Frequencies. These include the use of fungicides with less active ingredient, re- duced application rates, longer application. The frequent fungicide spray intervals and rates currently used by growers to control late blight are expensive

  2. Neutrinos from gamma-ray bursts: propagation of cosmic rays in their host galaxies

    E-Print Network [OSTI]

    Wang, Zi-Yi; Wang, Jun-Feng

    2015-01-01T23:59:59.000Z

    Gamma-ray bursts (GRBs) are proposed as candidate sources of ultra-high energy cosmic rays (UHECRs). We study the possibility that the PeV neutrinos recently observed by IceCube are produced by GRB cosmic rays interacting with the interstellar gas in the host galaxies. By studying the relation between the X-ray absorption column density N_H and the surface star-formation rate of GRB host galaxies, we find that N_H is a good indicator of the surface gas density of the host galaxies. Then we are able to calculate the neutrino production efficiency of CRs for GRBs with known N_H. We collect a sample of GRBs that have both measurements of N_H and accurate gamma-ray fluence, and attempt to calculate the accumulated neutrino flux based on the current knowledge about GRBs and their host galaxies. When the CR intensity produced by GRBs is normalized with the observed UHECR flux above $10^{19}{\\rm eV}$, the accumulated neutrino flux at PeV energies is estimated to be about $(0.3\\pm0.2)\\times10^{-8} \\rm{GeV\\ cm^{-2}\\ s...

  3. The Swift Gamma-Ray Burst Host Galaxy Legacy Survey - I. Sample Selection and Redshift Distribution

    E-Print Network [OSTI]

    Perley, D A; Schulze, S; Postigo, A de Ugarte; Hjorth, J; Berger, E; Cenko, S B; Chary, R; Cucchiara, A; Ellis, R; Fong, W; Fynbo, J P U; Gorosabel, J; Greiner, J; Jakobsson, P; Laskar, T; Levan, A J; Micha?owski, M J; Milvang-Jensen, B; Tanvir, N R; Th鰊e, C C; Wiersema, K

    2015-01-01T23:59:59.000Z

    We introduce the Swift Gamma-Ray Burst Host Galaxy Legacy Survey ("SHOALS"), a multi-observatory high-redshift galaxy survey targeting the largest unbiased sample of long-duration gamma-ray burst hosts yet assembled (119 in total). We describe the motivations of the survey and the development of our selection criteria, including an assessment of the impact of various observability metrics on the success rate of afterglow-based redshift measurement. We briefly outline our host-galaxy observational program, consisting of deep Spitzer/IRAC imaging of every field supplemented by similarly-deep, multi-color optical/NIR photometry, plus spectroscopy of events without pre-existing redshifts. Our optimized selection cuts combined with host-galaxy follow-up have so far enabled redshift measurements for 110 targets (92%) and placed upper limits on all but one of the remainder. About 20% of GRBs in the sample are heavily dust-obscured, and at most 2% originate from z>5.5. Using this sample we estimate the redshift-depen...

  4. Host/parasite interactions between Solenopsis invicta (Hymenoptera: Formicidae) and Thelohania solenopsae (Microsporida: Thelohaniidae)

    E-Print Network [OSTI]

    Hale, Michael Walker

    2007-09-17T23:59:59.000Z

    mounds and adoption rates, how T. solenopsae spores are affected by different stable temperatures. This study also examined the effects on T. solenopsae spores due to centrifugation out of the host cell, pH of the solution the spores are kept, and food...

  5. Host-IP Clustering Technique for Deep Web Characterization Denis Shestakov

    E-Print Network [OSTI]

    Hammerton, James

    Host-IP Clustering Technique for Deep Web Characterization Denis Shestakov Department of Media databases. This part of the Web, known as the deep Web, is to date relatively unexplored and even major are aimed at more accurate estimation of main parameters of the deep Web by sampling one national web domain

  6. Children's School May 2011 Children's School Co-Hosts NALS Conference

    E-Print Network [OSTI]

    Children's School May 2011 Children's School Co-Hosts NALS Conference Thanks to all the educators Affiliated Schools! We were honored by the presence and encouragement of H&SS Dean John Lehoczky, Psychology school's approach to early childhood education through offering tours, sharing a poster and presentations

  7. Hostile Takeover by Plasmodium: Reorganization of Parasite and Host Cell Membranes during Liver Stage

    E-Print Network [OSTI]

    Arnold, Jonathan

    MalaR (European Virtual Institute for Malaria Research) and Malsig (Signalling in life cycle stages of malaria is transmitted by female Anopheles mosquitoes and undergoes obligatory development within a parasitophorous to mask itself from the host immune system and bypass the numerous Kupffer cells on its way

  8. The relationship between host selection behaviour and offspring tness in a koinobiont parasitoid

    E-Print Network [OSTI]

    Rivero, Ana

    . Introduction A classic problem in parasitoid behavioural ecology is the prediction of which hosts a female foraging bout, depending both on the female's previous experience and hence perception of the environment-mail: Ana.Rivero@ed.ac.uk # 2000 Blackwell Science Ltd 467 Ecological Entomology (2000) 25, 467

  9. The metallicity and dust content of a redshift 5 gamma-ray burst host galaxy

    SciTech Connect (OSTI)

    Sparre, M.; Kr黨ler, T.; Fynbo, J. P. U.; Watson, D. J.; De Ugarte Postigo, A.; Hjorth, J.; Malesani, D. [Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 30, 2100 Copenhagen (Denmark); Hartoog, O. E.; Kaper, L. [Anton Pannekoek Institute for Astronomy, University of Amsterdam, Science Park 904, 1098 XH, Amsterdam (Netherlands); Wiersema, K. [Department of Physics and Astronomy, University of Leicester, University Road, Leicester, LE1 7RH (United Kingdom); D'Elia, V. [INAF/Rome Astronomical Observatory, via Frascati 33, I-00040 Monteporzio Catone (Roma) (Italy); Zafar, T. [European Southern Observatory, Karl-Schwarzschild-Strasse 2, D-85748 Garching (Germany); Afonso, P. M. J. [Physics and Astronomy Department, American River College, 4700 College Oak Drive, Sacramento, CA 95841 (United States); Covino, S. [INAF, Osservatorio Astronomico di Brera, via E. Bianchi 46, I-23807 Merate (Italy); Flores, H. [Laboratoire GEPI, Observatoire de Paris, CNRS-UMR8111, Universite Paris Diderot 5 place Jules Janssen, F-92195 Meudon (France); Goldoni, P. [APC, Astroparticule et Cosmologie, Universite Paris Diderot, CNRS/IN2P3, CEA/Irfu, Observatoire de Paris, Sorbonne Paris Cit, 10, Rue Alice Domon et L閛nie Duquet, F-75205 Paris, Cedex 13 (France); Greiner, J. [Max-Planck-Institut f黵 extraterrestrische Physik, Giessenbachstra遝, D-85748 Garching (Germany); Jakobsson, P. [Centre for Astrophysics and Cosmology, Science Institute, University of Iceland, Dunhagi 5, IS-107 Reykjavik (Iceland); Klose, S. [Th黵inger Landessternwarte Tautenburg, Sternwarte 5, D-07778 Tautenburg (Germany); Levan, A. J., E-mail: sparre@dark-cosmology.dk [Department of Physics, University of Warwick, Coventry CV4 7AL (United Kingdom); and others

    2014-04-20T23:59:59.000Z

    Observations of the afterglows of long gamma-ray bursts (GRBs) allow the study of star-forming galaxies across most of cosmic history. Here we present observations of GRB 111008A, from which we can measure metallicity, chemical abundance patterns, dust-to-metals ratio (DTM), and extinction of the GRB host galaxy at z = 5.0. The host absorption system is a damped Ly? absorber with a very large neutral hydrogen column density of log?N(H I)/cm{sup ?2}=22.300.06 and a metallicity of [S/H] = 1.70 0.10. It is the highest-redshift GRB with such a precise metallicity measurement. The presence of fine-structure lines confirms the z = 5.0 system as the GRB host galaxy and makes this the highest redshift where Fe II fine-structure lines have been detected. The afterglow is mildly reddened with A{sub V} = 0.11 0.04 mag, and the host galaxy has a DTM that is consistent with being equal to or lower than typical values in the Local Group.

  10. Selective Organic and Organometallic Reactions in Water-Soluble Host-Guest Supramolecular Systems

    SciTech Connect (OSTI)

    Pluth, Michael D.; Raymond, Kenneth N.; Bergman, Robert G.

    2008-02-16T23:59:59.000Z

    Inspired by the efficiency and selectivity of enzymes, synthetic chemists have designed and prepared a wide range of host molecules that can bind smaller molecules with their cavities; this area has become known as 'supramolecular' or 'host-guest' chemistry. Pioneered by Lehn, Cram, Pedersen, and Breslow, and followed up by a large number of more recent investigators, it has been found that the chemical environment in each assembly - defined by the size, shape, charge, and functional group availability - greatly influences the guest-binding characteristics of these compounds. In contrast to the large number of binding studies that have been carried out in this area, the exploration of chemistry - especially catalytic chemistry - that can take place inside supramolecular host cavities is still in its infancy. For example, until the work described here was carried out, very few examples of organometallic reactivity inside supramolecular hosts were known, especially in water solution. For that reason, our group and the group directed by Kenneth Raymond decided to take advantage of our complementary expertise and attempt to carry out metal-mediated C-H bond activation reactions in water-soluble supramolecular systems. This article begins by providing background from the Raymond group in supramolecular coordination chemistry and the Bergman group in C-H bond activation. It goes on to report the results of our combined efforts in supramolecular C-H activation reactions, followed by extensions of this work into a wider range of intracavity transformations.

  11. AGES CONSTRAINTS IN PEGMATITE PROVINCE RELATED TO CHARNOCKITIC HOST ROCKS IN MINAS GERAIS, BRAZIL

    E-Print Network [OSTI]

    Paris-Sud XI, Universit de

    AGES CONSTRAINTS IN PEGMATITE PROVINCE RELATED TO CHARNOCKITIC HOST ROCKS IN MINAS GERAIS, BRAZIL Fernando Machado de MELLO1 , Essaid BILAL2* , 1- Universidade Federal Rural do Rio de Janeiro, Brazil/ +33 4 7749 9707 Abstract Cambrian-Neoproterozoic granitoids suites in southeastern Brazil are the main

  12. Title: Working Together in Shale Gas Policy Hosts: Todd Cowen, Teresa Jordan and Christine Shoemaker

    E-Print Network [OSTI]

    Angenent, Lars T.

    Title: Working Together in Shale Gas Policy Hosts: Todd Cowen, Teresa Jordan and Christine and environmental groups. The Shale Gas Roundtable of the Institute of Politics at the University of Pittsburgh produced a report with several recommendations dealing especially with shale gas research, water use

  13. TOPIC: Shale Gas Emissions w/David Allen, Energy Institute HOST: Jeff Tester and Todd Cowen

    E-Print Network [OSTI]

    Angenent, Lars T.

    TOPIC: Shale Gas Emissions w/David Allen, Energy Institute HOST: Jeff Tester and Todd Cowen DATE fracturing of shale formations (shale gas) is projected by the Energy Information Administration to become the nation's energy landscape. However, the environmental impacts associated with ``fracking'' for shale gas

  14. Assessing Guest Diffusivities in Porous Hosts from Transient Concentration Profiles Lars Heinke,1

    E-Print Network [OSTI]

    Li, Jing

    deviate from the ideal textbook structure, with the possibility that these devia- tions (pore blockageAssessing Guest Diffusivities in Porous Hosts from Transient Concentration Profiles Lars Heinke,1 of mutual passages of the guest molecules in the chains of pore segments, thus quantifying departure from

  15. USFS Administrative Tour The Aspen FACE site hosted a visit of some 36 senior

    E-Print Network [OSTI]

    1 USFS Administrative Tour The Aspen FACE site hosted a visit of some 36 senior USFS administrators (USFS) welcomed the group to the site and Dave Karnosky (MTU) gave a brief overview of the Aspen FACE Global Change Program Director Rich Birdsey. Aspen FACE in the News On May 16, 2003, the Aspen FACE

  16. Infections and allergy --helminths, hygiene and host immune Rick M Maizels

    E-Print Network [OSTI]

    Maizels, Rick

    Infections and allergy -- helminths, hygiene and host immune regulation Rick M Maizels influence the development of allergies and other immunopathologies -- known as the `hygiene hypothesis to allergic disease [2]. The original `hygiene hypothesis' centred around the role of Th1-inducing microbial

  17. International Support On Hosting or Hiring Internationals Since 9/11

    E-Print Network [OSTI]

    Almor, Amit

    -Mail: isfs@sc.edu Website: http://hr.sc.edu/international.html #12;Hosting or Hiring Internationals | Page 2. Instructions are on the ISFS website; Best practice is to submit form both to Immigration & to International Support. State law sets special requirements for issuance of a S.C. driver's license E-Verify/FAR rules

  18. Communities of fungal endophytes in tropical forest grasses: highly diverse host-and habitat

    E-Print Network [OSTI]

    Coley, Phyllis

    Communities of fungal endophytes in tropical forest grasses: highly diverse host- and habitat: Charles W. Bacon Keywords: Barro Colorado Island Biodiversity Community assembly Fungal endophytes Poaceae- studied endophytes in the lowland forests of Panama. We used sequence data for 402 isolates from two

  19. Culturing and direct PCR suggest prevalent host generalism among diverse fungal endophytes of tropical forest grasses

    E-Print Network [OSTI]

    Coley, Phyllis

    Culturing and direct PCR suggest prevalent host generalism among diverse fungal endophytes examining endophytic fungi associated with grasses (Poaceae) have focused on agronomically important species and forest-edge communities. To provide a broader context for understanding grass-endophyte associations we

  20. The Endophytic System of Mediterranean Cytinus (Cytinaceae) Developing on Five Host Cistaceae Species

    E-Print Network [OSTI]

    Herrera, Carlos M.

    The Endophytic System of Mediterranean Cytinus (Cytinaceae) Developing on Five Host Cistaceae in the genus Cytinus, a holoparasite whose vegetative body is reduced to an endophytic system living within its scrublands. The aim of this work is to describe the endophytic systems of C. hypocistis and C. ruber

  1. Hosting Dynamic Data in the Cloud with Isis2 and the Ida DHT

    E-Print Network [OSTI]

    Keinan, Alon

    Hosting Dynamic Data in the Cloud with Isis2 and the Ida DHT Ken Birman and Heesung Sohn Dept, cloud storage and access technologies must be reexamined. Isis2 aims at such scenarios, offering a base called the Isis2 interactive data analysis infrastructure: Ida. Ida is a strongly-consistent distributed

  2. Discovery of the eucalypt pathogen Quambalaria eucalypti infecting a non-Eucalyptus host in Uruguay

    E-Print Network [OSTI]

    Discovery of the eucalypt pathogen Quambalaria eucalypti infecting a non-Eucalyptus host in Uruguay, Paysand煤, Uruguay. C Department of Microbiology and Plant Pathology, Forestry and Agricultural Agropecuaria, Ruta 48, km 10, Canelones, Uruguay. E Corresponding author. Email: caperez@fagro.edu.uy Abstract

  3. Automated, Retargetable Back-Annotation for Host Compiled Performance and Power Modeling

    E-Print Network [OSTI]

    Gerstlauer, Andreas

    and back- annotation of basic code blocks with all possible predeces- sors. Results from applying ourAutomated, Retargetable Back-Annotation for Host Compiled Performance and Power Modeling Suhas typical front- and back-end optimiza- tions by working at the compiler-generated intermediate rep

  4. DAX: A Widely Distributed Multi-tenant Storage Service for DBMS Hosting

    E-Print Network [OSTI]

    Aboulnaga, Ashraf

    DAX: A Widely Distributed Multi-tenant Storage Service for DBMS Hosting Rui Liu University data management needs that are best served by a SQL-based relational DBMS. It is not difficult to run a DBMS in the cloud, and in many cases one DBMS instance is enough to support an application's workload

  5. Scintillator having a MgAI.sub.2O.sub.4 host lattice

    DOE Patents [OSTI]

    Chen, Ching-Fong (Los Alamos, NM)

    2011-12-20T23:59:59.000Z

    A scintillator having a host lattice of MgAl.sub.2O.sub.4 was prepared by hot pressing under a vacuum environment a powder mixture of MgAl.sub.2O.sub.4, CeO.sub.2, and LiF.

  6. Library Hosted Catalogs Job Aid PURCH12/23/13L.Tran Page1

    E-Print Network [OSTI]

    California at Berkeley, University of

    , enter in the applicable search terms, and click the Go button. 2. The search results are shown items from preferred suppliers at University-specific pricing. Use Advanced Search options to enter, and then enter the applicable search item and the click Search button #12; Library Hosted Catalogs Job

  7. A Comprehensive Collection of Systems Biology Data Characterizing the Host Response to Viral Infection

    SciTech Connect (OSTI)

    Aevermann, Brian; Pickett, Brett E.; Kumar, Sanjeev; Klem, Edward B.; Agnihothram, Sudhakar; Askovich, Peter S.; Bankhead, Armand; Bolles, Meagan; Carter, Victoria; Chang, Jean H.; Clauss, Therese RW; Dash, Pradyot; Diercks, Alan H.; Eisfeld, Amie J.; Ellis, Amy L.; Fan, Shufang; Ferris, Martin T.; Gralinski, Lisa; Green, Richard; Gritsenko, Marina A.; Hatta, Masato; Heegel, Robert A.; Jacobs, Jon M.; Jeng, Sophia; Josset, Laurence; Kaiser, Shari M.; Kelly, Sarah; Law, Gale L.; Li, Chengjun; Li, Jiangning; Long, Casey; Luna, Maria L.; Matzke, Melissa M.; McDermott, Jason E.; Menachery, Vineet; Metz, Thomas O.; Mitchell, Hugh D.; Monroe, Matthew E.; Navarro, Garnet; Neumann, Gabriele; Podyminogin, Rebecca L.; Purvine, Samuel O.; Rosenberger, Carrie; Sanders, Catherine J.; Schepmoes, Athena A.; Shukla, Anil K.; Sims, Amy; Sova, Pavel; Tam, Vincent C.; Tchitchek, Nicholas; Thomas, Paul G.; Tilton, Susan C.; Totura, Allison L.; Wang, Jing; Webb-Robertson, Bobbie-Jo M.; Wen, Ji; Weiss, Jeffrey M.; Yang, Feng; Yount, Boyd; Zhang, Qibin; Mcweeney, Shannon K.; Smith, Richard D.; Waters, Katrina M.; Kawaoka, Yoshihiro; Baric, Ralph; Aderem, Alan; Katze, Michael G.; Scheuermann, Richard H.

    2014-10-14T23:59:59.000Z

    The Systems Biology for Infectious Diseases Research program was established by the U.S. National Institute of Allergy and Infectious Diseases to investigate host-pathogen interactions at a systems level. This program generated 47 transcriptomic and proteomic datasets from 30 studies that investigate in vivo and in vitro host responses to viral infections. Human pathogens in the Orthomyxoviridae and Coronaviridae families, especially pandemic H1N1 and avian H5N1 influenza A viruses and severe acute respiratory syndrome coronavirus (SARS-CoV), were investigated. Study validation was demonstrated via experimental quality control measures and meta-analysis of independent experiments performed under similar conditions. Primary assay results are archived at the GEO and PeptideAtlas public repositories, while processed statistical results together with standardized metadata are publically available at the Influenza Research Database (www.fludb.org) and the Virus Pathogen Resource (www.viprbrc.org). By comparing data from mutant versus wild-type virus and host strains, RNA versus protein differential expression, and infection with genetically similar strains, these data can be used to further investigate genetic and physiological determinants of host responses to viral infection.

  8. orbit their host star at distances closer than Mercury's orbit around the Sun (Fig. 1) --is

    E-Print Network [OSTI]

    Schnaufer, Achim

    ) -- is notunusualforanextrasolarplanetarysystem. Many similar dense configurations have been detected by the radial-velocity (Doppler) technique ofthe dynamical effect of the planets on their host stars (obtained through Doppler and transit. The Doppler technique measures tiny Doppler shifts in a parent star's light that are caused

  9. The Rockefeller Foundation to Host Bellagio Center Conference on Humanitarian Logistics: Networks for Africa

    E-Print Network [OSTI]

    Nagurney, Anna

    The Rockefeller Foundation to Host Bellagio Center Conference on Humanitarian Logistics: Networks to the Rockefeller Foundation; http://rockfound.org to organize a conference on "Humanitarian Logistics: Networks some of the underlying themes that will be discussed in depth. Logistics networks, in times of need

  10. allowing a longer period of infection within an individual host and by facilitating re-

    E-Print Network [OSTI]

    Cai, Long

    T cells and neutralizing antibodies. It augments viral load and thus accelerates the destruc- tion of CD4 cells. There is a highly dynamic balance of power between HIV and the immune system, which is slowly, dis- cussing genetic differences among hosts in theirimmuneresponsesandimmunemem- ory profiles

  11. -News Home Help EU offers 'sweetener' to Japan to let France host nuclear project

    E-Print Network [OSTI]

    to host a revolutionary nuclear fusion project. news web sites "I cannot elaborate on the sweetener, but I Wednesday after talks in Vienna on the International Thermonuclear Experimental Reactor (ITER). news web ( - ) -- which have supported the Japanese bid -- plus Russia and China, which back the EU bid.news web sites

  12. Phyllody of faba bean in the Sudan. I. Progress of symptom expression, host range and transmis-

    E-Print Network [OSTI]

    Paris-Sud XI, Universit de

    Phyllody of faba bean in the Sudan. I. Progress of symptom expression, host range and transmis bean phyllody was followed in a local susceptible cultivar, Hudeiba 72, graft-inoculated from naturally and slow development of disease, sometimes partial recovery. Symptom expression in faba bean plants

  13. Wild birds as possible hosts and vectors of mammalian strains of Chlamydia psittaci

    E-Print Network [OSTI]

    Johnson, Mark Caylor

    1982-01-01T23:59:59.000Z

    of eucaryot1c cells but does not affect procaryotic cells such as chlamydiae (1, 68). Nith inhibit1on of the host cell's growth, the cytoplasmic pools of amino ac1ds and nucleos1des are ava1lable to the chlamyd1ae. The organisms have a negative Gram...

  14. Demographics of the Galaxies Hosting Short-duration Gamma-Ray Bursts

    E-Print Network [OSTI]

    Fong, Wen-fai; Chornock, Ryan; Margutti, Raffaella; Levan, Andrew J; Tanvir, Nial R; Tunnicliffe, Rachel L; Czekala, Ian; Fox, Derek B; Perley, Daniel A; Cenko, S Bradley; Zauderer, B Ashley; Laskar, Tanmoy; Persson, S Eric; Monson, Andrew J; Kelson, Daniel D; Birk, Christoph; Murphy, David; Servillat, Mathieu; Anglada, Guillem

    2013-01-01T23:59:59.000Z

    We present observations of the afterglows and host galaxies of three short-duration gamma-ray bursts (GRBs): 100625A, 101219A and 110112A. We find that GRB 100625A occurred in a z=0.452 early-type galaxy with a stellar mass of 4.6e9 M_Sun and a stellar population age of 0.7 Gyr, and GRB 101219A originated in a star-forming galaxy at z=0.718 with a stellar mass of 1.4e9 M_Sun, a star formation rate of 16 M_Sun yr^-1, and a stellar population age of 50 Myr. We also report the discovery of the optical afterglow of GRB 110112A, which lacks a coincident host galaxy to i>26 mag and we cannot conclusively identify any field galaxy as a possible host. The bursts have inferred circumburst densities of ~1e-4-1 cm^-3, and isotropic-equivalent gamma-ray and kinetic energies of 1e50-1e51 erg. These events highlight the diversity of galaxies that host short GRBs. To quantify this diversity, we use the sample of 36 Swift short GRBs with robust associations to an environment (~1/2 of 68 short bursts detected by Swift to May ...

  15. Are Your Hosts Trading or Plotting? Telling P2P File-Sharing and Bots Apart

    E-Print Network [OSTI]

    North Carolina at Chapel Hill, University of

    performed by the infected hosts (e.g., spam forwarding, DDoS), but rather that are basic properties. In both cases, status information about available peers needs to be maintained constantly to ensure publicized and well-studied P2P botnet, Storm, built its communication protocol based on the Overnet network

  16. Are Your Hosts Trading or Plotting? Telling P2P File-Sharing and Bots Apart

    E-Print Network [OSTI]

    Reiter, Michael

    on particular attack activities performed by the infected hosts (e.g., spam forwarding, DDoS), but rather file-sharing, making it difficult to separate these two types of traffic. In both cases, status- tuated by the fact that one highly publicized and well- studied P2P botnet, Storm, built its

  17. Paper #194973 GEOCHEMICAL CHARACTERIZATION OF THE RESERVOIR HOSTING SHALE-GAS AND OIL in

    E-Print Network [OSTI]

    Paper #194973 GEOCHEMICAL CHARACTERIZATION OF THE RESERVOIR HOSTING SHALE-GAS AND OIL a reservoir for shale-gas and oil. We examined organic-rich black shale, known as Macasty shale, of Upper SHALE-GAS AND OIL in THE SUBSURFACE OF ANTICOSTI ISLAND, CANADA Key Words: Provenance, Anticosti Island

  18. FUNDAMENTAL PROPERTIES OF KEPLER PLANET-CANDIDATE HOST STARS USING ASTEROSEISMOLOGY

    SciTech Connect (OSTI)

    Huber, Daniel; Lissauer, Jack J.; Rowe, Jason F. [NASA Ames Research Center, Moffett Field, CA 94035 (United States); Chaplin, William J. [School of Physics and Astronomy, University of Birmingham, Birmingham B15 2TT (United Kingdom); Christensen-Dalsgaard, Jorgen; Kjeldsen, Hans; Handberg, Rasmus; Karoff, Christoffer; Lund, Mikkel N.; Lundkvist, Mia [Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120, DK-8000 Aarhus C (Denmark); Gilliland, Ronald L. [Center for Exoplanets and Habitable Worlds, The Pennsylvania State University, 525 Davey Lab, University Park, PA 16802 (United States); Buchhave, Lars A. [Niels Bohr Institute, University of Copenhagen, DK-2100 Copenhagen (Denmark); Fischer, Debra A.; Basu, Sarbani [Department of Astronomy, Yale University, New Haven, CT 06511 (United States); Sanchis-Ojeda, Roberto [Department of Physics, Massachusetts Institute of Technology, 77 Massachusetts Ave., Cambridge, MA 02139 (United States); Hekker, Saskia [Astronomical Institute ''Anton Pannekoek'', University of Amsterdam, Science Park 904, 1098 XH Amsterdam (Netherlands); Howard, Andrew W. [Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822 (United States); Isaacson, Howard; Marcy, Geoffrey W. [Department of Astronomy, University of California, Berkeley, CA 94720 (United States); Latham, David W., E-mail: daniel.huber@nasa.gov [Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138 (United States); and others

    2013-04-20T23:59:59.000Z

    We have used asteroseismology to determine fundamental properties for 66 Kepler planet-candidate host stars, with typical uncertainties of 3% and 7% in radius and mass, respectively. The results include new asteroseismic solutions for four host stars with confirmed planets (Kepler-4, Kepler-14, Kepler-23 and Kepler-25) and increase the total number of Kepler host stars with asteroseismic solutions to 77. A comparison with stellar properties in the planet-candidate catalog by Batalha et al. shows that radii for subgiants and giants obtained from spectroscopic follow-up are systematically too low by up to a factor of 1.5, while the properties for unevolved stars are in good agreement. We furthermore apply asteroseismology to confirm that a large majority of cool main-sequence hosts are indeed dwarfs and not misclassified giants. Using the revised stellar properties, we recalculate the radii for 107 planet candidates in our sample, and comment on candidates for which the radii change from a previously giant-planet/brown-dwarf/stellar regime to a sub-Jupiter size or vice versa. A comparison of stellar densities from asteroseismology with densities derived from transit models in Batalha et al. assuming circular orbits shows significant disagreement for more than half of the sample due to systematics in the modeled impact parameters or due to planet candidates that may be in eccentric orbits. Finally, we investigate tentative correlations between host-star masses and planet-candidate radii, orbital periods, and multiplicity, but caution that these results may be influenced by the small sample size and detection biases.

  19. THE RELATION BETWEEN BLACK HOLE MASS AND HOST SPHEROID STELLAR MASS OUT TO z {approx} 2

    SciTech Connect (OSTI)

    Bennert, Vardha N.; Auger, Matthew W.; Treu, Tommaso [Department of Physics, University of California, Santa Barbara, CA 93106 (United States); Woo, Jong-Hak [Astronomy Program, Department of Physics and Astronomy, Seoul National University (Korea, Republic of); Malkan, Matthew A., E-mail: vbennert@calpoly.edu, E-mail: tt@physics.ucsb.edu, E-mail: mauger@ast.cam.ac.uk, E-mail: woo@astro.snu.ac.kr, E-mail: malkan@astro.ucla.edu [Department of Physics and Astronomy, University of California, Los Angeles, CA 90095 (United States)

    2011-12-01T23:59:59.000Z

    We combine Hubble Space Telescope images from the Great Observatories Origins Deep Survey with archival Very Large Telescope and Keck spectra of a sample of 11 X-ray-selected broad-line active galactic nuclei in the redshift range 1 < z < 2 to study the black-hole-mass-stellar-mass relation out to a look-back time of 10 Gyr. Stellar masses of the spheroidal component (M{sub sph,*}) are derived from multi-filter surface photometry. Black hole masses (M{sub BH}) are estimated from the width of the broad Mg II emission line and the 3000 A nuclear luminosity. Comparing with a uniformly measured local sample and taking into account selection effects, we find evolution in the form M{sub BH}/M{sub sph,*}{proportional_to}(1 + z){sup 1.96{+-}}0{sup .55}, in agreement with our earlier studies based on spheroid luminosity. However, this result is more accurate because it does not require a correction for luminosity evolution and therefore avoids the related and dominant systematic uncertainty. We also measure total stellar masses (M{sub host,*}). Combining our sample with data from the literature, we find M{sub BH}/M{sub host,*}{proportional_to}(1 + z){sup 1.15{+-}0.15}, consistent with the hypothesis that black holes (in the range M{sub BH} {approx} 10{sup 8-9} M{sub Sun }) pre-date the formation of their host galaxies. Roughly, one-third of our objects reside in spiral galaxies; none of the host galaxies reveal signs of interaction or major merger activity. Combined with the slower evolution in host stellar masses compared to spheroid stellar masses, our results indicate that secular evolution or minor mergers play a non-negligible role in growing both BHs and spheroids.

  20. Variational Implicit-Solvent Modeling of Host-Guest Binding: A Case Study on Cucurbit[7]uril

    E-Print Network [OSTI]

    Li, Bo

    of Utah, Salt Lake City, UT 84112-5820, United States 5 Department of Mathematics, University of the individual VISM free-energy contributions shows that the major driving forces are water-mediated hydrophobic[n]uril hosts thanks to its good balance between the number of water molecules confined in the host cavity

  1. Managing Energy and Server Resources in Hosting Centers Jeffrey S. Chase, Darrell C. Anderson, Prachi N. Thakar, Amin M. Vahdat

    E-Print Network [OSTI]

    Sirer, Emin Gun

    of delivered performance. The system continuously moni- tors load and plans resource allotments by estimating bandwidth) to insulate its customers from demand surges and capital costs for excess capacity. HostingManaging Energy and Server Resources in Hosting Centers Jeffrey S. Chase, Darrell C. Anderson

  2. New Approaches to Improved Animal Health: Systems Biology and Modeling of Real Interactions of Pathogens and their Hosts

    E-Print Network [OSTI]

    decade or sousing comprehensive systems biology approaches linking genomics, proteomics, bioinformatics of computational systems biology analysis of host:pathogen interactions (the interactome) as a tool for enhanced are using computational systems biology methods to create interactome models of the actual host responses

  3. DEMOGRAPHICS OF THE GALAXIES HOSTING SHORT-DURATION GAMMA-RAY BURSTS

    SciTech Connect (OSTI)

    Fong, W.; Berger, E.; Chornock, R.; Margutti, R.; Czekala, I.; Zauderer, B. A.; Laskar, T.; Servillat, M. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Levan, A. J.; Tunnicliffe, R. L. [Department of Physics, University of Warwick, Coventry CV4 7AL (United Kingdom); Tanvir, N. R. [Department of Physics and Astronomy, University of Leicester, University Road, Leicester LE1 7RH (United Kingdom); Fox, D. B. [Department of Astronomy and Astrophysics, 525 Davey Laboratory, Pennsylvania State University, University Park, PA 16802 (United States); Perley, D. A. [Cahill Center for Astronomy and Astrophysics, Room 232, California Institute of Technology, Pasadena, CA 91125 (United States); Cenko, S. B. [Department of Astronomy, University of California, Berkeley, CA 94720-3411 (United States); Persson, S. E.; Monson, A. J.; Kelson, D. D.; Birk, C.; Murphy, D. [Observatories of the Carnegie Institution for Science, 813 Santa Barbara Street, Pasadena, CA 91101 (United States); Anglada, G. [Institut fuer Astrophysik, Friedrich-Hund-Platz 1, Universitaet Goettingen, D-37077 Goettingen (Germany)

    2013-05-20T23:59:59.000Z

    We present observations of the afterglows and host galaxies of three short-duration gamma-ray bursts (GRBs): 100625A, 101219A, and 110112A. We find that GRB 100625A occurred in a z = 0.452 early-type galaxy with a stellar mass of Almost-Equal-To 4.6 Multiplication-Sign 10{sup 9} M{sub Sun} and a stellar population age of Almost-Equal-To 0.7 Gyr, and GRB 101219A originated in a star-forming galaxy at z = 0.718 with a stellar mass of Almost-Equal-To 1.4 Multiplication-Sign 10{sup 9} M{sub Sun }, a star formation rate of Almost-Equal-To 16 M{sub Sun} yr{sup -1}, and a stellar population age of Almost-Equal-To 50 Myr. We also report the discovery of the optical afterglow of GRB 110112A, which lacks a coincident host galaxy to i {approx}> 26 mag, and we cannot conclusively identify any field galaxy as a possible host. From afterglow modeling, the bursts have inferred circumburst densities of Almost-Equal-To 10{sup -4}-1 cm{sup -3} and isotropic-equivalent gamma-ray and kinetic energies of Almost-Equal-To 10{sup 50}-10{sup 51} erg. These three events highlight the diversity of galactic environments that host short GRBs. To quantify this diversity, we use the sample of 36 Swift short GRBs with robust associations to an environment ({approx}1/2 of 68 short bursts detected by Swift to 2012 May) and classify bursts originating from four types of environments: late-type ( Almost-Equal-To 50%), early-type ( Almost-Equal-To 15%), inconclusive ( Almost-Equal-To 20%), and ''host-less'' (lacking a coincident host galaxy to limits of {approx}> 26 mag; Almost-Equal-To 15%). To find likely ranges for the true late- and early-type fractions, we assign each of the host-less bursts to either the late- or early-type category using probabilistic arguments and consider the scenario that all hosts in the inconclusive category are early-type galaxies to set an upper bound on the early-type fraction. We calculate most likely ranges for the late- and early-type fractions of Almost-Equal-To 60%-80% and Almost-Equal-To 20%-40%, respectively. We find no clear trend between gamma-ray duration and host type. We also find no change to the fractions when excluding events recently claimed as possible contaminants from the long GRB/collapsar population. Our reported demographics are consistent with a short GRB rate driven by both stellar mass and star formation.

  4. 3D climate modeling of Earth-like extrasolar planets orbiting different types of host stars

    E-Print Network [OSTI]

    Godolt, M; Hamann-Reinus, A; Kitzmann, D; Kunze, M; Langematz, U; von Paris, P; Patzer, A B C; Rauer, H; Stracke, B

    2015-01-01T23:59:59.000Z

    The potential habitability of a terrestrial planet is usually defined by the possible existence of liquid water on its surface. The potential presence of liquid water depends on many factors such as, most importantly, surface temperatures. The properties of the planetary atmosphere and its interaction with the radiative energy provided by the planet's host star are thereby of decisive importance. In this study we investigate the influence of different main-sequence stars upon the climate of Earth-like extrasolar planets and their potential habitability by applying a 3D Earth climate model accounting for local and dynamical processes. The calculations have been performed for planets with Earth-like atmospheres at orbital distances where the total amount of energy received from the various host stars equals the solar constant. In contrast to previous 3D modeling studies, we include the effect of ozone radiative heating upon the vertical temperature structure of the atmospheres. The global orbital mean results o...

