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Office of Legacy Management (LM)

! "..- - ; ! "..- - ; : : LY /b J:,;' "Environmental Impact Evaluation and Engineering Plan" for the Remedial Action at the Former Kellex Laboratory, Jersey City, New Jersey , Robert 3. Stem, Acting Director NEPA Affairs Division ECT is initiating the necessary activities required to accomplish the remedial action to co-t conditions of radiological contamination at the former Kellex site. The proposed action entails the excavation of some spotty areas of radiological contaminated soil. The details and findings of the Environmental Impact Evaluation of the proposed remedial action were discussed at a rseeting on June 22, 1979, that was attended by Hr. C. Kouts of your stuff. In addition, Plr. Kouts was given a copy of the subject report.


Verifying Test Hypotheses -HOL/TestGen Verifying Test Hypotheses -HOL/TestGen  

E-Print Network (OSTI)

Verifying Test Hypotheses - HOL/TestGen Verifying Test Hypotheses - HOL/TestGen An Experiment in Test and Proof Thomas Malcher January 20, 2014 1 / 20 #12;Verifying Test Hypotheses - HOL/TestGen HOL/TestGen Outline Introduction Test Hypotheses HOL/TestGen - Demo Verifying Test Hypotheses Conclusion 2 / 20 #12


Taking the hol out of HOL Nancy A. Day  

E-Print Network (OSTI)

process. A decade ago, there was a wide chasm between specialized automated methods such as model check- cludes a consistency checker, a simulator, and links to a model checker, and a theorem prover [3, 20 for the automated analysis of specifications expressed in higher-order logic (hol) independent of a conven- tional

Day, Nancy


The Economics of HOl1icultural Biotechnology  

E-Print Network (OSTI)

The Economics of HOl1icultural Biotechnology Julian M. Alston Kent J. Bradford Nicholas Kalaitzandonakes SUMMARY. Technological change has driven economic progress in agIiculture and will continue, Department of Agricultural and Resource Econom- ics, University of California, Davis and Associate Director

Bradford, Kent


Living SafeLy  

NLE Websites -- All DOE Office Websites (Extended Search)

Living SafeLy and Working around HigH-voLtage PoWer LineS 1 H igh-voltage power lines can be just as safe as the electrical wiring in our homes - or just as danger- ous. The key is...


Mapping the Cosmic Web with Ly? Emission  

Science Journals Connector (OSTI)

We use a high-resolution cosmological simulation to predict the distribution of H I Ly? emission from the low-redshift (z 0.5) intergalactic medium (IGM). Our simulation can be used to reliably compute the emission from optically thin regions of the IGM but not that of self-shielded gas. We therefore consider several models that bracket the expected emission from self-shielded regions. Most galaxies are surrounded by extended (102 kpc) "coronae" of optically thin gas with Ly? surface brightness close to the expected background. Most of these regions contain smaller cores of dense, cool gas. Unless self-shielded gas is able to cool to T 4.1 K, these cores are much brighter than the background. The Ly? coronae represent "cooling flows" of IGM gas accreting onto galaxies. We also estimate the number of Ly? photons produced through the reprocessing of stellar ionizing radiation in the interstellar medium of galaxies; while this mechanism is responsible for the brightest Ly? emission, it occurs on small physical scales and can be separated using high-resolution observations. In all cases, we find that Ly? emitters are numerous (with a space density of ~0.1 h3 Mpc-3) and closely trace the filamentary structure of the IGM, providing a new way to map gas inside the cosmic web.

Steven R. Furlanetto; Joop Schaye; Volker Springel; Lars Hernquist



Pontotoc Co. Greene Co. Hale Co. OAK GROVE C OAL D EGAS CEDAR COVE  

U.S. Energy Information Administration (EIA) Indexed Site




U.S. Energy Information Administration (EIA) Indexed Site



Ly-alpha emission from GRB host galaxies  

E-Print Network (OSTI)

Ly-alpha emission is indicative of on-going star formation in a dust-poor environment. Ly-alpha imaging is therefore a probe of the star formation rate and of the dust-content of Gamma-Ray Burst host galaxies. Both of these parameters are central to our understanding of GRB progenitors and of how the environments affect the propagation of afterglow emission out of host galaxies. We have started a program aimed at imaging high redshift (z>2) host galaxies of GRBs at the Ly-alpha resonance line from neutral hydrogen. Here were report the results from imaging of the fields of GRB 000301C and GRB 000926 and outline upcoming observations of further hosts.

J. P. U. Fynbo; P. Moller; B. Thomsen; J. Hjorth; J. Gorosabel; M. I. Andersen; M. P. Egholm; S. Holland; B. L Jensen; H. Pedersen; M. Weidinger



Building the bridge between Damped Ly-alpha Absorbers and Lyman Break galaxies  

E-Print Network (OSTI)

In 2000, we started the program ``Building the Bridge between Damped Ly-alpha Absorbers and Lyman-Break Galaxies: Ly-alpha Selection of Galaxies'' at the European Southern Observatory's Very Large Telescope. This project is an attempt to use Ly-alpha selection of high-z galaxies to bridge the gap between absorption- and emission-selected galaxies by creating a large database of z=3 galaxies belonging to the abundant population of faint (R>25.5) galaxies probed by the Damped Ly-alpha Absorbers (DLAs). Here we present the first results of our program, namely the results from a deep Ly-alpha study of the field of the z=2.85 DLA towards Q2138-4427.

J. P. U. Fynbo; C. Ledoux; P. Moller; B. Thomsen; I. Burud; B. Leibundgut



Spatially Resolved Gas Kinematics within a Ly$\\alpha$ Nebula: Evidence for Large-scale Rotation  

E-Print Network (OSTI)

We use spatially extended measurements of Ly$\\alpha$ as well as less optically thick emission lines from an $\\approx$80 kpc Ly$\\alpha$ nebula at $z\\approx1.67$ to assess the role of resonant scattering and to disentangle kinematic signatures from Ly$\\alpha$ radiative transfer effects. We find that the Ly$\\alpha$, CIV, HeII, and CIII] emission lines all tell a similar story in this system, and that the kinematics are broadly consistent with large-scale rotation. First, the observed surface brightness profiles are similar in extent in all four lines, strongly favoring a picture in which the Ly$\\alpha$ photons are produced in situ instead of being resonantly scattered from a central source. Second, we see low kinematic offsets between Ly$\\alpha$ and the less optically thick HeII line ($\\sim$100-200 km s$^{-1}$), providing further support for the argument that the Ly$\\alpha$ and other emission lines are all being produced within the spatially extended gas. Finally, the full velocity field of the system shows cohe...