  5. A novel test for host-symbiont codivergence indicates ancient origin of fungal endophytes in grasses

    E-Print Network [OSTI]

    Schardl, Chris L; Lindstrom, Adam; Speakman, Skyler; Stromberg, Arnold; Yoshida, Ruriko

    2007-01-01T23:59:59.000Z

    Significant phylogenetic codivergence between plant or animal hosts ($H$) and their symbionts or parasites ($P$) indicate the importance of their interactions on evolutionary time scales. However, valid and realistic methods to test for codivergence are not fully developed. One of the systems where possible codivergence has been of interest involves the large subfamily of temperate grasses (Pooideae) and their endophytic fungi (epichloae). These widespread symbioses often help protect host plants from herbivory and stresses, and affect species diversity and food web structures. Here we introduce the MRCALink (most-recent-common-ancestor link) method and use it to investigate the possibility of grass-epichlo\\"e codivergence. MRCALink applied to ultrametric $H$ and $P$ trees identifies all corresponding nodes for pairwise comparisons of MRCA ages. The result is compared to the space of random $H$ and $P$ tree pairs estimated by a Monte Carlo method.

  6. The Hydroxyl-Water Megamaser Connection. I. Water Emission Toward OH Megamaser Hosts

    E-Print Network [OSTI]

    Wiggins, Brandon K; Smidt, Joseph M

    2015-01-01T23:59:59.000Z

    Though megamasers are used to probe extragalactic phenomena, questions remain regarding their production and connection to galactic processes. The observation that water and hydroxyl megamasers rarely coexist in the same galaxy has given rise to the hypothesis that the two megamaser species appear in different phases of nuclear activity or that somehow their presence distinguishes different physical conditions in the medium. However, simultaneous hydroxyl and water megamaser emission has recently been detected in IC 694. Studies of this object are underway but, because many megamasers have not been surveyed for emission in the other molecule, it remains unclear whether IC 694 occupies a narrow phase of galaxy evolution or whether the relationship between megamaser species and galactic processes is more complicated than previously believed. In this paper, we present preliminary results of a systematic search for 22 GHz water maser emission among OH megamaser hosts to identify additional objects hosting both me...

  7. THE HOMOGENEOUS STUDY OF TRANSITING SYSTEMS (HoSTS). I. THE PILOT STUDY OF WASP-13

    SciTech Connect (OSTI)

    Gomez Maqueo Chew, Yilen; Cargile, Phillip; Hebb, Leslie; Stassun, Keivan G. [Department of Physics and Astronomy, Vanderbilt University, Nashville, TN 37235 (United States); Faedi, Francesca; Pollacco, Don [Department of Physics, University of Warwick, Coventry CV4 7AL (United Kingdom); Doyle, Amanda P.; Smalley, Barry [Astrophysics Group, Keele University, Staffordshire ST5 5BG (United Kingdom); Ghezzi, Luan; Cunha, Katia; Smith, Verne V. [Observatorio Nacional, Rua Gal. Jose Cristino 77, Rio de Janeiro, RJ 20921-400 (Brazil); Sousa, Sergio; Santos, Nuno C. [Centro de Astrofisica, Universidade do Porto, Rua das Estrelas, 4150-762 Porto (Portugal); Barros, Susana C. C. [LAM (Laboratoire d'Astrophysique de Marseille) UMR 7326, Aix Marseille Universite, CNRS, F-13388 Marseille (France); Schuler, Simon C. [Stewart Observatory, University of Arizona, Tucson, AZ 85721 (United States); Collier Cameron, Andrew, E-mail: yilen.gomez@vanderbilt.edu [School of Physics and Astronomy, University of St Andrews, St Andrews, Fife KY16 9SS (United Kingdom)

    2013-05-01T23:59:59.000Z

    We present the fundamental stellar and planetary properties of the transiting planetary system WASP-13 within the framework of the Homogeneous Study of Transiting Systems (HoSTS). HoSTS aims to derive the fundamental stellar (T{sub eff}, [Fe/H], M{sub *}, R{sub *}) and planetary (M{sub pl}, R{sub pl}, T{sub eq}) physical properties of known transiting planets using a consistent methodology and homogeneous high-quality data set. Four spectral analysis techniques are independently applied to a Keck+HIRES spectrum of WASP-13 considering two distinct cases: unconstrained parameters and constrained log g from transit light curves. We check the derived stellar temperature against that from a different temperature diagnostic based on an INT+IDS H{alpha} spectrum. The four unconstrained analyses render results that are in good agreement, and provide an improvement of 50% in the precision of T{sub eff}, and of 85% in [Fe/H] with respect to the WASP-13 discovery paper. The planetary parameters are then derived via the Monte Carlo Markov Chain modeling of the radial velocity and light curves, in iteration with stellar evolutionary models to derive realistic uncertainties. WASP-13 (1.187 {+-} 0.065 M{sub Sun }; 1.574 {+-} 0.048 R{sub Sun }) hosts a Saturn-mass, transiting planet (0.500 {+-} 0.037 M{sub Jup}; 1.407 {+-} 0.052 R{sub Jup}), and is at the end of its main-sequence lifetime (4-5.5 Gyr). Our analysis of WASP-13 showcases that both a detailed stellar characterization and transit modeling are necessary to well determine the fundamental properties of planetary systems, which are paramount in identifying and determining empirical relationships between transiting planets and their hosts.

  8. Effects of method of wheat streak mosaic virus transmission on the resistance of selected hosts

    E-Print Network [OSTI]

    Cho, Han Yong

    1969-01-01T23:59:59.000Z

    of these hybrids, which showed resistance to infection, were frequently reclassified as a susceptible host after reinoculation. The efficiency of transmission of WSMV to wheat by the mite, artist's airbrush, and carborundum rub inoculations were 49. 2, and 41... OF CONTENTS Chapter Page I INTRODUCTION II REVIEW OF THE LITERATURE III GENERAL MATERIALS AND METHODS Plant Materials Virus and Vector Virus Mite Transmission Carborundum rub Artist's airbrush Mite transmission 10 10 11 11 11 1. 2 12 12 13...

  9. Host recognition in Muscidifurax zaraptor (Hymenoptera :Pteromalidae): a parasitoid of the house fly

    E-Print Network [OSTI]

    Jones, Randy Russel

    2002-01-01T23:59:59.000Z

    al. 1996; Gilbert and Rayer 1985; Stamhuis et al. 1996; Walgenbach and Burkholder 1987) according to various changes in the behavior of the parasitoid as a result of the parasitoid being naive or experienced and the host being parasitized or non... the hide of animals and feeds on the blood. The feeding activity disturbs the animals and may affect weight gain and milk production of cattle (Bruce and Decker 1958; Campbell et al. 1977, 1987). Stable fly related reductions in livestock related...

  10. On the Fueling of Massive Black Holes and the Properties of their Host Spheroids

    E-Print Network [OSTI]

    Andres Escala

    2006-08-31T23:59:59.000Z

    We study the relation between nuclear massive black holes and their host spheroid gravitational potential. Using simple models, we analyze how gas is expected to be transported in the nuclear regions of galaxies. When we couple it with the expected gas lifetime given by the Kennicutt-Schmidt Law, this naturally leads to the `M_BH - M_virial' and `M_BH - sigma' relations. We also numerically test, using AMR simulations, our simple models for the mass transport with satisfactory results.

  11. Systematic Effects in Type-1a Supernovae Surveys from Host Galaxy Spectra

    SciTech Connect (OSTI)

    Strauss, Michael A. [Princeton University

    2013-08-23T23:59:59.000Z

    The physical relation between the properties of Type Ia supernovae and their host galaxies is investigated. Such supernovae are used to constrain the properties of dark energy, making it crucial to understand their physical properties and to check for systematic effects relating to the stellar populations of the progenitor stars from which these supernovae arose. This grant found strong evidence for two distinct populations of supernovae, and correlations between the progenitor stellar populations and the nature of the supernova light curves.

  12. CONSTRAINTS ON OBSCURED STAR FORMATION IN HOST GALAXIES OF GAMMA-RAY BURSTS

    SciTech Connect (OSTI)

    Hatsukade, Bunyo; Ohta, Kouji [Department of Astronomy, Kyoto University, Kyoto 606-8502 (Japan); Hashimoto, Tetsuya; Nakanishi, Kouichiro [National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588 (Japan); Tamura, Yoichi; Kohno, Kotaro, E-mail: hatsukade@kusastro.kyoto-u.ac.jp [Institute of Astronomy, the University of Tokyo, 2-21-1 Osawa, Mitaka, Tokyo 181-0015 (Japan)

    2012-04-01T23:59:59.000Z

    We present the results of the 16 cm wave band continuum observations of four host galaxies of gamma-ray bursts (GRBs) 990705, 021211, 041006, and 051022 using the Australia Telescope Compact Array. Radio emission was not detected in any of the host galaxies. The 2{sigma} upper limits on star formation rates derived from the radio observations of the host galaxies are 23, 45, 27, and 26 M{sub Sun} yr{sup -1}, respectively, which are less than about 10 times those derived from UV/optical observations, suggesting that they have no significant dust-obscured star formation. GRBs 021211 and 051022 are known as the so-called dark GRBs and our results imply that dark GRBs do not always occur in galaxies enshrouded by dust. Because large dust extinction was not observed in the afterglow of GRB 021211, our result suggests the possibility that the cause of the dark GRB is the intrinsic faintness of the optical afterglow. On the other hand, by considering the high column density observed in the afterglow of GRB 051022, the likely cause of the dark GRB is the dust extinction in the line of sight of the GRB.

  13. Identification of genetic loci that control mammary tumor susceptibility through the host microenvironment

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Zhang, Pengju; Lo, Alvin; Huang, Yurong; Huang, Ge; Liang, Guozhou; Mott, Joni; Karpen, Gary H.; Blakely, Eleanor A.; Bissell, Mina J.; Barcellos-Hoff, Mary Helen; et al

    2015-03-09T23:59:59.000Z

    The interplay between host genetics, tumor microenvironment and environmental exposure in cancer susceptibility remains poorly understood. Here we assessed the genetic control of stromal mediation of mammary tumor susceptibility to low dose ionizing radiation (LDIR) using backcrossed F1 into BALB/c (F1Bx) between cancer susceptible (BALB/c) and resistant (SPRET/EiJ) mouse strains. Tumor formation was evaluated after transplantation of non-irradiated Trp53-/- BALB/c mammary gland fragments into cleared fat pads of F1Bx hosts. Genome-wide linkage analysis revealed 2 genetic loci that constitute the baseline susceptibility via host microenvironment. However, once challenged with LDIR, we discovered 13 additional loci that were enriched for genesmore牷involved in cytokines, including TGF?1 signaling. Surprisingly, LDIR-treated F1Bx cohort significantly reduced incidence of mammary tumors from Trp53-/- fragments as well as prolonged tumor latency, compared to sham-treated controls. We demonstrated further that plasma levels of specific cytokines were significantly correlated with tumor latency. Using an ex vivo 3-D assay, we confirmed TGF?1 as a strong candidate for reduced mammary invasion in SPRET/EiJ, which could explain resistance of this strain to mammary cancer risk following LDIR. Our results open possible new avenues to understand mechanisms of genes operating via the stroma that affect cancer risk from external environmental exposures.珷less

  14. Radio constraints on heavily obscured star formation within dark gamma-ray burst host galaxies

    SciTech Connect (OSTI)

    Perley, D. A. [Department of Astronomy, California Institute of Technology, MC 249-17, 1200 East California Blvd., Pasadena, CA 91125 (United States); Perley, R. A., E-mail: dperley@astro.caltech.edu [National Radio Astronomy Observatory, P.O. Box O, Socorro, NM 87801 (United States)

    2013-12-01T23:59:59.000Z

    Highly dust-obscured starbursting galaxies (submillimeter galaxies and their ilk) represent the most extreme sites of star formation in the distant universe and contribute significantly to overall cosmic star formation beyond z > 1.5. Some stars formed in these environments may also explode as gamma-ray bursts (GRBs) and contribute to the population of 'dark' bursts. Here we present Very Large Array wideband radio-continuum observations of 15 heavily dust-obscured Swift GRBs to search for radio synchrotron emission associated with intense star formation in their host galaxies. Most of these targets (11) are not detected. Of the remaining four objects, one detection is marginal, and for two others we cannot yet rule out the contribution of a long-lived radio afterglow. The final detection is secure, but indicates a star formation rate (SFR) roughly consistent with the dust-corrected UV-inferred value. Most galaxies hosting obscured GRBs are therefore not forming stars at extreme rates, and the amount of optical extinction seen along a GRB afterglow sightline does not clearly correlate with the likelihood that the host has a sufficiently high SFR to be radio-detectable. While some submillimeter galaxies do readily produce GRBs, these GRBs are often not heavily obscured梥uggesting that the outer (modestly obscured) parts of these galaxies overproduce GRBs and the inner (heavily obscured) parts underproduce GRBs relative to their respective contributions to star formation, hinting at strong chemical or initial mass function gradients within these systems.

  15. A low-luminosity type-1 QSO sample: II. Overluminous host spheroidals or undermassive black holes?

    E-Print Network [OSTI]

    Busch, Gerold; Valencia-S., M髇ica; Moser, Lydia; Fischer, Sebastian; Eckart, Andreas; Scharw鋍hter, Julia; Gadotti, Dimitri A; Wisotzki, Lutz

    2013-01-01T23:59:59.000Z

    Recognizing the properties of the host galaxies of quasi-stellar objects (QSOs) is essential to understand the suspected coevolution of central supermassive black holes (BHs) and their host galaxies. We selected a subsample of the Hamburg/ESO survey for bright UV-excess QSOs, containing only the 99 nearest QSOs with redshift z<=0.06, that are close enough to allow detailed structural analysis. From this "low-luminosity type-1 QSO sample", we observed 20 galaxies and performed aperture photometry and bulge-disk-bar-AGN-decomposition with BUDDA on near-infrared J, H, K band images. From the photometric decomposition of these 20 objects and visual inspection of images of another 26, we find that ~50% of the hosts are disk galaxies and most of them (86%) are barred. Stellar masses, calculated from parametric models based on inactive galaxy colors, range from 2x10^9 M_sun to 2x10^11 M_sun. Black hole masses measured from single epoch spectroscopy range from 1x10^6 M_sun to 5x10^8 M_sun. In comparison to higher ...

  16. City of San Jose to host Renewable Energy From Waste Conference 2014 November 18-20, 2014, Double Tree by Hilton, San Jose, California

    E-Print Network [OSTI]

    City of San Jose to host Renewable Energy From Waste Conference 2014 for the second Renewable Energy From Waste Conference, to be hosted by the City of San, California. Following the overwhelming success of the 2013 event, Renewable Energy

  17. Host Genetic Control of the Microbiome in Humans and Maise or Relating Host Genetic Variation to the Microbiome (2011 JGI User Meeting)

    ScienceCinema (OSTI)

    Ley, Ruth [Cornell University

    2011-06-03T23:59:59.000Z

    The U.S. Department of Energy Joint Genome Institute (JGI) invited scientists interested in the application of genomics to bioenergy and environmental issues, as well as all current and prospective users and collaborators, to attend the annual DOE JGI Genomics of Energy & Environment Meeting held March 22-24, 2011 in Walnut Creek, Calif. The emphasis of this meeting was on the genomics of renewable energy strategies, carbon cycling, environmental gene discovery, and engineering of fuel-producing organisms. The meeting features presentations by leading scientists advancing these topics. Ruth Ley of Cornell University gives a presentation on "Relating Host Genetic Variation to the Microbiome" at the 6th annual Genomics of Energy & Environment Meeting on March 23, 2011.

  18. Host Genetic Control of the Microbiome in Humans and Maise or Relating Host Genetic Variation to the Microbiome (2011 JGI User Meeting)

    SciTech Connect (OSTI)

    Ley, Ruth [Cornell University] [Cornell University

    2011-03-23T23:59:59.000Z

    The U.S. Department of Energy Joint Genome Institute (JGI) invited scientists interested in the application of genomics to bioenergy and environmental issues, as well as all current and prospective users and collaborators, to attend the annual DOE JGI Genomics of Energy & Environment Meeting held March 22-24, 2011 in Walnut Creek, Calif. The emphasis of this meeting was on the genomics of renewable energy strategies, carbon cycling, environmental gene discovery, and engineering of fuel-producing organisms. The meeting features presentations by leading scientists advancing these topics. Ruth Ley of Cornell University gives a presentation on "Relating Host Genetic Variation to the Microbiome" at the 6th annual Genomics of Energy & Environment Meeting on March 23, 2011.

  19. Another short-burst host galaxy with an optically obscured high star formation rate: The case of GRB 071227

    SciTech Connect (OSTI)

    Nicuesa Guelbenzu, A.; Klose, S.; Kann, D. A.; Rossi, A.; Schmidl, S. [Th黵inger Landessternwarte Tautenburg, Sternwarte 5, D-07778 Tautenburg (Germany); Micha?owski, M. J.; McKenzie, M. R. G. [Scottish Universities Physics Alliance, Institute for Astronomy, University of Edinburgh, Royal Observatory, Edinburgh, EH9 3HJ (United Kingdom); Savaglio, S.; Greiner, J. [Max-Planck-Institut f黵 Extraterrestrische Physik, Giessenbachstra遝, D-85748 Garching (Germany); Hunt, L. K. [INAF-Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I-50125 Firenze (Italy); Gorosabel, J. [Instituto de Astrof韘ica de Andaluc韆, Consejo Superior de Investigaciones Cient韋icas (IAA-CSIC), Glorieta de la Astronom韆 s/n, E-18008 Granada (Spain); Palazzi, E. [INAF-IASF Bologna, Via Gobetti 101, I-40129 Bologna (Italy)

    2014-07-01T23:59:59.000Z

    We report on radio continuum observations of the host galaxy of the short gamma-ray burst 071227 (z = 0.381) with the Australia Telescope Compact Array. We detect the galaxy in the 5.5 GHz band with an integrated flux density of F {sub ?} = 43 11 ?Jy, corresponding to an unobscured star-formation rate of about 24 M {sub ?} yr{sup 1}, 40 times higher than what was found from optical emission lines. Among the ?30 well-identified and studied host galaxies of short bursts this is the third case where the host is found to undergo an episode of intense star formation. This suggests that a fraction of all short-burst progenitors hosted in star-forming galaxies could be physically related to recent star formation activity, implying a relatively short merger timescale.

  20. UAS Placement Agreement This is an agreement between the student, the module organizer and the host organization/mentor

    E-Print Network [OSTI]

    Agnor, Craig B.

    and the host organization/mentor teacher. It is a negotiated document that sets out the anticipated tasks-mail ___________________________________________________ Name of Mentor Teacher ___________________________________________________ Address ___________________________________________________ Mentor Teacher ___________________________________________________ Academic Adviser

  1. Phylogenetic relationships, host affinity, and geographic structure of boreal and arctic endophytes from three major plant lineages

    E-Print Network [OSTI]

    Arnold, A. Elizabeth

    Phylogenetic relationships, host affinity, and geographic structure of boreal and arctic endophytes Although associated with all plants, fungal endophytes (microfungi that live within healthy plant tissues, or phylogenetic relationships. We surveyed endophytic Ascomycota from healthy photosyn- thetic tissues of three

  2. Parasitism shaping host life-history evolution: adaptive responses in a marine gastropod to infection by trematodes

    E-Print Network [OSTI]

    Fredensborg, Brian L; Poulin, R

    2006-01-01T23:59:59.000Z

    theory predicts that hosts infected by par- asites that negatively in?uence survival andtheory is that there will be trade-offs between ?tness components such as growth, reproduction and survival (

  3. Detailed search US supports Japanese bid to host ITER as France urges Europe to go it alone

    E-Print Network [OSTI]

    support of his country for the Japanese bid to host the international thermonuclear site (ITER thermonuclear site if the French candidate is not selected for the international project. However

  4. Systems Biology Analysis of Brucella Infected Peyers Patch Reveals Rapid Invasion with Modest Transient Perturbations of the Host Transcriptome

    E-Print Network [OSTI]

    Rossetti, Carlos A.; Drake, Kenneth L.; Siddavatam, Prasad; Lawhon, Sara D.; Nunes, Jairo E.; Gull, Tamara; Khare, Sangeeta; Everts, Robin E.; Lewin, Harris A.; Adams, Leslie Garry

    2013-12-09T23:59:59.000Z

    Brucella melitensis causes the most severe and acute symptoms of all Brucella species in human beings and infects hosts primarily through the oral route. The epithelium covering domed villi of jejunal-ileal Peyer抯 patches ...

  5. Effects of two naphthoquinone compounds on wheat seedlings, germination of urediospores of Puccinia graminis tritici and the host parasite relationship

    E-Print Network [OSTI]

    Rodriguez Campos, Enrique

    1964-01-01T23:59:59.000Z

    EFFECTS OF TWO NAPHTHOQUINONE COMPOUNDS ON WHEAT SEEDLINGS, GERMINATION OF UREDIOSPORES OF PUCCINIA GRAMINIS TRITICI AND THE HOST PARASITE RELATIONSHIP A thesis Enrique Rodrigues Campos Submitted to the Graduate College of Texas Ak... TRITICI AND THE HOST PARASITE RELATIONSHIP A thesis by Enrique Rodriguez Campos Approved. as to style and content by: Ch irman of Committee omm tee Member o ittee ember Committee Member ACKNOWLEDGMENTS The author wishes to acknowledge Dr. Maurice...

  6. Mutual Impacts on a Specialist Herbivore and its Host Plants: Variation in Insect Morphology and Plant Tolerance

    E-Print Network [OSTI]

    Chinchilla-Ramirez, Milena

    2014-12-04T23:59:59.000Z

    MUTUAL IMPACTS IN A SPECIALIST HERBIVORE AND ITS HOST PLANTS: VARIATION IN INSECT MORPHOLOGY AND PLANT TOLERANCE A Thesis by MILENA CHINCHILLA-RAMIREZ Submitted to the Office of Graduate and Professional Studies of Texas A... Subject: Entomology Copyright 2014 Milena Chinchilla-Ramirez ii ABSTRACT In one study, a suite of host plants from the genus Zea L. (Poaceae) and the specialist herbivore Dalbulus maidis (DeLong and Wolcott) (Hemiptera: Cicadellidae) were used...

  7. Dynamic interplay between spin-crossover and host-guest function in a nanoporous metal-organic framework material.

    SciTech Connect (OSTI)

    Southon, P. D.; Liu, L.; Fellows, E. A.; Price, D. J.; Halder, G. J.; Chapman, K. W.; Moubaraki, B.; Murray, K. S.; Letard, J.F.; Kepert, C. J.; Univ. Sydney; Monash Univ.; Universite Bordeaux

    2009-01-01T23:59:59.000Z

    The nanoporous metal-organic framework [Fe(pz)Ni(CN){sub 4}], 1 (where pz is pyrazine), exhibits hysteretic spin-crossover at ambient conditions and is robust to the adsorption and desorption of a wide range of small molecular guests, both gases (N{sub 2}, O{sub 2}, CO{sub 2}) and vapors (methanol, ethanol, acetone, acetonitrile, and toluene). Through the comprehensive analysis of structure, host-guest properties, and spin-crossover behaviors, it is found that this pillared Hofmann system uniquely displays both guest-exchange-induced changes to spin-crossover and spin-crossover-induced changes to host-guest properties, with direct dynamic interplay between these two phenomena. Guest desorption and adsorption cause pronounced changes to the spin-crossover behavior according to a systematic trend in which larger guests stabilize the high-spin state and therefore depress the spin-crossover temperature of the host lattice. When stabilizing the alternate spin state of the host at any given temperature, these processes directly stimulate the spin-crossover process, providing a chemisensing function. Exploitation of the bistability of the host allows the modification of adsorption properties at a fixed temperature through control of the host spin state, with each state shown to display differing chemical affinities to guest sorption. Guest desorption then adsorption, and vice versa, can be used to switch between spin states in the bistable temperature region, adding a guest-dependent memory effect to this system.

  8. The host galaxies of fast-ejecta core-collapse supernovae

    SciTech Connect (OSTI)

    Kelly, Patrick L.; Filippenko, Alexei V. [Department of Astronomy, University of California, Berkeley, CA 94720-3411 (United States); Modjaz, Maryam [CCPP, New York University, 4 Washington Place, New York, NY 10003 (United States); Kocevski, Daniel [NASA Goddard Space Flight Center, Code 662, Greenbelt, MD 20771 (United States)

    2014-07-01T23:59:59.000Z

    Spectra of broad-lined Type Ic supernovae (SNe Ic-BL), the only kind of SN observed at the locations of long-duration gamma-ray bursts (LGRBs), exhibit wide features indicative of high ejecta velocities (?0.1c). We study the host galaxies of a sample of 245 low-redshift (z < 0.2) core-collapse SNe, including 17 SNe Ic-BL, discovered by galaxy-untargeted searches, and 15 optically luminous and dust-obscured z < 1.2 LGRBs. We show that, in comparison with Sloan Digital Sky Survey galaxies having similar stellar masses, the hosts of low-redshift SNe Ic-BL and z < 1.2 LGRBs have high stellar mass and star formation rate densities. Core-collapse SNe having typical ejecta velocities, in contrast, show no preference for such galaxies. Moreover, we find that the hosts of SNe Ic-BL, unlike those of SNe Ib/Ic and SNe II, exhibit high gas velocity dispersions for their stellar masses. The patterns likely reflect variations among star-forming environments and suggest that LGRBs can be used as probes of conditions in high-redshift galaxies. They may be caused by efficient formation of massive binary progenitor systems in densely star-forming regions, or, less probably, a higher fraction of stars created with the initial masses required for an SN Ic-BL or LGRB. Finally, we show that the preference of SNe Ic-BL and LGRBs for galaxies with high stellar mass and star formation rate densities cannot be attributed to a preference for low metal abundances but must reflect the influence of a separate environmental factor.

  9. Confirming Fundamental Parameters of the Exoplanet Host Star epsilon Eridani Using the Navy Optical Interferometer

    E-Print Network [OSTI]

    Baines, Ellyn K

    2011-01-01T23:59:59.000Z

    We measured the angular diameter of the exoplanet host star epsilon Eridani using the Navy Optical Interferometer. We determined its physical radius, effective temperature, and mass by combining our measurement with the star's parallax, photometry from the literature, and the Yonsei-Yale isochrones (Yi et al. 2001), respectively. We used the resulting stellar mass of 0.82 +/- 0.05 M_Sun plus the mass function from Benedict et al. (2006) to calculate the planet's mass, which is 1.53 +/- 0.22 M_Jupiter. Using our new effective temperature, we also estimated the extent of the habitable zone for the system.

  10. CONFIRMING FUNDAMENTAL PROPERTIES OF THE EXOPLANET HOST STAR {epsilon} ERIDANI USING THE NAVY OPTICAL INTERFEROMETER

    SciTech Connect (OSTI)

    Baines, Ellyn K.; Armstrong, J. Thomas, E-mail: ellyn.baines@nrl.navy.mil, E-mail: tarmstr@crater.nrl.navy.mil [Remote Sensing Division, Naval Research Laboratory, 4555 Overlook Avenue SW, Washington, DC 20375 (United States)

    2012-01-10T23:59:59.000Z

    We measured the angular diameter of the exoplanet host star {epsilon} Eridani using the Navy Optical Interferometer. We determined its physical radius, effective temperature, and mass by combining our measurement with the star's parallax, photometry from the literature, and the Yonsei-Yale isochrones, respectively. We used the resulting stellar mass of 0.82 {+-} 0.05 M{sub Sun} plus the mass function from Benedict et al. to calculate the planet's mass, which is 1.53 {+-} 0.22 M{sub Jupiter}. Using our new effective temperature, we also estimated the extent of the habitable zone for the system.

  11. Natural and experimental host range of the Maize Dwarf Mosaic Virus in Texas

    E-Print Network [OSTI]

    Leisy, Ralph Herbert

    1968-01-01T23:59:59.000Z

    in. adjacent to, or in the vicinity of virus infected f'elds were collected for virus assay and for experimental susceptibility studies. Virus assays were (sade by mechanically inoculating suscep- tible host plants with the extracted sap of each... with MDMV, the grasses wh'ch were collected for determination of natural susceptibility and which proved to be free of the virus were grown in isolation and mechanically inocu- lated with the extracted sap of MDfliV (isolate Tx66-BBJg-I) infected AKS 614...

  12. DOE and Northwest Partners Host Three-Day Market Introduction Workshop in Portland

    Broader source: Energy.gov [DOE]

    More than 270 attendees gathered in Portland, OR to participate in the "Voices for SSL Efficiency" Solid-State Lighting Workshop on July 9-11, 2008. The workshop, hosted by DOE, Bonneville Power Administration, Energy Trust of Oregon, Northwest Energy Efficiency Alliance, and Puget Sound Energy, was the third DOE meeting to explore how Federal, State, and private-sector organizations can work together to guide market introduction of high-performance SSL products. The workshop brought together a diverse gathering of participants energy efficiency organizations, utilities, government, and industry to share insights, ideas, and updates on the rapidly evolving SSL market.

  13. News Release: DOE to Host Public Scoping Meetings on Uranium Leasing PEIS |

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels DataDepartment of Energy Your Density Isn'tOrigin of Contamination in Many DevilsForumEngines |NewStateDepartment of Energy to Host

  14. DOE Hosts Record Number of Attendees at Annual Small Business Conference |

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels DataDepartment of Energy Your Density Isn't Your Destiny: Theof"Wave theJulyD&D Project|StatementDOEDepartment of Energy Hosts

  15. DOE to Host a Booth at Offshore WINDPOWER | Department of Energy

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels DataDepartment of Energy Your Density Isn't Your Destiny: Theof"WaveInteractionsMaterials |ProductionDepartment ofDOE to Host a Booth

  16. TOMORROW: Secretary Chu To Host Earth Day Live Chat | Department of Energy

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page onYouTube YouTube Note: Since the.pdfBreakingMayDepartment ofEnergy State7/109T.M. BullFEDERALOFAmerica'sPaulTo Host

  17. DOE to Host a Booth at Offshore WINDPOWER | Department of Energy

    Energy Savers [EERE]

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directed offOCHCO OverviewAttachments4 ChairsEnergyawards contract for sludgeDOE to Host a Booth at

  18. U.S. Department of Energy Hosts Booth at WINDPOWER | Department of Energy

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page onYouTube YouTube Note: Since the.pdfBreakingMayDepartmentTestFeed Families" | Department ofHosts Booth at WINDPOWER

  19. Webinar: How to Host a Youth Climate Summit | Department of Energy

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page onYouTube YouTube Note: SinceDevelopment | Department ofPartnerships ToolkitWaste Heatv3) | Department ofHow to Host a

  20. Selecting a Host DOE Laboratory | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level:Energy: Grid Integration Redefining What'sis Taking Over OurThe Iron4(SC)Principal Investigators'RayScience andSelecting a Host DOE

  1. Selecting a Host DOE Laboratory | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level:Energy: Grid Integration Redefining What'sis Taking Over OurThe Iron4(SC)Principal Investigators'RayScience andSelecting a Host

  2. Selecting a Host DOE Laboratory/Facility | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level:Energy: Grid Integration Redefining What'sis Taking Over OurThe Iron4(SC)Principal Investigators'RayScience andSelecting a HostHow to

  3. NERSC Hosts HS Students on Job Shadow Day- NERSC Center News, Mar 15, 2011

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office of Science (SC)Integrated Codes |IsLove Your1AllocationsNOVA Portal: Submit2014ftpHosts HS Students

  4. Massive relic galaxies challenge the co-evolution of SMBHs and their host galaxies

    E-Print Network [OSTI]

    Ferr-Mateu, Anna; Trujillo, Ignacio; Balcells, Marc; Bosch, Remco C E van den

    2015-01-01T23:59:59.000Z

    We study a sample of eight massive galaxies that are extreme outliers (3-5$\\sigma$) in the M$_{\\bullet}$-M$_\\mathrm{bulge}$ local scaling relation. Two of these galaxies are confirmed to host extremely large super massive black holes (SMBHs), whereas the virial mass estimates for the other six are also consistent with having abnormally large SMBHs. From the analysis of their star formation histories and their structural properties we find that all these extreme outliers can be considered as relic galaxies from the early (z$\\sim$2) Universe: i.e. they are compact (R$_{\\mathrm{e}}$$<$2 kpc) and have purely old stellar populations (t$\\gtrsim$10 Gyr). In order to explain the nature of such deviations from the local relations, we propose a scenario in which the hosts of these \\"uber-massive SMBHs are galaxies that have followed a different evolutionary path than the two-phase growth channel assumed for massive galaxies. Once the SMBH and the core of the galaxy are formed at z$\\sim$2, the galaxy skips the second...

  5. Approaches to LLW disposal site selection and current progress of host states

    SciTech Connect (OSTI)

    Walsh, J.J.; Kerr, T.A.

    1990-11-01T23:59:59.000Z

    In accordance with the Low-Level Radioactive Waste Policy Amendments Act of 1985 and under the guidance of 10 CFR 61, States have begun entering into compacts to establish and operate regional disposal facilities for low-level radioactive waste. The progress a state makes in implementing a process to identify a specific location for a disposal site is one indication of the level of a state's commitment to meeting its responsibilities under Federal law and interstate compact agreements. During the past few years, several States have been engaged in site selection processes. The purpose of this report is to summarize the site selection approaches of some of the Host States (California, Michigan, Nebraska, New York, North Carolina, Texas, and Illinois), and their progress to date. An additional purpose of the report is to discern whether the Host States's site selection processes were heavily influenced by any common factors. One factor each state held in common was that political and public processes exerted a powerful influence on the site selection process at virtually every stage. 1 ref.

  6. Far-infrared observations of an unbiased sample of gamma-ray burst host galaxies

    E-Print Network [OSTI]

    Kohn, Saul A; Bourne, Nathan; Baes, Maarten; Fritz, Jacopo; Cooray, Asantha; De Looze, Ilse; De Zotti, Gianfranco; Dannerbauer, Helmut; Dunne, Loretta; Dye, Simon; Eales, Stephen; Furlanetto, Cristina; Gonzalez-Nuevo, Joaquin; Ibar, Edo; Ivison, Rob J; Maddox, Steve J; Scott, Douglas; Smith, Daniel J B; Smith, Matthew W L; Symeonidis, Myrto; Valiante, Elisabetta

    2015-01-01T23:59:59.000Z

    Gamma-ray bursts (GRBs) are the most energetic phenomena in the Universe; believed to result from the collapse and subsequent explosion of massive stars. Even though it has profound consequences for our understanding of their nature and selection biases, little is known about the dust properties of the galaxies hosting GRBs. We present analysis of the far-infrared properties of an unbiased sample of 21 GRB host galaxies (at an average redshift of $z\\,=\\,3.1$) located in the {\\it Herschel} Astrophysical Terahertz Large Area Survey (H-ATLAS), the {\\it Herschel} Virgo Cluster Survey (HeViCS), the {\\it Herschel} Fornax Cluster Survey (HeFoCS), the {\\it Herschel} Stripe 82 Survey (HerS) and the {\\it Herschel} Multi-tiered Extragalactic Survey (HerMES), totalling $880$ deg$^2$, or $\\sim 3$\\% of the sky in total. Our sample selection is serendipitous, based only on whether the X-ray position of a GRB lies within a large-scale {\\it Herschel} survey -- therefore our sample can be considered completely unbiased. Using ...

  7. Cyber-Physical System Security With Deceptive Virtual Hosts for Industrial Control Networks

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Vollmer, Todd; Manic, Milos

    2014-05-01T23:59:59.000Z

    A challenge facing industrial control network administrators is protecting the typically large number of connected assets for which they are responsible. These cyber devices may be tightly coupled with the physical processes they control and human induced failures risk dire real-world consequences. Dynamic virtual honeypots are effective tools for observing and attracting network intruder activity. This paper presents a design and implementation for self-configuring honeypots that passively examine control system network traffic and actively adapt to the observed environment. In contrast to prior work in the field, six tools were analyzed for suitability of network entity information gathering. Ettercap, anmore牷established network security tool not commonly used in this capacity, outperformed the other tools and was chosen for implementation. Utilizing Ettercap XML output, a novel four-step algorithm was developed for autonomous creation and update of a Honeyd configuration. This algorithm was tested on an existing small campus grid and sensor network by execution of a collaborative usage scenario. Automatically created virtual hosts were deployed in concert with an anomaly behavior (AB) system in an attack scenario. Virtual hosts were automatically configured with unique emulated network stack behaviors for 92% of the targeted devices. The AB system alerted on 100% of the monitored emulated devices.珷less

  8. The APOGEE Spectroscopic Survey of Kepler Planet Hosts: Feasibility, Efficiency, and First Results

    E-Print Network [OSTI]

    Fleming, Scott W; Deshpande, Rohit; Bender, Chad F; Terrien, Ryan C; Marchwinski, Robert C; Wang, Ji; Roy, Arpita; Stassun, Keivan G; Prieto, Carlos Allende; Cunha, Katia; Smith, Verne V; Agol, Eric; Ak, Hasan; Bastien, Fabienne A; Bizyaev, Dmitry; Crepp, Justin R; Ford, Eric B; Frinchaboy, Peter M; Garc韆-Hern醤dez, Domingo An韇al; P閞ez, Ana Elia Garc韆; Gaudi, B Scott; Ge, Jian; Hearty, Fred; Ma, Bo; Majewski, Steve R; M閟z醨os, Szabolcs; Nidever, David L; Pan, Kaike; Pepper, Joshua; Pinsonneault, Marc H; Schiavon, Ricardo P; Schneider, Donald P; Wilson, John C; Zamora, Olga; Zasowski, Gail

    2015-01-01T23:59:59.000Z

    The Kepler mission has yielded a large number of planet candidates from among the Kepler Objects of Interest (KOIs), but spectroscopic follow-up of these relatively faint stars is a serious bottleneck in confirming and characterizing these systems. We present motivation and survey design for an ongoing project with the SDSS-III multiplexed APOGEE near-infrared spectrograph to monitor hundreds of KOI host stars. We report some of our first results using representative targets from our sample, which include current planet candidates that we find to be false positives, as well as candidates listed as false positives that we do not find to be spectroscopic binaries. With this survey, KOI hosts are observed over ~20 epochs at a radial velocity precision of 100-200 m/s. These observations can easily identify a majority of false positives caused by physically-associated stellar or substellar binaries, and in many cases, fully characterize their orbits. We demonstrate that APOGEE is capable of achieving RV precision ...

  9. Precision Measurement of the Decay Rate of 7Be in Host Materials

    E-Print Network [OSTI]

    Y. Nir-El; G. Haquin; Z. Yungreiss; M. Hass; G. Goldring; S. K. Chamoli; B. S. Nara Singh; S. Lakshmi; U. Koester; N. Champault; A. Dorsival; G. Georgiev; V. N. Fedoseyev; B. A. Marsh; D. Schumann; G. Heidenreich; S. Teichmann

    2006-12-03T23:59:59.000Z

    A controlled and precise determination of the cross-sections of the fusion reactions 7Be(p,gamma)8B and 3He(4He,gamma)7Be, which play an important role in determining the solar neutrino flux, necessitates the knowledge of a precise value of the electron-capture half-life of 7Be. This half-life may depend on the material hosting the 7Be atoms via small modifications of the electron density around the 7Be nucleus. In this brief communication we report on the measurement of 7Be implanted in four materials: copper, aluminum, sapphire and PVC. The four results are consistent with a null host dependence within two standard deviations and their weighted average of 53.236(39)d agrees very well with the adopted value in the literature, 53.22(6)d. The present results may exhibit a slight (0.22%) increase of the half-life at room temperature for metals compared to insulators that requires further studies.

  10. Sub-millimeter emission from type Ia supernova host galaxies at z=0.5

    E-Print Network [OSTI]

    D. Farrah; M. Fox; M. Rowan-Robinson; D. Clements; J. Afonso

    2003-12-03T23:59:59.000Z

    We present deep sub-millimetre observations of seventeen galaxies at z=0.5, selected through being hosts of a type 1a supernova. Two galaxies are detected directly, and the sample is detected statistically with a mean 850 micron flux of 1.01mJy +/- 0.33mJy, which is 25% - 135% higher than locally. We infer that the mean value of A_v in normal galaxies at z=0.5 is comparable to or greater than the mean A_v in local normal galaxies, in agreement with galaxy chemical evolution models and indirect observational evidence. Scaling from the local value given by Rowan-Robinson (2003) gives a mean extinction at z=0.5 of A_v = 0.56 +/- 0.17. The dust in the brightest sub-mm object in our sample is best interpreted as normal `cirrus' dust similar to that seen locally. The detection rate of our sample suggests that some sources found in blank-field sub-mm surveys may not be high redshift starbursts, but rather cirrus galaxies at moderate redshifts and with lower star formation rates. Finally, an increase in host dust extinction with redshift may impact the cosmological results from distant supernova searches. This emphasizes the need to carefully monitor dust extinction when using type Ia supernovae to measure the cosmological parameters.

  11. The Application Hosting Environment: Lightweight Middleware for Grid-Based Computational Science

    E-Print Network [OSTI]

    P. V. Coveney; R. S. Saksena; S. J. Zasada; M. McKeown; S. Pickles

    2006-11-27T23:59:59.000Z

    Grid computing is distributed computing performed transparently across multiple administrative domains. Grid middleware, which is meant to enable access to grid resources, is currently widely seen as being too heavyweight and, in consequence, unwieldy for general scientific use. Its heavyweight nature, especially on the client-side, has severely restricted the uptake of grid technology by computational scientists. In this paper, we describe the Application Hosting Environment (AHE) which we have developed to address some of these problems. The AHE is a lightweight, easily deployable environment designed to allow the scientist to quickly and easily run legacy applications on distributed grid resources. It provides a higher level abstraction of a grid than is offered by existing grid middleware schemes such as the Globus Toolkit. As a result the computational scientist does not need to know the details of any particular underlying grid middleware and is isolated from any changes to it on the distributed resources. The functionality provided by the AHE is `application-centric': applications are exposed as web services with a well-defined standards-compliant interface. This allows the computational scientist to start and manage application instances on a grid in a transparent manner, thus greatly simplifying the user experience. We describe how a range of computational science codes have been hosted within the AHE and how the design of the AHE allows us to implement complex workflows for deployment on grid infrastructure.

  12. Hubble space telescope high-resolution imaging of Kepler small and cool exoplanet host stars

    SciTech Connect (OSTI)

    Gilliland, Ronald L.; Cartier, Kimberly M. S.; Wright, Jason T. [Department of Astronomy and Astrophysics, and Center for Exoplanets and Habitable Worlds, The Pennsylvania State University, 525 Davey Lab, University Park, PA 16802 (United States); Adams, Elisabeth R. [Planetary Science Institute, 1700 East Fort Lowell, Suite 106, Tucson, AZ 85719 (United States); Ciardi, David R. [NASA Exoplanet Science Institute/Caltech, Pasadena, CA 91125 (United States); Kalas, Paul, E-mail: gillil@stsci.edu [Astronomy Department, University of California, Berkeley, CA 94720 (United States)

    2015-01-01T23:59:59.000Z

    High-resolution imaging is an important tool for follow-up study of exoplanet candidates found via transit detection with the Kepler mission. We discuss here Hubble Space Telescope imaging with the WFC3 of 23 stars that host particularly interesting Kepler planet candidates based on their small size and cool equilibrium temperature estimates. Results include detections, exclusion of background stars that could be a source of false positives for the transits, and detection of physically associated companions in a number of cases providing dilution measures necessary for planet parameter refinement. For six Kepler objects of interest, we find that there is ambiguity regarding which star hosts the transiting planet(s), with potentially strong implications for planetary characteristics. Our sample is evenly distributed in G, K, and M spectral types. Albeit with a small sample size, we find that physically associated binaries are more common than expected at each spectral type, reaching a factor of 10 frequency excess in M. We document the program detection sensitivities, detections, and deliverables to the Kepler follow-up program archive.

  13. Energy input from quasars regulates the growth and activity of black holes and their host galaxies

    E-Print Network [OSTI]

    Tiziana Di Matteo; Volker Springel; Lars Hernquist

    2005-02-09T23:59:59.000Z

    In the early Universe, while galaxies were still forming, black holes as massive as a billion solar masses powered quasars. Supermassive black holes are found at the centers of most galaxies today, where their masses are related to the velocity dispersions of stars in their host galaxies and hence to the mass of the central bulge of the galaxy. This suggests a link between the growth of the black holes and the host galaxies, which has indeed been assumed for a number of years. But the origin of the observed relation between black hole mass and stellar velocity dispersion, and its connection with the evolution of galaxies have remained unclear. Here we report simulations that simultaneously follow star formation and the growth of black holes during galaxy-galaxy collisions. We find that in addition to generating a burst of star formation, a merger leads to strong inflows that feed gas to the supermassive black hole and thereby power the quasar. The energy released by the quasar expels enough gas to quench both star formation and further black hole growth. This determines the lifetime of the quasar phase (approaching 100 million years) and explains the relationship between the black hole mass and the stellar velocity dispersion.

  14. The Host Galaxies of Narrow-Line Seyfert 1s: Nuclear Dust Morphology and Starburst Rings

    E-Print Network [OSTI]

    R. P. Deo; D. M. Crenshaw; S. B. Kraemer

    2006-03-29T23:59:59.000Z

    We present a study of the nuclear morphology of a sample of narrow- and broad-line Seyfert 1 galaxies (NLS1's and BLS1's) based on broad-band images in the Hubble Space Telescope archives. In our previous study, we found that large-scale stellar bars at > 1 kpc from the nucleus are more common in NLS1's than BLS1's. In this paper we find that NLS1's preferentially have grand-design dust spirals within approx. 1 kpc of their centers. We also find that NLS1's have a higher fraction of nuclear star-forming rings than BLS1's. We find that many of the morphological differences are due to the presence or absence of a large-scale stellar bar within the spiral host galaxy. In general, barred Seyfert 1s tend to have grand-design dust spirals at their centers, confirming the results of other researchers. The high fraction of grand-design nuclear dust spirals and stellar nuclear rings observed in NLS1's host galaxies suggests a means for efficient fueling of their nuclei to support their high Eddington ratios.

  15. Co-evolution of nuclear star clusters, massive black holes and their host galaxies

    E-Print Network [OSTI]

    Antonini, Fabio; Silk, Joseph

    2015-01-01T23:59:59.000Z

    Studying how nuclear star clusters (NSCs) form and how they are related to the growth of the central massive black holes (MBHs) and their host galaxies is fundamental for our understanding of the evolution of galaxies and the processes that have shaped their central structures. We present the results of a semi-analytical galaxy formation model that follows the evolution of dark matter halos along merger trees, as well as that of the baryonic components. This model allows us to study the evolution of NSCs in a cosmological context, by taking into account the growth of NSCs due to both dynamical friction-driven migration of stellar clusters and star formation triggered by infalling gas, while also accounting for dynamical heating from (binary) MBHs. We find that in-situ star formation contributes a significant fraction (up to ~40%) of the total mass of NSCs in our model. Both NSC growth through in-situ star formation and through star cluster migration are found to generate NSC -- host galaxy scaling correlation...

  16. REVISITING THE FIRST GALAXIES: THE EFFECTS OF POPULATION III STARS ON THEIR HOST GALAXIES

    SciTech Connect (OSTI)

    Muratov, Alexander L.; Gnedin, Oleg Y.; Zemp, Marcel [Department of Astronomy, University of Michigan, Ann Arbor, MI 48109 (United States); Gnedin, Nickolay Y., E-mail: muratov@umich.edu [Particle Astrophysics Center, Fermi National Accelerator Laboratory, Batavia, IL 60510 (United States)

    2013-08-01T23:59:59.000Z

    We revisit the formation and evolution of the first galaxies using new hydrodynamic cosmological simulations with the adaptive refinement tree code. Our simulations feature a recently developed model for H{sub 2} formation and dissociation, and a star formation recipe that is based on molecular rather than atomic gas. Here, we develop and implement a recipe for the formation of metal-free Population III (Pop III) stars in galaxy-scale simulations that resolve primordial clouds with sufficiently high density. We base our recipe on the results of prior zoom-in simulations that resolved the protostellar collapse in pre-galactic objects. We find the epoch during which Pop III stars dominated the energy and metal budget of the first galaxies to be short-lived. Galaxies that host Pop III stars do not retain dynamical signatures of their thermal and radiative feedback for more than 10{sup 8} years after the lives of the stars end in pair-instability supernovae, even when we consider the maximum reasonable efficiency of the feedback. Though metals ejected by the supernovae can travel well beyond the virial radius of the host galaxy, they typically begin to fall back quickly, and do not enrich a large fraction of the intergalactic medium. Galaxies with a total mass in excess of 3 Multiplication-Sign 10{sup 6} M{sub Sun} re-accrete most of their baryons and transition to metal-enriched Pop II star formation.

  17. Cyber-Physical System Security With Deceptive Virtual Hosts for Industrial Control Networks

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Vollmer, Todd; Manic, Milos

    2014-05-01T23:59:59.000Z

    A challenge facing industrial control network administrators is protecting the typically large number of connected assets for which they are responsible. These cyber devices may be tightly coupled with the physical processes they control and human induced failures risk dire real-world consequences. Dynamic virtual honeypots are effective tools for observing and attracting network intruder activity. This paper presents a design and implementation for self-configuring honeypots that passively examine control system network traffic and actively adapt to the observed environment. In contrast to prior work in the field, six tools were analyzed for suitability of network entity information gathering. Ettercap, an established network security tool not commonly used in this capacity, outperformed the other tools and was chosen for implementation. Utilizing Ettercap XML output, a novel four-step algorithm was developed for autonomous creation and update of a Honeyd configuration. This algorithm was tested on an existing small campus grid and sensor network by execution of a collaborative usage scenario. Automatically created virtual hosts were deployed in concert with an anomaly behavior (AB) system in an attack scenario. Virtual hosts were automatically configured with unique emulated network stack behaviors for 92% of the targeted devices. The AB system alerted on 100% of the monitored emulated devices.

  18. Hydrogen-poor superluminous supernovae and long-duration gamma-ray bursts have similar host galaxies

    SciTech Connect (OSTI)

    Lunnan, R.; Chornock, R.; Berger, E.; Laskar, T.; Fong, W.; Sanders, N. E.; Challis, P. M.; Drout, M. R.; Foley, R. J.; Kirshner, R. P.; Leibler, C.; Marion, G. H.; Milisavljevic, D.; Narayan, G. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Rest, A. [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States); Huber, M. E. [Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822 (United States); McCrum, M.; Smartt, S. J.; Smith, K. W. [Astrophysics Research Centre, School of Mathematics and Physics, Queen's University Belfast, Belfast BT7 1NN (United Kingdom); Scolnic, D., E-mail: rlunnan@cfa.harvard.edu [Department of Physics and Astronomy, Johns Hopkins University, 3400 North Charles Street, Baltimore, MD 21218 (United States); and others

    2014-06-01T23:59:59.000Z

    We present optical spectroscopy and optical/near-IR photometry of 31 host galaxies of hydrogen-poor superluminous supernovae (SLSNe), including 15 events from the Pan-STARRS1 Medium Deep Survey. Our sample spans the redshift range 0.1 ? z ? 1.6, and is the first comprehensive host galaxy study of this specific subclass of cosmic explosions. Combining the multi-band photometry and emission-line measurements, we determine the luminosities, stellar masses, star formation rates, and metallicities. We find that, as a whole, the hosts of SLSNe are a low-luminosity ((M{sub B} ) ? 17.3 mag), low stellar mass ((M {sub *}) ? 2 10{sup 8} M {sub ?}) population, with a high median specific star formation rate ((sSFR) ? 2 Gyr{sup 1}). The median metallicity of our spectroscopic sample is low, 12 + log (O/H) ? 8.35 ? 0.45 Z {sub ?}, although at least one host galaxy has solar metallicity. The host galaxies of H-poor SLSNe are statistically distinct from the hosts of GOODS core-collapse SNe (which cover a similar redshift range), but resemble the host galaxies of long-duration gamma-ray bursts (LGRBs) in terms of stellar mass, SFR, sSFR, and metallicity. This result indicates that the environmental causes leading to massive stars forming either SLSNe or LGRBs are similar, and in particular that SLSNe are more effectively formed in low metallicity environments. We speculate that the key ingredient is large core angular momentum, leading to a rapidly spinning magnetar in SLSNe and an accreting black hole in LGRBs.

  19. Proton Mediated Chemistry and Catalysis in a Self-Assembled Supramolecular Host

    SciTech Connect (OSTI)

    Pluth, Michael; Bergman, Robert; Raymond, Kenneth

    2009-04-10T23:59:59.000Z

    Synthetic supramolecular host assemblies can impart unique reactivity to encapsulated guest molecules. Synthetic host molecules have been developed to carry out complex reactions within their cavities, despite the fact that they lack the type of specifically tailored functional groups normally located in the analogous active sites of enzymes. Over the past decade, the Raymond group has developed a series of self-assembled supramolecules and the Bergman group has developed and studied a number of catalytic transformations. In this Account, we detail recent collaborative work between these two groups, focusing on chemical catalysis stemming from the encapsulation of protonated guests and expanding to acid catalysis in basic solution. We initially investigated the ability of a water-soluble, self-assembled supramolecular host molecule to encapsulate protonated guests in its hydrophobic core. Our study of encapsulated protonated amines revealed rich host-guest chemistry. We established that self-exchange (that is, in-out guest movement) rates of protonated amines were dependent on the steric bulk of the amine rather than its basicity. The host molecule has purely rotational tetrahedral (T) symmetry, so guests with geminal N-methyl groups (and their attendant mirror plane) were effectively desymmetrized; this allowed for the observation and quantification of the barriers for nitrogen inversion followed by bond rotation. Furthermore, small nitrogen heterocycles, such as N-alkylaziridines, N-alkylazetidines, and N-alkylpyrrolidines, were found to be encapsulated as proton-bound homodimers or homotrimers. We further investigated the thermodynamic stabilization of protonated amines, showing that encapsulation makes the amines more basic in the cavity. Encapsulation raises the effective basicity of protonated amines by up to 4.5 pK{sub a} units, a difference almost as large as that between the moderate and strong bases carbonate and hydroxide. The thermodynamic stabilization of protonated guests was translated into chemical catalysis by taking advantage of the potential for accelerating reactions that take place via positively charged transition states, which could be potentially stabilized by encapsulation. Orthoformates, generally stable in neutral or basic solution, were found to be suitable substrates for catalytic hydrolysis by the assembly. Orthoformates small enough to undergo encapsulation were readily hydrolyzed by the assembly in basic solution, with rate acceleration factors up to 3900 compared with those of the corresponding uncatalyzed reactions. Furthering the analogy to enzymes that obey Michaelis-Menten kinetics, we observed competitive inhibition with the inhibitor NPr{sub 4}{sup +}, thereby confirming that the interior cavity of the assembly was the active site for catalysis. Mechanistic studies revealed that the assembly is required for catalysis and that the rate-limiting step of the reaction involves proton transfer from hydronium to the encapsulated substrate. Encapsulation in the assembly changes the orthoformate hydrolysis from an A-1 mechanism (in which decomposition of the protonated substrate is the rate-limiting step) to an A-S{sub E}2 mechanism (in which proton transfer is the rate-limiting step). The study of hydrolysis in the assembly was next extended to acetals, which were also catalytically hydrolyzed by the assembly in basic solution. Acetal hydrolysis changed from the A-1 mechanism in solution to an A-2 mechanism inside the assembly, where attack of water on the protonated substrate is rate limiting. This work provides rare examples of assembly-catalyzed reactions that proceed with substantial rate accelerations despite the absence of functional groups in the cavity and with mechanisms fully elucidated by quantitative kinetic studies.

  20. LONG GRBs ARE METALLICITY-BIASED TRACERS OF STAR FORMATION: EVIDENCE FROM HOST GALAXIES AND REDSHIFT DISTRIBUTION

    SciTech Connect (OSTI)

    Wang, F. Y.; Dai, Z. G., E-mail: fayinwang@nju.edu.cn, E-mail: dzg@nju.edu.cn [School of Astronomy and Space Science, Nanjing University, Nanjing 210093 (China)

    2014-07-01T23:59:59.000Z

    We investigate the mass distribution of long gamma-ray burst (GRB) host galaxies and the redshift distribution of long GRBs by considering that long GRBs occur in low-metallicity environments. We calculate the upper limit on the stellar mass of a galaxy which can produce long GRBs by utilizing the mass-metallicity (M-Z) relation of galaxies. After comparing with the observed GRB host galaxies masses, we find that the observed GRB host galaxy masses can fit the predicted masses well if GRBs occur in low-metallicity 12 + log (O/H){sub KK04} < 8.7. GRB host galaxies have low metallicity, low mass, and high star formation rate compared with galaxies of seventh data release of the Sloan Digital Sky Survey. We also study the cumulative redshift distribution of the latest Swift long GRBs by adding dark GRBs and 10 new GRBs redshifts from the TOUGH survey. The observed discrepancy between the GRB rate and the star formation history can be reconciled by considering that GRBs tend to occur in low-metallicity galaxies with 12 + log (O/H){sub KK04} < 8.7. We conclude that the metallicity cutoff that can produce long GRBs is about 12 + log (O/H){sub KK04} < 8.7 from the host mass distribution and redshift distribution.

  1. The Dependence of the $A_V$ Prior for SN\\,Ia on Host Mass and Disk Inclination

    E-Print Network [OSTI]

    Holwerda, B W; Kenworthy, M A; Mack, K J

    2015-01-01T23:59:59.000Z

    Supernovae type Ia (SNIa) are used as "standard candles" for cosmological distance scales. To fit their light curve shape -- absolute luminosity relation, one needs to assume an intrinsic color and a likelihood of host galaxy extinction or a convolution of these, a color distribution prior. The host galaxy extinction prior is typically assumed to be an exponential drop-off for the current supernova programs ($P(A_V) \\propto e^{-A_V/\\tau_0}$). We explore the validity of this prior using the distribution of extinction values inferred when two galaxies accidentally overlap (an occulting galaxy pair). We correct the supernova luminosity distances from the SDSS-III Supernova projects (SDSS-SN) by matching the host galaxies to one of three templates from occulting galaxy pairs based on the host galaxy mass and the $A_V$-bias - prior-scale ($\\tau_0$) relation from Jha et al. (2007). We find that introducing an $A_V$ prior that depends on host mass results in lowered luminosity distances for the SDSS-SN on average bu...

  2. A Multi-Omic View of Host-Pathogen-Commensal Interplay in Salmonella-Mediated Intestinal Infection

    SciTech Connect (OSTI)

    Kaiser, Brooke LD; Li, Jie; Sanford, James A.; Kim, Young-Mo; Kronewitter, Scott R.; Jones, Marcus B.; Peterson, Christine; Peterson, Scott N.; Frank, Bryan C.; Purvine, Samuel O.; Brown, Joseph N.; Metz, Thomas O.; Smith, Richard D.; Heffron, Fred; Adkins, Joshua N.

    2013-06-26T23:59:59.000Z

    The potential for commensal microorganisms indigenous to a host (the 憁icrobiome or 憁icrobiota) to alter infection outcome by influencing host-pathogen interplay is largely unknown. We used a multi-omics 搒ystems approach, incorporating proteomics, metabolomics, glycomics, and metagenomics, to explore the molecular interplay between the murine host, the pathogen Salmonella enterica serovar Typhimurium (S. Typhimurium), and commensal gut microorganisms during intestinal infection with S. Typhimurium. We find proteomic evidence that S. Typhimurium thrives within the infected 129/SvJ mouse gut without antibiotic pre-treatment, inducing inflammation and disrupting the intestinal microbiome (e.g., suppressing Bacteroidetes and Firmicutes while promoting growth of Salmonella and Enterococcus). Alteration of the host microbiome population structure was highly correlated with gut environmental changes, including the accumulation of metabolites normally consumed by commensal microbiota. Finally, the less characterized phase of S. Typhimurium抯 lifecycle was investigated, and both proteomic and glycomic evidence suggests S. Typhimurium may take advantage of increased fucose moieties to metabolize fucose while growing in the gut. The application of multiple omics measurements to Salmonella-induced intestinal inflammation provides insights into complex molecular strategies employed during pathogenesis between host, pathogen, and the microbiome.

  3. NO CORRELATION BETWEEN HOST GALAXY METALLICITY AND GAMMA-RAY ENERGY RELEASE FOR LONG-DURATION GAMMA-RAY BURSTS

    SciTech Connect (OSTI)

    Levesque, Emily M.; Kewley, Lisa J. [Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822 (United States); Soderberg, Alicia M.; Berger, Edo, E-mail: emsque@ifa.hawaii.ed, E-mail: kewley@ifa.hawaii.ed, E-mail: asoderbe@cfa.harvard.ed, E-mail: eberger@cfa.harvard.ed [Smithsonian Astrophysical Observatory, 60 Garden St., MS-20, Cambridge, MA 02138 (United States)

    2010-12-10T23:59:59.000Z

    We compare the redshifts, host galaxy metallicities, and isotropic (E{sub {gamma}},iso) and beaming-corrected (E{sub {gamma}}) gamma-ray energy release of 16 long-duration gamma-ray bursts (LGRBs) at z < 1. From this comparison, we find no statistically significant correlation between host metallicity and redshift, E{sub {gamma}},iso, or E{sub {gamma}}. These results are at odds with previous theoretical and observational predictions of an inverse correlation between gamma-ray energy release and host metallicity, as well as the standard predictions of metallicity-driven wind effects in stellar evolutionary models. We consider the implications that these results have for LGRB progenitor scenarios, and discuss our current understanding of the role that metallicity plays in the production of LGRBs.

  4. External and Internal Guest Binding of a Highly Charged Supramolecular Host in Water: Deconvoluting the Very Different Thermodynamics

    SciTech Connect (OSTI)

    Sgarlata, Carmelo; Mugridge, Jeffrey; Pluth, Michael; Tiedemann,, Bryan; Zito, Valeria; Arena, Giuseppe; Raymond, Kenneth N.

    2009-07-22T23:59:59.000Z

    NMR, UV-vis and isothermal titration calorimetry (ITC) measurements probe different aspects of competing host-guest equilibria as simple alkylammonium guest molecules interact with both the exterior (ion-association) and interior (encapsulation) of the [Ga{sub 4}L{sub 6}]{sup 12-} supramolecular assembly in water. Data obtained by each independent technique measure different components of the host-guest equilibria and only when analyzed together does a complete picture of the solution thermodynamics emerge. Striking differences between the internal and external guest binding are found. External binding is enthalpy driven and mainly due to attractive interactions between the guests and the exterior surface of the assembly while encapsulation is entropy driven as a result of desolvation and release of solvent molecules from the host cavity.

  5. Homogeneous spectroscopic parameters for bright planet host stars from the northern hemisphere

    E-Print Network [OSTI]

    Sousa, S G; Mortier, A; Tsantaki, M; Adibekyan, V; Mena, E Delgado; Israelian, G; Rojas-Ayala, B; Neves, V

    2015-01-01T23:59:59.000Z

    Aims. In this work we derive new precise and homogeneous parameters for 37 stars with planets. For this purpose, we analyze high resolution spectra obtained by the NARVAL spectrograph for a sample composed of bright planet host stars in the northern hemisphere. The new parameters are included in the SWEET-Cat online catalogue. Methods. To ensure that the catalogue is homogeneous, we use our standard spectroscopic analysis procedure, ARES+MOOG, to derive effective temperatures, surface gravities, and metallicities. These spectroscopic stellar parameters are then used as input to compute the stellar mass and radius, which are fundamental for the derivation of the planetary mass and radius. Results. We show that the spectroscopic parameters, masses, and radii are generally in good agreement with the values available in online databases of exoplanets. There are some exceptions, especially for the evolved stars. These are analyzed in detail focusing on the effect of the stellar mass on the derived planetary mass. ...

  6. Low-phonon-frequency chalcogenide crystalline hosts for rare earth lasers operating beyond three microns

    DOE Patents [OSTI]

    Payne, Stephen A. (Castro Valley, CA); Page, Ralph H. (San Ramon, CA); Schaffers, Kathleen I. (Pleasanton, CA); Nostrand, Michael C. (Livermore, CA); Krupke, William F. (Pleasanton, CA); Schunemann, Peter G. (Malden, MA)

    2000-01-01T23:59:59.000Z

    The invention comprises a RE-doped MA.sub.2 X.sub.4 crystalline gain medium, where M includes a divalent ion such as Mg, Ca, Sr, Ba, Pb, Eu, or Yb; A is selected from trivalent ions including Al, Ga, and In; X is one of the chalcogenide ions S, Se, and Te; and RE represents the trivalent rare earth ions. The MA.sub.2 X.sub.4 gain medium can be employed in a laser oscillator or a laser amplifier. Possible pump sources include diode lasers, as well as other laser pump sources. The laser wavelengths generated are greater than 3 microns, as becomes possible because of the low phonon frequency of this host medium. The invention may be used to seed optical devices such as optical parametric oscillators and other lasers.

  7. Parent Stars of Extrasolar Planets. XV. Host Star Rotation Revisited with {\\it Kepler} Data

    E-Print Network [OSTI]

    Gonzalez, Guillermo

    2015-01-01T23:59:59.000Z

    We employed published rotation periods of {\\it Kepler} field stars to test whether stars hosting planets tend to rotate more slowly than stars without known planets. Spectroscopic vsini observations of nearby stars with planets have indicated that they tend to have smaller visni values. We employ data for {\\it Kepler} Objects of Interest (KOIs) from the first 16 quarters of its original mission; stellar parameters are based on the analysis of the first 17 quarters. We confirm that KOI stars rotate more slowly with much greater confidence than we had previously found for nearby stars with planets. Furthermore, we find that stars with planets of all types rotate more slowly, not just stars with giant planets.

  8. The integration of multiple OS-9 stations with a VAX/VMS host via Ethernet

    SciTech Connect (OSTI)

    Charity, T. (CERN/EF, Geneva (CH))

    1989-10-01T23:59:59.000Z

    In this paper a method for providing embedded microprocessors with virtual disk storage capacity and remote terminal access from a VAX/VMS host via Ethernet is described. The underlying Ethernet driver permits different network protocols to be co-resident in the microprocessors. The system described is in use in many experiments at CERN and elsewhere, and provides a cheap and effective method for sharing data and programs between microprocessors and VAX/VMS systems. Existing approaches to these problems required sole use of a dedicated intelligent network interface, and were biased towards VMEbus systems. One of the goals of the design was to provide a highly transparent and easy-to-use development environment such that users would appear to be working on dedicated microprocessor workstations, unaware of the underlying network connections.

  9. Subcellular proteomic analysis of host-pathogen interactions using human monocytes exposed to Yersinia pestis and Yersinia pseudotuberculosis

    SciTech Connect (OSTI)

    Zhang, C G; Gonzales, A D; Choi, M W; Chromy, B A; Fitch, J P; McCutchen-Maloney, S L

    2004-05-20T23:59:59.000Z

    Yersinia pestis, the etiological agent of plague, is of concern to human health both from an infectious disease and a civilian biodefense perspective. While Y. pestis and Y. pseudotuberculosis share more than 90% DNA homology, they have significantly different clinical manifestations. Plague is often fatal if untreated, yet Y. pseudotuberculosis causes severe intestinal distress and is rarely fatal. A better understanding of host response to these closely related pathogens may help explain the different mechanisms of virulence and pathogenesis that result in such different clinical outcomes. The aim of this study was to characterize host protein expression changes in human monocyte-like U937 cells after exposure to Y. pestis and Y. pseudotuberculosis. In order to gain global proteomic coverage of host response, proteins from cytoplasmic, nuclear and membrane fractions of host cells were studied by 2-dimensional differential gel electrophoresis (2-D DIGE) and relative protein expression differences were quantitated. Differentially expressed proteins, with at least 1.5 fold expression changes and p values of 0.01 or less, were identified by MALDI-MS or LC/MS/MS. With these criteria, differential expression was detected in 16 human proteins after Y. pestis exposure and 13 human proteins after Y. pseudotuberculosis exposure, of which only two of the differentially expressed proteins identified were shared between the two exposures. Proteins identified in this study are reported to be involved in a wide spectrum of cellular functions and host defense mechanisms including apoptosis, cytoskeletal rearrangement, protein synthesis and degradation, DNA replication and transcription, metabolism, protein folding, and cell signaling. Notably, the differential expression patterns observed can distinguish the two pathogen exposures from each other and from unexposed host cells. The functions of the differentially expressed proteins identified provide insight on the different virulence and pathogenic mechanisms of Y. pestis and Y. pseudotuberculosis.

  10. Uranium and its relationship to host rock mineralogy in an unoxidized roll front in the Jackson group, South Texas

    E-Print Network [OSTI]

    Prasse, Eric Martin

    1978-01-01T23:59:59.000Z

    of the requirement for the degree of MASTER OF SCIENCE December 1978 Major Subject: Geology URANIUM AND ITS RELATIONSHIP TO HOST ROCK MINERALOGY IN AN UNOXIDIZED ROLL FRONT IN THE JACKSON GROUP, SOUTH TEXAS A Thesis by ERIC MARTIN PRASSE Approved as to style... and content by: Chairman of Committee r Head of Department Member Member December 1978 :& ~'8% 055 ABSTRACT Uranium and its Relat1onship to Host Rock Mineralogy in an Unox1dized Roll Front in the Jackson Group, South Texas (December, 1978) Eric...

  11. Systems Biology Analysis of Brucella Infected Peyers Patch Reveals Rapid Invasion with Modest Transient Perturbations of the Host Transcriptome

    E-Print Network [OSTI]

    Rossetti, Carlos A.; Drake, Kenneth L.; Siddavatam, Prasad; Lawhon, Sara D.; Nunes, Jairo E.; Gull, Tamara; Khare, Sangeeta; Everts, Robin E.; Lewin, Harris A.; Adams, Leslie Garry

    2013-12-09T23:59:59.000Z

    Systems Biology Analysis of Brucella Infected Peyer抯 Patch Reveals Rapid Invasion with Modest Transient Perturbations of the Host Transcriptome Carlos A. Rossetti1, Kenneth L. Drake2, Prasad Siddavatam2, Sara D. Lawhon1, Jairo E. S. Nunes1... mechanisms. Citation: Rossetti CA, Drake KL, Siddavatam P, Lawhon SD, Nunes JES, et al. (2013) Systems Biology Analysis of Brucella Infected Peyer抯 Patch Reveals Rapid Invasion with Modest Transient Perturbations of the Host Transcriptome. PLoS ONE 8(12): e...

  12. Hypothetical Distance Learning Program Costs Model A framework for thinking about the comprehensive costs of hosting a DL program

    E-Print Network [OSTI]

    Snider, Barry B.

    Hypothetical Distance Learning Program Costs Model A framework for thinking about the comprehensive costs of hosting a DL program Start-Up Ongoing Explanation 100,000$ 100,000$ FTE needed to develop any or repurpose old courses for the online context. Infrastructure Costs tbd tbd Cost of adding or improving

  13. Host-defense peptides isolated from the skin secretions of the Northern red-legged frog Rana aurora aurora

    E-Print Network [OSTI]

    Davidson, Carlos

    Host-defense peptides isolated from the skin secretions of the Northern red-legged frog Rana aurora aurora J. Michael Conlona,*, Agnes Sonnevendb , Carlos Davidsonc , Anni Demandtd , Thierry Jouennee-stimulated skin secretions of the Northern red-legged frog Rana aurora aurora and their primary structures

  14. Know the Star, Know the Planet. III. Discovery of Late-Type Companions to Two Exoplanet Host Stars

    E-Print Network [OSTI]

    Roberts,, Lewis C; Mason, Brian D; Riddle, Reed L; Hartkopf, William I; Law, Nicholas M; Baranec, Christoph

    2015-01-01T23:59:59.000Z

    We discuss two multiple star systems that host known exoplanets: HD 2638 and 30 Ari B. Adaptive optics imagery revealed an additional stellar companion to both stars. We collected multi-epoch images of the systems with Robo-AO and the PALM-3000 adaptive optics systems at Palomar Observatory and provide relative photometry and astrometry. The astrometry indicates that the companions share common proper motion with their respective primaries. Both of the new companions have projected separations less than 30 AU from the exoplanet host star. Using the projected separations to compute orbital periods of the new stellar companions, HD 2638 has a period of 130 yrs and 30 Ari B has a period of 80 years. Previous studies have shown that the true period is most likely within a factor of three of these estimated values. The additional component to the 30 Ari makes it the second confirmed quadruple system known to host an exoplanet. HD 2638 hosts a hot Jupiter and the discovery of a new companion strengthens the connect...

  15. During the month of November, the Department hosted an unusual guest from Kazakhstan, Zhanna Yessengaliyeva. Kazakhstan is a country

    E-Print Network [OSTI]

    Pringle, James "Jamie"

    During the month of November, the Department hosted an unusual guest from Kazakhstan, Zhanna Yessengaliyeva. Kazakhstan is a country in Central Asia and Eastern Europe. Kazakhstan is the ninth largest) is larger than Western Europe. 16.6 million people live in Kazakhstan, its population density is less than 6

  16. Japan, EU adamant about their proposals to host ITER, put off negotiations to next year; Joint construction plan involving Japan,

    E-Print Network [OSTI]

    Japan, EU adamant about their proposals to host ITER, put off negotiations to next year; Joint construction plan involving Japan, U.S. South Korea also emerging NIHON KEIZAI, December 20, 2004 Japan are likely to enter a crucial stage early in the next year. In addition to Japan and the EU, the United

  17. Major Mergers Host the Most Luminous Red Quasars at z ~ 2: A Hubble Space Telescope WFC3/IR Study

    E-Print Network [OSTI]

    Glikman, Eilat; Mailly, Madeline; Schawinski, Kevin; Urry, C M; Lacy, M

    2015-01-01T23:59:59.000Z

    We used the Hubble Space Telescope WFC3 near-infrared camera to image the host galaxies of a sample of eleven luminous, dust-reddened quasars at z ~ 2 -- the peak epoch of black hole growth and star formation in the Universe -- to test the merger-driven picture for the co-evolution of galaxies and their nuclear black holes. The red quasars come from the FIRST+2MASS red quasar survey and a newer, deeper, UKIDSS+FIRST sample. These dust-reddened quasars are the most intrinsically luminous quasars in the Universe at all redshifts, and may represent the dust-clearing transitional phase in the merger-driven black hole growth scenario. Probing the host galaxies in rest-frame visible light, the HST images reveal that 8/10 of these quasars have actively merging hosts, while one source is reddened by an intervening lower redshift galaxy along the line-of-sight. We study the morphological properties of the quasar hosts using parametric Sersic fits as well as the non-parametric estimators (Gini coefficient, M_{20} and a...