Prescott, Moire K M; Dey, Arjun



Levels of the Rab GDP dissociation inhibitor (GDI) are altered in the prenatal restrain stress mouse model of schizophrenia and are differentially regulated by the mGlu2/3 receptor agonists, LY379268 and LY354740  

Science Journals Connector (OSTI)

Abstract LY379268 and LY354740, two agonists of mGlu2/3 metabotropic glutamate receptors, display different potencies in mouse models of schizophrenia. This differential effect of the two drugs remains unexplained. We performed a proteomic analysis in cultured cortical neurons challenged with either LY379268 or LY354740. Among the few proteins that were differentially influenced by the two drugs, Rab GDP dissociation inhibitor-? (Rab GDI?) was down-regulated by LY379268 and showed a trend to an up-regulation in response to LY354740. In cultured hippocampal neurons, LY379268 selectively down-regulated the ? isoform of Rab GDI. Rab GDI inhibits the activity of the synaptic vesicle-associated protein, Rab3A, and is reduced in the brain of schizophrenic patients. We examined the expression of Rab GDI in mice exposed to prenatal stress (“PRS mice”), which have been described as a putative model of schizophrenia. Rab GDI? protein levels were increased in the hippocampus of PRS mice at postnatal days (PND)1 and 21, but not at PND60. At PND21, PRS mice also showed a reduced depolarization-evoked [3H]d-aspartate release in hippocampal synaptosomes. The increase in Rab GDI? levels in the hippocampus of PRS mice was reversed by a 7-days treatment with LY379268 (1 or 10 mg/kg, i.p.), but not by treatment with equal doses of LY354740. These data strengthen the validity of PRS mice as a model of schizophrenia, and show for the first time a pharmacodynamic difference between LY379268 and LY354740 which might be taken into account in an attempt to explain the differential effect of the two drugs across mouse models.

Rosamaria Orlando; Marina Borro; Marta Motolese; Gemma Molinaro; Sergio Scaccianoce; Alessandra Caruso; Luigi di Nuzzo; Filippo Caraci; Francesco Matrisciano; Anna Pittaluga; Jerome Mairesse; Maurizio Simmaco; Robert Nisticò; James A. Monn; Ferdinando Nicoletti



Properties of Ly-alpha and Gamma Ray Burst selected starbursts at high redshifts  

E-Print Network (OSTI)

Selection of starbursts through either deep narrow band imaging of redshifted Ly-alpha emitters, or localisation of host galaxies of gamma-ray bursts both give access to starburst galaxies that are significantly fainter than what is currently available from selection techniques based on the continuum (such as Lyman-break selection). We here present results from a survey for Ly-alpha emitters at z=3, conducted at the European Southern Observatory's Very Large Telescope. Furthermore, we briefly describe the properties of host galaxies of gamma-ray bursts at z>2. The majority of both Ly-alpha and gamma-ray burst selected starbursts are fainter than the flux limit of the Lyman-break galaxy sample, suggesting that a significant fraction of the integrated star formation at z~3 is located in galaxies at the faint end of the luminosity function.

J. P. U. Fynbo; B. Krog; K. Nilsson; G. Bjornsson; J. Hjorth; P. Jakobsson; C. Ledoux; P. Moller; B. Thomsen



Ly-alpha Emission from a Lyman Limit Absorber at z=3.036  

E-Print Network (OSTI)

Deep, 17.8 hours, narrow band imaging obtained at the ESO 3.5m New Technology Telescope has revealed extended (galaxy sized) Ly-alpha emission from a high redshift Lyman limit absorber. The absorber is a z(abs) approx. z(em) Lyman limit absorber seen in the spectrum of Q1205-30 at z(em)=3.036. The Ly-alpha luminosity of the emission line object is 12-14 x 10e41 h^-2 erg/s for Omega(matter)=1. The size and morphology of the Ly-alpha emitter are both near--identical to those of a previously reported emission line object associated with a DLA at z=1.934 (Fynbo et al. 1999a), suggesting a close connection between Lyman limit absorbers and DLAs. We also detect six candidate Ly-alpha emitting galaxies in the surrounding field at projected distances of 156-444 h^-1 kpc with Ly-alpha luminosities ranging from 3.3 to 9.5 x 10e41 h^-2 erg/s for Omega(matter)=1. Assuming no obscuration of Ly-alpha photons by dust this corresponds to star formation rates in the range 0.3-0.9 h^-2 M(sun)/yr. Comparing this to the the Lyman break galaxies in current ground based samples only make up the very bright end of the high redshift galaxy luminosity function. A significant, and possibly dominating, population of high redshift galaxies are not found in the ground based Lyman break surveys.

J. U. Fynbo; B. Thomsen; P. Moller



Inhibition of peptidoglycan biosynthesis in gram-positive bacteria by LY146032.  

Science Journals Connector (OSTI)

...UDP-MurNAc-pentapeptide precursor in the cytoplasm of intact bacteria (12, 14). Surprisingly, however, inhibition by LY146032 in intact S. aureus as well as B. megaterium...Cambridge. 19. Ringrose, P. S. 1985. Warhead delivery and suicide substrates as...

N E Allen; J N Hobbs; W E Alborn Jr



Immune responses in mice deficient in Ly-GDI, a lymphoid-specific regulator of Rho \\{GTPases\\}  

Science Journals Connector (OSTI)

Ly-GDI (lymphoid-specific guanosine diphosphate (GDP) dissociation inhibitor), also called D4-GDI, is preferentially expressed in hematopoietic tissues including bone marrow, thymus, spleen and lymph nodes. It binds to the small guanosine triphosphate (GTP)-binding protein Rho and inhibits GDP dissociation from Rho proteins. To explore the function of Ly-GDI in lymphocytes, we have generated Ly-GDI-deficient mice by gene targeting. These mice showed no striking abnormalities of lymphoid development or thymocyte selection. The mice also exhibited, for the most part, normal immune responses including lymphocyte proliferation, IL-2 production, cytotoxic T lymphocyte activity, antibody production, antigen processing and presentation, immune cell aggregation and migration, and protection against an intracellular protozoan. However, Ly-GDI-deficient mice exhibited deregulated T and B cell interactions after in vitro cultivation of mixed lymphocyte populations in concanavalin A (Con A) leading to overexpansion of B lymphocytes. Further studies revealed that Ly-GDI deficiency decreased IL-2 withdrawal apoptosis of lymph node cells while dexamethasone- and T cell receptor-induced apoptosis remained intact. These data implicate the regulation of the Rho \\{GTPase\\} by Ly-GDI in lymphocyte survival and responsiveness, but suggest that these functions may be partially complemented by other Rho regulatory proteins when the LyGDI protein is deficient.