  18. Gas/solvent-induced transformation and expansion of a nonporous solid to 1:1 host guest form

    SciTech Connect (OSTI)

    Thallapally, Praveen K.; McGrail, B. Peter; Dalgarno, Scott J.; Atwood, Jerry L.

    2008-07-01T23:59:59.000Z

    Herein we report the gas (CO2, N2O and propane) and solvent (CS2 and acetone) induced transformation and expansion of guest free thermodynamic form of a p-tert-butylcalix [4]arene to 1:1 host guest form.

  19. Short title: Endophytes of grasses Culturing and direct PCR suggest prevalent host generalism among diverse fungal endophytes of

    E-Print Network [OSTI]

    Arnold, A. Elizabeth

    Short title: Endophytes of grasses Culturing and direct PCR suggest prevalent host generalism among diverse fungal endophytes of tropical forest grasses K. Lindsay Higgins Phyllis D. Coley Thomas A. Kursar: Most studies examining endophytic fungi associated with grasses (Poaceae) have focused on agronomically

  20. The host of GRB/XRF 030528 - an actively star forming galaxy at z=0.782

    E-Print Network [OSTI]

    Rau, A

    2005-01-01T23:59:59.000Z

    An important parameter for the distinction of X-ray flashes, X-ray rich bursts and Gamma-ray bursts in the rest frame is the distance to the explosion site. Here we report on the spectroscopic redshift determination of the host galaxy of XRF/GRB 030528 using the ESO VLT FORS2 instrument. From the strong oxygen and hydrogen emission lines the redshift was measured to be z=0.782+-0.001. Obtaining the line luminosities and ratios we find that the host is consistent with being an actively star forming galaxy with sub-solar metallicity. With a stellar mass of ~10E10 Msun the host is placed among the most massive GRB host galaxies at a similar redshift. Estimating the redshifted properties of the prompt emission, we find that XRF/GRB 030528 would be classified as an X-ray rich bursts in the rest frame rather than an X-ray flash in the typically used observer frame.

  1. Human enhancement and the future of work Report from a joint workshop hosted by the Academy of Medical

    E-Print Network [OSTI]

    Cambridge, University of

    Human enhancement and the future of work Report from a joint workshop hosted by the Academy of Medical Sciences, the British Academy, the Royal Academy of Engineering and the Royal Society. November 2012 #12;Academy of Medical Sciences The independent Academy of Medical Sciences promotes advances

  2. 0044-5231/03/242/02-107 $ 15.00/0 Review of Biogeography, Host Range and Evolution

    E-Print Network [OSTI]

    Lehmann, Gerlind

    . Tachinid flies of the Ormiini possess a conspicuously inflated prosternal region, enabling them to detect radiation. To emphasise further research in this impor- tant group of parasitoids, their biogeography 1993), but tachinid flies of the Ormiini are atypical because they use sound for host-detection (CADE

  3. Development and Utilization of Host Materials for White Phosphorescent Organic Light-Emitting Diodes

    SciTech Connect (OSTI)

    Tang, Ching; Chen, Shaw

    2013-05-31T23:59:59.000Z

    Our project was primarily focused on the MYPP 2015 goal for white phosphorescent organic devices (PhOLEDs or phosphorescent organic light-emitting diodes) for solid-state lighting with long lifetimes and high efficiencies. Our central activity was to synthesize and evaluate a new class of host materials for blue phosphors in the PhOLEDs, known to be a weak link in the device operating lifetime. The work was a collaborative effort between three groups, one primarily responsible for chemical design and characterization (Chen), one primarily responsible for device development (Tang) and one primarily responsible for mechanistic studies and degradation analysis (Rothberg). The host materials were designed with a novel architecture that chemically links groups with good ability to move electrons with those having good ability to move 揾oles (positive charges), the main premise being that we could suppress the instability associated with physical separation and crystallization of the electron conducting and hole conducting materials that might cause the devices to fail. We found that these materials do prevent crystallization and that this will increase device lifetimes but that efficiencies were reduced substantially due to interactions between the materials creating new low energy 揷harge transfer states that are non-luminescent. Therefore, while our proposed strategy could in principle improve device lifetimes, we were unable to find a materials combination where the efficiency was not substantially compromised. In the course of our project, we made several important contributions that are peripherally related to the main project goal. First, we were able to prepare the proposed new family of materials and develop synthetic routes to make them efficiently. These types of materials that can transport both electrons and holes may yet have important roles to play in organic device technology. Second we developed an important new method for controlling the deposition profile of material so that arbitrary concentration gradients can be implemented in layers with mixed composition. These concentration profiles are known to increase device efficiency and longevity and we confirmed that experimentally. Third, we investigated a new method for analyzing degradation in devices using mass spectrometry to look for degradation products. We showed that these methods are not simple to interpret unambiguously and need to be used with caution.

  4. Managing Energy and Server Resources in Hosting Centers Jeffrey S. Chase, Darrell C. Anderson, Prachi N. Thakar, Amin M. Vahdat \\Lambda

    E-Print Network [OSTI]

    Chase, Jeffrey S.

    resource allotments by estimating the value of their effects on service performance. A greedy resource surges and capital costs for excess capacity. Hosting centers face familiar operating system challengesManaging Energy and Server Resources in Hosting Centers Jeffrey S. Chase, Darrell C. Anderson

  5. Abstract--With the increasing deployment of overlay networks, a mobile host with a range of network interfaces can be connected

    E-Print Network [OSTI]

    Atkinson, Robert C

    Hierarchical MIPv6. Address management strategy in mobile host multihoming context is investigatedAbstract--With the increasing deployment of overlay networks, a mobile host with a range of network interfaces can be connected to multiple access networks simultaneously. Such multihoming technology can

  6. IMPROVED CATALYSTS FOR HEAVY OIL UPGRADING BASED ON ZEOLITE Y NANOPARTICLES ENCAPSULATED IN STABLE NANOPOROUS HOSTS

    SciTech Connect (OSTI)

    Conrad Ingram; Mark Mitchell

    2004-06-30T23:59:59.000Z

    The focus of this project is to improve the catalytic performance of zeolite Y for heavy petroleum hydrocracking by synthesizing nanoparticles of the zeolite ({approx}20-30 nm) inside nanoporous silicate or aluminosilicate hosts of similar pore diameters. The encapsulated zeolite nanoparticles are expected to possess pores of reduced diffusional path lengths, hence hydrocarbon substrates will diffuse in, are converted and the products quickly diffused out. This is expected to prevent over-reaction, hence minimizing pore blockage and active sites deactivation. In this phase of the project, research activities were focused on refining procedures to: (a) improve the synthesis of ordered, high surface area nanoporous silica, such as SBA-15, with expanded pore size using trimethylbenzene as additive to the parent SBA-15 synthesis mixture; and (b) reduce the particle size of zeolite Y such that they can be effectively incorporated into the nanoporous silicas. The synthesis of high surface ordered nanoporous silica containing enlarged pores of diameter of 25 nm (larger than the standard size of 8.4 nm) using trimethylbenzene as a pore size expander was accomplished. The synthesis of zeolite Y nanoparticles with median pore size of approximately 50 nm (smaller than the 80 nm typically obtained with TMAOH) using combined TMABr/TMAOH as organic additives was also accomplished.

  7. IMPROVED CATALYSTS FOR HEAVY OIL UPGRADING BASED ON ZEOLITE Y NANOPARTICLES ENCAPSULATED IN STABLE NANOPOROUS HOSTS

    SciTech Connect (OSTI)

    Conrad Ingram

    2003-09-03T23:59:59.000Z

    The focus of this project is to improve the catalytic performance of zeolite Y for petroleum hydrocracking by synthesizing nanoparticles of the zeolite ({approx}20-25 nm) inside nanoporous silicate or aluminosilicate hosts. The encapsulated zeolite nanoparticles are expected to possess reduced diffusional path lengths, hence hydrocarbon substrates will diffuse in, are converted and the products quickly diffused out. This is expected to prevent over-reaction and the blocking of the zeolite pores and active sites will be minimized. In this phase of the project, procedures for the synthesis of ordered nanoporous silica, such as SBA-15, using block copolymers and nonionic surfactant were successful reproduced. Expansion of the pores sizes of the nanoporous silica using trimethylbenzene is suggested based on shift in the major X-Ray Diffraction peak in the products to lower 2 angles compared with the parent SBA-15 material. The synthesis of ordered nanoporous materials with aluminum incorporated in the predominantly silicate framework was attempted but is not yet successful, and the procedures needs will be repeated and modified as necessary. Nanoparticles of zeolite Y of particle sizes in the range 40 nm to 120 nm were synthesized in the presence of TMAOH as the particle size controlling additive.

  8. Origin of the Metallicity Dependence of Exoplanet Host Stars in the Protoplanetary Disk Mass Distribution

    E-Print Network [OSTI]

    Wyatt, M C; Greaves, J S

    2007-01-01T23:59:59.000Z

    The probability of a star hosting a planet that is detectable in radial velocity surveys increases Ppl(Z) oc 10^2Z, where Z is metallicity. Core accretion models reproduce this trend, since the protoplanetary disk of a high metallicity star has a high density of solids and so forms cores which accrete gas before the primordial gas disk dissipates. This paper considers the origin of the form of Ppl(Z). We introduce a simple model in which detectable planets form when the mass of solids in the protoplanetary disk, Ms, exceeds a critical value. In this model the form of Ppl(Z) is a direct reflection of the distribution of protoplanetary disk masses, Mg, and the observed Ppl(Z) is reproduced if P(Mg>Mg') oc 1/Mg'^2. We argue that a protoplanetary disk's sub-mm dust mass is a pristine indicator of the mass available for planet-building and find the observed sub-mm disk mass distribution is consistent with the observed Ppl(Z) if Ms>0.5M_J is required to form detectable planets. Any planet formation model which impo...

  9. Development of a Phosphate Ceramic as a Host for Halide-contaminated Plutonium Pyrochemical Reprocessing Wastes

    SciTech Connect (OSTI)

    Metcalfe, Brian; Fong, Shirley K.; Gerrard, Lee A.; Donald, Ian W.; Strachan, Denis M.; Scheele, Randall D.

    2007-03-31T23:59:59.000Z

    The presence of halide anions in four types of wastes arising from the pyrochemical reprocessing of plutonium required an immobilization process to be developed in which not only the actinide cations but also the halide anions were immobilized in a durable waste form. At AWE, we have developed such a process using Ca3(PO4)2 as the host material. Successful trials of the process with actinide- and Cl-bearing Type I waste were carried out at PNNL where the immobilization of the waste in a form resistant to aqueous leaching was confirmed. Normalized mass losses determined at 40癈 and 28 days were 12 x 10-6 g?m-2 and 2.7 x 10-3 g?m-2 for Pu and Cl, respectively. Accelerated radiation-induced damage effects are being determined with specimens containing 238Pu. No changes in the crystalline lattice have been detected with XRD after the 239Pu equivalent of 400 years ageing. Confirmation of the process for Type II waste (a oxyhydroxide-based waste) is currently underway at PNNL. Differences in the ionic state of Pu in the four types of waste have required different surrogates to be used. Samarium chloride was used successfully as a surrogate for both Pu(III) and Am(III) chlorides. Initial investigations into the use of HfO2 as the surrogate for Pu(IV) oxide in Type II waste indicated no significant differences.

  10. ON THE SURVIVAL OF BROWN DWARFS AND PLANETS ENGULFED BY THEIR GIANT HOST STAR

    SciTech Connect (OSTI)

    Passy, Jean-Claude; Mac Low, Mordecai-Mark [Department of Astrophysics, American Museum of Natural History, New York, NY (United States); De Marco, Orsola [Department of Physics and Astronomy, Macquarie University, Sydney, NSW (Australia)

    2012-11-10T23:59:59.000Z

    The recent discovery of two Earth-mass planets in close orbits around an evolved star has raised questions as to whether substellar companions can survive encounters with their host stars. We consider whether these companions could have been stripped of significant amounts of mass during the phase when they orbited through the dense inner envelopes of the giant. We apply the criterion derived by Murray et al. for disruption of gravitationally bound objects by ram pressure to determine whether mass loss may have played a role in the histories of these and other recently discovered low-mass companions to evolved stars. We find that the brown dwarf and Jovian-mass objects circling WD 0137-349, SDSS J08205+0008, and HIP 13044 are most unlikely to have lost significant mass during the common envelope phase. However, the Earth-mass planets found around KIC 05807616 could well be the remnants of one or two Jovian-mass planets that lost extensive mass during the common envelope phase.

  11. The galaxy - dark matter halo connection: which galaxy properties are correlated with the host halo mass?

    E-Print Network [OSTI]

    Contreras, S; Norberg, P; Padilla, N

    2015-01-01T23:59:59.000Z

    We demonstrate how the properties of a galaxy depend on the mass of its host dark matter subhalo, using two independent models of galaxy formation. For the cases of stellar mass and black hole mass, the median property value displays a monotonic dependence on subhalo mass. The slope of the relation changes for subhalo masses for which heating by active galactic nuclei becomes important. The median property values are predicted to be remarkably similar for central and satellite galaxies. The two models predict considerable scatter around the median property value, though the size of the scatter is model dependent. There is only modest evolution with redshift in the median galaxy property at a fixed subhalo mass. Properties such as cold gas mass and star formation rate, however, are predicted to have a complex dependence on subhalo mass. In these cases subhalo mass is not a good indicator of the value of the galaxy property. We illustrate how the predictions in the galaxy property - subhalo mass plane differ fr...

  12. Structural Consequences of Anionic Host-Cationic Guest Interactions in a Supramolecular Assembly

    SciTech Connect (OSTI)

    Pluth, Michael D.; Johnson, Darren W.; Szigethy, Geza; Davis, Anna V.; Teat, Simon J.; Oliver, Allen G.; Bergman, Robert G.; Raymond, Kenneth N.

    2008-07-09T23:59:59.000Z

    The molecular structure of the self-assembled supramolecular assembly [M{sub 4}L{sub 6}]{sup 12-} has been explored with different metals (M = Ga{sup III}, Fe{sup III}, Ti{sup IV}) and different encapsulated guests (NEt{sub 4}{sup +}, BnNMe{sub 3}{sup +}, Cp{sub 2}Co{sup +}, Cp*{sub 2}Co{sup +}) by X-ray crystallography. While the identity of the metal ions at the vertices of the M{sub 4}L{sub 6} structure is found to have little effect on the assembly structure, encapsulated guests significantly distort the size and shape of the interior cavity of the assembly. Cations on the exterior of the assembly are found to interact with the assembly through either {pi}-{pi}, cation-{pi}, or CH-{pi} interactions. In some cases, the exterior guests interact with only one assembly, but cations with the ability to form multiple {pi}-{pi} interactions are able to interact with adjacent assemblies in the crystal lattice. The solvent accessible cavity of the assembly is modeled using the rolling probe method and found to range from 253-434 {angstrom}{sup 3}, depending on the encapsulated guest. Based on the volume of the guest and the volume of the cavity, the packing coefficient for each host-guest complex is found to range from 0.47-0.67.

  13. The Host Galaxies and Narrow Line Regions of Four Double-Peaked [OIII] AGN

    E-Print Network [OSTI]

    Villforth, C

    2015-01-01T23:59:59.000Z

    Major gas-rich mergers of galaxies are expected to play an important role in triggering and fuelling luminous AGN. We present deep multi-band (u/r/z) imaging and long slit spectroscopy of four double-peaked [OIII] emitting AGN, a class of objects associated with either kcp-separated binary AGN or final stage major mergers, though AGN with complex narrow-line regions are known contaminants. Such objects are of interest since they represent the onset of AGN activity during the merger process. Three of the objects studied have been confirmed as major mergers using near-infrared imaging, one is a confirmed X-ray binary AGN. All AGN are luminous and have redshifts of 0.1 < z < 0.4. Deep r-band images show that a majority (3/4) of the sources have disturbed host morphologies and tidal features, while the remaining source is morphologically undisturbed down to low surface brightness limits. The lack of morphological disturbances in this galaxy despite the fact that is is a close binary AGN suggests that the me...

  14. METHANE HYDRATE STUDIES: DELINEATING PROPERTIES OF HOST SEDIMENTS TO ESTABLISH REPRODUCIBLE DECOMPOSITION KINETICS.

    SciTech Connect (OSTI)

    Mahajan, Devinder; Jones, Keith W.; Feng, Huan; Winters, William J.

    2004-12-01T23:59:59.000Z

    The use of methane hydrate as an energy source requires development of a reliable method for its extraction from its highly dispersed locations in oceanic margin sediments and permafrost. The high pressure (up to 70 MPa) and low temperature (272 K to 278 K) conditions under which hydrates are stable in the marine environment can be mimicked in a laboratory setting and several kinetic studies of pure methane hydrate decomposition have been reported. However, the effect of host sediments on methane hydrate occurrence and decomposition are required to develop reliable hydrate models. In this paper, we describe methods to measure sediment properties as they relate to pore-space methane gas hydrate. Traditional geotechnical techniques are compared to the micrometer level by use of the synchrotron Computed Microtomography (CMT) technique. CMT was used to measure the porosity at the micrometer level and to show pore-space pathways through field samples. Porosities for three sediment samples: one from a site on Georges Bank and two from the known Blake Ridge methane hydrate site, from different depths below the mud line were measured by traditional drying and by the new CMT techniques and found to be in good agreement. The integration of the two analytical approaches is necessary to enable better understanding of methane hydrate interactions with the surrounding sediment particles.

  15. THE OPTICALLY UNBIASED GRB HOST (TOUGH) SURVEY. VI. RADIO OBSERVATIONS AT z {approx}< 1 AND CONSISTENCY WITH TYPICAL STAR-FORMING GALAXIES

    SciTech Connect (OSTI)

    Michalowski, M. J.; Dunlop, J. S. [SUPA (Scottish Universities Physics Alliance), Institute for Astronomy, University of Edinburgh, Royal Observatory, Edinburgh EH9 3HJ (United Kingdom); Kamble, A.; Kaplan, D. L. [Physics Department, University of Wisconsin-Milwaukee, Milwaukee, WI 53211 (United States); Hjorth, J.; Malesani, D.; Fynbo, J. P. U.; Kruehler, T. [Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 30, DK-2100 Copenhagen O (Denmark); Reinfrank, R. F. [CSIRO Astronomy and Space Science, P.O. Box 76, Epping, NSW 1710 (Australia); Bonavera, L. [Instituto de Fisica de Cantabria, CSIC-Universidad de Cantabria, Avda. de los Castros s/n, E-39005 Santander (Spain); Castro Ceron, J. M. [Department of Radio Astronomy, Madrid Deep Space Communications Complex (INTA-NASA/INSA), Ctra. M-531, km. 7, E-28.294 Robledo de Chavela (Madrid) (Spain); Ibar, E. [UK Astronomy Technology Centre, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ (United Kingdom); Garrett, M. A. [Netherlands Institute for Radio Astronomy (ASTRON), Postbus 2, 7990 AA Dwingeloo (Netherlands); Jakobsson, P. [Centre for Astrophysics and Cosmology, Science Institute, University of Iceland, Dunhagi 5, 107 Reykjavik (Iceland); Levan, A. J. [Department of Physics, University of Warwick, Coventry CV4 7AL (United Kingdom); Massardi, M. [INAF-Istituto di Radioastronomia, via Gobetti 101, I-40129 Bologna (Italy); Pal, S. [ICRAR, University of Western Australia, 35 Stirling Highway, Crawley, WA (Australia); Sollerman, J. [Oskar Klein Centre, Department of Astronomy, AlbaNova, Stockholm University, SE-10691 Stockholm (Sweden); Tanvir, N. R. [Department of Physics and Astronomy, University of Leicester, University Road, Leicester LE1 7RH (United Kingdom); Van der Horst, A. J., E-mail: mm@roe.ac.uk [Astronomical Institute 'Anton Pannekoek', University of Amsterdam, Science Park 904, 1098XH Amsterdam (Netherlands); and others

    2012-08-20T23:59:59.000Z

    The objective of this paper is to determine the level of obscured star formation activity and dust attenuation in a sample of gamma-ray burst (GRB) hosts, and to test the hypothesis that GRB hosts have properties consistent with those of the general star-forming galaxy populations. We present a radio continuum survey of all z < 1 GRB hosts in The Optically Unbiased GRB Host (TOUGH) sample supplemented with radio data for all (mostly pre-Swift) GRB-SN hosts discovered before 2006 October. We present new radio data for 22 objects and have obtained a detection for three of them (GRB 980425, 021211, 031203; none in the TOUGH sample), increasing the number of radio-detected GRB hosts from two to five. The star formation rate (SFR) for the GRB 021211 host of {approx}825 M{sub Sun} yr{sup -1}, the highest ever reported for a GRB host, places it in the category of ultraluminous infrared galaxies. We found that at least {approx}63% of GRB hosts have SFR < 100 M{sub Sun} yr{sup -1} and at most {approx}8% can have SFR > 500 M{sub Sun} yr{sup -1}. For the undetected hosts the mean radio flux (<35 {mu}Jy 3{sigma}) corresponds to an average SFR < 15 M{sub Sun} yr{sup -1}. Moreover, {approx}> 88% of the z {approx}< 1 GRB hosts have ultraviolet dust attenuation A{sub UV} < 6.7 mag (visual attenuation A{sub V} < 3 mag). Hence, we did not find evidence for large dust obscuration in a majority of GRB hosts. Finally, we found that the distributions of SFRs and A{sub UV} of GRB hosts are consistent with those of Lyman break galaxies, H{alpha} emitters at similar redshifts, and of galaxies from cosmological simulations. The similarity of the GRB population with other star-forming galaxies is consistent with the hypothesis that GRBs, a least at z {approx}< 1, trace a large fraction of all star formation, and are therefore less biased indicators than once thought.

  16. Origin of the Metallicity Dependence of Exoplanet Host Stars in the Protoplanetary Disk Mass Distribution

    E-Print Network [OSTI]

    M. C. Wyatt; C. J. Clarke; J. S. Greaves

    2007-07-18T23:59:59.000Z

    The probability of a star hosting a planet that is detectable in radial velocity surveys increases Ppl(Z) oc 10^2Z, where Z is metallicity. Core accretion models reproduce this trend, since the protoplanetary disk of a high metallicity star has a high density of solids and so forms cores which accrete gas before the primordial gas disk dissipates. This paper considers the origin of the form of Ppl(Z). We introduce a simple model in which detectable planets form when the mass of solids in the protoplanetary disk, Ms, exceeds a critical value. In this model the form of Ppl(Z) is a direct reflection of the distribution of protoplanetary disk masses, Mg, and the observed Ppl(Z) is reproduced if P(Mg>Mg') oc 1/Mg'^2. We argue that a protoplanetary disk's sub-mm dust mass is a pristine indicator of the mass available for planet-building and find the observed sub-mm disk mass distribution is consistent with the observed Ppl(Z) if Ms>0.5M_J is required to form detectable planets. Any planet formation model which imposes a critical solid mass for planet formation would reproduce the observed Ppl(Z), and core accretion models are empirically consistent with a threshold criterion. We identify 7 protoplanetary disks which, by rigid application of this criterion, would be expected to form detectable planets. A testable prediction is that Ppl(Z) should flatten both for Z>0.5dex and as more distant and lower mass planets are discovered. Further, combining this model with one in which the evolution of a star's debris disk is also influenced by the solid mass in its protoplanetary disk, results in the prediction that debris disks detected around stars with planets should be more infrared luminous than those around stars without planets in tentative agreement with recent observations.

  17. Development of a Phosphate Ceramic as a Host for Halide-Contaminated Plutonium Pyrochemical Reprocessing Wastes

    SciTech Connect (OSTI)

    Metcalfe, Brian; Fong, Shirley; Gerrard, Lee; Donald, Ian [MSRD, AWE plc, AWE Aldermaston, Reading, RG7 4PR (United Kingdom); Strachan, Denis; Scheele, Randall [PNNL, Richland, WA, 99352 (United States)

    2007-07-01T23:59:59.000Z

    The presence of halide anions in four types of wastes arising from the pyrochemical reprocessing of plutonium required an immobilization process to be developed in which not only the actinide cations but also the halide anions were immobilized in a durable, leach resistant form. AWE has developed such a process using Ca{sub 3}(PO{sub 4}){sub 2} as the host material. Successful trials of the process using actinide-doped Type I waste (essentially a chloride-based waste) were carried out at PNNL where the immobilization of the waste in a form resistant to aqueous leaching was confirmed. Normalized mass losses determined using a modified MCC-1 test at 40 deg. C/28 days were 12 x 10{sup -6} g.m{sup -2} and 2.7 x 10{sup -3} g.m{sup -2} for Pu and Cl, respectively. Accelerated radiation-induced damage effects are being determined with specimens containing {sup 238}Pu. No changes in the crystalline lattice have been detected with XRD after the {sup 239}Pu equivalent of 400 years ageing. Confirmation of the process for Type II waste (an oxyhydroxide-based waste) is currently underway at PNNL. Differences in the ionic state of plutonium in the four types of waste have required different surrogates to be used. Samarium chloride was used successfully as a surrogate for both Pu(III) and Am(III) chlorides. Early investigations into the use of HfO{sub 2} as the surrogate for Pu(IV) oxide in Type II waste showed some apparent differences in the phase assemblages of the surrogate and actinide-based products. However XRD examination of the products at higher resolution has demonstrated there is no significant difference and that for this work HfO{sub 2} is a suitable surrogate for PuO{sub 2}. (authors)

  18. Low-Energy Nuclear Reactions of Protons in Host Metals at Picometre Distance

    SciTech Connect (OSTI)

    Heinrich Hora; George H. Miley; Jak C. Kelly

    2000-11-12T23:59:59.000Z

    A review is given for the explanation of the measurements of Miley et al. of a fully reproducible generation of nuclei of the whole periodic table by protons in host metals during a several-weeks reaction. Similar low-energy nuclear reactions (LENR) were observed by other groups. The fact that the heavy nuclides are not due to pollution can be seen from the fact that such very rare elements as thulium and terbium were detected by unique K-shell X-ray spectra. The nuclear reaction energy goes into the heavy nuclei as measured from much bigger traces in CR39 than from alphas. The fact that any reaction of the protons results in stable daughter nuclei is confirmed by the fact that the highest energy gain is resulting with stable reaction products. This has been explained in Ref. 2, and the energy gain for the heavy element generation by a compound reaction was discussed. The explanation is based on the model of the authors from 1989 to assume free motion of the protons contrary to localized crystalline states. A relation of the reaction time U on distance d of the reacting nuclei by a power law with an exponent 34.8 was derived. Based on few reproducible D-D reactions, a reaction time near the range of megaseconds and a reaction distance of nanometers was concluded. A splendid confirmation of the picometre-megasecond reactions was achieved by Li et al. from his direct quantum mechanical calculations of the hot fusion D-T reactions based on a one-step selective resonance tunneling model. Li et al. were able for the first time to derive the cross sections of the hot fusion. Li's application to picometre distance showed megasecond reaction times with no neutron or gamma emission. Because of the imaginary part in the Schroedinger potential, the problem of the level width is reduced by damping.

  19. STAR FORMATION IN LINER HOST GALAXIES AT z {approx} 0.3

    SciTech Connect (OSTI)

    Tommasin, Silvia; Netzer, Hagai; Sternberg, Amiel [School of Physics and Astronomy, Tel Aviv University, Tel Aviv 69978 (Israel); Nordon, Raanan; Lutz, Dieter; Berta, Stefano; Magnelli, Benjamin [MPE, Postfach 1312, 85741 Garching (Germany); Bongiorno, Angela [INAF-Oservatorio Astronomico di Roma, via Frascati 33, 00040 Monte Porzio Catone (Roma) (Italy); Le Floc'h, Emeric; Riguccini, Laurie [Laboratoire AIM, CEA/DSM-CNRS-Universite Paris Diderot, IRFU/Service d'Astrophysique, Bat 709, CEA-Saclay, 91191 Gif-sur-Yvette Cedex (France); Pozzi, Francesca [Dipartimento di Astronomia, Universita degli Studi di Bologna, via Ranzani 1, 40127 Bologna (Italy)

    2012-07-10T23:59:59.000Z

    We present the results of a Herschel-PACS study of a sample of 97 low-ionization nuclear emission-line regions (LINERs) at redshift z {approx} 0.3 selected from the zCOSMOS survey. Of these sources, 34 are detected in at least one PACS band, enabling reliable estimates of the far-infrared L{sub FIR} luminosities, and a comparison to the FIR luminosities of local LINERs. Many of our PACS-detected LINERs are also UV sources detected by GALEX. Assuming that the FIR is produced in young dusty star-forming regions, the typical star formation rates (SFRs) for the host galaxies in our sample are {approx}10 M{sub Sun} yr{sup -1}, 1-2 orders of magnitude larger than in many local LINERs. Given stellar masses inferred from optical/NIR photometry of the (unobscured) evolved stellar populations, we find that the entire sample lies close to the star-forming 'main sequence' for galaxies at redshift 0.3. For young star-forming regions, the H{alpha}- and UV-based estimates of the SFRs are much smaller than the FIR-based estimates, by factors {approx}30, even assuming that all of the H{alpha} emission is produced by O-star ionization rather than by the active galactic nuclei (AGNs). These discrepancies may be due to large (and uncertain) extinctions toward the young stellar systems. Alternatively, the H{alpha} and UV emissions could be tracing residual star formation in an older, less obscured population with decaying star formation. We also compare L{sub SF} and L(AGN) in local LINERs and in our sample. Finally, we comment on the problematic use of several line diagnostic diagrams in cases with an estimated obscuration similar to that in the sample under study.

  20. Electrically switchable polymer liquid crystal and polymer birefringent flake in fluid host systems and optical devices utilizing same

    DOE Patents [OSTI]

    Marshall, Kenneth L.; Kosc, Tanya Z.; Jacobs, Stephen D.; Faris, Sadeg M.; Li, Le

    2003-12-16T23:59:59.000Z

    Flakes or platelets of polymer liquid crystals (PLC) or other birefringent polymers (BP) suspended in a fluid host medium constitute a system that can function as the active element in an electrically switchable optical device when the suspension is either contained between a pair of rigid substrates bearing transparent conductive coatings or dispersed as microcapsules within the body of a flexible host polymer. Optical properties of these flake materials include large effective optical path length, different polarization states and high angular sensitivity in their selective reflection or birefringence. The flakes or platelets of these devices need only a 3-20.degree. rotation about the normal to the cell surface to achieve switching characteristics obtainable with prior devices using particle rotation or translation.

  1. Genomics Approaches to Study Molecular and Cellular Mechanisms of Host Response to Avian Influenza Virus in Chickens

    E-Print Network [OSTI]

    Wang, Ying

    2012-02-14T23:59:59.000Z

    tropism and the pathogenesis of viral diseases (Cullen, 2006a). On the other hand, viruses encode viral miRNAs to protect themselves against cellular antiviral responses (Gupta, et al., 2006). Host miRNAs play important roles in antiviral... direct negative effect on the replication of retrovirus primate foamy virus type 1 (PFV-1), which is mediated through the down- regulation of replication-essential viral proteins encoded by open reading frame 2 (ORF2) ( Lecellier, et al., 2005; Cullen...

  2. Refractory oxide hosts for a high power, broadly tunable laser with high quantum efficiency and method of making same

    DOE Patents [OSTI]

    Chen, Yok (Oak Ridge, TN); Gonzalez, Roberto (Madrid, ES)

    1986-01-01T23:59:59.000Z

    Refractory oxide crystals having high-quantum efficiency and high thermal stability for use as broadly tunable laser host materials. The crystals are formed by removing hydrogen from a single crystal of the oxide material to a level below about 10.sup.12 protons per cm.sup.3 and subsequently thermochemically reducing the oxygen content of the crystal to form sufficient oxygen anion vacancies so that short-lived F.sup.+ luminescence is produced when the crystal is optically excited.

  3. Primordial pollution of globular clusters within their host dwarfs embedded in dark matter halos at high redshifts

    E-Print Network [OSTI]

    Kenji Bekki

    2005-12-19T23:59:59.000Z

    Recent observational studies have revealed star-to-star abundance inhomogeneity among light elements (e.g., C, N, O, Na, and Al) of stars on the main sequence in the Galactic globular clusters (GCs). One of promising interpretations for this result is that the observed abundance inhomogeneity is due to the second generation of stars formed from ejecta of the first generation of evolved stars (e.g., AGB stars) within GCs. However it remains unclear whether and how this primordial pollution can occur within GCs. We here propose a new scenario in which primordial pollution of GCs is highly likely to occur if GCs are located in the central regions of high redshift dark matter subhalos that can host low-mass dwarf galaxies. In this scenario, gas ejected from the first generation of stars of GCs can be effectively trapped in the deep gravitational potential of their host halos and consequently can be consumed for the formation of the second generation of stars without losing a significant amount of gas by ram pressure stripping of interstellar and intergalactic medium. During merging of these halos with the proto-Galaxy, the halos are completely destroyed owing to the strong tidal field of the Galaxy. The self-polluted GCs located initially in the central regions of the halos can survive from tidal destruction owing to their compactness and finally become the Galactic halo GCs. In this scenario, ejecta of field stars surrounding the central GCs can be also converted into stars within their host dwarfs and finally become the second generation of stars of GCs. We also discuss the origin of the difference in the degree of abundance inhomogeneity between different GCs, such as $\\omega$ Centauri and NGC 6752, in terms of the difference in physical properties between host halos from which GC originate.

  4. Host habitat location mediated by olfactory stimuli in anaphes iole (hymenoptera: mymaridae), an egg parasitoid of lygus hesperus (hemiptera: miridae)

    E-Print Network [OSTI]

    Manrique, Veronica

    2005-02-17T23:59:59.000Z

    HOST HABITAT LOCATION MEDIATED BY OLFACTORY STIMULI IN ANAPHES IOLE (HYMENOPTERA: MYMARIDAE), AN EGG PARASITOID OF LYGUS HESPERUS (HEMIPTERA: MIRIDAE) A Thesis by VERONICA MANRIQUE Submitted to the Office of Graduate Studies of Texas A... PARASITOID OF LYGUS HESPERUS (HEMIPTERA: MIRIDAE) A Thesis by VERONICA MANRIQUE Submitted to Texas A&M University in partial fulfillment of the requirements for the degree of MASTER OF SCIENCE Approved as to style and content by...

  5. Refractory oxide hosts for a high power, broadly tunable laser with high quantum efficiency and method of making same

    DOE Patents [OSTI]

    Chen, Yok; Gonzalez, R.

    1985-07-03T23:59:59.000Z

    Refractory oxide crystals having high-quantum efficiency and high thermal stability for use as broadly tunable laser host materials. The crystals are formed by removing hydrogen from a single crystal of the oxide material to a level below about 10/sup 12/ protons per cm/sup 3/ and subsequently thermochemically reducing the oxygen content of the crystal to form sufficient oxygen anion vacancies so that short-lived F/sup +/ luminescence is produced when the crystal is optically excited.

  6. The Art of Seduction and Affect Economy: Neoliberal Class Struggle and Gender Politics in a Tokyo Host Club

    E-Print Network [OSTI]

    Takeyama, Akiko

    2008-01-01T23:59:59.000Z

    ). Such affective labor is observed in today抯 formal and informal service industry, including but not limited to: tourism, sexual amusement, counseling, self-help seminars, aesthetic and relaxation salons, nannies, maid, and so on (Cruikshank 1993; Ehrenreich... of Japan抯 ephemeral, fad-driven subculture, but a constitutive element of Japan抯 affect economy梐n economy rooted in postindustrial consumerism and neoliberal globalization. The first host club establishment, in fact, opened in the mid-1960s, in Tokyo...

  7. Chronic graft-versus-host disease in the rat radiation chimera. III. Immunology and immunopathology in rapidly induced models

    SciTech Connect (OSTI)

    Beschorner, W.E.; Tutschka, P.J.; Santos, G.W.

    1983-03-01T23:59:59.000Z

    Although chronic graft-versus-host disease (GVHD) frequently develops in the long-term rat radiation chimera, we present three additional models in which a histologically similar disease is rapidly induced. These include adoptive transfer of spleen and bone marrow from rats with spontaneous chronic GVHD into lethally irradiated rats of the primary host strain; sublethal irradiation of stable chimeras followed by a booster transplant; and transfer of spleen cells of chimeras recovering from acute GVHD into second-party (primary recipient strain) or third-party hosts. Some immunopathologic and immune abnormalities associated with spontaneous chronic GVHD were not observed in one or more of the induced models. Thus, IgM deposition in the skin, antinuclear antibodies, and vasculitis appear to be paraphenomena. On the other hand, lymphoid hypocellularity of the thymic medulla, immaturity of splenic follicles, and nonspecific suppressor cells were consistently present in the long term chimeras, and in all models. These abnormalities therefore may be pathogenetically important, or closely related to the development of chronic GVHD.