Li Yin; Pamela Schwartzberg; Tanya M. Scharton-kerstenj; Louis Staudt; Michael Lenardo



The Gas Reservoir for present day Galaxies : Damped Ly-alpha Absorption Systems  

E-Print Network (OSTI)

We present results from an ongoing search for galaxy counterparts of a subgroup of Quasar Absorption Line Systems called Damped Ly-alpha Absorbers (DLAs). DLAs have several characteristics that make them essential in the process of understanding how galaxies formed in the early universe and evolved to the galaxies we see today in the local universe. Finally we compare DLAs with recent findings of a population of starforming galaxies at high redshifts, so called Lyman-break galaxies.

J. U. Fynbo; B. Thomsen; P. Moller



White dwarf atmosphere models with Ly-$?$ opacity in the analysis of the white dwarf cooling sequence of NGC 6397  

E-Print Network (OSTI)

We discuss the importance of pure hydrogen white dwarf atmosphere models with Ly-$\\rm \\alpha$ far red wing opacity in the analysis of the white dwarf cooling sequence of the globular cluster NGC 6397. Our recently improved atmosphere models account for the previously missing opacity from the Ly-$\\rm \\alpha$ hydrogen line broadened by collisions of the absorbing hydrogen atoms with molecular and atomic hydrogen. These models are the first that well reproduce the UV colors and spectral energy distributions of cool white dwarfs with $T_{\\rm eff}white dwarf cooling sequence using atmosphere models that do not include the correct Ly-$\\alpha$ opacity is underestimated by $\\sim 0.5$ Gyr. Our analysis shows that it is essential to use white dwarf atmosphere models with Ly-$\\rm \\alpha$ opacity for precise dating of old stellar populations from white dwarf cooling sequences.

Piotr M. Kowalski



Chandra Detection of OVIII Ly-alpha Absorption from an Overdense Region in the Intergalactic Medium  

E-Print Network (OSTI)

We report the first detection of an OVIII Ly-alpha absorption line associated with an overdense region in the intergalactic medium (IGM) along the sightline towards PKS 2155-304 with the Chandra Low Energy Transmission Grating Spectrometer (LETGS). The absorption line is detected at 4.5 sigma level with cz~16,600 km/s. At the same velocity Shull et al.(1998) detected a small group of spiral galaxies (with an overdensity of delta_gal ~ 100) and low metallicity HI Ly-alpha clouds. We constrain the intragroup gas that gives rise to the OVIII Ly-alpha line to a baryon density in the range 1e-5 solar abundance. These estimates are in accordance with those of the warm/hot intergalactic medium (WHIM) that are predicted from hydrodynamic simulations. Extrapolating from this single detection implies a large fraction of the ``missing baryons'' (~ 10%, or ~ 30-40% of the WHIM) are probed by the OVIII absorber.

T. Fang; H. L. Marshall; J. C. Lee; D. S. Davis; C. R. Canizares



Evidence of patchy hydrogen reionization from an extreme Ly$\\alpha$ trough below redshift six  

E-Print Network (OSTI)

We report the discovery of an extremely long ($\\sim$110 Mpc/$h$) and dark ($\\tau_{\\rm eff} \\gtrsim 7$) Ly$\\alpha$ trough extending down to $z \\simeq 5.5$ towards the $z_{\\rm em} \\simeq 6.0$ quasar ULAS J0148+0600. We use these new data in combination with Ly$\\alpha$ forest measurements from 42 quasars at $4.5 \\le z_{\\rm em} \\le 6.4$ to conduct an updated analysis of the line-of-sight variance in the intergalactic Ly$\\alpha$ opacity over $4 \\le z \\le 6$. We find that the scatter in transmission among lines of sight near $z \\sim 6$ significantly exceeds theoretical expectations for either a uniform ultraviolet background (UVB) or simple fluctuating UVB models in which the mean free path to ionizing photons is spatially invariant. The data, particularly near $z \\simeq 5.6$-5.8, instead require fluctuations in the volume-weighted hydrogen neutral fraction that are a factor three or more beyond those expected from density variations alone. We argue that these fluctuations are most likely driven by large-scale vari...

Becker, George D; Madau, Piero; Pettini, Max; Ryan-Weber, Emma V; Venemans, Bram P


Note: This page contains sample records for the topic "vleet hol ly" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


A simple analytical model for the abundance of damped Ly-?absorbers  

E-Print Network (OSTI)

A simple analytical model for estimating the fraction (\\Omega_{gas}) of matter in gaseous form within the collapsed dark matter (DM) haloes is presented. The model is developed using (i) the Press-Schechter formalism to estimate the fraction of baryons in DM haloes, and (ii) the observational estimates of the star formation rate at different redshifts. The prediction for \\Omega_{gas} from the model is in broad agreement with the observed abundance of the damped Ly-\\alpha systems. Furthermore, it can be used for estimating the circular velocities of the collapsed haloes at different redshifts, which could be compared with future observations.

T. Roy Choudhury; T. Padmanabhan



An on-going multi-wavelength survey of Ly-alpha emitters at redshifts z = 2 - 8  

E-Print Network (OSTI)

In the last decade, the technique of finding Ly-alpha emitters through narrow-band imaging has become a promising method of detecting high redshift galaxies. Ly-alpha emitters have been found from redshifts z ~ 2, up to the highest redshift source known to date at z = 6.96. Several surveys are also underway to find z = 7 - 9 sources. But these very high redshift sources are too faint to be studied in great detail, and more information can be found from studying the same class of objects at lower redshifts. Here we present our survey strategy to determine the nature of Ly-alpha emitters at lower redshifts, through multi-wavelength surveys, and our plans to extend the survey to redshift z = 8.8.

Kim K. Nilsson; Johan P. U. Fynbo; Palle Moller; Alvaro Orsi



Synergy of CO/[CII]/Ly$\\alpha$ Line Intensity Mapping with the SKA  

E-Print Network (OSTI)

We present the science enabled by cross-correlations of the SKA1-LOW 21-cm EoR surveys with other line mapping programs. In particular, we identify and investigate potential synergies with planned programs, such as the line intensity mapping of redshifted CO rotational lines, [CII] and Ly-$\\alpha$ emissions during reionization. We briefly describe how these tracers of the star-formation rate at $z \\sim 8$ can be modeled jointly before forecasting their auto- and cross-power spectra measurements with the nominal 21cm EoR survey. The use of multiple line tracers would be invaluable to validate and enrich our understanding of the EoR.

Chang, Tzu-Ching; Santos, Mario; Silva, Marta; Aguirre, James; Doré, Olivier; Pritchard, Jonathan



with Earth's Theia component; thus, it is present-ly not possible to obtain information on D17  

E-Print Network (OSTI)

with Earth's Theia component; thus, it is present- ly not possible to obtain information on D17 O of the proto-Earth. An alternative explanation for the isotope difference between Earth and the Moon is that the D17 O value of Earth was modified by late- accreting material (late veneer) after the for- mation

Napp, Nils


Effects of excitation laser wavelength on Ly-a and He-a line emission from nitrogen plasmas  

E-Print Network (OSTI)

are soft x-ray lasers,6,7 laser-produced plasma (LPP) sources,8­11 and higher har- monics from laser heatedEffects of excitation laser wavelength on Ly-a and He-a line emission from nitrogen plasmas S. S November 2012; accepted 27 December 2012; published online 11 January 2013) Laser-produced nitrogen plasmas

Harilal, S. S.


Edward S. Van Vleet, Peter M. Williams. Sampling sea surface films ...  

Science Journals Connector (OSTI)

May 21, 1979 ... tive of naturally occurring films. Stainless steel .... rally occuring sea surface films present in uncontaminated areas ... radiation; an-. HAM. 1979.




SciTech Connect

We search for evidence of diffuse Ly? emission from extended neutral hydrogen surrounding Ly? emitting galaxies (LAEs) using deep narrow-band images of the Extended Chandra Deep Field South. By stacking the profiles of 187 LAEs at z = 2.06, 241 LAEs at z = 3.10, and 179 LAEs at z = 3.12, and carefully performing low-surface brightness photometry, we obtain mean surface brightness maps that reach 9.9, 8.7, and 6.2 × 10{sup –19} erg cm{sup –2} s{sup –1} arcsec{sup –2} in the emission line. We undertake a thorough investigation of systematic uncertainties in our surface brightness measurements and find that our limits are 5-10 times larger than would be expected from Poisson background fluctuations; these uncertainties are often underestimated in the literature. At z ? 3.1, we find evidence for extended halos with small-scale lengths of 5-8 kpc in some but not all of our sub-samples. We demonstrate that sub-samples of LAEs with low equivalent widths and brighter continuum magnitudes are more likely to possess such halos. At z ? 2.1, we find no evidence of extended Ly? emission down to our detection limits. Through Monte-Carlo simulations, we also show that we would have detected large diffuse LAE halos if they were present in our data sets. We compare these findings to other measurements in the literature and discuss possible instrumental and astrophysical reasons for the discrepancies.

Feldmeier, John J. [Department of Physics and Astronomy, Youngstown State University, Youngstown, OH 44555 (United States); Hagen, Alex; Ciardullo, Robin; Gronwall, Caryl; Hagen, Lea M. Z. [Department of Astronomy and Astrophysics, The Pennsylvania State University, University Park, PA 16802 (United States); Gawiser, Eric; Kurczynski, Peter [Department of Physics and Astronomy, Rutgers, The State University of New Jersey, Piscataway, NJ 08854 (United States); Guaita, Lucia [Oskar Klein Cosmology Centre, Department of Astronomy, Stockholm University, SE-106 91 Stolkholm (Sweden); Bond, Nicholas A. [Cosmology Laboratory (Code 665), NASA Goddard Space Flight Center, Greenbelt, MD 20771 (United States); Acquaviva, Viviana [Department of Physics, New York City College of Technology, City University of New York, 300 Jay Street, Brooklyn, NY 11201 (United States); Blanc, Guillermo A. [Observatories of the Carnegie Institution of Washington, 813 Santa Barbara Street, Pasadena, CA 91101 (United States); Orsi, Alvaro, E-mail: jjfeldmeier@ysu.edu [Departamento de Astronomía y Astrofísica, Pontificia Universidad Católica, Av. Vicuña Mackenna 4860, Santiago (Chile)




SciTech Connect

We use 2167 Sloan Digital Sky Survey quasar spectra to search for low-density oxygen in the intergalactic medium (IGM). Oxygen absorption is detected on a pixel-by-pixel basis by its correlation with Ly{alpha} forest absorption. We have developed a novel locally calibrated pixel (LCP) search method that uses adjacent regions of the spectrum to calibrate interlopers and spectral artifacts, which would otherwise limit the measurement of O VI absorption. Despite the challenges presented by searching for weak O VI within the Ly{alpha} forest in spectra of moderate resolution and signal-to-noise, we find a highly significant detection of absorption by oxygen at 2.7 < z < 3.2 (the null hypothesis has a {chi}{sup 2} = 80 for nine data points). We interpret our results using synthetic spectra generated from a log-normal density field assuming a mixed quasar-galaxy photoionizing background and that it dominates the ionization fraction of detected O VI. The LCP search data can be fit by a constant metallicity model with [O/H] = -2.15{sup +0.07}{sub -0.09} but also by models in which low-density regions are unenriched and higher density regions have a higher metallicity. The density-dependent enrichment model by Aguirre et al. is also an acceptable fit. All our successful models have similar mass-weighted oxygen abundance, corresponding to [(O/H){sub MW}] = -2.45 {+-} 0.06. This result can be used to find the cosmic oxygen density in the Ly{alpha} forest, {Omega}{sub Oxy,IGM} = 1.4({+-}0.2) x 10{sup -6} {approx} 3 x 10{sup -4{Omega}}{sub b}. This is the tightest constraint on the mass-weighted mean oxygen abundance and the cosmic oxygen density in the Ly{alpha} forest to date and indicates that it contains {approx}16% of the total expected metal production by star formation up to z = 3.