  8. On the afterglow and host galaxy of GRB 021004: A comprehensivestudy with the Hubble Space Telescope1

    SciTech Connect (OSTI)

    Fynbo, J.P.U.; Gorosabel, J.; Smette, A.; Fruchter, A.; Hjorth,J.; Pedersen, K.; Levan, A.; Burud, I.; Sahu, K.; Vreeswijk, P.M.; Bergeron, E.; Kouveliotou1, C.; Tanvir, N.; Thorsett11, S.E.; Wijers,R.A.M.J.; Castro Ceron, J.M.; Castro-Tirado, A.; Garnavich, P.; Holland,S.T.; Jakobsson, P.; Moller, P.; Nugent, P.; Pian, E.; Rhoads, J.; Thomsen, B.; Watson, D.; Woosley, S.

    2004-12-01T23:59:59.000Z

    We report on Hubble Space Telescope (HST) observations of the late-time afterglow and host galaxy of GRB 021004 (z = 2.33).Although this gamma-ray burst (GRB) is one of the best observed so far in terms of sampling in the time domain, multi-wavelength coverage and polarimetric observations, there is large disagreement between different measurements and interpretations of this burst in the literature. We have observed the field of GRB 021004 with the HST at multiple epochs from 3 days until almost 10 months after the burst. With STI S prism and G430L spectroscopy we cover the spectral region from about 2000 Angstrom to 5700 Angstrom corresponding to 600 1700 Angstrom in the rest frame. From the limit on the flux recovery bluewards of the Lyman-limit we constrain the H I column density to be above 1 x 1018 cm-2 (5 sigma). Based on ACS and N ICMOS imaging we find that the afterglow evolved a chromatically within the errors (any variation must be less then 5 percent) during the period of HST observations. The color changes observed by other authors during the first four days must be related to a 'noisy' phenomenon superimposed on an afterglow component with a constant spectral shape. This also means that the cooling break has remained on the blue side of the optical part of the spectrum for at least two weeks after the explosion. The optical to X-ray slope OX is consistent with being the same at 1.4 and 52.4 days after the burst. This indicates that the cooling frequency is constant and hence, according to fireball models, that the circumburst medium has a constant density profile. The late-time slope of the light curve (alpha 2, F nu proportional to t-alpha2) is in the range 2 = 1.8-1.9, although inconsistent with a single power-law. This could be due to a late-time flattening caused by the transition to non-relativistic expansion or due to excess emission (a 'bump' in the light curve) about 7 days afterburst. The host galaxy is like most previously studied GRB hosts a (very) blue starburst galaxy with no evidence for dust and with strong Ly emission. The star-formation rate of the host is about 10 M solar mass yr-1 based on both the strength of the UV continuum and on the Ly alpha luminosity. The spectral energy distribution of the host implies an age in the range 30-100 Myr for the dominant stellar population.

  9. JOURNAL DE PHYSIQUE Colloque C5, supple'ment au no 5, Tome 40, Mai 1979, page C5-54 Hyperfine fields of S-rare earth impurities in noble hosts

    E-Print Network [OSTI]

    Paris-Sud XI, Universit de

    that the trivalent rare earth (e.g. Gd3+)contributes two s-p electrons, for monovalent hosts like noble metals fields of S-rare earth impurities in noble hosts A. Troper, 0.L. T. de Menezes and A. A. Gomes Centro previously developed for rare earth impurities diluted in s-p hosts [I]. Numerical results for the hyperfine

  10. RADII OF RAPIDLY ROTATING STARS, WITH APPLICATION TO TRANSITING-PLANET HOSTS

    SciTech Connect (OSTI)

    Brown, Timothy M., E-mail: tbrown@lcogt.ne [Las Cumbres Observatory Global Telescope, Goleta, CA 93117 (United States)

    2010-01-20T23:59:59.000Z

    The currently favored method for estimating radii and other parameters of transiting-planet host stars is to match theoretical models to observations of the stellar mean density rho{sub *}, the effective temperature T{sub eff}, and the composition parameter [Z]. This explicitly model-dependent approach is based on readily available observations, and results in small formal errors. Its performance will be central to the reliability of results from ground-based transit surveys such as TrES, HAT, and SuperWASP, as well as to the space-borne missions MOST, CoRoT, and Kepler. Here, I use two calibration samples of stars (eclipsing binaries (EBs) and stars for which asteroseismic analyses are available) having well-determined masses and radii to estimate the accuracy and systematic errors inherent in the rho{sub *} method. When matching to the Yonsei-Yale stellar evolution models, I find the most important systematic error results from selection bias favoring rapidly rotating (hence probably magnetically active) stars among the EB sample. If unaccounted for, this bias leads to a mass-dependent underestimate of stellar radii by as much as 4% for stars of 0.4 M{sub sun}, decreasing to zero for masses above about 1.4 M{sub sun}. Relative errors in estimated stellar masses are three times larger than those in radii. The asteroseismic sample suggests (albeit with significant uncertainty) that systematic errors are small for slowly rotating, inactive stars. Systematic errors arising from failings of the Yonsei-Yale models of inactive stars probably exist, but are difficult to assess because of the small number of well-characterized comparison stars having low mass and slow rotation. Poor information about [Z] is an important source of random error, and may be a minor source of systematic error as well. With suitable corrections for rotation, it is likely that systematic errors in the rho{sub *} method can be comparable to or smaller than the random errors, yielding radii that are accurate to about 2% for most stars.

  11. Helicobacter pylori cytotoxin-associated gene A (CagA) subverts the apoptosis-stimulating protein of p53 (ASPP2) tumor suppressor pathway of the host

    E-Print Network [OSTI]

    Buti, Ludovico

    Type I strains of Helicobacter pylori (Hp) possess a pathogenicity island, cag, that encodes the effector protein cytotoxin-associated gene A (CagA) and a type four secretion system. After translocation into the host cell, ...

  12. Safeguarding Health Information: Building Assurance through HIPAA Security Hosted by the HHS Office for Civil Rights (OCR) and the National Institute of Standards and Technology (NIST)

    E-Print Network [OSTI]

    1 Safeguarding Health Information: Building Assurance through HIPAA Security Hosted by the HHS, Acting Chief, Computer Security Division, Information Technology Laboratory (ITL), NIST 9 Data Using Encryption Matthew Scholl, Computer Security Division, Information Technology Laboratory

  13. Cosmos greenstone terrane: Insights into an Archaean volcanic arc, associated with komatiite-hosted nickel sulphide mineralisation, from U-Pb dating, volcanic stratigraphy and geochemistry

    E-Print Network [OSTI]

    De Joux, Alexandra; Joux, Alexandra de

    2014-06-30T23:59:59.000Z

    The Neoarchaean Agnew-Wiluna greenstone belt (AWB) of the Kalgoorlie Terrane, within the Eastern Goldfields Superterrane (EGS) of the Yilgarn Craton, Western Australia, contains several world-class, komatiite-hosted, ...

  14. Host Galaxy Extinction of SNIa: Co-evolution of ISM Structure and Extinction Law with Star-Formation

    E-Print Network [OSTI]

    B. W. Holwerda

    2008-01-31T23:59:59.000Z

    This paper presents a mechanism that may modify the extinction law for SNIa observed at higher redshift. Starting from the observations that (1) SNIa occur predominantly in spiral galaxies, (2) star-formation ejects ISM out of the plane of spirals, (3) star-formation alters the extinction properties of the dust in the ISM, and (4) there is substantially more star-formation at higher redshift, I propose that spiral galaxies have a dustier halo in the past than they do now. The ejected material's lower value of $R_V$ will lead to a lower average value ($\\bar{R}_V$) for SNIa observed at higher redshift. Two relations in SNIa observations indicate evolution of the average $R_V$: the relation of observed $R_V$ with inclination of the host galaxy at low redshift and the matching of the distribution of extinction values ($A_V$) for SNIa in different redshift intervals. The inclination effect does point to a halo with lower $R_V$ values. In contrast, the distributions of $A_V$ values match best for a $\\bar{R}_V(z)$ evolution that mimics the relation of SNIa dimming with redshift attributed to the cosmological constant. However, even in the worse case scenario, the evolution $\\bar{R}_V$ can not fully explain the dimming of SNIa: host galaxy extinction law evolution is not a viable alternative to account for the dimming of SNIa. Future observations of SNIa --multi-color lightcurves and spectra-- will solve separately for values of $A_V$ and $R_V$ for each SNIa . Solving for evolution of $\\bar{R}_V$ (and $A_V$) with redshift will be important for the coming generation of cosmological SNIa measurements and has the bonus science of insight into the distribution of dust-rich ISM in the host galaxies in the distant past.

  15. PS1-10bzj: A FAST, HYDROGEN-POOR SUPERLUMINOUS SUPERNOVA IN A METAL-POOR HOST GALAXY

    SciTech Connect (OSTI)

    Lunnan, R.; Chornock, R.; Berger, E.; Milisavljevic, D.; Drout, M.; Sanders, N. E.; Challis, P. M.; Czekala, I.; Foley, R. J.; Fong, W.; Kirshner, R. P.; Leibler, C.; Marion, G. H.; Narayan, G. [Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138 (United States); Huber, M. E. [Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822 (United States); McCrum, M.; Smartt, S. J. [Astrophysics Research Centre, School of Mathematics and Physics, Queen's University Belfast, Belfast BT7 1NN (United Kingdom); Rest, A. [Space Telescope Science Institute, 3700 San Martin Dr., Baltimore, MD 21218 (United States); Roth, K. C. [Gemini Observatory, 670 N. Aohoku Place, Hilo, HI 96720 (United States); Scolnic, D., E-mail: rlunnan@cfa.harvard.edu [Department of Physics and Astronomy, Johns Hopkins University, 3400 North Charles Street, Baltimore, MD 21218 (United States); and others

    2013-07-10T23:59:59.000Z

    We present observations and analysis of PS1-10bzj, a superluminous supernova (SLSN) discovered in the Pan-STARRS Medium Deep Survey at a redshift z = 0.650. Spectroscopically, PS1-10bzj is similar to the hydrogen-poor SLSNe 2005ap and SCP 06F6, though with a steeper rise and lower peak luminosity (M{sub bol} {approx_equal} -21.4 mag) than previous events. We construct a bolometric light curve, and show that while PS1-10bzj's energetics were less extreme than previous events, its luminosity still cannot be explained by radioactive nickel decay alone. We explore both a magnetar spin-down and circumstellar interaction scenario and find that either can fit the data. PS1-10bzj is located in the Extended Chandra Deep Field South and the host galaxy is imaged in a number of surveys, including with the Hubble Space Telescope. The host is a compact dwarf galaxy (M{sub B} Almost-Equal-To -18 mag, diameter {approx}< 800 pc), with a low stellar mass (M{sub *} Almost-Equal-To 2.4 Multiplication-Sign 10{sup 7} M{sub Sun }), young stellar population ({tau}{sub *} Almost-Equal-To 5 Myr), and a star formation rate of {approx}2-3 M{sub Sun} yr{sup -1}. The specific star formation rate is the highest seen in an SLSN host so far ({approx}100 Gyr{sup -1}). We detect the [O III] {lambda}4363 line, and find a low metallicity: 12 + (O/H) = 7.8 {+-} 0.2 ({approx_equal} 0.1 Z{sub Sun }). Together, this indicates that at least some of the progenitors of SLSNe come from young, low-metallicity populations.

  16. Rhizoctonia spp. associated with brown patch of St. Augustinegrass: isolate characterization, host range, and screening for resistance

    E-Print Network [OSTI]

    Hurd, Bernadette Murphy

    1982-01-01T23:59:59.000Z

    Resistance CONCLUSION LITERATURE CITED 13 13 18 18 25 27 34 41 45 VITA 50 LIST OF TABLES Page TABLE 1. Dates St. Augustinegrsss displaying brown patch symptoms was collected, location of the collection sites, and type of host tissue from..., drained, and placed under a laminar- flow hood on paper towels for 10 min to remove excess water. The cut end of each tip was dipped in molten Paraplast (Lancer Co. , St. Louis, NO. , 63103) to seal the wound. One tip was placed in each of the WA...

  17. Uranium and its relationship to host rock mineralogy in an unoxidized roll front in the Jackson group, South Texas

    E-Print Network [OSTI]

    Prasse, Eric Martin

    1978-01-01T23:59:59.000Z

    /Tordilla Sandstone Dubose Deweesville Sandstone Conquista Clay Dilworth Sandstone tion of uran1um bearing solutions to take place. Sandstone is the most common uranium host rock because its perme- ability permits the flow of m1nera11z1ng solutions through... to the flow of uranium bear1ng solutions during mineralization . In addition, the Deweesvi lie contai ns a shaly lens in its middle which is the upper boundary of several ore bod1es ( Dickinson and Sullivan, 1976), including the deposit studied 1 n...

  18. Physiochemical disparity of mismatched HLA class I alloantigens and risk of acute graft-versus-host disease

    E-Print Network [OSTI]

    Kosmoliaptsis, V.; J鰎is, M. M.; Mallon, D. H.; Lankester, A. C.; von dem Borne, P. A.; Kuball, J.; Bierings, M.; Cornelissen, J. J.; Groenendijk朣ijnke, M. E.; van der Holt, B.; Bradley, J. A.; Oudshoorn, M.; van Rood, Jon J.; Taylor, C. J.; Claas, F. H. J.

    2015-01-26T23:59:59.000Z

    ) 13 (24) 9 (16) 0.488 36 (21) 20 (12) 0.023 Diagnosis, n (%) 0.642 0.997 Acute leukemia 27 (45) 24 (44) 23 (40) 74 (43) 75 (45) Chronic leukemia 6 (10) 11 (20) 8 (14) 25 (15) 24 (14) Plasma cell disorder 5 (8) 2 (4) 3 (5) 10... 1 Physiochemical disparity of mismatched HLA class I alloantigens and risk of acute graft-versus-1 host disease following HSCT 2 Running title: Physiochemical HLA disparity and acute GvHD 3 V. Kosmoliaptsis1,2*, M. M. J鰎is3,4, D. H. Mallon1, A...

  19. WISE colours and star-formation in the host galaxies of radio-loud narrow-line Seyfert 1

    E-Print Network [OSTI]

    Caccianiga, A; Ballo, L; Foschini, L; Maccacaro, T; Della Ceca, R; Severgnini, P; Marcha, M J; Mateos, S; Sani, E

    2015-01-01T23:59:59.000Z

    We investigate the mid-infrared properties of the largest (42 objects) sample of radio-loud narrow-line Seyfert 1 (RL NLS1) collected to date, using data from the Wide-field Infrared Survey Explorer (WISE). We analyse the mid-IR colours of these objects and compare them to what is expected from different combinations of AGN and galaxy templates. We find that, in general, the host-galaxy emission gives an importan contribution to the observed mid-IR flux in particular at the longest wavelengths (W3, at 12micron, and W4, at 22micron). In about half of the sources (22 objects) we observe a very red mid-IR colour (W4-W3>2.5) that can be explained only using a starburst galaxy template (M82). Using the 22micron luminosities, corrected for the AGN contribution, we have then estimated the star-formation rate for 20 of these "red" RL NLS1, finding values ranging from 10 to 500 Msun/y. For the RL NLS1 showing bluer colours, instead, we cannot exclude the presence of a star-forming host galaxy although, on average, we ...

  20. The Central Kiloparsec of Seyfert and Inactive Host Galaxies: a Comparison of Two-Dimensional Stellar and Gaseous Kinematics

    E-Print Network [OSTI]

    Gaelle Dumas; Carole Mundell; Eric Emsellem; Neil Nagar

    2007-05-29T23:59:59.000Z

    We investigate the properties of the two-dimensional distribution and kinematics of ionised gas and stars in the central kiloparsecs of a matched sample of nearby active (Seyfert) and inactive galaxies, using the SAURON Integral Field Unit on the William Herschel Telescope. The ionised gas distributions show a range of low excitation regions such as star formation rings in Seyferts and inactive galaxies, and high excitation regions related to photoionisation by the AGN. The stellar kinematics of all galaxies in the sample show regular rotation patterns typical of disc-like systems, with kinematic axes which are well aligned with those derived from the outer photometry and which provide a reliable representation of the galactic line of nodes. After removal of the non-gravitational components due to e.g. AGN-driven outflows, the ionised gas kinematics in both the Seyfert and inactive galaxies are also dominated by rotation with global alignment between stars and gas in most galaxies. This result is consistent with previous findings from photometric studies that the large-scale light distribution of Seyfert hosts are similar to inactive hosts. However, fully exploiting the two-dimensional nature of our spectroscopic data, deviations from axisymmetric rotation in the gaseous velocity fields are identified that suggest the gaseous kinematics are more disturbed at small radii in the Seyfert galaxies compared with the inactive galaxies, providing a tentative link between nuclear gaseous streaming and nuclear activity.

  1. Critical importance of the de novo pyrimidine biosynthesis pathway for Trypanosoma cruzi growth in the mammalian host cell cytoplasm

    SciTech Connect (OSTI)

    Hashimoto, Muneaki, E-mail: muneaki@juntendo.ac.jp [Department of Molecular and Cellular Parasitology, Juntendo University School of Medicine, 2-1-1 Hongo, Bunkyo-ku, Tokyo 113-8421 (Japan)] [Department of Molecular and Cellular Parasitology, Juntendo University School of Medicine, 2-1-1 Hongo, Bunkyo-ku, Tokyo 113-8421 (Japan); Morales, Jorge; Fukai, Yoshihisa; Suzuki, Shigeo; Takamiya, Shinzaburo; Tsubouchi, Akiko; Inoue, Syou [Department of Molecular and Cellular Parasitology, Juntendo University School of Medicine, 2-1-1 Hongo, Bunkyo-ku, Tokyo 113-8421 (Japan)] [Department of Molecular and Cellular Parasitology, Juntendo University School of Medicine, 2-1-1 Hongo, Bunkyo-ku, Tokyo 113-8421 (Japan); Inoue, Masayuki [Graduate School of Pharmaceutical Sciences, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033 (Japan)] [Graduate School of Pharmaceutical Sciences, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033 (Japan); Kita, Kiyoshi [Department of Biomedical Chemistry, Graduate School of Medicine, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033 (Japan)] [Department of Biomedical Chemistry, Graduate School of Medicine, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033 (Japan); Harada, Shigeharu [Department of Applied Biology, Graduate School of Science and Technology, Kyoto Institute of Technology, Sakyo-ku, Kyoto 606-8585 (Japan)] [Department of Applied Biology, Graduate School of Science and Technology, Kyoto Institute of Technology, Sakyo-ku, Kyoto 606-8585 (Japan); Tanaka, Akiko [Systems and Structural Biology Center, RIKEN, Tsurumi, Yokohama 230-0045 (Japan)] [Systems and Structural Biology Center, RIKEN, Tsurumi, Yokohama 230-0045 (Japan); Aoki, Takashi [Department of Molecular and Cellular Parasitology, Juntendo University School of Medicine, 2-1-1 Hongo, Bunkyo-ku, Tokyo 113-8421 (Japan)] [Department of Molecular and Cellular Parasitology, Juntendo University School of Medicine, 2-1-1 Hongo, Bunkyo-ku, Tokyo 113-8421 (Japan); Nara, Takeshi, E-mail: tnara@juntendo.ac.jp [Department of Molecular and Cellular Parasitology, Juntendo University School of Medicine, 2-1-1 Hongo, Bunkyo-ku, Tokyo 113-8421 (Japan)] [Department of Molecular and Cellular Parasitology, Juntendo University School of Medicine, 2-1-1 Hongo, Bunkyo-ku, Tokyo 113-8421 (Japan)

    2012-01-20T23:59:59.000Z

    Highlights: Black-Right-Pointing-Pointer We established Trypanosoma cruzi lacking the gene for carbamoyl phosphate synthetase II. Black-Right-Pointing-Pointer Disruption of the cpsII gene significantly reduced the growth of epimastigotes. Black-Right-Pointing-Pointer In particular, the CPSII-null mutant severely retarded intracellular growth. Black-Right-Pointing-Pointer The de novo pyrimidine pathway is critical for the parasite growth in the host cell. -- Abstract: The intracellular parasitic protist Trypanosoma cruzi is the causative agent of Chagas disease in Latin America. In general, pyrimidine nucleotides are supplied by both de novo biosynthesis and salvage pathways. While epimastigotes-an insect form-possess both activities, amastigotes-an intracellular replicating form of T. cruzi-are unable to mediate the uptake of pyrimidine. However, the requirement of de novo pyrimidine biosynthesis for parasite growth and survival has not yet been elucidated. Carbamoyl-phosphate synthetase II (CPSII) is the first and rate-limiting enzyme of the de novo biosynthetic pathway, and increased CPSII activity is associated with the rapid proliferation of tumor cells. In the present study, we showed that disruption of the T. cruzicpsII gene significantly reduced parasite growth. In particular, the growth of amastigotes lacking the cpsII gene was severely suppressed. Thus, the de novo pyrimidine pathway is important for proliferation of T. cruzi in the host cell cytoplasm and represents a promising target for chemotherapy against Chagas disease.

  2. HOST GALAXIES, CLUSTERING, EDDINGTON RATIOS, AND EVOLUTION OF RADIO, X-RAY, AND INFRARED-SELECTED AGNs

    SciTech Connect (OSTI)

    Hickox, Ryan C.; Jones, Christine; Forman, William R.; Murray, Stephen S.; Brodwin, Mark; Narayan, Ramesh; Kenter, Almus; Caldwell, Nelson; Anderson, Michael E. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Kochanek, Christopher S. [Department of Astronomy and Center for Cosmology and Astroparticle Physics, Ohio State University, 140 West 18th Avenue, Columbus, OH 43210-1173 (United States); Eisenstein, Daniel [Steward Observatory, 933 North Cherry Avenue, Tucson, AZ 85721 (United States); Jannuzi, Buell T.; Dey, Arjun [National Optical Astronomy Observatory, Tucson, AZ 85726-6732 (United States); Brown, Michael J. I. [School of Physics, Monash University, Clayton 3800, Victoria (Australia); Stern, Daniel; Eisenhardt, Peter R.; Gorjian, Varoujan [Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109 (United States); Cool, Richard J. [Princeton University Observatory, Peyton Hall, Princeton, NJ 08544-1001 (United States)], E-mail: rhickox@cfa.harvard.edu

    2009-05-01T23:59:59.000Z

    We explore the connection between different classes of active galactic nuclei (AGNs) and the evolution of their host galaxies, by deriving host galaxy properties, clustering, and Eddington ratios of AGNs selected in the radio, X-ray, and infrared (IR) wavebands. We study a sample of 585 AGNs at 0.25 < z < 0.8 using redshifts from the AGN and Galaxy Evolution Survey (AGES). We select AGNs with observations in the radio at 1.4 GHz from the Westerbork Synthesis Radio Telescope, X-rays from the Chandra XBooetes Survey, and mid-IR from the Spitzer IRAC Shallow Survey. The radio, X-ray, and IR AGN samples show only modest overlap, indicating that to the flux limits of the survey, they represent largely distinct classes of AGNs. We derive host galaxy colors and luminosities, as well as Eddington ratios, for obscured or optically faint AGNs. We also measure the two-point cross-correlation between AGNs and galaxies on scales of 0.3-10 h {sup -1} Mpc, and derive typical dark matter halo masses. We find that: (1) radio AGNs are mainly found in luminous red sequence galaxies, are strongly clustered (with M {sub halo} {approx} 3 x 10{sup 13} h {sup -1} M {sub sun}), and have very low Eddington ratios {lambda} {approx}< 10{sup -3}; (2) X-ray-selected AGNs are preferentially found in galaxies that lie in the 'green valley' of color-magnitude space and are clustered similar to the typical AGES galaxies (M {sub halo} {approx} 10{sup 13} h {sup -1} M {sub sun}), with 10{sup -3} {approx}< {lambda} {approx}< 1; (3) IR AGNs reside in slightly bluer, slightly less luminous galaxies than X-ray AGNs, are weakly clustered (M {sub halo} {approx}< 10{sup 12} h {sup -1} M {sub sun}), and have {lambda}>10{sup -2}. We interpret these results in terms of a simple model of AGN and galaxy evolution, whereby a 'quasar' phase and the growth of the stellar bulge occurs when a galaxy's dark matter halo reaches a critical mass between {approx}10{sup 12} and 10{sup 13} M {sub sun}. After this event, star formation ceases and AGN accretion shifts from radiatively efficient (optical- and IR-bright) to radiatively inefficient (optically faint, radio-bright) modes.

  3. Host cells and methods for producing 3-methyl-2-buten-1-ol, 3-methyl-3-buten-1-ol, and 3-methyl-butan-1-ol

    DOE Patents [OSTI]

    Chou, Howard H. (Berkeley, CA); Keasling, Jay D. (Berkeley, CA)

    2011-07-26T23:59:59.000Z

    The invention provides for a method for producing a 5-carbon alcohol in a genetically modified host cell. In one embodiment, the method comprises culturing a genetically modified host cell which expresses a first enzyme capable of catalyzing the dephosphorylation of an isopentenyl pyrophosphate (IPP) or dimethylallyl diphosphate (DMAPP), such as a Bacillus subtilis phosphatase (YhfR), under a suitable condition so that 5-carbon alcohol is 3-methyl-2-buten-1-ol and/or 3-methyl-3-buten-1-ol is produced. Optionally, the host cell may further comprise a second enzyme capable of reducing a 3-methyl-2-buten-1-ol to 3-methyl-butan-1-ol, such as a reductase.

  4. Electrically Addressable Optical Devices Using A System Of Composite Layered Flakes Suspended In A Fluid Host To Obtain Angularly Depende

    DOE Patents [OSTI]

    Kosc, Tanya Z. (Rochester, NY); Marshall, Kenneth L. (Henrietta, NY); Jacobs, Stephen D. (Pittsford, NY)

    2004-12-07T23:59:59.000Z

    Composite or layered flakes having a plurality of layers of different materials, which may be dielectric materials, conductive materials, or liquid crystalline materials suspended in a fluid host and subjected to an electric field, provide optical effects dependent upon the angle or orientation of the flakes in the applied electric field. The optical effects depend upon the composition and thickness of the layers, producing reflectance, interference, additive and/or subtractive color effects. The composition of layered flakes may also be selected to enhance and/or alter the dielectric properties of flakes, whereby flake motion in an electric field is also enhanced and/or altered. The devices are useful as active electro-optical displays, polarizers, filters, light modulators, and wherever controllable polarizing, reflecting and transmissive optical properties are desired.

  5. A population of massive, luminous galaxies hosting heavily dust-obscured gamma-ray bursts: Implications for the use of GRBs as tracers of cosmic star formation

    SciTech Connect (OSTI)

    Perley, D. A. [Department of Astronomy, California Institute of Technology, MC 249-17, 1200 East California Blvd., Pasadena, CA 91125 (United States); Levan, A. J. [Department of Physics, University of Warwick, Coventry CV4 7AL (United Kingdom); Tanvir, N. R. [Department of Physics and Astronomy, University of Leicester, Leicester LE1 7RH (United Kingdom); Cenko, S. B.; Bloom, J. S.; Filippenko, A. V.; Morgan, A. N. [Department of Astronomy, University of California, Berkeley, CA 94720-3411 (United States); Hjorth, J.; Kr黨ler, T.; Fynbo, J. P. U.; Milvang-Jensen, B. [Dark Cosmology Centre, Niels Bohr Institute, Copenhagen (Denmark); Fruchter, A.; Kalirai, J. [Space Telescope Science Institute, Baltimore, MD 21218 (United States); Jakobsson, P. [Centre for Astrophysics and Cosmology, Science Institute, University of Iceland, Dunhagi 5, 107 Reykjav韐 (Iceland); Prochaska, J. X. [Department of Astronomy and Astrophysics, UCO/Lick Observatory, University of California, Santa Cruz, CA 95064 (United States); Silverman, J. M., E-mail: dperley@astro.caltech.edu [Department of Astronomy, University of Texas, Austin, TX 78712 (United States)

    2013-12-01T23:59:59.000Z

    We present observations and analysis of the host galaxies of 23 heavily dust-obscured gamma-ray bursts (GRBs) observed by the Swift satellite during the years 2005-2009, representing all GRBs with an unambiguous host-frame extinction of A{sub V} > 1 mag from this period. Deep observations with Keck, Gemini, Very Large Telescope, Hubble Space Telescope, and Spitzer successfully detect the host galaxies and establish spectroscopic or photometric redshifts for all 23 events, enabling us to provide measurements of the intrinsic host star formation rates, stellar masses, and mean extinctions. Compared to the hosts of unobscured GRBs at similar redshifts, we find that the hosts of dust-obscured GRBs are (on average) more massive by about an order of magnitude and also more rapidly star forming and dust obscured. While this demonstrates that GRBs populate all types of star-forming galaxies, including the most massive, luminous systems at z ? 2, at redshifts below 1.5 the overall GRB population continues to show a highly significant aversion to massive galaxies and a preference for low-mass systems relative to what would be expected given a purely star-formation-rate-selected galaxy sample. This supports the notion that the GRB rate is strongly dependent on metallicity, and may suggest that the most massive galaxies in the universe underwent a transition in their chemical properties ?9 Gyr ago. We also conclude that, based on the absence of unobscured GRBs in massive galaxies and the absence of obscured GRBs in low-mass galaxies, the dust distributions of the lowest-mass and the highest-mass galaxies are relatively homogeneous, while intermediate-mass galaxies (?10{sup 9} M {sub ?}) have diverse internal properties.

  6. The Genomes of the Fungal Plant Pathogens Cladosporium fulvum and Dothistroma septosporum Reveal Adaptation to Different Hosts and Lifestyles But Also Signatures of Common Ancestry

    SciTech Connect (OSTI)

    de Wit, Pierre J. G. M.; van der Burgt, Ate; Okmen, Bilal; Stergiopoulos, Ioannis; Abd-Elsalam, Kamel A.; Aerts, Andrea L.; Bahkali, Ali H.; Beenen, Henriek G.; Chettri, Oranav; Cos, Murray P.; Datema, Erwin; de Vries, Ronald P.; DHillon, Braham; Ganley, Austen R.; Griffiths, Scott A.; Guo, Yanan; Gamelin, Richard C.; Henrissat, Bernard; Kabir, M. Shahjahan; Jashni, Mansoor Karimi; Kema, Gert; Klaubauf, Sylvia; Lapidus, Alla; Levasseur, Anthony; Lindquist, Erika; Mehrabi, Rahim; Ohm, Robin A.; Owen, Timothy J.; Salamov, Asaf; Schwelm, Arne; Schijlen, Elio; Sun, Hui; van den Burg, Harrold A.; van Burg, Roeland C. H. J.; Zhang, Shuguang; Goodwin, Stephen B.; Grigoriev, Igor V.; Collemare, Jerome; Bradshaw, Rosie E.

    2012-05-04T23:59:59.000Z

    We sequenced and compared the genomes of the Dothideomycete fungal plant pathogens Cladosporium fulvum (Cfu) (syn. Passalora fulva) and Dothistroma septosporum (Dse) that are closely related phylogenetically, but have different lifestyles and hosts. Although both fungi grow extracellularly in close contact with host mesophyll cells, Cfu is a biotroph infecting tomato, while Dse is a hemibiotroph infecting pine. The genomes of these fungi have a similar set of genes (70percent of gene content in both genomes are homologs), but differ significantly in size (Cfu >61.1-Mb; Dse 31.2-Mb), which is mainly due to the difference in repeat content (47.2percent in Cfu versus 3.2percent in Dse). Recent adaptation to different lifestyles and hosts is suggested by diverged sets of genes. Cfu contains an tomatinase gene that we predict might be required for detoxification of tomatine, while this gene is absent in Dse. Many genes encoding secreted proteins are unique to each species and the repeat-rich areas in Cfu are enriched for these species-specific genes. In contrast, conserved genes suggest common host ancestry. Homologs of Cfu effector genes, including Ecp2 and Avr4, are present in Dse and induce a Cf-Ecp2- and Cf-4-mediated hypersensitive response, respectively. Strikingly, genes involved in production of the toxin dothistromin, a likely virulence factor for Dse, are conserved in Cfu, but their expression differs markedly with essentially no expression by Cfu in planta. Likewise, Cfu has a carbohydrate-degrading enzyme catalog that is more similar to that of necrotrophs or hemibiotrophs and a larger pectinolytic gene arsenal than Dse, but many of these genes are not expressed in planta or are pseudogenized. Overall, comparison of their genomes suggests that these closely related plant pathogens had a common ancestral host but since adapted to different hosts and lifestyles by a combination of differentiated gene content, pseudogenization, and gene regulation.

  7. QSO hosts and environments at z=0.9 to 4.2: JHK images with adaptive optics

    E-Print Network [OSTI]

    J. B. Hutchings; D. Crampton; S. L. Morris; D. Durand; E. Steinbring

    1998-12-08T23:59:59.000Z

    We have observed nine QSOs with redshifts 0.85 to 4.16 at near-IR wavelengths with the adaptive optics bonnette of the Canada-France-Hawaii telescope. Exposure times ranged from 1500 to 24000s (mostly near 7000s) in J, H, or K bands, with pixels 0.035 arcsec on the sky. The FWHM of the co-added images at the location of the quasars are typically 0.16 arcsec. Including another QSO published previously, we find associated QSO structure in at least eight of ten objects, including the QSO at z = 4.16. The structures seen in all cases include long faint features which appear to be tidal tails. In four cases we have also resolved the QSO host galaxy, but find them to be smooth and symmetrical: future PSF removal may expand this result. Including one object previously reported, of the nine objects with more extended structure, five are radio-loud, and all but one of these appear to be in a dense small group of compact galaxy companions. The radio-quiet objects do not occupy the same dense environments, as seen in the NIR. In this small sample we do not find any apparent trends of these properties with redshift, over the range 0.8 < z < 2.4. The colors of the host galaxies and companions are consistent with young stellar populations at the QSO redshift. Our observations suggest that adaptive optic observations in the visible region will exhibit luminous signatures of the substantial star-formation activity that must be occurring.

  8. The host outer membrane proteins OmpA and OmpC are associated with the Shigella phage Sf6 virion

    SciTech Connect (OSTI)

    Zhao Haiyan, E-mail: zhaohy@ku.ed [Department of Molecular Biosciences, University of Kansas, 1200 Sunnyside Avenue, Lawrence, KS 66045 (United States); Sequeira, Reuben D., E-mail: sequen@ku.ed [Department of Molecular Biosciences, University of Kansas, 1200 Sunnyside Avenue, Lawrence, KS 66045 (United States); Galeva, Nadezhda A., E-mail: galeva@ku.ed [Analytical Proteomics Laboratory, Structural Biology Center, University of Kansas, 2034 Becker Drive, Lawrence, KS 66047 (United States); Tang Liang, E-mail: tangl@ku.ed [Department of Molecular Biosciences, University of Kansas, 1200 Sunnyside Avenue, Lawrence, KS 66045 (United States)

    2011-01-20T23:59:59.000Z

    Assembly of dsDNA bacteriophage is a precisely programmed process. Potential roles of host cell components in phage assembly haven't been well understood. It was previously reported that two unidentified proteins were present in bacteriophage Sf6 virion (Casjens et al, 2004, J.Mol.Biol. 339, 379-394, Fig. 2A). Using tandem mass spectrometry, we have identified the two proteins as outer membrane proteins (OMPs) OmpA and OmpC from its host Shigella flexneri. The transmission electron cryo-microscopy structure of Sf6 shows significant density at specific sites at the phage capsid inner surface. This density fit well with the characteristic beta-barrel domains of OMPs, thus may be due to the two host proteins. Locations of this density suggest a role in Sf6 morphogenesis reminiscent of phage-encoded cementing proteins. These data indicate a new, OMP-related phage:host linkage, adding to previous knowledge that some lambdoid bacteriophage genomes contain OmpC-like genes that express phage-encoded porins in the lysogenic state.

  9. France gets nuclear fusion plant France will get to host the project to build a 10bn-euro (6.6bn) nuclear fusion reactor, in

    E-Print Network [OSTI]

    ) nuclear fusion reactor, in the face of strong competition from Japan. The International Thermonuclear division, which is responsible for the UK's thermonuclear fusion programme, said the decisionFrance gets nuclear fusion plant France will get to host the project to build a 10bn-euro (6.6bn

  10. Context-dependent protein folding of a virulence peptide in the bacterial and host environments: structure of an SycH朰opH chaperone杄ffector complex

    SciTech Connect (OSTI)

    Vujanac, Milos; Stebbins, C. Erec, E-mail: stebbins@rockefeller.edu [The Rockefeller University, New York, NY 10065 (United States)

    2013-04-01T23:59:59.000Z

    The structure of a SycH朰opH chaperone杄ffector complex from Yersinia reveals the bacterial state of a protein that adopts different folds in the host and pathogen environments. Yersinia pestis injects numerous bacterial proteins into host cells through an organic nanomachine called the type 3 secretion system. One such substrate is the tyrosine phosphatase YopH, which requires an interaction with a cognate chaperone in order to be effectively injected. Here, the first crystal structure of a SycH朰opH complex is reported, determined to 1.9 resolution. The structure reveals the presence of (i) a nonglobular polypeptide in YopH, (ii) a so-called ?-motif in YopH and (iii) a conserved hydrophobic patch in SycH that recognizes the ?-motif. Biochemical studies establish that the ?-motif is critical to the stability of this complex. Finally, since previous work has shown that the N-terminal portion of YopH adopts a globular fold that is functional in the host cell, aspects of how this polypeptide adopts radically different folds in the host and in the bacterial environments are analysed.