Pieri, Matthew M.; Frank, Stephan; Mathur, Smita; Weinberg, David H. [Department of Astronomy, Ohio State University, 140 West 18th Avenue, Columbus, OH 43210 (United States); York, Donald G. [Department of Astronomy and Astrophysics, University of Chicago, Chicago, IL 60637 (United States); Oppenheimer, Benjamin D., E-mail: mpieri@astronomy.ohio-state.ed [Astronomy Department, University of Arizona, Tucson, AZ 85721 (United States)



Pharmacological characterization of LY233053: A structurally novel tetrazole-substituted competitive N-methyl-D-aspartic acid antagonist with a short duration of action  

SciTech Connect

This study reports the activity of a structurally novel excitatory amino acid receptor antagonist, LY233053 (cis-(+-)-4-((2H-tetrazol-5-yl)methyl)piperidine-2-carboxylic acid), the first tetrazole-containing competitive N-methyl-D-aspartic acid (NMDA) antagonist. LY233053 potently inhibited NMDA receptor binding to rat brain membranes as shown by the in vitro displacement of (3H) CGS19755 (IC50 = 107 +/- 7 nM). No appreciable affinity in (3H)alpha-amino-3-hydroxy-5-methylisoxazole-4-propionic acid (AMPA) or (3H)kainate binding assays was observed (IC50 values greater than 10,000 nM). In vitro NMDA receptor antagonist activity was further demonstrated by selective inhibition of NMDA-induced depolarization in cortical wedges (IC50 = 4.2 +/- 0.4 microM vs. 40 microM NMDA). LY233053 was effective after in vivo systemic administration in a number of animal models. In neonatal rats, LY233053 selectively blocked NMDA-induced convulsions (ED50 = 14.5 mg/kg i.p.) with a relatively short duration of action (2-4 hr). In pigeons, LY233053 potently antagonized (ED50 = 1.3 mg/kg i.m.) the behavioral suppressant effects of 10 mg/kg of NMDA. However, a dose of 160 mg/kg, i.m., was required to produce phencyclidine-like catalepsy in pigeons. In mice, LY233053 protected against maximal electroshock-induced seizures at lower doses (ED50 = 19.9 mg/kg i.p.) than those that impaired horizontal screen performance (ED50 = 40.9 mg/kg i.p.). Cholinergic and GABAergic neuronal degenerations after striatal infusion of NMDA were prevented by single or multiple i.p. doses of LY233053. In summary, the antagonist activity of LY233053 after systemic administration demonstrates potential therapeutic value in conditions of neuronal cell loss due to NMDA receptor excitotoxicity.

Schoepp, D.D.; Ornstein, P.L.; Leander, J.D.; Lodge, D.; Salhoff, C.R.; Zeman, S.; Zimmerman, D.M. (Eli Lilly and Company, Indianapolis, IN (USA))




SciTech Connect

The Ly{alpha} line of He II at 304 Angstrom-Sign is one of the spectral lines of choice for EUV channels of narrowband imagers on board space telescopes, which provide spectacular intensity images of the outer solar atmosphere. Since the magnetic field information is encoded in the polarization of the spectral line radiation, it is important to investigate whether the He II line radiation from the solar disk can be polarized, along with its magnetic sensitivity. Here we report some theoretical predictions concerning the linear polarization signals produced by scattering processes in this strong emission line of the solar transition region, taking into account radiative transfer and the Hanle effect caused by the presence of organized and random magnetic fields. We find that the fractional polarization amplitudes are significant ({approx}1%), even when considering the wavelength-integrated signals. Interestingly, the scattering polarization of the Ly{alpha} line of He II starts to be sensitive to the Hanle effect for magnetic strengths B {approx}> 100 G (i.e., for magnetic strengths of the order of and larger than the Hanle saturation field of the hydrogen Ly{alpha} line at 1216 Angstrom-Sign ). We therefore propose simultaneous observations of the scattering polarization in both Ly{alpha} lines to facilitate magnetic field measurements in the upper solar chromosphere. Even the development of a narrowband imaging polarimeter for the He II 304 Angstrom-Sign line alone would be already of great diagnostic value for probing the solar transition region.

Trujillo Bueno, Javier; Stepan, Jiri; Belluzzi, Luca, E-mail: jtb@iac.es, E-mail: stepan@iac.es, E-mail: belluzzi@iac.es [Instituto de Astrofisica de Canarias, 38205 La Laguna, Tenerife (Spain)



http://hol.sagepub.com/ The Holocene  

E-Print Network (OSTI)

Fialkiewicz-Koziel, Sarah A Finkelstein, Mariusz Galka, Michelle Garneau, Dan Andersson, Christopher Bochicchio, Keith Barber, Lisa R Belyea, Joan Bunbury, Frank M Chambers, Daniel J Charman, Julie Loisel Camill,3 Jukka Alm,4 Matthew J Amesbury,5 David Anderson,6 Sofia Andersson,7 Christopher Bochicchio,1

Turetsky, Merritt



SciTech Connect

By combining data from the NASA Wide-field Infrared Survey Explorer (WISE) mission with optical spectroscopy from the W. M. Keck telescope, we discover a mid-IR color criterion that yields a 78% success rate in identifying rare, typically radio-quiet, 1.6 {approx}< z {approx}< 4.6 dusty Ly{alpha} emitters (LAEs). Of these, at least 37% have emission extended on scales of 30-100 kpc and are considered Ly{alpha} ''blobs'' (LABs). The objects have a surface density of only {approx}0.1 deg{sup -2}, making them rare enough that they have been largely missed in deep, small area surveys. We measured spectroscopic redshifts for 92 of these galaxies, and find that the LAEs (LABs) have a median redshift of 2.3 (2.5). The WISE photometry coupled with data from Herschel (Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA) reveals that these galaxies are in the Hyper Luminous IR galaxy regime (L{sub IR} {approx}> 10{sup 13}-10{sup 14} L{sub Sun }) and have warm colors. They are typically more luminous and warmer than other dusty, z {approx} 2 populations such as submillimeter-selected galaxies and dust-obscured galaxies. These traits are commonly associated with the dust being illuminated by intense active galactic nucleus activity. We hypothesize that the combination of spatially extended Ly{alpha}, large amounts of warm IR-luminous dust, and rarity (implying a short-lived phase) can be explained if the galaxies are undergoing brief, intense ''feedback'' transforming them from an extreme dusty starburst/QSO into a mature galaxy.