  11. South Africa is shortlisted to host a major scientific facility -the Square Kilometre Array (SKA). The SKA is a next-generation radio telescope

    E-Print Network [OSTI]

    Jarrett, Thomas H.

    South Africa is shortlisted to host a major scientific facility - the Square Kilometre Array (SKA instrument in a radio-quiet area in the arid Karoo region of South Africa's Northern Cape Province. Further the fron- tiers of science and technology, South Africa's SKA project attracts the brightest and most

  12. Influence of the host cell factors CK2, hTERT, and PML, on the antiviral response to herpes simplex virus type I infection

    E-Print Network [OSTI]

    Smith, Miles Christian

    2013-08-31T23:59:59.000Z

    deploys a variety of defenses to limit the extent to which the virus can replicate. This thesis is the summation of projects that examined the impact of three host cell factors - those being CK2, hTERT, and PML - on HSV-1 replication. CK2 is a cellular...

  13. Cheer Clinic The Oregon State Cheerleaders will be hosting a cheer clinics this winter, for kids ages 2-13. The clinic is limited to the first 150

    E-Print Network [OSTI]

    Escher, Christine

    Cheer Clinic The Oregon State Cheerleaders will be hosting a cheer clinics this winter, for kids ages 2-13. The clinic is limited to the first 150 participants that sign up. The clinic includes a t information call the Oregon State Marketing office at (541)737.1085. Jr. Cheer Clinic2008 Cheer Clinic Oregon

  14. The Puerto Rico Weather Camp 2013 is a summer experience hosted by the NOAA Center for Atmospheric Sciences at UPR Mayagez (UPRM) and co-sponsored by the

    E-Print Network [OSTI]

    Gilbes, Fernando

    The Puerto Rico Weather Camp 2013 is a summer experience hosted by the NOAA Center for Atmospheric forecasters and administrators, Emergency Management officers, and TV weather broadcasters. The Puerto Rico in the vicinity of La Parguera, Lajas (southwestern Puerto Rico). Applicants must be rising sophomore, junior

  15. The Puerto Rico Weather Camp 2012 is a summer experience hosted by the NOAA Center for Atmospheric Sciences at UPR Mayagez (UPRM) and co-sponsored by the

    E-Print Network [OSTI]

    Gilbes, Fernando

    The Puerto Rico Weather Camp 2012 is a summer experience hosted by the NOAA Center for Atmospheric forecasters and administrators, Emergency Management officers, and TV weather broadcasters. The Puerto Rico in the vicinity of La Parguera, Lajas (southwestern Puerto Rico). Applicants must be rising sophomore, junior

  16. Sea Level Rise Summit June 20-22 in Boca Raton FAU's Center for Environmental Studies within the Charles E. Schmidt College of Science will host a "Risk

    E-Print Network [OSTI]

    Fernandez, Eduardo

    Sea Level Rise Summit June 20-22 in Boca Raton FAU's Center for Environmental Studies within the Charles E. Schmidt College of Science will host a "Risk and Response: Sea Level Rise Summit" on Wednesday planning of agencies, institutions and civic society to sea level rise and compare the Florida situation

  17. Inelastic hosts as electrodes for high-capacity lithium-ion batteries Kejie Zhao, Matt Pharr, Joost J. Vlassak, and Zhigang Suoa

    E-Print Network [OSTI]

    in commercial lithium-ion batteries for both cathodes e.g., LiCoO2 and anodes e.g., graphite . By contrastInelastic hosts as electrodes for high-capacity lithium-ion batteries Kejie Zhao, Matt Pharr, Joost for high-capacity lithium-ion batteries. Upon absorbing lithium, silicon swells several times its volume

  18. Koizumi says Japan still hoping to host international nuclear fusion ... http://asia.news.yahoo.com/050614/ap/d8an68i81.html 1 of 2 6/14/05 7:48 AM

    E-Print Network [OSTI]

    Koizumi says Japan still hoping to host international nuclear fusion ... http-- New Yahoo! Asia News Search Yahoo! News advertisement Tuesday June 14, 12:59 PM Koizumi says Japan still hoping to host international nuclear fusion reactor Contentious negotiations between Japan

  19. 1 hour, 25 minutes ago Japan will ask the European Union to declare it a "joint host" of a revolutionary nuclear energy project even if the reactor is located in

    E-Print Network [OSTI]

    " of a revolutionary nuclear energy project even if the reactor is located in France, a newspaper said. The Nihon to 'joint host' revolutionary nuclear reactor 6/6/05 8:23 AMPrint Story: Japan to ask EU to 'joint host' revolutionary nuclear reactor on Yahoo! News Page 1 of 1http://news.yahoo.com/s/afp/20050606/sc

  20. DISCOVERY OF A 1.6 YEAR MAGNETIC ACTIVITY CYCLE IN THE EXOPLANET HOST STAR {iota} HOROLOGII

    SciTech Connect (OSTI)

    Metcalfe, T. S.; Judge, P. G.; Knoelker, M.; Mathur, S.; Rempel, M. [High Altitude Observatory, NCAR, P.O. Box 3000, Boulder, CO 80307 (United States); Basu, S. [Department of Astronomy, Yale University, P.O. Box 208101, New Haven, CT 06520 (United States); Henry, T. J. [Department of Physics and Astronomy, Georgia State University, Atlanta, GA 30302 (United States); Soderblom, D. R. [Space Telescope Science Institute, 3700 San Martin Dr., Baltimore, MD 21218 (United States)

    2010-11-10T23:59:59.000Z

    The Mount Wilson Ca HK survey revealed magnetic activity variations in a large sample of solar-type stars with timescales ranging from 2.5 to 25 years. This broad range of cycle periods is thought to reflect differences in the rotational properties and the depths of the surface convection zones for stars with various masses and ages. In 2007, we initiated a long-term monitoring campaign of Ca II H and K emission for a sample of 57 southern solar-type stars to measure their magnetic activity cycles and their rotational properties when possible. We report the discovery of a 1.6 year magnetic activity cycle in the exoplanet host star {iota} Horologii and obtain an estimate of the rotation period that is consistent with Hyades membership. This is the shortest activity cycle so far measured for a solar-type star and may be related to the short-timescale magnetic variations recently identified in the Sun and HD 49933 from helioseismic and asteroseismic measurements. Future asteroseismic observations of {iota} Hor can be compared to those obtained near the magnetic minimum in 2006 to search for cycle-induced shifts in the oscillation frequencies. If such short activity cycles are common in F stars, then NASA's Kepler mission should observe their effects in many of its long-term asteroseismic targets.

  1. An upper limit on the ratio between the Extreme Ultraviolet and the bolometric luminosities of stars hosting habitable planets

    E-Print Network [OSTI]

    Sengupta, Sujan

    2015-01-01T23:59:59.000Z

    A large number of terrestrial planets in the classical habitable zone of stars of different spectral types has already been discovered and many are expected to be discovered in near future. However, owing to the lack of knowledge on the atmospheric properties, the ambient environment of such planets are unknown. It is known that sufficient amount of Extreme Ultraviolet (EUV) radiation from the star can drive hydrodynamic outflow of hydrogen that may drag heavier species from the atmosphere of the planet. If the rate of mass loss is sufficiently high then substantial amount of volatiles would escape causing the planet to become uninhabitable. Considering energy-limited hydrodynamical mass loss with an escape rate that causes oxygen to escape along with hydrogen, I present an upper limit for the ratio between the EUV and the bolometric luminosities of stars which constrains the habitability of planets around them. Application of the limit to planet-hosting stars with known EUV luminosities implies that many M-t...

  2. The Effect of Host Star Spectral Energy Distribution and Ice-Albedo Feedback on the Climate of Extrasolar Planets

    E-Print Network [OSTI]

    Shields, Aomawa L; Bitz, Cecilia M; Pierrehumbert, Raymond T; Joshi, Manoj M; Robinson, Tyler D

    2013-01-01T23:59:59.000Z

    Planetary climate can be affected by the interaction of the host star spectral energy distribution with the wavelength-dependent reflectivity of ice and snow. Here we explore this effect using a one dimensional (1-D), line-by-line, radiative-transfer model to calculate broadband planetary albedos as input to a seasonally varying, 1-D energy-balance climate model. A three-dimensional general circulation model is also used to explore the atmosphere's response to changes in incoming stellar radiation, or instellation, and surface albedo. Using this hierarchy of models we simulate planets covered by ocean, land, and water ice of varying grain size, with incident radiation from stars of different spectral types. Terrestrial planets orbiting stars with higher near-UV radiation exhibit a stronger ice-albedo feedback. We find that ice-covered conditions occur on an F-dwarf planet with only a 2% reduction in instellation relative to the present instellation on Earth, assuming fixed CO2 (present atmospheric level on Ea...

  3. Electrically actuatable doped polymer flakes and electrically addressable optical devices using suspensions of doped polymer flakes in a fluid host

    DOE Patents [OSTI]

    Trajkovska-Petkoska, Anka; Jacobs, Stephen D.; Marshall, Kenneth L.; Kosc, Tanya Z.

    2010-05-11T23:59:59.000Z

    Doped electrically actuatable (electrically addressable or switchable) polymer flakes have enhanced and controllable electric field induced motion by virtue of doping a polymer material that functions as the base flake matrix with either a distribution of insoluble dopant particles or a dopant material that is completely soluble in the base flake matrix. The base flake matrix may be a polymer liquid crystal material, and the dopants generally have higher dielectric permittivity and/or conductivity than the electrically actuatable polymer base flake matrix. The dopant distribution within the base flake matrix may be either homogeneous or non-homogeneous. In the latter case, the non-homogeneous distribution of dopant provides a dielectric permittivity and/or conductivity gradient within the body of the flakes. The dopant can also be a carbon-containing material (either soluble or insoluble in the base flake matrix) that absorbs light so as to reduce the unpolarized scattered light component reflected from the flakes, thereby enhancing the effective intensity of circularly polarized light reflected from the flakes when the flakes are oriented into a light reflecting state. Electro-optic devices contain these doped flakes suspended in a host fluid can be addressed with an applied electric field, thus controlling the orientation of the flakes between a bright reflecting state and a non-reflecting dark state.

  4. Confirming HD 23478 as a new magnetic B star hosting an H$\\alpha$-bright centrifugal magnetosphere

    E-Print Network [OSTI]

    Sikora, James; Bohlender, David; Neiner, Coralie; Oksala, Mary; Shultz, Matt; Cohen, David; ud-Doula, Asif; Grunhut, Jason; Monin, Dmitry; Owocki, Stan; Petit, V閞onique; Rivinius, Thomas; Townsend, Richard

    2015-01-01T23:59:59.000Z

    In this paper we report 23 magnetic field measurements of the B3IV star HD 23478: 12 obtained from high resolution Stokes $V$ spectra using the ESPaDOnS (CFHT) and Narval (TBL) spectropolarimeters, and 11 from medium resolution Stokes $V$ spectra obtained with the DimaPol spectropolarimeter (DAO). HD 23478 was one of two rapidly rotating stars identified as potential "centrifugal magnetosphere" hosts based on IR observations from the Apache Point Observatory Galactic Evolution Experiment survey. We derive basic physical properties of this star including its mass ($M=6.1^{+0.8}_{-0.7}\\,M_\\odot$), effective temperature ($T_{\\rm eff}=20\\pm2\\,$kK), radius ($R=2.7^{+1.6}_{-0.9}\\,R_\\odot$), and age ($\\tau_{\\rm age}=3^{+37}_{-1}\\,$Myr). We repeatedly detect weakly-variable Zeeman signatures in metal, He and H lines in all our observations corresponding to a longitudinal magnetic field of $\\langle B_z\\rangle\\approx-2.0\\,$kG. The rotational period is inferred from Hipparcos photometry ($P_{\\rm rot}=1.0498(4)\\,$d). Und...

  5. Towards a Comprehensive Fueling-Controlled Theory on the Growth of Massive Black Holes and Host Spheroids

    E-Print Network [OSTI]

    Andres Escala

    2007-05-30T23:59:59.000Z

    We study the relation between nuclear massive black holes and their host spheroid gravitational potential. Using AMR numerical simulations, we analyze how gas is transported in the nuclear (central kpc) regions of galaxies. We study the gas fueling onto the inner accretion disk (sub-pc scale) and the star formation in a massive nuclear disk like those generally found in proto-spheroids (ULIRGs, SCUBA Galaxies). These sub-pc resolution simulation of gas fueling that is mainly depleted by star formation naturally satisfy the `M_BH - $M_virial' relation, with a scatter considerably less than the observed one. We found a generalized version of Kennicutt-Schmidt Law for starbursts is satisfied, in which the total gas depletion rate (dot{M}_gas = dot{M}_BH + dot{M}_SF) is the one that scales as M_gas/t_orbital. We also found that the `M_BH - sigma' relation is a byproduct of the `M_BH - M_virial' relation in the fueling controlled scenario.

  6. Membrane Protein Crystallization in Lipidic Mesophases. Hosting Lipid Effects on the Crystallization and Structure of a Transmembrane Peptide

    SciTech Connect (OSTI)

    Hfer, Nicole; Aragao, David; Lyons, Joseph A.; Caffrey, Martin (Trinity)

    2011-09-28T23:59:59.000Z

    Gramicidin is an apolar pentadecapeptide antibiotic consisting of alternating d- and l-amino acids. It functions, in part, by creating pores in membranes of susceptible cells rendering them leaky to monovalent cations. The peptide should be able to traverse the host membrane either as a double-stranded, intertwined double helix (DSDH) or as a head-to-head single-stranded helix (HHSH). Current structure models are based on macromolecular X-ray crystallography (MX) and nuclear magnetic resonance (NMR). However, the HHSH form has only been observed by NMR. The shape and size of the different gramicidin conformations differ. We speculated therefore that reconstituting it into a lipidic mesophase with bilayers of different microstructures would preferentially stabilize one form over the other. By using such mesophases for in meso crystallogenesis, the expectation was that at least one would generate crystals of gramicidin in the HHSH form for structure determination by MX. This was tested using commercial and in-house synthesized lipids that support in meso crystallogenesis. Lipid acyl chain lengths were varied from 14 to 18 carbons to provide mesophases with a range of bilayer thicknesses. Unexpectedly, all lipids produced high-quality, structure-grade crystals with gramicidin only in the DSDH conformation.

  7. SMB Host Processor Overhead

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    There are two benchmarks included here. The msgrate test measures the sustained MPI message rate using a communication pattern found in many real applications. For a complete...

  8. SMB Host Processor Overhead

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office of Scienceand Requirements RecentlyElectronicResourcesjobs RunningSEABRV2/01/12SMB SMB Description

  9. WIPP Hosts Stakeholder Workshop

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level:Energy: Grid Integration Redefining What'sis Taking Over OurThe Iron SpinPrincetonUsing Maps1 -VisualizingVoteFundingComputers GetFebruary15,

  10. Down-regulation of gibberellic acid in poplar has negligible effects on host-plant suitability and insect pest response

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Buhl, Christine; Strauss, Steven H.; Lindroth, Richard L.

    2015-02-01T23:59:59.000Z

    Abstract Endogenous levels and signaling of gibberellin plant hormones such as gibberellic acid (GA) have been genetically down-regulated to create semi-dwarf varieties of poplar. The potential benefits of semi-dwarf stature include reduced risk of wind damage, improved stress tolerance, and improved wood quality. Despite these benefits, modification of growth traits may have consequences for non-target traits that confer defense against insect herbivores. According to the growth-differentiation balance hypothesis, reductions in growth may shift allocation of carbon from growth to chemical resistance traits, thereby altering plant defense. To date, host-plant suitability and pest response have not been comprehensively evaluated in GA down-regulated plants. We quantified chemical resistance and nitrogen (an index of protein) in GA down-regulated and wild-type poplar (Populus alba P. tremula) genotypes. We also evaluated performance of both generalist (Lymantria dispar) and specialist (Chrysomela scripta) insect pests reared on these genotypes. Our evaluation of resistance traits in four GA down-regulated genotypes revealed increased phenolic glycosides in one modified genotype and reduced lignin in two modified genotypes relative to the non-transgenic wild type. Nitrogen levels did not vary significantly among the experimental genotypes. Generalists reared on the four GA down-regulated genotypes exhibited reduced performance on only one modified genotype relative to the wild type. Specialists, however, performed similarly across all genotypes. Results from this study indicate that although some non-target traits varied among GA down-regulated genotypes, the differences in poplar pest susceptibility were modest and highly genotype-specific.

  11. Down-regulation of gibberellic acid in poplar has negligible effects on host-plant suitability and insect pest response

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Buhl, Christine; Strauss, Steven H.; Lindroth, Richard L.

    2015-02-01T23:59:59.000Z

    Abstract Endogenous levels and signaling of gibberellin plant hormones such as gibberellic acid (GA) have been genetically down-regulated to create semi-dwarf varieties of poplar. The potential benefits of semi-dwarf stature include reduced risk of wind damage, improved stress tolerance, and improved wood quality. Despite these benefits, modification of growth traits may have consequences for non-target traits that confer defense against insect herbivores. According to the growth-differentiation balance hypothesis, reductions in growth may shift allocation of carbon from growth to chemical resistance traits, thereby altering plant defense. To date, host-plant suitability and pest response have not been comprehensively evaluated in GAmore牷down-regulated plants. We quantified chemical resistance and nitrogen (an index of protein) in GA down-regulated and wild-type poplar (Populus alba P. tremula) genotypes. We also evaluated performance of both generalist (Lymantria dispar) and specialist (Chrysomela scripta) insect pests reared on these genotypes. Our evaluation of resistance traits in four GA down-regulated genotypes revealed increased phenolic glycosides in one modified genotype and reduced lignin in two modified genotypes relative to the non-transgenic wild type. Nitrogen levels did not vary significantly among the experimental genotypes. Generalists reared on the four GA down-regulated genotypes exhibited reduced performance on only one modified genotype relative to the wild type. Specialists, however, performed similarly across all genotypes. Results from this study indicate that although some non-target traits varied among GA down-regulated genotypes, the differences in poplar pest susceptibility were modest and highly genotype-specific.珷less

  12. Determining the Dust Extinction of Gamma-ray Burst Host Galaxies: A Direct Method Based on Optical and X-ray Photometry

    E-Print Network [OSTI]

    Yuan Li; Aigen Li; Daming Wei

    2007-12-17T23:59:59.000Z

    The dust extinction of gamma-ray bursts (GRBs) host galaxies, containing important clues to the nature of GRB progenitors and crucial for dereddening, is still poorly known. Here we propose a straightforward method to determine the extinction of GRB host galaxies by comparing the observed optical spectra to the intrinsic ones extrapolated from the X-ray spectra. The rationale for this method is from the standard fireball model: if the optical flux decay index equals to that of the X-ray flux, then there is no break frequency between the optical and X-ray bands, therefore we can derive the intrinsic optical flux from the X-ray spectra. We apply this method to three GRBs of which the optical and X-ray fluxes have the same decay indices and another one with inferred cooling break frequency, and obtain the rest-frame extinction curves of their host galaxies. The derived extinction curves are gray and do not resemble any extinction curves of local galaxies (e.g. the Milk Way, the Small/Large Magellanic Clouds, or nearby starburst galaxies). The amount of extinction is rather large (with visual extinction $A_V$ $\\sim$ 1.6--3.4$\\magni$). We model the derived extinction curves in terms of the silicate-graphite interstellar grain model. As expected from the ``gray'' nature of the derived extinction curve, the dust size distribution is skewed to large grains. We determine, for the first time, the local dust-to-gas ratios of GRB host galaxies using the model-derived dust parameters and the hydrogen column densities determined from X-ray absorptions.

  13. Comparison of light out-coupling enhancements in single-layer blue-phosphorescent organic light emitting diodes using small-molecule or polymer hosts

    SciTech Connect (OSTI)

    Chang, Yung-Ting [Institute of Chemistry, Academia Sinica, Taipei, Taiwan 11529, Taiwan (China); Department of Electrical Engineering, Graduate Institute of Photonics and Optoelectronics, National Taiwan University, Taipei, Taiwan 10617, Taiwan (China); Liu, Shun-Wei [Department of Electronic Engineering, Mingchi University of Technology, New Taipei, Taiwan 24301, Taiwan (China); Yuan, Chih-Hsien; Lee, Chih-Chien [Department of Electronic Engineering, National Taiwan University of Science and Technology, Taipei, Taiwan 10607, Taiwan (China); Ho, Yu-Hsuan; Wei, Pei-Kuen [Research Center for Applied Science Academia Sinica, Taipei, Taiwan 11527, Taiwan (China); Chen, Kuan-Yu [Chilin Technology Co., LTD, Tainan City, Taiwan 71758, Taiwan (China); Lee, Yi-Ting; Wu, Min-Fei; Chen, Chin-Ti, E-mail: cchen@chem.sinica.edu.tw, E-mail: chihiwu@cc.ee.ntu.edu.tw [Institute of Chemistry, Academia Sinica, Taipei, Taiwan 11529, Taiwan (China); Wu, Chih-I, E-mail: cchen@chem.sinica.edu.tw, E-mail: chihiwu@cc.ee.ntu.edu.tw [Department of Electrical Engineering, Graduate Institute of Photonics and Optoelectronics, National Taiwan University, Taipei, Taiwan 10617, Taiwan (China)

    2013-11-07T23:59:59.000Z

    Single-layer blue phosphorescence organic light emitting diodes (OLEDs) with either small-molecule or polymer hosts are fabricated using solution process and the performances of devices with different hosts are investigated. The small-molecule device exhibits luminous efficiency of 14.7?cd/A and maximum power efficiency of 8.39?lm/W, which is the highest among blue phosphorescence OLEDs with single-layer solution process and small molecular hosts. Using the same solution process for all devices, comparison of light out-coupling enhancement, with brightness enhancement film (BEF), between small-molecule and polymer based OLEDs is realized. Due to different dipole orientation and anisotropic refractive index, polymer-based OLEDs would trap less light than small molecule-based OLEDs internally, about 37% better based simulation results. In spite of better electrical and spectroscopic characteristics, including ambipolar characteristics, higher carrier mobility, higher photoluminescence quantum yield, and larger triplet state energy, the overall light out-coupling efficiency of small molecule-based devices is worse than that of polymer-based devices without BEF. However, with BEF for light out-coupling enhancement, the improved ratio in luminous flux and luminous efficiency for small molecule based device is 1.64 and 1.57, respectively, which are significantly better than those of PVK (poly-9-vinylcarbazole) devices. In addition to the theoretical optical simulation, the experimental data also confirm the origins of differential light-outcoupling enhancement. The maximum luminous efficiency and power efficiency are enhanced from 14.7?cd/A and 8.39?lm/W to 23?cd/A and 13.2?lm/W, respectively, with laminated BEF, which are both the highest so far for single-layer solution-process blue phosphorescence OLEDs with small molecule hosts.

  14. Determination of mechanisms of host plant resistance to the Banks grass mite Oligonychus pratensis (Banks) (Acari: Tetranychidae) in selected maize inbreds

    E-Print Network [OSTI]

    Krakowsky, Matthew David

    1999-01-01T23:59:59.000Z

    on the host plant. Plexiglas cages (Archer et al 1997), small plastic cages snapped onto the leaves (Trichilo and Leigh, 1985), cages placed over the entire plant (Ruggle and Gutierrez, 1995), and detached leaves in petri dishes (Rodriguez, 1953, Mansour... the entire plant. Detached leaf culture presents the easiest method of containing mites on the substrate of interest and allowing for daily observation. Rodriguez (1953) used 2cm diameter leaf sections floating in a petri dish containing a sucrose solution...

  15. Type Ia Supernova Properties as a Function of the Distance to the Host Galaxy in the SDSS-II SN Survey

    SciTech Connect (OSTI)

    Galbany, Lluis [Institut de Fisica d'Altes Energies (IFAE), Barcelona (Spain); et al.

    2012-08-20T23:59:59.000Z

    We use type-Ia supernovae (SNe Ia) discovered by the SDSS-II SN Survey to search for dependencies between SN Ia properties and the projected distance to the host galaxy center, using the distance as a proxy for local galaxy properties (local star-formation rate, local metallicity, etc.). The sample consists of almost 200 spectroscopically or photometrically confirmed SNe Ia at redshifts below 0.25. The sample is split into two groups depending on the morphology of the host galaxy. We fit light-curves using both MLCS2k2 and SALT2, and determine color (AV, c) and light-curve shape (delta, x1) parameters for each SN Ia, as well as its residual in the Hubble diagram. We then correlate these parameters with both the physical and the normalized distances to the center of the host galaxy and look for trends in the mean values and scatters of these parameters with increasing distance. The most significant (at the 4-sigma level) finding is that the average fitted AV from MLCS2k2 and c from SALT2 decrease with the projected distance for SNe Ia in spiral galaxies. We also find indications that SNe in elliptical galaxies tend to have narrower light-curves if they explode at larger distances, although this may be due to selection effects in our sample. We do not find strong correlations between the residuals of the distance moduli with respect to the Hubble flow and the galactocentric distances, which indicates a limited correlation between SN magnitudes after standardization and local host metallicity.

  16. Determining the Dust Extinction of Gamma-ray Burst Host Galaxies: A Direct Method Based on Optical and X-ray Photometry

    E-Print Network [OSTI]

    Li, Yuan; Wei, Daming

    2007-01-01T23:59:59.000Z

    The dust extinction of gamma-ray bursts (GRBs) host galaxies, containing important clues to the nature of GRB progenitors and crucial for dereddening, is still poorly known. Here we propose a straightforward method to determine the extinction of GRB host galaxies by comparing the observed optical spectra to the intrinsic ones extrapolated from the X-ray spectra. The rationale for this method is from the standard fireball model: if the optical flux decay index equals to that of the X-ray flux, then there is no break frequency between the optical and X-ray bands, therefore we can derive the intrinsic optical flux from the X-ray spectra. We apply this method to three GRBs of which the optical and X-ray fluxes have the same decay indices and another one with inferred cooling break frequency, and obtain the rest-frame extinction curves of their host galaxies. The derived extinction curves are gray and do not resemble any extinction curves of local galaxies (e.g. the Milk Way, the Small/Large Magellanic Clouds, or ...

  17. On the nature of the z=0 X-ray absorbers: II. The contrast between local and AGN host galaxy absorption

    E-Print Network [OSTI]

    Rik J. Williams; Smita Mathur; Fabrizio Nicastro

    2007-09-24T23:59:59.000Z

    We search for highly-ionized gas near three AGN host galaxies using the Chandra low-energy transmission grating spectrograph. Strong absorption lines from such gas are seen at z=0, most likely from one or more of the following components: (1) a Galactic corona, (2) the Local Group medium, and (3) an extended warm-hot intergalactic medium (WHIM) filament passing through our local overdensity. Since AGNs reside within host galaxies that are also expected to sit within cosmically overdense regions, similar absorption resulting from these three components should appear at the AGN redshifts as well. However, no such absorption is seen. The lack of strong absorption lines is likely a result of the gas in these host galaxies and surrounding galaxy clusters being much hotter, and hence more highly ionized, than the gas in the Local Group+Galaxy system. We conclude that WHIM filaments produce no measurable absorption lines at the AGN redshifts, and therefore contribute at most a small fraction of the observed z=0 warm-hot gas.

  18. Regional Nuclear Workforce Development in the Central Savannah...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Nuclear Workforce Development in the Central Savannah River Area Dr. Susan A. Winsor Aiken Technical College President: P.O. Box 696, Aiken, SC 29802, winsors@atc.edu Mindy Mets...

  19. Bachelor of Fine Arts Lindsey Michelle Allen, Art

    E-Print Network [OSTI]

    Gering, Jon C.

    Bachelor of Fine Arts Lindsey Michelle Allen, Art Todd Christopher Baran, Art Mindy Lynnette Bryant Emily Dian Buford, Psychology Brennen Gail Bushnell, English Andrea Jeanne Calvin, English Erica Marie

  20. REPBLICA DE MOAMBIQUE CONSELHO NACIONAL DE COMBATE AO HIV/SIDA

    E-Print Network [OSTI]

    Klein, Ophir

    -Grasse, Willi McFarland, Mindy Hochgesang, Karen White, and Donald Whitson. For their participation, Leopoldina Ali, Rito Muzazila, Mauricio Santos, Kenneth Gimbel-Sherr, Annelien Groten. In addition

  1. DISCOVERY AND EARLY MULTI-WAVELENGTH MEASUREMENTS OF THE ENERGETIC TYPE IC SUPERNOVA PTF12GZK: A MASSIVE-STAR EXPLOSION IN A DWARF HOST GALAXY

    SciTech Connect (OSTI)

    Ben-Ami, Sagi; Gal-Yam, Avishay; Yaron, Ofer; Arcavi, Iair [Department of Particle Physics and Astrophysics, The Weizmann Institute of Science, Rehovot 76100 (Israel); Filippenko, Alexei V.; Cenko, S. Bradley [Department of Astronomy, University of California, Berkeley, CA 94720-3411 (United States); Mazzali, Paolo A. [INAF, Osservatorio Astronomico di Padova, Vicolo Osservatorio 5, I-35122 Padova (Italy); Modjaz, Maryam [New York University, Center for Cosmology and Particle Physics, Department of Physics, 4 Washington Place, New York, NY 10003 (United States); Horesh, Assaf; Kulkarni, Shrinivas R.; Perley, Daniel [Cahill Center for Astrophysics, California Institute of Technology, Pasadena, CA 91125 (United States); Howell, D. Andrew; Graham, Melissa L.; Sand, David J. [Las Cumbres Observatory Global Telescope Network, 6740 Cortona Drive, Suite 102, Santa Barbara, CA 93117 (United States); Horst, J. Chuck; Leonard, Douglas C. [Department of Astronomy, San Diego State University, San Diego, CA 92182 (United States); Im, Myunshin; Jeon, Yiseul [CEOU/Astronomy Program, Department of Physics and Astronomy, Seoul National University, Seoul (Korea, Republic of); Pian, Elena [Kavli Institute for Theoretical Physics, Kohn Hall, University of California, Santa Barbara, CA 93106-4030 (United States); Sullivan, Mark, E-mail: sagi.ben-ami@weizmann.ac.il [Department of Physics (Astrophysics), University of Oxford, DWB, Keble Road, Oxford, OX1 3RH (United Kingdom); and others

    2012-12-01T23:59:59.000Z

    We present the discovery and extensive early-time observations of the Type Ic supernova (SN) PTF12gzk. Our light curves show a rise of 0.8 mag within 2.5 hr. Power-law fits (f(t){proportional_to}(t - t{sub 0}) {sup n}) to these data constrain the explosion date to within one day. We cannot rule out a quadratic fireball model, but higher values of n are possible as well for larger areas in the fit parameter space. Our bolometric light curve and a dense spectral sequence are used to estimate the physical parameters of the exploding star and of the explosion. We show that the photometric evolution of PTF12gzk is slower than that of most SNe Ic. The high ejecta expansion velocities we measure ({approx}30, 000 km s{sup -1} derived from line minima four days after explosion) are similar to the observed velocities of broad-lined SNe Ic associated with gamma-ray bursts (GRBs) rather than to normal SN Ic velocities. Yet, this SN does not show the persistent broad lines that are typical of broad-lined SNe Ic. The host-galaxy characteristics are also consistent with GRB-SN hosts, and not with normal SN Ic hosts. By comparison with the spectroscopically similar SN 2004aw, we suggest that the observed properties of PTF12gzk indicate an initial progenitor mass of 25-35 M{sub Sun} and a large ((5-10) Multiplication-Sign 10{sup 51} erg) kinetic energy, the later being close to the regime of GRB-SN properties.

  2. Silicon and Nickel Enrichment in Planet-Host Stars: Observations and Implications for the Core-Accretion Theory of Planet Formation

    E-Print Network [OSTI]

    Sarah E. Robinson; Gregory Laughlin; Peter Bodenheimer; Debra Fischer

    2006-01-27T23:59:59.000Z

    We present evidence that stars with planets exhibit statistically significant silicon and nickel enrichment over the general metal-rich population. We also present simulations which predict silicon enhancement of planet hosts within the context of the core-accretion hypothesis for giant planet formation. Because silicon and oxygen are both alpha elements, [Si/Fe] traces [O/Fe], so the silicon enhancement in planet hosts predicts that these stars are oxygen-rich as well. We present new numerical simulations of planet formation by core accretion that establish the timescale on which a Jovian planet reaches rapid gas accretion, t_rga, as a function of solid surface density sigma_solid: (t_rga / 1 Myr) = (sigma_solid / 25.0 g cm^{-2})^{-1.44}. This relation enables us to construct Monte Carlo simulations that predict the fraction of star-disk systems that form planets as a function of [Fe/H], [Si/Fe], disk mass, outer disk radius and disk lifetime. Our simulations reproduce both the known planet-metallicity correlation and the planet-silicon correlation reported in this paper. The simulations predict that 16% of Solar-type stars form Jupiter-mass planets, in agreement with 12% predicted from extrapolation of the observed planet frequency-semimajor axis distribution. Although a simple interpretation of core accretion predicts that the planet-silicon correlation should be much stronger than the planet-nickel correlation, we observe the same degree of silicon and nickel enhancement in planet hosts. If this result persists once more planets have been discovered, it might indicate a complexity in the chemistry of planet formation beyond the simple accumulation of solids in the core accretion theory.

  3. Societal-Equity-Enhancing Criteria and Facility-Host Incentives Supporting Five Key Elements in the January 2012 Blue Ribbon Commission Report - 13015

    SciTech Connect (OSTI)

    Eriksson, Leif G. [Nuclear Waste Dispositions, 535 N. Interlachen Avenue, Unit 303, Winter Park, Florida 32789 (United States)] [Nuclear Waste Dispositions, 535 N. Interlachen Avenue, Unit 303, Winter Park, Florida 32789 (United States); Dials, George E. [B and W Conversion Services LLC, 1020 Monarch Road, Suite 300, Lexington, Kentucky 40513 (United States)] [B and W Conversion Services LLC, 1020 Monarch Road, Suite 300, Lexington, Kentucky 40513 (United States); George, Critz H. [Retired DOE and Consultant, 1218 Countryside Lane, Albuquerque, New Mexico, 87114 (United States)] [Retired DOE and Consultant, 1218 Countryside Lane, Albuquerque, New Mexico, 87114 (United States)

    2013-07-01T23:59:59.000Z

    In February 2009, the Obama Administration announced it would abandon USA's only candidate SNF/HLW-disposal facility since 1987. In 2010, all related activities were stopped and the Blue Ribbon Commission on America's Nuclear Future was established 'to recommend a new strategy for managing the back end of the nuclear fuel cycle', which it did in January 2012, emphasizing eight key elements. However, Key Element 1, 'A new, consent-based approach to siting future nuclear facilities', is qualitative/indeterminate rather than quantitative/measurable. It is thus highly-susceptible to semantic permutations that could extend rather than, as intended, expedite the siting of future nuclear facilities unless it also defines: a) Whose consent is needed?; and b) What constitutes consent? The following 'generic', radiation-risk- and societal-equity-based criteria address these questions: 1. Identify areas affected by projected radiation and other health risks from: a. The proposed nuclear facility (facility stakeholders); and b. The related nuclear-materials-transportation routes (transportation stakeholders); then 2. Surround each stakeholder area with a buffer zone and use this enlarged foot print to identify: a. Stakeholder hosts; and b. Areas not hosting any stakeholder category (interested parties). 3. Define 'consent-based' as being at least 60 percent of the 'population' in the respective stakeholder category and apply this yardstick to both 'in favor' and 'against' votes. Although criteria 1 and 2 also need facility-based definitions to make Key Element 1 measurable, the described siting approach, augmented by related facility-host incentives, would expedite the schedule and reduce the cost for achieving Key Elements 4-6 and 8, politics permitting. (authors)

  4. Optical amplifier operating at 1.3 microns useful for telecommunications and based on dysprosium-doped metal chloride host materials

    DOE Patents [OSTI]

    Page, R.H.; Schaffers, K.I.; Payne, S.A.; Krupke, W.F.; Beach, R.J.

    1997-12-02T23:59:59.000Z

    Dysprosium-doped metal chloride materials offer laser properties advantageous for use as optical amplifiers in the 1.3 {micro}m telecommunications fiber optic network. The upper laser level is characterized by a millisecond lifetime, the host material possesses a moderately low refractive index, and the gain peak occurs near 1.31 {micro}m. Related halide materials, including bromides and iodides, are also useful. The Dy{sup 3+}-doped metal chlorides can be pumped with laser diodes and yield 1.3 {micro}m signal gain levels significantly beyond those currently available. 9 figs.

  5. Optical amplifier operating at 1.3 microns useful for telecommunications and based on dysprosium-doped metal chloride host materials

    DOE Patents [OSTI]

    Page, Ralph H. (San Ramon, CA); Schaffers, Kathleen I. (Pleasanton, CA); Payne, Stephen A. (Castro Valley, CA); Krupke, William F. (Pleasanton, CA); Beach, Raymond J. (Livermore, CA)

    1997-01-01T23:59:59.000Z

    Dysprosium-doped metal chloride materials offer laser properties advantageous for use as optical amplifiers in the 1.3 .mu.m telecommunications fiber optic network. The upper laser level is characterized by a millisecond lifetime, the host material possesses a moderately low refractive index, and the gain peak occurs near 1.31 .mu.m. Related halide materials, including bromides and iodides, are also useful. The Dy.sup.3+ -doped metal chlorides can be pumped with laser diodes and yield 1.3 .mu.m signal gain levels significantly beyond those currently available.

  6. Plasmids in the driving seat: The regulatory RNA Rcd gives plasmid ColE1 control over division and growth of its E. coli host

    E-Print Network [OSTI]

    Gaimster, Hannah; Summers, David

    2014-11-11T23:59:59.000Z

    al., 1993; Colloms et al., 1990; Stirling et al., 1988, 1989; Summers and Sherratt, 1984). The plasmid and host cooperate in this process because, although the cer recom- bination site is of necessity on the plasmid, four essential proteins (XerC, Xer... ) ???? Stirling, C.J., et al., 1988. The arginine repressor is essential for plasmid stabilizing site-specific recombination at the ColE1 cer locus. EMBO J. 7, 43894395. Stirling, C.J., et al., 1989. xerB, an Escherichia coli gene required for plasmid ColE1 site...

  7. CHARACTERIZING THE COOL KEPLER OBJECTS OF INTERESTS. NEW EFFECTIVE TEMPERATURES, METALLICITIES, MASSES, AND RADII OF LOW-MASS KEPLER PLANET-CANDIDATE HOST STARS

    SciTech Connect (OSTI)

    Muirhead, Philip S. [Current address: Department of Astronomy, California Institute of Technology, 1200 East California Boulevard, MC 249-17, Pasadena, CA 91125 (United States); Hamren, Katherine [Current address: Department of Astronomy and Astrophysics, University of California Santa Cruz, 1156 High Street, Santa Cruz, CA 95064 (United States); Schlawin, Everett; Lloyd, James P. [Department of Astronomy, Cornell University, 122 Sciences Drive, Ithaca, NY 14853 (United States); Rojas-Ayala, Barbara [Current address: Department of Astrophysics, American Museum of Natural History, Central Park West at 79th Street, New York, NY 10024 (United States); Covey, Kevin R., E-mail: philm@astro.caltech.edu [Hubble Fellow. (United States)

    2012-05-10T23:59:59.000Z

    We report stellar parameters for late-K and M-type planet-candidate host stars announced by the Kepler Mission. We obtained medium-resolution, K-band spectra of 84 cool (T{sub eff} {approx}< 4400 K) Kepler Objects of Interest (KOIs) from Borucki et al. We identified one object as a giant (KOI 977); for the remaining dwarfs, we measured effective temperatures (T{sub eff}) and metallicities [M/H] using the K-band spectral indices of Rojas-Ayala et al. We determine the masses (M{sub *}) and radii (R{sub *}) of the cool KOIs by interpolation onto the Dartmouth evolutionary isochrones. The resultant stellar radii are significantly less than the values reported in the Kepler Input Catalog and, by construction, correlate better with T{sub eff}. Applying the published KOI transit parameters to our stellar radius measurements, we report new physical radii for the planet candidates. Recalculating the equilibrium temperatures of the planet-candidates assuming Earth's albedo and re-radiation fraction, we find that three of the planet-candidates are terrestrial sized with orbital semimajor axes that lie within the habitable zones of their host stars (KOI 463.01, KOI 812.03, and KOI 854.01). The stellar parameters presented in this Letter serve as a resource for prioritization of future follow-up efforts to validate and characterize the cool KOI planet candidates.

  8. Know The Star, Know the Planet. IV. A Stellar Companion to the Host star of the Eccentric Exoplanet HD 8673b

    E-Print Network [OSTI]

    Roberts,, Lewis C; Neyman, Christopher R; Wu, Yanqin; Riddle, Reed L; Shelton, J Christopher; Angione, John; Baranec, Christoph; Bouchez, Antonin; Bui, Khanh; Burruss, Rick; Burse, Mahesh; Chordia, Pravin; Croner, Ernest; Das, Hillol; Dekany, Richard G; Guiwits, Stephen; Hale, David; Henning, John; Law, Shrinivas Kulkarni Nicholas; McKenna, Dan; Milburn, Jennifer; Palmer, Dean; Punnadi, Sujit; Ramaprakash, A N; Roberts, Jennifer E; Tendulkar, Shriharsh P; Trinh, Thang; Troy, Mitchell; Truong, Tuan; Zolkower, Jeff

    2015-01-01T23:59:59.000Z

    HD 8673 hosts a massive exoplanet in a highly eccentric orbit (e=0.723). Based on two epochs of speckle interferometry a previous publication identi?ed a candidate stellar companion. We observed HD 8673 multiple times with the 10 m Keck II telescope, the 5 m Hale telescope, the 3.63 m AEOS telescope and the 1.5m Palomar telescope in a variety of ?lters with the aim of con?rming and characterizing the stellar companion. We did not detect the candidate companion, which we now conclude was a false detection, but we did detect a fainter companion. We collected astrometry and photometry of the companion on six epochs in a variety of ?lters. The measured di?erential photometry enabled us to determine that the companion is an early M dwarf with a mass estimate of 0.33-0.45 M?. The companion has a projected separation of 10 AU, which is one of the smallest projected separations of an exoplanet host binary system. Based on the limited astrometry collected, we are able to constrain the orbit of the stellar companion to...

  9. ALMA DETECTION OF THE VIBRATIONALLY EXCITED HCN J = 4-3 EMISSION LINE IN THE AGN-HOSTING LUMINOUS INFRARED GALAXY IRAS 205514250

    SciTech Connect (OSTI)

    Imanishi, Masatoshi [Subaru Telescope, 650 North A'ohoku Place, Hilo, Hawaii, 96720 (United States); Nakanishi, Kouichiro, E-mail: masa.imanishi@nao.ac.jp [Joint ALMA Observatory, Alonso de C髍dova 3107, Vitacura 763-0355, Santiago de Chile (Chile)

    2013-10-01T23:59:59.000Z

    We present results from our ALMA Cycle 0 observations, at the frequencies around the HCN, HCO{sup +}, and HNC J = 4-3 transition lines, of the luminous infrared galaxy IRAS 205514250 at z = 0.043, which is known to host an energetically important obscured active galactic nucleus (AGN). In addition to the targeted HCN, HCO{sup +}, and HNC J = 4-3 emission lines, two additional strong emission lines are seen, which we attribute to H{sub 2}S and CH{sub 3}CN(+CCH). The HCN-to-HCO{sup +} J = 4-3 flux ratio (?0.7) is higher than in the other starburst-dominated galaxy (?0.2) observed in our ALMA Cycle 0 program. We tentatively (?5?) detected the vibrationally excited (v {sub 2} = 1) HCN J = 4-3 (l = 1f) emission line, which is important for testing an infrared radiative pumping scenario for HCN. This is the second detection of this molecular transition in external galaxies. The most likely reason for this detection is not only the high flux of this emission line, but also the small molecular line widths observed in this galaxy, suggesting that vibrational excitation of HCN may be relatively common in AGN-hosting galaxies.

  10. GALAXY ZOO: THE FUNDAMENTALLY DIFFERENT CO-EVOLUTION OF SUPERMASSIVE BLACK HOLES AND THEIR EARLY- AND LATE-TYPE HOST GALAXIES

    SciTech Connect (OSTI)

    Schawinski, Kevin; Urry, C. Megan [Department of Physics, Yale University, New Haven, CT 06511 (United States); Virani, Shanil; Coppi, Paolo; Cardamone, Carolin N. [Yale Center for Astronomy and Astrophysics, Yale University, P.O. Box 208121, New Haven, CT 06520 (United States); Bamford, Steven P. [Centre for Astronomy and Particle Theory, University of Nottingham, University Park, Nottingham, NG7 2RD (United Kingdom); Treister, Ezequiel [Institute for Astronomy, 2680 Woodlawn Drive, University of Hawaii, Honolulu, HI 96822 (United States); Lintott, Chris J.; Kaviraj, Sugata [Department of Physics, University of Oxford, Keble Road, Oxford, OX1 3RH (United Kingdom); Sarzi, Marc [Centre for Astrophysics Research, University of Hertfordshire, College Lane, Hatfield, Herts AL10 9AB (United Kingdom); Keel, William C. [Department of Physics and Astronomy, 206 Gallalee Hall, 514 University Blvd., University of Alabama, Tuscaloosa, AL 35487-0324 (United States); Masters, Karen L.; Nichol, Robert C.; Thomas, Daniel [Institute of Cosmology and Gravitation, University of Portsmouth, Mercantile House, Hampshire Terrace, Portsmouth, PO1 2EG (United Kingdom); Ross, Nicholas P. [Department of Astronomy and Astrophysics, 525 Davey Laboratory, Pennsylvania State University, University Park, PA 16802 (United States); Andreescu, Dan [LinkLab, 4506 Graystone Avenue, Bronx, NY 10471 (United States); Murray, Phil [Fingerprint Digital Media, 9 Victoria Close, Newtownards, Co. Down, Northern Ireland, BT23 7GY (United Kingdom); Raddick, M. Jordan; Szalay, Alex S. [Department of Physics and Astronomy, Johns Hopkins University, Homewood Campus, Baltimore, MD 21218 (United States); Slosar, Anze, E-mail: kevin.schawinski@yale.ed [Berkeley Center for Cosmological Physics, Lawrence Berkeley National Laboratory and Physics Department, University of California, Berkeley, CA 94720 (United States)

    2010-03-01T23:59:59.000Z

    We use data from the Sloan Digital Sky Survey and visual classifications of morphology from the Galaxy Zoo project to study black hole growth in the nearby universe (z < 0.05) and to break down the active galactic nucleus (AGN) host galaxy population by color, stellar mass, and morphology. We find that the black hole growth at luminosities L[O{sub III}]>10{sup 40} erg s{sup -1} in early- and late-type galaxies is fundamentally different. AGN host galaxies as a population have a broad range of stellar masses (10{sup 10}-10{sup 11} M{sub sun}), reside in the green valley of the color-mass diagram and their central black holes have median masses around 10{sup 6.5} M{sub sun}. However, by comparing early- and late-type AGN host galaxies to their non-active counterparts, we find several key differences: in early-type galaxies, it is preferentially the galaxies with the least massive black holes that are growing, while in late-type galaxies, it is preferentially the most massive black holes that are growing. The duty cycle of AGNs in early-type galaxies is strongly peaked in the green valley below the low-mass end (10{sup 10} M{sub sun}) of the red sequence at stellar masses where there is a steady supply of blue cloud progenitors. The duty cycle of AGNs in late-type galaxies on the other hand peaks in massive (10{sup 11} M{sub sun}) green and red late-types which generally do not have a corresponding blue cloud population of similar mass. At high-Eddington ratios (L/L{sub Edd}>0.1), the only population with a substantial fraction of AGNs are the low-mass green valley early-type galaxies. Finally, the Milky Way likely resides in the 'sweet spot' on the color-mass diagram where the AGN duty cycle of late-type galaxies is highest. We discuss the implications of these results for our understanding of the role of AGNs in the evolution of galaxies.

  11. Optical devices having flakes suspended in a host fluid to provide a flake/fluid system providing flakes with angularly dependent optical properties in response to an alternating current electric field due to the dielectric properties of the system

    DOE Patents [OSTI]

    Kosc, Tanya Z. (Rochester, NY); Marshall, Kenneth L. (Rochester, NY); Jacobs, Stephen D. (Pittsford, NY)

    2006-05-09T23:59:59.000Z

    Optical devices utilizing flakes (also called platelets) suspended in a host fluid have optical characteristics, such as reflective properties, which are angular dependent in response to an AC field. The reflectivity may be Bragg-like, and the characteristics are obtained through the use of flakes of liquid crystal material, such as polymer liquid crystal (PLC) materials including polymer cholesteric liquid crystal (PCLC) and polymer nematic liquid crystal (PNLC) material or birefringent polymers (BP). The host fluid may be propylene carbonate, poly(ethylene glycol) or other fluids or fluid mixtures having fluid conductivity to support conductivity in the flake/host system. AC field dependent rotation of 90.degree. can be obtained at rates and field intensities dependent upon the frequency and magnitude of the AC field. The devices are useful in providing displays, polarizers, filters, spatial light modulators and wherever switchable polarizing, reflecting, and transmission properties are desired.

  12. Interaction of Close-in Planets with the Magnetosphere of their Host Stars I: Diffusion, Ohmic Dissipation of Time Dependent Field, Planetary Inflation, and Mass Loss

    E-Print Network [OSTI]

    Randy O. Laine; Douglas N. C. Lin; Shawfeng Dong

    2008-04-07T23:59:59.000Z

    The unanticipated discovery of the first close-in planet around 51 Peg has rekindled the notion that shortly after their formation outside the snow line, some planets may have migrated to the proximity of their host stars because of their tidal interaction with their nascent disks. If these planets indeed migrated to their present-day location, their survival would require a halting mechanism in the proximity of their host stars. Most T Tauri stars have strong magnetic fields which can clear out a cavity in the innermost regions of their circumstellar disks and impose magnetic induction on the nearby young planets. Here we consider the possibility that a magnetic coupling between young stars and planets could quench the planet's orbital evolution. After a brief discussion of the complexity of the full problem, we focus our discussion on evaluating the permeation and ohmic dissipation of the time dependent component of the stellar magnetic field in the planet's interior. Adopting a model first introduced by C. G. Campbell for interacting binary stars, we determine the modulation of the planetary response to the tilted magnetic field of a non-synchronously spinning star. We first compute the conductivity in the young planets, which indicates that the stellar field can penetrate well into the planet's envelope in a synodic period. For various orbital configurations, we show that the energy dissipation rate inside the planet is sufficient to induce short-period planets to inflate. This process results in mass loss via Roche lobe overflow and in the halting of the planet's orbital migration.

  13. LDP lawmakers to ask Koizumi to show resolve to host fusion reactor http://asia.news.yahoo.com/050317/kyodo/d88shocg0.html 1 of 2 3/17/05 5:11 AM

    E-Print Network [OSTI]

    's interest in hosting the world's first nuclear fusion reactor. The ruling party lawmakers reached six parties, expected to be a major focus. Tadamori Oshima, a former agriculture, forestry, is the latest stage in a decade-long quest to develop nuclear fusion power since the plan emerged during a 1985

  14. As part of its continuing cloud computing series, the National Institute of Standards and Technology is hosting a new forum on Cloud and Mobility. Join experts in the fields of cloud, mobility, and measurement for thought-provoking

    E-Print Network [OSTI]

    and Technology is hosting a new forum on Cloud and Mobility. Join experts in the fields of cloud, mobility sessions, and networking. New Frontiers in IT and Measurement Science Rapid advances in mobile cloud computing are bringing sweeping changes to the way mobile computing and communication services are delivered

  15. This is an electronic version of the article published as Napoleon, M.E. and King, B.H. 1999. Offspring sex ratio response to host size in the parasitoid wasp

    E-Print Network [OSTI]

    King, Bethia H.

    29 This is an electronic version of the article published as Napoleon, M.E. and King, B.H. 1999 response to host size in the parasitoid wasp Spalangia endius M. E. Napoleon1 and B. H. King M.E. Napoleon1

  16. Geochemistry of the Banded Iron Formations and their Host Rocks in the Eastern Desert of Egypt BACKUS, Ethan L.1, GAGNON, Kelli E.1, EL-SHAZLY, Aley K.1, and KHALIL, Khalil Isaac2

    E-Print Network [OSTI]

    El-Shazly, Aley

    Geochemistry of the Banded Iron Formations and their Host Rocks in the Eastern Desert of Egypt University, Egypt Sponsored by NSF-OISE-1004021 Session 92:T3. Sigma Gamma Epsilon Undergraduate Research over 30,000 km2 in the central Eastern Desert of Egypt. The deposits most resemble Algoma-type iron

  17. Photoluminescence properties of rare earths (Eu{sup 3+}, Tb{sup 3+}, Dy{sup 3+} and Tm{sup 3+}) activated NaInW{sub 2}O{sub 8} wolframite host lattice

    SciTech Connect (OSTI)

    Asiri Naidu, S.; Boudin, S. [Laboratoire de Cristallographie et Sciences des Materiaux, ENSICAEN, Universite de Caen, CNRS, 6 Bd Marechal Juin, F-14050 Caen (France); Varadaraju, U.V. [Department of Chemistry, Indian Institute of Technology Madras, Chennai 600036 (India); Raveau, B., E-mail: bernard.raveau@ensicaen.fr [Laboratoire de Cristallographie et Sciences des Materiaux, ENSICAEN, Universite de Caen, CNRS, 6 Bd Marechal Juin, F-14050 Caen (France)

    2012-01-15T23:59:59.000Z

    The photoluminescence (PL) studies on NaIn{sub 1-x}RE{sub x}W{sub 2}O{sub 8}, with RE=Eu{sup 3+}, Tb{sup 3+}, Dy{sup 3+} and Tm{sup 3+} phases have shown that the relative contribution of the host lattice and of the intra-f-f emission of the activators to the PL varies with the nature of the rare earth cation. In the case of Dy{sup 3+} and Tm{sup 3+} activators, with yellow and blue emission, respectively, the energy transfer from host to the activator plays a major role. In contrast for Eu{sup 3+}, with intense red emission, the host absorption is less pronounced and the intra-f-f transitions of the Eu{sup 3+} ions play a major role, whereas for Tb{sup 3+} intra-f-f transitions are only observed, giving rise to green emission. - Graphical abstract: NaInW{sub 2}O{sub 8} double tungstate doped with Eu{sup 3+}, Dy{sup 3+}, Tb{sup 3+}and Tm{sup 3+} shows characteristic emission of intense red for Eu{sup 3+}, yellow for Dy{sup 3+}, green for Tb{sup 3+} and blue for Tm{sup 3+}. Highlights: Black-Right-Pointing-Pointer Characteristic emissions of rare earths (Eu{sup 3+}, Tb{sup 3+}, Dy{sup 3+} and Tm{sup 3+}) are observed NaInW{sub 2}O{sub 8} wolframite. Black-Right-Pointing-Pointer Energy transfer from host to the activators (Eu{sup 3+} Dy{sup 3+} Tm{sup 3+} is observed. Black-Right-Pointing-Pointer PL properties of rare earth ions depend on minor structural variations in the host lattice.

  18. 16-12-12Web Archiv e (naf wa.org)-Hosted By Hurricane Electric -Resurrection Of Ex... 1/3naf wa.org/.../11052-resurrection-of -extinct-enzy mes-rev eals-ev olutionary -strategy -f or-the-inv enti...

    E-Print Network [OSTI]

    16-12-12Web Archiv e (naf wa.org)-Hosted By Hurricane Electric - Resurrection Of Ex... 1/3naf wa Archiv e (naf wa.org)-Hosted By Hurricane Electric - Resurrection Of Ex... naf wa.org/.../11052

  19. Cosmic Evolution of Black Holes and Spheroids. V. The Relation Between Black Hole Mass and Host Galaxy Luminosity for a Sample of 79 Active Galaxies

    E-Print Network [OSTI]

    Park, Daeseong; Bennert, Vardha N; Treu, Tommaso; Auger, Matthew W; Malkan, Matthew A

    2014-01-01T23:59:59.000Z

    We investigate the cosmic evolution of the black hole (BH) mass -- bulge luminosity relation using a sample of 52 active galaxies at $z \\sim 0.36$ and $z \\sim 0.57$ in the BH mass range of $10^{7.4-9.1} M_{\\odot}$. By consistently applying multi-component spectral and structural decomposition to high-quality Keck spectra and high-resolution HST images, BH masses ($M_{\\rm BH}$) are estimated using the H$\\beta$ broad emission line combined with the 5100 \\AA\\ nuclear luminosity, and bulge luminosities ($L_{\\rm bul}$) are derived from surface photometry. Comparing the resulting $M_{\\rm BH}-L_{\\rm bul}$ relation to local active galaxies and taking into account selection effects, we find evolution of the form $M_{\\rm BH} / L_{\\rm bul} \\propto (1+z)^{\\gamma}$ with $\\gamma=1.8\\pm0.7$, consistent with BH growth preceding that of the host galaxies. Including an additional sample of 27 active galaxies with $0.5

  20. Discrimination between energy transfer and back transfer processes for GaAs host and Er luminescent dopants using electric response analysis

    SciTech Connect (OSTI)

    Ishii, Masashi, E-mail: ISHII.Masashi@nims.go.jp [National Institute for Materials Science (NIMS), Tsukuba, Ibaraki 305-0047 (Japan); Koizumi, Atsushi; Fujiwara, Yasufumi [Division of Materials and Manufacturing Science, Graduate School of Engineering Osaka University, Suita, Osaka 565-0871 (Japan); Takeda, Yoshikazu [Nagoya Industrial Science Research Institute, Nagoya, Aichi 464-0819 (Japan)

    2014-04-07T23:59:59.000Z

    The energy transfer and back transfer processes of GaAs co-doped with Er and O (GaAs:Er,O) were experimentally distinguished by using a frequency response analysis of the AC photocurrent. The results were achieved by using the difference in the frequency dispersion between (1) the dispersion of the energy transfer, which is triggered by the trapping of free charges in the GaAs host and is represented with the Debye relaxation response and (2) the dispersion of the energy back transfer, which is induced by non-radiative transition of 4f bound electrons in the Er dopants and is described with a Lorentzian. The Debye relaxation response found in GaAs:Er,O provided a charge trapping time that was dependent on temperature, which was well correlated with the thermal quenching property of intense intra-4f-shell luminescence. The spectral shape of the Lorentzian dependence on the temperature was explained with the thermal excitation of Er 4f electrons and release of trapped charges in GaAs. The thermal excitation and release of charges consistently explained the characteristics of weak 4f luminescence in low- and high-temperature regions, respectively.

  1. The Tip of the Red Giant Branch Distances to Type Ia Supernova Host Galaxies. III. NGC 4038/39 and NGC 5584

    E-Print Network [OSTI]

    Jang, In Sung

    2015-01-01T23:59:59.000Z

    We present the tip of the red giant branch (TRGB) distances to Type Ia supernova (SNe Ia) host galaxies NGC 4038/39 and NGC 5584. Based on the deep images constructed using archival Hubble Space Telescope data, we detect red giant branch stars in each galaxy. VI photometry of the resolved stars and corresponding I-band luminosity functions show the TRGB to be at I_{TRGB} = 27.67 \\pm 0.05 for NGC 4038/39 and I_{TRGB} = 27.77 \\pm 0.04 for NGC 5584. From these estimates, we determine the distance modulus to NGC 4038/39 to be (m-M)_0 = 31.67 \\pm 0.05 (random) \\pm 0.12 (systematic) (corresponding to a linear distance of 21.58 \\pm 0.50 \\pm 1.19 Mpc) and the distance modulus to NGC 5584 to be (m-M)_0 = 31.76 \\pm 0.04 (random) \\pm 0.12 (systematic) (corresponding to a linear distance of 22.49 \\pm 0.41 \\pm 1.24 Mpc). We derive a mean absolute maximum magnitude of SNe Ia of M_V = -19.29 \\pm 0.08 from the distance estimates of five SNe Ia (including two SNe in this study and three SNe Ia from our previous studies), and ...

  2. NAVY PRECISION OPTICAL INTERFEROMETER OBSERVATIONS OF THE EXOPLANET HOST {kappa} CORONAE BOREALIS AND THEIR IMPLICATIONS FOR THE STAR'S AND PLANET'S MASSES AND AGES

    SciTech Connect (OSTI)

    Baines, Ellyn K.; Armstrong, J. Thomas [Remote Sensing Division, Naval Research Laboratory, 4555 Overlook Avenue SW, Washington, DC 20375 (United States); Van Belle, Gerard T., E-mail: ellyn.baines@nrl.navy.mil [Lowell Observatory, Flagstaff, AZ 86001 (United States)

    2013-07-01T23:59:59.000Z

    We used the Navy Precision Optical Interferometer to measure the limb-darkened angular diameter of the exoplanet host star {kappa} CrB and obtained a value of 1.543 {+-} 0.009 mas. We calculated its physical radius (5.06 {+-} 0.04 R{sub Sun }) and used photometric measurements from the literature with our diameter to determine {kappa} CrB's effective temperature (4788 {+-} 17 K) and luminosity (12.13 {+-} 0.09 L{sub Sun }). We then placed the star on an Hertzsprung-Russell diagram to ascertain the star's age (3.42{sup +0.32}{sub -0.25} Gyr) and mass (1.47 {+-} 0.04 M{sub Sun }) using a metallicity of [Fe/H] = +0.15. With this mass, we calculated the system's mass function with the orbital elements from a variety of sources, which produced a range of planetary masses: m{sub p}sin i = 1.61-1.88 M{sub Jup}. We also updated the extent of the habitable zone for the system using our new temperature.

  3. Simple Host?Guest Chemistry To Modulate the Process of Concentration and Crystallization of Membrane Proteins by Detergent Capture in a Microfluidic Device

    SciTech Connect (OSTI)

    Li, Liang; Nachtergaele, Sigrid; Seddon, Annela M.; Tereshko, Valentina; Ponomarenko, Nina; Ismagilov, Rustem F. (UC)

    2009-01-15T23:59:59.000Z

    This paper utilizes cyclodextrin-based host-guest chemistry in a microfluidic device to modulate the crystallization of membrane proteins and the process of concentration of membrane protein samples. Methyl-{beta}-cyclodextrin (MBCD) can efficiently capture a wide variety of detergents commonly used for the stabilization of membrane proteins by sequestering detergent monomers. Reaction Center (RC) from Blastochloris viridis was used here as a model system. In the process of concentrating membrane protein samples, MBCD was shown to break up free detergent micelles and prevent them from being concentrated. The addition of an optimal amount of MBCD to the RC sample captured loosely bound detergent from the protein-detergent complex and improved sample homogeneity, as characterized by dynamic light scattering. Using plug-based microfluidics, RC crystals were grown in the presence of MBCD, giving a different morphology and space group than crystals grown without MBCD. The crystal structure of RC crystallized in the presence of MBCD was consistent with the changes in packing and crystal contacts hypothesized for removal of loosely bound detergent. The incorporation of MBCD into a plug-based microfluidic crystallization method allows efficient use of limited membrane protein sample by reducing the amount of protein required and combining sparse matrix screening and optimization in one experiment. The use of MBCD for detergent capture can be expanded to develop cyclodextrin-derived molecules for fine-tuned detergent capture and thus modulate membrane protein crystallization in an even more controllable way.

  4. Hosting Dept. Host Visiting Speaker Speaker's Institution Purpose PRELIMINARY

    E-Print Network [OSTI]

    MacMillan, Andrew

    Biochemistry Fliegel/Sykes Natalie Goto University of Ottawa external MMI Foley, Edan Savraj Grewal University, Robert Kenneth Harder University of British Columbia external MMI Kane, Kevin James Di Santo Dept external Biochemistry Schang, Luis James Ronald Davie University of Manitoba STRG retreat Cell Biol. Simmen

  5. Information Systems Host: Sanjeev Dewan

    E-Print Network [OSTI]

    Loudon, Catherine

    Ghose is an Associate Professor of Information, Operations, and Management Sciences and the Robert L by its shared technology infrastructure. He has worked on product reviews, reputation and rating systems, sponsored search advertising, mobile commerce, mobile apps, mobile ads, crowd funding, and online markets

  6. Hosting Web Pages at NERSC

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office of Science (SC) EnvironmentalGyroSol茅(tm) HarmonicbetandEnergy 2010 A File

  7. Westinghouse to host education fair

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level:Energy: Grid Integration Redefining What'sis Taking Over OurThe Iron SpinPrincetonUsing Maps1DOETHEWeeklyTRU Solutions LLC

  8. NERSC Hosts Digital Stargazing Portal

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office of Science (SC)Integrated Codes |IsLove Your1AllocationsNOVA Portal: Submit2014ftp

  9. Chronic graft-versus-host disease in the rat radiation chimera: I. clinical features, hematology, histology, and immunopathology in long-term chimeras

    SciTech Connect (OSTI)

    Beschorner, W.E.; Tutschka, P.J.; Santos, G.W.

    1982-04-01T23:59:59.000Z

    The clinical features, pathology, and immunopathology of chronic graft-versus-host disease (GVHD) developing in the long-term rat radiation chimera are described. At 6 to 12 months post-transplant, the previously stable ACI/LEW chimeras developed patchy to diffuse severe hair loss and thickened skin folds, and had microscopic features resembling scleroderma, Sjogren's syndrome, and chronic hepatitis. Skin histology showed dermal inflammation and acanthosis with atrophy of the appendages, with progression to dermal sclerosis. The liver revealed chronic hepatitis with bile duct injury and proliferation and periportal piecemeal necrosis. The tongue had considerable submucosal inflammation, muscular necrosis, and atrophy and arteritis. The serous salivary glands, lacrimal glands, and bronchi had lymphocytic inflammation and injury to duct, acinar, and mucosal columnar epithelium. The thymus had lymphocyte depletion of the medulla with prominent epithelium. The spleen and lymph nodes had poorly developed germinal centers but increased numbers of plasma cells. IgM was observed along the basement membrane and around the basal cells of the skin and tongue and along the basement membrane of the bile ducts. IgM was present also in the arteries of the tongue. Immunoglobulins eluted from the skin, cross-reacted with the bile duct epithelium and usually with both ACI and Lewis skin. Increased titers of speckled antinuclear antibodies were present in the serum of rats with chronic (GVHD). Chronic GVHD in the long-term rat radiation chimera is very similar to human chronic GVHD and is a potentially excellent model for autoimmune disorders including scleroderma, Sjorgren's syndrome, and chronic hepatitis.

  10. An examination of electronic file transfer between host and microcomputers for the AMPMODNET/AIMNET (Army Material Plan Modernization Network/Acquisition Information Management Network) classified network environment

    SciTech Connect (OSTI)

    Hake, K.A.

    1990-11-01T23:59:59.000Z

    This report presents the results of investigation and testing conducted by Oak Ridge National Laboratory (ORNL) for the Project Manager -- Acquisition Information Management (PM-AIM), and the United States Army Materiel Command Headquarters (HQ-AMC). It concerns the establishment of file transfer capabilities on the Army Materiel Plan Modernization (AMPMOD) classified computer system. The discussion provides a general context for micro-to-mainframe connectivity and focuses specifically upon two possible solutions for file transfer capabilities. The second section of this report contains a statement of the problem to be examined, a brief description of the institutional setting of the investigation, and a concise declaration of purpose. The third section lays a conceptual foundation for micro-to-mainframe connectivity and provides a more detailed description of the AMPMOD computing environment. It gives emphasis to the generalized International Business Machines, Inc. (IBM) standard of connectivity because of the predominance of this vendor in the AMPMOD computing environment. The fourth section discusses two test cases as possible solutions for file transfer. The first solution used is the IBM 3270 Control Program telecommunications and terminal emulation software. A version of this software was available on all the IBM Tempest Personal Computer 3s. The second solution used is Distributed Office Support System host electronic mail software with Personal Services/Personal Computer microcomputer e-mail software running with IBM 3270 Workstation Program for terminal emulation. Test conditions and results are presented for both test cases. The fifth section provides a summary of findings for the two possible solutions tested for AMPMOD file transfer. The report concludes with observations on current AMPMOD understanding of file transfer and includes recommendations for future consideration by the sponsor.

  11. Host diversity begets parasite diversity: bird final hosts and trematodes in snail intermediate hosts

    E-Print Network [OSTI]

    Hechinger, R F; Lafferty, K D

    2005-01-01T23:59:59.000Z

    Natural Reserve System抯 Carpinteria Salt Marsh Reserve, andtwo types of habitat in Carpinteria Salt Marsh (34824 0 N,community structure in Carpinteria Salt Marsh. Our ?ndings

  12. Study on proliferative responses to host Ia antigens in allogeneic bone marrow chimera in mice: sequential analysis of the reactivity and characterization of the cells involved in the responses

    SciTech Connect (OSTI)

    Iwabuchi, K.; Ogasawara, K.; Ogasawara, M.; Yasumizu, R.; Noguchi, M.; Geng, L.; Fujita, M.; Good, R.A.; Onoe, K.

    1987-01-01T23:59:59.000Z

    Irradiation bone marrow chimeras were established by reconstitution of lethally irradiated AKR mice with C57BL/10 marrow cells to permit serial analysis of the developing reactivities of lymphocytes from such chimeras, (B10----AKR), against donor, host, or third party antigens. We found that substantial proliferative responses to Ia antigens of the recipient strain and also to third party antigens were generated by the thymocytes obtained from the irradiation chimeras at an early stage after bone marrow reconstitution. The majority of the responding thymocytes had surfaces lacking demonstrable peanut agglutinin receptors and were donor type Thy-1+, Ly-2-, and L3T4+ in both anti-recipient and anti-third party MLR. In anti-host responses, however, Ly-2+ thymocytes seemed to be at least partially involved. This capacity of thymus cells to mount a response to antigens of the recipient strain declined shortly thereafter, whereas the capacity to mount MLR against third party antigens persisted. The spleen cells of (B10----AKR) chimeras at the same time developed a more durable capability to exhibit anti-host reactivities and a permanent capability of reacting to third party allo-antigens. The stimulator antigens were Ia molecules on the stimulator cells in both anti-recipient and anti-third party MLR. The responding splenocytes were of donor origin and most of them had Thy-1+, Ly-1+2-, and L3T4+ phenotype.

  13. A Statistical Framework for Microbial Source Attribution: Measuring Uncertainty in Host Transmission Events Inferred from Genetic Data (Part 2 of a 2 Part Report)

    SciTech Connect (OSTI)

    Allen, J; Velsko, S

    2009-11-16T23:59:59.000Z

    This report explores the question of whether meaningful conclusions can be drawn regarding the transmission relationship between two microbial samples on the basis of differences observed between the two sample's respective genomes. Unlike similar forensic applications using human DNA, the rapid rate of microbial genome evolution combined with the dynamics of infectious disease require a shift in thinking on what it means for two samples to 'match' in support of a forensic hypothesis. Previous outbreaks for SARS-CoV, FMDV and HIV were examined to investigate the question of how microbial sequence data can be used to draw inferences that link two infected individuals by direct transmission. The results are counter intuitive with respect to human DNA forensic applications in that some genetic change rather than exact matching improve confidence in inferring direct transmission links, however, too much genetic change poses challenges, which can weaken confidence in inferred links. High rates of infection coupled with relatively weak selective pressure observed in the SARS-CoV and FMDV data lead to fairly low confidence for direct transmission links. Confidence values for forensic hypotheses increased when testing for the possibility that samples are separated by at most a few intermediate hosts. Moreover, the observed outbreak conditions support the potential to provide high confidence values for hypothesis that exclude direct transmission links. Transmission inferences are based on the total number of observed or inferred genetic changes separating two sequences rather than uniquely weighing the importance of any one genetic mismatch. Thus, inferences are surprisingly robust in the presence of sequencing errors provided the error rates are randomly distributed across all samples in the reference outbreak database and the novel sequence samples in question. When the number of observed nucleotide mutations are limited due to characteristics of the outbreak or the availability of only partial rather than whole genome sequencing, indel information was shown to have the potential to improve performance but only for select outbreak conditions. In examined HIV transmission cases, extended evolution proved to be the limiting factor in assigning high confidence to transmission links, however, the potential to correct for extended evolution not associated with transmission events is demonstrated. Outbreak specific conditions such as selective pressure (in the form of varying mutation rate), are shown to impact the strength of inference made and a Monte Carlo simulation tool is introduced, which is used to provide upper and lower bounds on the confidence values associated with a forensic hypothesis.