Bridge, Carrie R. [California Institute of Technology, MS249-17, Pasadena, CA 91125 (United States); Blain, Andrew [Department of Physics and Astronomy, University of Leicester, LE1 7RH Leicester (United Kingdom); Borys, Colin J. K.; Griffith, Roger L.; Tsai, Chao-Wei [Infrared Processing and Analysis Center, California Institute of Technology, MS 100-22, Pasadena, CA 91125 (United States); Petty, Sara; Farrah, Duncan [Department of Physics, Virginia Polytechnic Institute and State University, Blacksburg, VA 24061 (United States); Benford, Dominic [NASA Goddard Space Flight Center, Greenbelt, MD 20771 (United States); Eisenhardt, Peter; Stern, Daniel; Wu Jingwen [Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Dr., Pasadena, CA 91109 (United States); Jarrett, Tom [Astronomy Department, University of Cape Town, Rondebosch 7701 (South Africa); Lonsdale, Carol [National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 22903 (United States); Stanford, Spencer A. [Department of Physics, University of California Davis, One Shields Ave., Davis, CA 95616 (United States); Wright, Edward L., E-mail: bridge@astro.caltech.edu [Astronomy Department, University of California Los Angeles, Los Angeles, CA 90095 (United States)



The {ital b} Distribution and the Velocity Structure of Absorption Peaks in the Ly{alpha} Forest  

SciTech Connect

A theory is developed that relates the observed {ital b} parameter of a Ly{alpha} absorption line to the velocity curvature of the corresponding peak in the optical depth fluctuation. Its relation to the traditional interpretation of {ital b} as the thermal broadening width is discussed. It is demonstrated that, independent of the details of the cosmological model, the differential {ital b} distribution has a high-{ital b} asymptote of dN/db{proportional_to}b{sup {minus}m}, where m{ge}5, when we make the reasonable assumption that low-curvature fluctuations are statistically favored over high-curvature ones. There in general always exist lines much broader than the thermal width. We develop a linear perturbative analysis of the optical depth fluctuation, which yields a single-parameter prediction for the full {ital b} distribution. In addition to exhibiting the high-velocity tail, it qualitatively explains the observed sharp low-{ital b} cutoff{emdash}a simple reflection of the fact that high-curvature fluctuations are relatively rare. Although the existence of the high-{ital b} asymptote, which is independent of the validity of the linear expansion, is consistent with the observed {ital b} distribution, a detailed comparison of the linear prediction with six observational data sets indicates that higher order corrections are not negligible. The perturbative analysis nonetheless offers valuable insights into the dependence of the {ital b} distribution on cosmological parameters such as {Omega} and the power spectrum. A key parameter is the effective smoothing scale of the optical depth fluctuation, which is in turn determined by three scales: the thermal broadening width, the baryon smoothing scale (approximately the Jeans scale), and the observation/simulation resolution. The first two are determined by reionization history, but are comparable in general, whereas the third varies by about an order of magnitude in current hydrodynamic simulations. Studies with non{endash}resolution-dominated {ital b} distributions can be used to probe the reionization history of the universe. {copyright} {ital {copyright} 1999.} {ital The American Astronomical Society}

Hui, L. [NASA/Fermilab Astrophysics Center, Fermi National Accelerator Laboratory, Batavia, IL 60510 (United States)] [NASA/Fermilab Astrophysics Center, Fermi National Accelerator Laboratory, Batavia, IL 60510 (United States); Rutledge, R.E. [Max-Planck-Institut fuer extraterrestrische Physik, Postfach 1603, D-85740 Garching (Germany)] [Max-Planck-Institut fuer extraterrestrische Physik, Postfach 1603, D-85740 Garching (Germany)



The [ital b] Distribution and the Velocity Structure of Absorption Peaks in the Ly[alpha] Forest  

SciTech Connect

A theory is developed that relates the observed [ital b] parameter of a Ly[alpha] absorption line to the velocity curvature of the corresponding peak in the optical depth fluctuation. Its relation to the traditional interpretation of [ital b] as the thermal broadening width is discussed. It is demonstrated that, independent of the details of the cosmological model, the differential [ital b] distribution has a high-[ital b] asymptote of dN/db[proportional to]b[sup [minus]m], where m[ge]5, when we make the reasonable assumption that low-curvature fluctuations are statistically favored over high-curvature ones. There in general always exist lines much broader than the thermal width. We develop a linear perturbative analysis of the optical depth fluctuation, which yields a single-parameter prediction for the full [ital b] distribution. In addition to exhibiting the high-velocity tail, it qualitatively explains the observed sharp low-[ital b] cutoff[emdash]a simple reflection of the fact that high-curvature fluctuations are relatively rare. Although the existence of the high-[ital b] asymptote, which is independent of the validity of the linear expansion, is consistent with the observed [ital b] distribution, a detailed comparison of the linear prediction with six observational data sets indicates that higher order corrections are not negligible. The perturbative analysis nonetheless offers valuable insights into the dependence of the [ital b] distribution on cosmological parameters such as [Omega] and the power spectrum. A key parameter is the effective smoothing scale of the optical depth fluctuation, which is in turn determined by three scales: the thermal broadening width, the baryon smoothing scale (approximately the Jeans scale), and the observation/simulation resolution. The first two are determined by reionization history, but are comparable in general, whereas the third varies by about an order of magnitude in current hydrodynamic simulations. Studies with non[endash]resolution-dominated [ital b] distributions can be used to probe the reionization history of the universe. [copyright] [ital [copyright] 1999.] [ital The American Astronomical Society

Hui, L. (NASA/Fermilab Astrophysics Center, Fermi National Accelerator Laboratory, Batavia, IL 60510 (United States)); Rutledge, R.E. (Max-Planck-Institut fuer extraterrestrische Physik, Postfach 1603, D-85740 Garching (Germany))



Intergalactic Medium Emission Observations with the Cosmic Web Imager. II. Discovery of Extended, Kinematically Linked Emission around SSA22 Ly? Blob 2  

Science Journals Connector (OSTI)

The intergalactic medium (IGM) is the dominant reservoir of baryons, delineates the large-scale structure of the universe at low to moderate overdensities, and provides gas from which galaxies form and evolve. Simulations of a cold-dark-matter- (CDM-) dominated universe predict that the IGM is distributed in a cosmic web of filaments and that galaxies should form along and at the intersections of these filaments. While observations of QSO absorption lines and the large-scale distribution of galaxies have confirmed the CDM paradigm, the cosmic web of IGM has never been confirmed by direct imaging. Here we report our observation of the Ly? blob 2 (LAB2) in SSA22 with the Cosmic Web Imager (CWI). This is an integral field spectrograph optimized for low surface brightness, extended emission. With 22 hr of total on- and off-source exposure, CWI has revealed that LAB2 has extended Ly? emission that is organized into azimuthal zones consistent with filaments. We perform numerous tests with simulations and the data to secure the robustness of this result, which relies on data with modest signal-to-noise ratios. We have developed a smoothing algorithm that permits visualization of data cube slices along image or spectral image planes. With both raw and smoothed data cubes we demonstrate that the filaments are kinematically associated with LAB2 and display double-peaked profiles characteristic of optically thick Ly? emission. The flux is 10-20 times brighter than expected for the average emission from the IGM but is consistent with boosted fluorescence from a buried QSO or gravitation cooling radiation. Using simple emission models, we infer a baryon mass in the filaments of at least 1-4 ? 1011 M ?, and the dark halo mass is at least 2 ? 1012 M ?. The spatial-kinematic morphology is more consistent with inflow from the cosmic web than outflow from LAB2, although an outflow feature maybe present at one azimuth. LAB2 and the surrounding gas have significant and coaligned angular momentum, strengthening the case for their association.

D. Christopher Martin; Daphne Chang; Matt Matuszewski; Patrick Morrissey; Shahin Rahman; Anna Moore; Charles C. Steidel; Yuichi Matsuda



The sources of extended continuum emission towards Q0151+048A : The host galaxy and the Damped Ly-alpha Absorber  

E-Print Network (OSTI)

We present deep imaging in the U, B and I bands obtained under excellent seeing conditions of the double quasar Q0151+048A,B and of the Damped Ly-alpha (DLA) absorbing galaxy at z(abs) = 1.9342 named S4. We analyse the data employing two separate and independent methods. First we deconvolve the images using the MCS algorithm, secondly we decompose the images via an object based iteration process where we fit models to objects without any attempt to improve the resolution of the data. Our detailed analysis of the images reveals, somewhat surprisingly, that extended objects centred on the quasars themselves are much brighter continuum sources than the DLA galaxy. Due to the complexity caused by the many superimposed objects, we are unable to certify whether or not continuum emission from the DLA galaxy is detected. Continuum emission from the extended objects centred on the positions of the quasars is clearly seen, and the objects are tentatively identified as the ``host galaxies'' of the quasars. The flux of those host galaxies is of order 2--6% of the quasar flux, and the light profile of the brighter of the two is clearly best fit with a de Vaucouleurs profile. We discuss two alternative interpretations of the origin of the extended flux: i) the early stage of a massive elliptical galaxy in the process of forming the bulk of its stars, and ii) quasar light scattered by dust.

J. U. Fynbo; I. Burud; P. Moller




SciTech Connect

Recent theoretical investigations have pointed out that the cores of the Ly{alpha} lines of H I and He II should show measurable scattering polarization signals when observing the solar disk, and that the magnetic sensitivity, through the Hanle effect, of such linear polarization signals is suitable for exploring the magnetism of the solar transition region. Such investigations were carried out in the limit of complete frequency redistribution (CRD) and neglecting quantum interference between the two upper J-levels of each line. Here we relax both approximations and show that the joint action of partial frequency redistribution and J-state interference produces much more complex fractional linear polarization (Q/I) profiles, with large amplitudes in their wings. Such wing polarization signals turn out to be very sensitive to the temperature structure of the atmospheric model, so that they can be exploited for constraining the thermal properties of the solar chromosphere. Finally, we show that the approximation of CRD without J-state interference is however suitable for estimating the amplitude of the linear polarization signals in the core of the lines, where the Hanle effect operates.

Belluzzi, Luca; Trujillo Bueno, Javier [Instituto de Astrofisica de Canarias, E-38205 La Laguna, Tenerife (Spain); Stepan, Jiri [Astronomical Institute ASCR, Ondrejov (Czech Republic)




SciTech Connect

We present the elemental abundance and H{sub 2} content measurements of a damped Ly{alpha} (DLA) system with an extremely large H I column density, log N(H I) (cm{sup -2}) = 22.0 {+-} 0.10, at z{sub abs} = 3.287 toward the QSO SDSS J081634+144612. We measure column densities of H{sub 2}, C I, C I*, Zn II, Fe II, Cr II, Ni II, and Si II from a high signal-to-noise and high spectral resolution VLT-UVES spectrum. The overall metallicity of the system is [Zn/H] = -1.10 {+-} 0.10 relative to solar. Two molecular hydrogen absorption components are seen at z = 3.28667 and 3.28742 (a velocity separation of Almost-Equal-To 52 km s{sup -1}) in rotational levels up to J = 3. We derive a total H{sub 2} column density of log N(H{sub 2}) (cm{sup -2}) = 18.66 and a mean molecular fraction of f = 2N(H{sub 2})/[2N(H{sub 2}) + N(H I)] = 10{sup -3.04{+-}0.37}, typical of known H{sub 2}-bearing DLA systems. From the observed abundance ratios we conclude that dust is present in the interstellar medium of this galaxy, with an enhanced abundance in the H{sub 2}-bearing clouds. However, the total amount of dust along the line of sight is not large and does not produce any significant reddening of the background QSO. The physical conditions in the H{sub 2}-bearing clouds are constrained directly from the column densities of H{sub 2} in different rotational levels, C I and C I*. The kinetic temperature is found to be T Almost-Equal-To 75 K and the particle density lies in the range n{sub H} = 50-80 cm{sup -3}. The neutral hydrogen column density of this DLA is similar to the mean H I column density of DLAs observed at the redshift of {gamma}-ray bursts (GRBs). We explore the relationship between GRB-DLAs and the high column density end of QSO-DLAs finding that the properties (metallicity and depletion) of DLAs with log N(H I) > 21.5 in the two populations do not appear to be significantly different.