  14. THE TIP OF THE RED GIANT BRANCH DISTANCES TO TYPE Ia SUPERNOVA HOST GALAXIES. II. M66 AND M96 IN THE LEO I GROUP

    SciTech Connect (OSTI)

    Lee, Myung Gyoon; Jang, In Sung, E-mail: mglee@astro.snu.ac.kr, E-mail: isjang@astro.snu.ac.kr [Astronomy Program, Department of Physics and Astronomy, Seoul National University, Gwanak-gu, Seoul 151-742 (Korea, Republic of)

    2013-08-10T23:59:59.000Z

    M66 and M96 in the Leo I Group are nearby spiral galaxies hosting Type Ia supernovae (SNe Ia). We estimate the distances to these galaxies from the luminosity of the tip of the red giant branch (TRGB). We obtain VI photometry of resolved stars in these galaxies from F555W and F814W images in the Hubble Space Telescope archive. From the luminosity function of these red giants, we find the TRGB I-band magnitude to be I{sub TRGB} = 26.20 {+-} 0.03 for M66 and 26.21 {+-} 0.03 for M96. These values yield distance modulus (m - M){sub 0} = 30.12 {+-} 0.03(random) {+-} 0.12(systematic) for M66 and (m - M){sub 0} = 30.15 {+-} 0.03(random) {+-} 0.12(systematic) for M96. These results show that they are indeed the members of the same group. With these results we derive absolute maximum magnitudes of two SNe (SN 1989B in M66 and SN 1998bu in M96). V-band magnitudes of these SNe Ia are {approx}0.2 mag fainter than SN 2011fe in M101, one of the nearest recent SNe Ia. We also derive near-infrared magnitudes for SN 1998bu. Optical magnitudes of three SNe Ia (SN 1989B, SN 1998bu, and SN 2011fe) based on TRGB analysis yield a Hubble constant, H{sub 0} = 68.4 {+-} 2.6(random) {+-} 3.7(systematic) km s{sup -1} Mpc{sup -1}. This value is similar to the values derived from recent WMAP9 results, H{sub 0} = 69.32 {+-} 0.80 km s{sup -1} Mpc{sup -1}, and from Planck results, H{sub 0} = 67.3 {+-} 1.2 km s{sup -1} Mpc{sup -1}, but smaller than other recent determinations based on Cepheid calibration for SNe Ia luminosity, H{sub 0} = 74 {+-} 3 km s{sup -1} Mpc{sup -1}.

  15. Bacteriophage ?MAM1, a Viunalikevirus, Is a Broad-Host-Range, High-Efficiency Generalized Transducer That Infects Environmental and Clinical Isolates of the Enterobacterial Genera Serratia and Kluyvera

    E-Print Network [OSTI]

    Matilda, Miguel A.; Salmond, George P. C.

    2014-01-01T23:59:59.000Z

    The generated transducing particles adsorb normally and inject DNA into a recipient 63 bacterium. The injected bacterial DNA may integrate by homologous recombination into 64 the genome of the recipient host, resulting in a stable bacterial transductant (14... .o.i. The mixture was incubated at 30 169 篊 for 30 minutes (1 h for Sma 12), pelleted by centrifugation (4.000 g for 10 min at 4 篊) 170 8 and washed twice with 10 ml of LB to remove any remaining lysate. The cells were 171 resuspended in 5 ml of LB and 100...

  16. Effect of Spin-Crossover-Induced Pore Contraction on CO{sub 2}-Host Interactions in the Porous Coordination Polymers [Fe(pyrazine)M(CN){sub 4}] (M = Ni, Pt)

    SciTech Connect (OSTI)

    Culp, Jeffrey T.; Chen, De-Li; Liu, Jinchen; Chirdon, Danielle; Kauffman, Kristi; Goodman, Angela; Johnson, J. Karl

    2013-02-01T23:59:59.000Z

    Variable-temperature in situ ATR-FTIR spectra are presented for the porous spin-crossover compounds [Fe(pyrazine)- Ni(CN){sub 4}] and [Fe(pyrazine)Pt(CN){sub 4}] under CO{sub 2} pressures of up to 8 bar. Significant shifts in the ?{sub 3} and ?{sub 2} IR absorption bands of adsorbed CO{sub 2} are observed as the host materials undergo transition between low- and high-spin states. Computational models used to determine the packing arrangement of CO{sub 2} within the pore structures show a preferred orientation of one of the adsorbed CO{sub 2} molecules with close O=C=O贩稨 contacts with the pyrazine pillar ligands. The interaction is a consequence of the commensurate distance of the inter-pyrazine separations and the length of the CO{sub 2} molecule, which allows the adsorbed CO{sub 2} to effectively bridge the pyrazine pillars in the structure. The models were used to assign the distinct shifts in the IR absorption bands of the adsorbed CO{sub 2} that arise from changes in the O=C=O贩稨 contacts that strengthen and weaken in correlation with changes in the Fe朜 bond lengths as the spin state of Fe changes. The results indicate that spin-crossover compounds can function as a unique type of flexible sorbent in which the pore contractions associated with spin transition can affect the strength of CO{sub 2}host interactions.

  17. Navy Warfare Development Command (NWDC) is hosting a Pacific Rim Innovation Symposium on October 10-11, 2012, at the SPAWAR Center in San Diego, Ca., for junior leaders from E-5 to O-5. The event is scheduled to start at 12:00

    E-Print Network [OSTI]

    Navy Warfare Development Command (NWDC) is hosting a Pacific Rim Innovation Symposium on October 10 will be brought forward to senior Navy leadership. Agenda: 10 OCT (All Times Pacific Daylight Time) 1200 Welcome of Breakout Group Issues 1730 Adjourn for the Day 11 OCT 1200 Navy Innovation Resources, CAPT David Tyler, ACo

  18. The 2014 Oregon State Cheerleaders and Dancers will be hosting a clinic for kids in grades K -5. The clinic is limited to the first 150 participants. The clinic includes a t-shirt and a ticket for the participant to the game. All participants must have th

    E-Print Network [OSTI]

    Escher, Christine

    The 2014 Oregon State Cheerleaders and Dancers will be hosting a clinic for kids in grades K - 5. The clinic is limited to the first 150 participants. The clinic includes a t-shirt and a ticket by a legal guardian. Cheer Clinic and Peformance at the Oregon State Women's Basketball Game vs. WSU Sunday

  19. UT Arlington Nedderman Society Membership Roster

    E-Print Network [OSTI]

    Huang, Haiying

    Randall R. Butler, Ph.D. William D. Caldwell Jonathan Campbell and Tanya Dowdey Alan R. Cannon #12;Estella David and Molly Albart Julie S. Alexander Cheri D. Allen Cheryl A. Anderson, Ph.D. Jason Anderson Mindi Ruthie Brock Lance and Amber Brown Julie A. Brown John and Amalia Buckwalter Brian Builta and Sarah

  20. New Hampshire 4-H Serving to Learn, Learning to Serve

    E-Print Network [OSTI]

    New Hampshire, University of

    humane society shelters to feed and groom animals and clean cages or hold an adopt-a-pet week in cooperation with a local pet center or humane society. Child Care Provide free on-site child care services and community centers. Teach seniors how to use email and the internet. Mindy Turner, New Mexico 4-H Youth

  1. Geothermal Technologies Office Hosts Collegiate Competition

    Office of Energy Efficiency and Renewable Energy (EERE)

    To further accelerate the adoption of geothermal energy, the United States Department of Energy is sponsoring a Geothermal Case Study Challenge (CSC) to aggregate geothermal data that can help us...

  2. Cell Host & Microbe Adenovirus Transport via Direct

    E-Print Network [OSTI]

    Gross, Steven

    as a naked capsid using the microtubule motor cyto- plasmic dynein. How the dynein complex is recruited of viruses are instead consistent with trans- port by microtubule motors (Do hner et al., 2005). Recent evidence has implicated cytoplasmic dynein in the translocation of herpes simplex virus, adenovirus

  3. Viral metagenomics in host-associated systems

    E-Print Network [OSTI]

    Willner, Dana Leigh

    2010-01-01T23:59:59.000Z

    cesium chloride density gradient centrifugation and DNase I treatment was for removing human genomic contamination

  4. Mechanical engineering Department Seminar Hosts: White & Bishop

    E-Print Network [OSTI]

    Lin, Xi

    by detecting and elim- inating seizures seconds before they occur Stretchable, bendable lithium-ion batteries, complete with integrated wireless recharging systems, which could hasten the development of flexible smart Technology photos courtesy of John Rogers / Photography by Evan Sears Reproduced with permission from

  5. Ethanol production in non-recombinant hosts

    DOE Patents [OSTI]

    Kim, Youngnyun; Shanmugam, Keelnatham; Ingram, Lonnie O.

    2013-06-18T23:59:59.000Z

    Non-recombinant bacteria that produce ethanol as the primary fermentation product, associated nucleic acids and polypeptides, methods for producing ethanol using the bacteria, and kits are disclosed.

  6. EM Hosts Used Fuel Management Workshop

    Broader source: Energy.gov [DOE]

    WASHINGTON, D.C. EM抯 Office of Nuclear Materials Disposition held a workshop with Swedish executives earlier this month to learn about their approaches to designing a national waste management program.

  7. Open Access to Financing + Solar Hosting

    Broader source: Energy.gov [DOE]

    This presentation summarizes the information given by GridParity Finance during the DOE SunShot Grand Challenge: Summit and Technology Forum, June 13-14, 2012.

  8. Assessment of Farmland Hosting Renewable Energy Systems

    Broader source: Energy.gov [DOE]

    In New Jersey, under the Farmland Assessment Act, farmland actively devoted to an agricultural or horticultural use is assessed at its productivity value. This practice generally results in a lower...

  9. Purdue Hosts CAARMS9 - Purdue University

    E-Print Network [OSTI]

    Sally

    2003-07-31T23:59:59.000Z

    problems come from petroleum engineering and environmental engineer- ing. ... on by tough economic times. ...... area of nondestructive evaluation of frozen.

  10. Supplement 15, Parasite-Subject Catalogue: Hosts

    E-Print Network [OSTI]

    Humphrey, Judith M.; Segal, Dorothy B.; Beard, Mary I.; Edwards, Shirley J.; Kirby, Margie D.

    1966-01-01T23:59:59.000Z

    Persia Jack, K. M., 1962 a, 289 Persia Jack, K. M., 1962 a, 272, 277 all from Angola Jack, K. M., 1962 a, 283 French Guinea Jack, K. M., 1962 a, 287 British Somaliland, Upper Egypt, Abyssinia Jack, K. M., 1962 a, 287 Kurdistan, Cyprus, South...

  11. Comparative phosphoproteomics reveals components of host cell...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    only hyper-cytotoxic but also were phagocytosed at much higher rates compared to the wild type parent strain. To elucidate the cellular signaling underlying this enhanced...

  12. Host and Derivative Product Modeling and Synthesis

    E-Print Network [OSTI]

    Davis, Matthew Louis Turner

    2010-10-12T23:59:59.000Z

    , implementation, and refinement of design methodologies is the notion that both the structure of the development process and the structure of the developed product are key factors in creating value in a firm抯 product line. With respect to the latter key factor...

  13. ORNL to Host Tennessee Solar Initiative

    E-Print Network [OSTI]

    if Americans prove unable to adapt their life styles to electric cars or to the idea that it will be cheaper. The development of dramatic new technologies for battery storage or the electric grid will be of little value

  14. Class Host: Johnson County Sheriff's Office Criminalistics

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625govInstrumentstdmadapInactiveVisiting the TWPSuccessAlamosCharacterization2 Permit Modification Request ReviseClass

  15. OREM Hosts Community Workshop | Department of Energy

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page onYouTube YouTube Note: Since the.pdfBreaking ofOilNEWResponse to Time-BasedDecember 23,Misc Cases T H EOPOWER

  16. Laboratory hosts 12th annual HAZMAT Challenge

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office of Science (SC)Integrated Codes |Is Your Home asLCLSLaboratory DirectorsRecovery ActLaboratory12th

  17. Junior Solar Sprint Host Guide Book

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOEThe Bonneville PowerCherries 82981-1cnHigh SchoolIn12electron beamJoin2015 BonnevilleJulyJune1June49,6

  18. DOE hosts public hearings in Idaho Falls

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOEThe Bonneville Power Administration wouldDECOMPOSITION OF CALCIUMCOSTDOE SolarPrinter-friendly iconofhosts public

  19. WIPP Hosts All-Hazards Planning Meeting

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level:Energy: Grid Integration Redefining What'sis Taking Over OurThe Iron SpinPrincetonUsing Maps1 -VisualizingVoteFundingComputers GetFebruary

  20. OREM Hosts Community Workshop | Department of Energy

    Broader source: Energy.gov (indexed) [DOE]

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742Energy ChinaofSchaeferAprilOverview |November(NationalORDER CONDITIONALLY GRANTING

  1. Essential requirement of I-A region-identical host bone marrow or bone marrow-derived cells for tumor neutralization by primed L3T4+ T cells

    SciTech Connect (OSTI)

    Ozawa, H.; Iwaguchi, T.; Kataoka, T.

    1987-12-01T23:59:59.000Z

    The antitumor activity of Meth A-hyperimmunized BALB/c mouse spleen cells (Meth A-Im-SPL) was assayed by the Winn test in H-2 incompatible bone marrow chimeras in closed colony CD-1 (nu/nu), inbred DDD/1(nu/nu) (H-2s), or inbred BALB/c(nu/nu) (H-2d) mice as recipients. We found that Meth A-Im-SPL suppressed Meth A growth in the chimera nude mice which were reconstituted with bone marrow cells of the H-2d haplotype (i.e., BALB/c, DBA/2 and B10.D2), but not in the chimeras which were reconstituted with bone marrow cells of the H-2a, H-2b, or H-2k haplotype (i.e., B10.A, B10, and B10.BR). These results suggested that H-2 restriction occurred between Meth A-Im-SPL and bone marrow or bone marrow-derived cells in tumor neutralization. Furthermore, Meth A-Im-SPL did not suppress Meth 1 tumors (antigenically distinct from Meth A tumors) in the presence or absence of mitomycin C-treated Meth A in a Winn assay. These results suggested that there is tumor specificity in the effector phase as well as in the induction phase. The phenotype of the effectors in the Meth A-Im-SPL was Thy-1.2+ and L3T4+, because Meth A-Im-SPL lost their antitumor activity with pretreatment with anti-Thy-1.2 monoclonal antibody (mAb) and complement or anti-L3T4 mAb and complement, but not with anti-Lyt-2.2 mAb and complement or complement alone. Positively purified L3T4+ T cells from Meth A-Im-SPL (Meth A-Im-L3T4), obtained by the panning method, suppressed the tumor growth in the chimera nude mice which were reconstituted with bone marrow cells of B10.KEA2 mice (that were I-A region-identical with Meth A-Im-L3T4 cells but not others in H-2) as well as B10.D2 cells (that were fully identical with Meth A-Im-L3T4 cells in H-2). We conclude that Meth A-Im-SPL (L3T4+) neutralized the tumors in collaboration with I-A region-identical host bone marrow or bone marrow-derived cells, and the neutralization was not accompanied by the bystander effect.

  2. Ancient host shifts followed by host conservatism in a group of ant parasitoids

    E-Print Network [OSTI]

    Murray, E. A; Carmichael, A. E; Heraty, J. M

    2013-01-01T23:59:59.000Z

    QLD: Great Sandy NP Australia: ACT: Canberra, JerrabomberraSEQ: Lansborough Australia: ACT: Canberra Nature Prk. BlackQLD, Mt. Glorious Australia: ACT: Canberra. Black Mtn. South

  3. A mathematical model for coupling within-host and between-host ...

    E-Print Network [OSTI]

    Zhilan Feng

    2012-10-12T23:59:59.000Z

    Oct 10, 2012 ... b Programa de Matem醫icas Aplicadas y Computaci髇, Instituto Mexicano del Petr髄eo, Mexico. 7 c Facultad de Matem醫icas, Universidad...

  4. A mathematical model for coupling within-host and between-host ...

    E-Print Network [OSTI]

    Zhilan Feng

    2013-09-15T23:59:59.000Z

    Oct 4, 2012 ... b Programa de Matem醫icas Aplicadas y Computaci髇, Instituto Mexicano del Petr髄eo, Mexico c Facultad de Matem醫icas, Universidad...

  5. DOE Host: Gene Turner LANL Technical Hosts: Terrill Lemke and Steve Veenis

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOEThe Bonneville Power Administration wouldDECOMPOSITION OF CALCIUMCOST MANAGEMENT REPORT Page8 DOE DOE

  6. Recipient allocation preferences and organizational choices: a fit perspective

    E-Print Network [OSTI]

    Gogus, Celile Itir

    2007-04-25T23:59:59.000Z

    . Christopher O. L. H. Porter was one of the most influential people throughout my graduate career, I thank him for his tremendous help with this dissertation and also for our work in the Team Research Lab. Mindy Bergman and Angelo DeNisi were very helpful... the relationship between different outcome types and choice of an allocation preference almost exclusively focused on the outcome categories proposed by the social exchange theory (Foa & Foa, 1975). The theory identifies six outcome categories that may...

  7. Recipient allocation preferences and organizational choices: a fit perspective

    E-Print Network [OSTI]

    Gogus, Celile Itir

    2007-04-25T23:59:59.000Z

    . Christopher O. L. H. Porter was one of the most influential people throughout my graduate career, I thank him for his tremendous help with this dissertation and also for our work in the Team Research Lab. Mindy Bergman and Angelo DeNisi were very helpful... the relationship between different outcome types and choice of an allocation preference almost exclusively focused on the outcome categories proposed by the social exchange theory (Foa & Foa, 1975). The theory identifies six outcome categories that may...

  8. agn host galaxies: Topics by E-print Network

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    levels. A large number of stellar features are measured both in the optical and near-infrared. We find the nuclear stellar population to be related to the level of activity. These...

  9. agns host galaxy: Topics by E-print Network

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    levels. A large number of stellar features are measured both in the optical and near-infrared. We find the nuclear stellar population to be related to the level of activity. These...

  10. agn host galaxy: Topics by E-print Network

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    levels. A large number of stellar features are measured both in the optical and near-infrared. We find the nuclear stellar population to be related to the level of activity. These...

  11. Coevolution of Supermassive Black Holes and Their Host Galaxies

    E-Print Network [OSTI]

    Hiner, Kyle Devon

    2012-01-01T23:59:59.000Z

    A3 A5 (Myr) F0 F5 F8 G0 G5 G8 K0 K2 K5 K7 M0 M8 Table 2.3:spectral types: A2, A3, G4, G8, K0, and K3. We have comparedSp Type A0 A3 A5 F0 F5 F8 G0 G5 G8 K0 K2 K2 K5 K5 K7 M0 M8

  12. High average power laser using a transverse flowing liquid host

    DOE Patents [OSTI]

    Ault, Earl R.; Comaskey, Brian J.; Kuklo, Thomas C.

    2003-07-29T23:59:59.000Z

    A laser includes an optical cavity. A diode laser pumping device is located within the optical cavity. An aprotic lasing liquid containing neodymium rare earth ions fills the optical cavity. A circulation system that provides a closed loop for circulating the aprotic lasing liquid into and out of the optical cavity includes a pump and a heat exchanger.

  13. adenovirus host cell: Topics by E-print Network

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    modeling of physical conditions in the molecular ISM. We find that the CO-emitting gas is warmer, denser, and less optically thick than that found in typical Galactic...

  14. affects host cell: Topics by E-print Network

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Biology and Medicine Websites Summary: Figure S1, related to Figure 2. M1T15448 GAS replicate efficiently in the cytosol of epithelial cells replication of GAS. (A)...

  15. aureus host cell: Topics by E-print Network

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    modeling of physical conditions in the molecular ISM. We find that the CO-emitting gas is warmer, denser, and less optically thick than that found in typical Galactic...

  16. altered host cell: Topics by E-print Network

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    modeling of physical conditions in the molecular ISM. We find that the CO-emitting gas is warmer, denser, and less optically thick than that found in typical Galactic...

  17. A Seafloor Microbial Biome Hosted within Incipient Ferromanganese...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Santelli, Orcutt et al. 2008). Yet microbially-mediated basalt alteration and energy conservation has not been directly demonstrated on the seafloor. By using synchrotron-based...

  18. Evaluation of tick-host-landscape interactions using spatial analysis

    E-Print Network [OSTI]

    Bush, Beau R

    1997-01-01T23:59:59.000Z

    for antennae, battery power, and computer interfacing (Fig. 2). From the prototype, twenty more tracking units were manufactured in our laboratory. GPS caiamta data cceeieelhy thc GPS eaccieacia Sec ccar DGPS ecwpeciSca gaia in lihKL iheaeat RXCM Caccac... (RTCM) data provided by the Trimble 4000 base station. . Cow tracking unit with view of internal component configuration within anodized aluminum box. . View of cow harness with tracking unit, battery and foam insulator . . . . . 10 Side view...

  19. animal reservoir hosts: Topics by E-print Network

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AND SIMULATION OF A MATURE FIELD USING AN INTEGRATED APPROACH University of Kansas - KU ScholarWorks Summary: Reservoir characterization involves various studies...

  20. Department of Energy Hosts First Steering Committee Meeting on...

    Energy Savers [EERE]

    source that powers growing economies, while greatly reducing greenhouse gas emissions and air pollution." The Action Plan, which was signed in April 2007, fulfilled the commitment...

  1. Supplement 17, Part 7, Parasite-Subject Catalogue: Hosts

    E-Print Network [OSTI]

    Edwards, Shirley J.; Kirby, Margie D.; Segal, Dorothy B.; Humphrey, Judith M.

    1971-01-01T23:59:59.000Z

    bile bile duct(s) blood blood vessel body cavity bone brain bronchi caecum cloaca bexiga de ar arteria arteria bile bilis canale epatico ducto biliario sangue sangue vaso sanguigno vaso de sangue osso cerebro bronchi cieco cloaca...

  2. Supplement 18, Part 7, Parasite-Subject Catalogue: Hosts

    E-Print Network [OSTI]

    Edwards, Shirley J.; Kirby, Margie D.; Crawley, Lila R.; Rayburn, Jane D.; Shaw, Judith H.; Walker, Martha L.

    1974-01-01T23:59:59.000Z

    ducto biliario sangue sangue vaso sanguigno vaso de sangue osso cerebro bronchi cieco cloaca clrebro bronquios connective tissue tessuto connetti- vo crop diaphragm duodenum ear esophagus eye feces gall bladder gill(s) gizzard heart...

  3. Senior DOE Official to Host Press Call on Electricity Advisory...

    Energy Savers [EERE]

    for policy and program initiatives surrounding generation adequacy, energy efficiency and demand response, transmission adequacy; deployment of energy storage technologies; and...

  4. Peer Review Lab Inspection Form Safety Officer Hosting Inspection

    E-Print Network [OSTI]

    /freezer is used for cold storage of flammable liquids? Yes No N/A 19. Chemical containers are properly labeled

  5. alternative host matrix: Topics by E-print Network

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    the model and its extensions well suited for studying the phase diagram of QCD. James C. Osborn 2004-03-11 29 Molecular Dynamics of Matrix-Assisted Laser Desorption of Leucine...

  6. Cell Host & Microbe Invasive and Adherent Bacterial Pathogens

    E-Print Network [OSTI]

    Kirchhausen, Tomas

    ,9 Alejandro Toledo-Arana,1,2,3,9 Ann E. Lin,4 Jost Enninga,6,7 Javier Pizarro-Cerda ,1,2,3 B. Brett Finlay,4

  7. Mammalian Host Responses to Proinflammatory Stimuli by Microbial Pathogens

    E-Print Network [OSTI]

    Clark, Robin Teresa

    2010-01-01T23:59:59.000Z

    response in Helicobacter pylori gastritis. Ann Med, 2009.Y. , et al. , Helicobacter pylori potentiates epithelial:is highly produced in Helicobacter pylori-infected gastric

  8. NREL: News - NREL to Host Photovoltaics Presentation at 2014...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    power is needed to power a generator set to approximate the energy output of an average solar panel. Denver Solar Day coincides with the opening day of the 40th IEEE...

  9. altered pulmonary host: Topics by E-print Network

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    by lying down, with no complaints of hoarseness or dysphonia. He denied fever, fatigue, cough, chest pain, sweats, weight loss, reflux, arthralgias, myalgias and rash. He also...

  10. DOE Hosts Festival to Collect Items for Area Food Banks

    Broader source: Energy.gov [DOE]

    WASHINGTON, D.C. Deputy Secretary of Energy Daniel Poneman and a representative of the Capital Area Food Bank are among the guest speakers at an event this Tuesday, July 31, to collect food items for the DOE Feeds Families drive.

  11. NNSA Hosts Cybersecurity Consortium Members Following White House...

    National Nuclear Security Administration (NNSA)

    Livermore National Laboratory and Sandia National Laboratory in California and New Mexico. Vice President Biden and Secretary of Energy Ernest Moniz highlighted DOENNSA's...

  12. Can an evolving Universe host a static event horizon?

    E-Print Network [OSTI]

    Aharon Davidson; Shimon Rubin; Yosef Verbin

    2012-11-09T23:59:59.000Z

    We prove the existence of general relativistic perfect fluid black hole solutions, and demonstrate the phenomenon for the $P=w\\rho$ class of equations of state. While admitting a local time-like Killing vector on the event horizon itself, the various black hole configurations are necessarily time dependent (thereby avoiding a well known no-go theorem) away from the horizon. Consistently, Hawking's imaginary time periodicity is globally manifest on the entire spacetime manifold.

  13. Supplement 20, Part 7, Parasite-Subject Catalogue: Hosts

    E-Print Network [OSTI]

    Shaw, Judith H.; Edwards, Shirley J.; Rayburn, Jane D.; Tolson, Deborah A.; Hood, Martha W.

    1976-01-01T23:59:59.000Z

    at the Times-Beaconin Manahawkin (Lenni Lenape Indian for "land of good corn") and living in Lakehurst ("Land of the Crashing Airships"). In her rather piebald career, she has worked in professional theatre public relations, as a janitor in a high school...

  14. Host and pathogen transcriptional profiles of acute Brucella melitensis infection

    E-Print Network [OSTI]

    Rossetti, Carlos Alberto

    2009-05-15T23:59:59.000Z

    to macrophages and cells of the reticulo-endotelial system, Brucella has predilection for the gravid uterus ultimately causing abortion with huge numbers of organisms being expelled in the fetus and fetal fluids (4). In the placenta, Brucella replicate...

  15. Nonlinear optical crystal optimized for Ytterbium laser host wavelengths

    DOE Patents [OSTI]

    Ebbers, Christopher A. (Pleasanton, CA); Schaffers, Kathleen I. (Livermore, CA)

    2008-05-27T23:59:59.000Z

    A material for harmonic generation has been made by substitutional changes to the crystal LaCa.sub.4 (BO.sub.3).sub.3 also known as LaCOB in the form Re1.sub.xRe2.sub.yRe3.sub.zCa.sub.4(B0.sub.3).sub.3O where Re1 and Re2, (rare earth ion 1 and rare earth ion 2) are selected from the group consisting of Sc, Yttrium, La, Ce, Pr, Nd, Sm, Eu, Gd, Th, Dy, Ho, Er, Tm, Yb, and Lu; Re3 is Lanthanum; and x+y+z=1.

  16. Nonlinear optical crystal optimized for ytterbium laser host wavelengths

    DOE Patents [OSTI]

    Ebbers, Christopher A. (Livermore, CA); Schaffers, Kathleen I. (Pleasanton, CA)

    2007-08-21T23:59:59.000Z

    A material for harmonic generation has been made by substitutional changes to the crystal LaCa.sub.4(BO.sub.3).sub.3 also known as LaCOB in the form Re1.sub.xRe2.sub.yRe3.sub.zCa.sub.4(B0.sub.3).sub.3O where Re1 and Re2, (rare earth ion 1 and rare earth ion 2) are selected from the group consisting of Sc, Yttrium, La, Ce, Pr, Nd, Sm, Eu, Gd, Tb, Dy, Ho, Er, Tm, Yb, and Lu; Re3 is Lanthanum; and x+y+z=1.

  17. Nonlinear optical crystal optimized for Ytterbium laser host wavelengths

    DOE Patents [OSTI]

    Ebbers, Christopher A. (Livermore, CA); Schaffers, Kathleen I. (Pleasanton, CA)

    2007-02-20T23:59:59.000Z

    A material for harmonic generation has been made by substitutional changes to the crystal LaCa.sub.4 (BO.sub.3).sub.3 also known as LaCOB in the form Re1.sub.xRe2.sub.yRe3.sub.zCa.sub.4(BO.sub.3).sub.3O where Re1 and Re2, (rare earth ion 1 and rare earth ion 2) are selected from the group consisting of Sc, Yttrium, La, Ce, Pr, Nd, Sm, Eu, Gd, Tb, Dy, Ho, Er, Tm, Yb, and Lu; Re3 is Lanthanum; and x+y+z=1.

  18. DOE to Host Three Alaska Native Village Renewable Energy Project...

    Office of Environmental Management (EM)

    in an the initial facilitation workshop for Alaska Energy Ambassadors held at the U.S. Fish & Wildlife Service Regional Office in Anchorage in September. Photo by Jared Temanson,...

  19. Checklist of Host-Parasite Interactions of the Order Crocodylia

    E-Print Network [OSTI]

    Tellez, Marisa

    2013-01-01T23:59:59.000Z

    Griphobilharzia amoena Platt, Blair, Purdie and Melvillelungs, liver, and spleen. Platt et al. (1991); BloodGriphobilharzia amoena Platt, Blair, Purdie and Melville

  20. RESEARCH Open Access Investigating host dependence of xylose

    E-Print Network [OSTI]

    Zhao, Huimin

    it can reduce the cost of feedstock for bioethanol production and substantially minimize the emission

  1. Characterization of a Broad Host Range Tailocin from Burkholderia

    E-Print Network [OSTI]

    Duarte, Iris

    2012-10-19T23:59:59.000Z

    lipopolysaccharide (LPS) was conducted to determine the receptor site and it was determined that L-rhamnose and alpha-glucose associated with the LPS core were the receptors. Genetic analysis and targeted mutagenesis of the tailocin encoding genes was conducted...

  2. Implementing CDM projects Guidebook to Host Country Legal Issues

    E-Print Network [OSTI]

    University of Denmark, or Baker & McKenzie. This report is intended as a public resource for stakeholders undertaking activities that reduce greenhouse gas emissions, whether under the Kyoto Protocol's Clean Development Mechanism or other market-based instruments for carbon trading. While this guidebook provides

  3. MinorityAffairs,AlumniAssociation Host Outreach Program

    E-Print Network [OSTI]

    Jones, Michelle

    , as well as its value in creating a positive work/life environment for all employees. No state of Pennsylvania and at the University of Illinois. She earned her Ph.D. from the Massachusetts Institute diversity seminar through its Management Advancement for the Public Service (MAPS) series. Titled "Diversity

  4. Jefferson Lab hosts 23 teams for Virginia High School Science...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    High School Science Bowl on Feb. 11 February 3, 2006 Some of the brightest young minds in the Commonwealth will meet at the Department of Energy's Jefferson Lab on Saturday, Feb....

  5. SPECIAL SEMINAR Hosted by the University of Nebraska-Lincoln

    E-Print Network [OSTI]

    Farritor, Shane

    . The ES program focuses on four areas: solar energy, wind and wave energy, fuel cells, and biomass and Biomolecular Engineering and Nebraska EPSCoR Sustainable Energy Funding Opportunities at NSF Monday, October 4 energy through the Energy for Sustainability (ES) program and through other programs, especially those

  6. Secretary Chu to Host Media Briefing on Energy Department FY...

    Energy Savers [EERE]

    Year 2013 Budget Request, outlining the proposed investments in an all-of-the-above energy strategy that includes critical innovation, in the job-creating clean energy...

  7. REVIEWS AND SYNTHESES Local adaptation in host use among marine

    E-Print Network [OSTI]

    Sotka, Erik

    , local adaptation, selection. Ecology Letters (2005) 8: 448颅459 I N T R O DU C T I O N Population, abundance and ecological roles of organisms (Fox & Morrow 1981; Mopper & Strauss 1998), helps to maintain, there is a lingering perception that populations in the sea rarely locally adapt, and are more likely to evolve

  8. DOE and MEEA Host Fourth Annual SSL Market Introduction Workshop...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    installations in downtown Chicago, including the Merchandise Mart and the Wit Hotel. DOE SSL Portfolio Manager James Brodrick and MEEA Executive Director Wendy Jaehn kicked off...

  9. DOE and Northeast Energy Efficiency Partnerships Host Two-Day...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    and updates on the rapidly evolving SSL market. SSL Essentials and Lessons Learned DOE SSL Portfolio Manager James Brodrick kicked off the workshop by highlighting the pace of...

  10. DOE and Northwest Partners Host Three-Day Market Introduction...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    on the rapidly evolving SSL market. SSL Tutorials Address Technology Basics On Day 1, DOE SSL Portfolio Manager James Brodrick kicked off the workshop with an overview of DOE...

  11. Supplement 16, Part 7, Parasite-Subject Catalogue, Hosts

    E-Print Network [OSTI]

    Segal, Dorothy B.; Humphrey, Judith M.; Edwards, Shirley J.; Kirby, Margie D.

    1968-01-01T23:59:59.000Z

    n. sp. Congo Accipiter trivirgatus Price, R. D., 1964 a, 148 Kurodaia fulvofasciata Philippine Islands and Formosa [Acerina cernua] ersha Bauer, 0. N., [1949 a], 153 Henneguya creplini all from Yenisei river Plistophora acerinae Trichodina... Ob and Irtysh rivers Bauer, 0. N., [1949 a], 153 all from Yenisei river Phyllodistomum pseudofolium Tetracotyle ovata Bunodera luciopercae Cotylurus variegatus [Acerina cernua] ersh Bunodera luciopercae Tetracotyle percae Acerina cernua L...

  12. Histone deacetylase inhibitor therapy in graft-versus-host-disease

    E-Print Network [OSTI]

    How, Melissa

    2014-01-01T23:59:59.000Z

    passed through a disposable strainer to remove any clumps.be filtered through a 70 祄 strainer to remove any large

  13. Host cell factors involved in retrovirus replication and disease pathogenesis

    E-Print Network [OSTI]

    Seidel, Shannon Beth

    2012-01-01T23:59:59.000Z

    suspension through a 70uM cell strainer and incubated in ACKa 70uM nylon mesh cell strainer and washed through usingrun through a 70uM cell strainer into cell culture media (

  14. Deputy Secretary Poneman's Remarks at a Conference Hosted by...

    Office of Environmental Management (EM)

    the months and years ahead as we lay the groundwork for an expanding nuclear energy industry worldwide that will reduce air pollution, create new jobs and protect our national...

  15. Under Secretary D'Agostino to Host Conference Call Announcing...

    Broader source: Energy.gov (indexed) [DOE]

    has reached a major milestone in the Department's efforts to clean up the Cold War legacy at the Savannah River Site (SRS) in South Carolina. WHAT: U.S. Department of...

  16. RESEARCH LUNCHEON SERIES Co-hosted by the Departments of

    E-Print Network [OSTI]

    Farritor, Shane

    storage devices such as supercapacitors and batteries. Recently, our group has developed two different interests are focused on nanostructured, solution-processed optoelectronic devices, including solar cells-based Ionogel Formation for Biomedical and Energy Storage Applications Dr. Matthew Panzer Assistant Professor

  17. Solar ALMA Observations - A new view of our host star

    E-Print Network [OSTI]

    Wedemeyer, Sven; Brajsa, Roman; Barta, Miroslav; Shimojo, Masumi; Hales, Antonio; Yagoubov, Pavel; Hudson, Hugh

    2015-01-01T23:59:59.000Z

    ALMA provides the necessary spatial, temporal and spectral resolution to explore central questions in contemporary solar physics with potentially far-reaching implications for stellar atmospheres and plasma physics. It can uniquely constraint the thermal and magnetic field structure in the solar chromosphere with measurements that are highly complementary to simultaneous observations with other ground-based and space-borne instruments. Here, we highlight selected science cases.

  18. A HOST-BASED SECURITY ASSESSMENT ARCHITECTURE FOR INDUSTRIAL CONTROL

    E-Print Network [OSTI]

    Ou, Xinming "Simon"

    for this is their involvement in a country's critical infrastructures such as electrical, telephone, water, energy, etc the environment, or causing a loss of production, generation, or distribution of public utilities [1]. This makes. These systems can be vulnerable to a variety of attacks leading to devastating consequences like loss

  19. Is host castration an evolutionary strategy of bot flies?

    E-Print Network [OSTI]

    Timm, Robert M.; Lee, Richard E., Jr.

    1982-03-01T23:59:59.000Z

    . Genetics of speciation. Amer. Natur. 109:83-92 -. 1978. Speciation and sexual selection in Hawaiian Drosophila, p. 93-107. In P. F. Brus- sard (ed.), Ecological Genetics: The Interface. Springer-Verlag, N.Y. JOHNSON,W. R., AND W. B. HEED. Chromosomal... of the status of the genus Cephenemyia Ltr. 1818. Can. J. Zool. 33:75-98. CHANDLER,A. C., AND C. P. READ. 1961. Intro- duction to Parasitology. John Wiley & Sons, N.Y. 822 p. CHENG, T. C. 1973. General Parasitology. Academ- ic Press, N.Y. 965 p. DALMAT...

  20. algal hosts cystoseira: Topics by E-print Network

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    of both models represents 1,463.45 km2 on the island that can be developed for algaebased bioenergy Gilbes, Fernando 62 Behavioural Response in Plants: Adjustment in Algal...