Guimaraes, R. [Programa de Modelagem Computacional-SENAI-Cimatec, 41650-010 Salvador, Bahia (Brazil); Noterdaeme, P.; Petitjean, P. [UPMC-CNRS, UMR7095, Institut d'Astrophysique de Paris, 98bis Blvd. Arago, F-75014 Paris (France); Ledoux, C. [European Southern Observatory, Alonso de Cordova 3107, Casilla 19001, Vitacura, Santiago 19 (Chile); Srianand, R.; Rahmani, H. [Inter-University Centre for Astronomy and Astrophysics, Post Bag 4, Ganeshkhind, Pune 411007 (India); Lopez, S., E-mail: rguimara@eso.org [Departamento de Astronomia, Universidad de Chile, Casilla 36-D, Santiago (Chile)



A SEARCH FOR C II 158 {mu}m LINE EMISSION IN HCM 6A, A Ly{alpha} EMITTER AT z = 6.56  

SciTech Connect

We report a Plateau de Bure Interferometer search for C II 158 {mu}m emission from HCM 6A, a lensed Ly{alpha} emitter (LAE) at z = 6.56. Our non-detections of C II 158 {mu}m line emission and 1.2 mm radio continuum emission yield 3{sigma} limits of L{sub CII} < 6.4 x 10{sup 7} x ({Delta}V/100 km s{sup -1}){sup 1/2} L{sub Sun} for the C II 158 {mu}m line luminosity and S{sub 1.2mm} < 0.68 mJy for the 1.2 mm flux density. The local conversion factor between L{sub CII} and the star formation rate (SFR) yields an SFR < 4.7 M{sub Sun} yr{sup -1}, Almost-Equal-To 2 times lower than that inferred from the ultraviolet (UV) continuum, suggesting that the local factor may not be applicable in high-z LAEs. The non-detection of 1.2 mm continuum emission yields a total SFR < 28 M{sub Sun} yr{sup -1}; any obscured star formation is thus within a factor of two of the visible star formation. Our best-fit model to the rest-frame UV/optical spectral energy distribution of HCM 6A yields a stellar mass of 1.3 Multiplication-Sign 10{sup 9} M{sub Sun} and an SFR of Almost-Equal-To 10 M{sub Sun} yr{sup -1}, with negligible dust obscuration. We fortuitously detect CO J = 3-2 emission from a z = 0.375 galaxy in the foreground cluster A370, and obtain a CO line luminosity of L'(CO) > (8.95 {+-} 0.79) Multiplication-Sign 10{sup 8} K km s{sup -1} pc{sup 2} and a molecular gas mass of M(H{sub 2}) > (4.12 {+-} 0.36) Multiplication-Sign 10{sup 9} M{sub Sun }, for a CO-to-H{sub 2} conversion factor of 4.6 M{sub Sun} (K km s{sup -1} pc{sup 2}){sup -1}.

Kanekar, Nissim [National Centre for Radio Astrophysics, Tata Institute of Fundamental Research, Pune 411 007 (India); Wagg, Jeff [European Southern Observatory, Alonso de Cordova 3107, Vitacura, Casilla 19001, Santiago 19 (Chile); Chary, Ranga Ram [U.S. Planck Data Center, MS220-6 Caltech, Pasadena, CA 91125 (United States); Carilli, Christopher L., E-mail: nkanekar@ncra.tifr.res.in [National Radio Astronomy Observatory, P.O. Box O, Socorro, NM 87801 (United States)



The Subaru Ly? blob survey: a sample of 100-kpc Ly? blobs at z = 3  

Science Journals Connector (OSTI)

......All-Sky Point Source Catalog, NASA/IPAC Infrared Science Archive, http://irsa.ipac.caltech.edu/applications/Gator/ . Dey A. , et al, 2005, ApJ, 629, 654. Dijkstra M. , Loeb A., 2009, MNRAS, 400, 1109. Faucher-Giguere C......

Y. Matsuda; T. Yamada; T. Hayashino; R. Yamauchi; Y. Nakamura; N. Morimoto; M. Ouchi; Y. Ono; K. Kousai; E. Nakamura; M. Horie; T. Fujii; M. Umemura; M. Mori


Note: This page contains sample records for the topic "vleet hol ly" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


HolT Hunter: Software for Identifying and Characterizing Low-Strain DNA Holliday Triangles  

SciTech Connect

Synthetic DNA nanostructures are most commonly held together via Holliday junctions. These junctions allow for a wide variety of different angles between the double helices they connect. Nevertheless, only constructs with a very limited selection of angles have been built, to date, because of the computational complexity of identifying structures that fit together with low strain at odd angles. I have developed an algorithm that finds over 95% of the possible solutions by breaking the problem down into two portions. First, there is a problem of how smooth rods can form triangles by lying across one another. This problem is easily handled by numerical computation. Second, there is the question of how distorted DNA double helices would need to be to fit onto the rod structure. This strain is calculated directly. The algorithm has been implemented in a Mathematica 8 notebook called Holliday Triangle Hunter. A large database of solutions has been identified. Additional interface software is available to facilitate drawing and viewing models.

Sherman W. B.



Automatic In Situ Identification of Plankton Matthew B. Blaschko, Gary Holness, Marwan A. Mattar, Dimitri Lisin,  

E-Print Network (OSTI)

micro­organisms known as plankton. As the foundation of the food chain for marine life, plankton Cytometer And Microscope (FlowCAM), that detects par­ ticles from a stream of water siphoned directly from challenge. We expect that upon completion, our system will become a use­ ful tool for marine biologists

Massachusetts at Amherst, University of


Julian Ly Davis, Ph.D. 315 Engineering Lab  

E-Print Network (OSTI)

, Virginia Tech, Thesis: Design of a Smart Fluid Rankine Cycle, Advisor: Mark S. Cramer TEACHING 2008

Dumont, Elizabeth R.


On the use of Ly? emitters as probes of reionization  

Science Journals Connector (OSTI)

......with the massively parallel, hybrid (mpi+openmp) code cubep3m...forces are calculated on two grids: a fine grid covering the...By chi2 minimization on a grid, we find that the best fit...acknowledge the Swedish National Infrastructure for Computing (SNIC) resources......

Hannes Jensen; Peter Laursen; Garrelt Mellema; Ilian T. Iliev; Jesper Sommer-Larsen; Paul R. Shapiro



public EvEnts APRIL to JuLy 2011  

E-Print Network (OSTI)

Ey (bEc (socsc) '01) Head of Sustainability and Responsible Investment at Colonial First State When 14 Hans C Freeman lecture 15 Sydney Science Forums 16 Architecture, Design and Planning 18 university sustainability. NB: this lecture commences at 5.30pm. sydney.edu.au/china_studies_centre tuesday 29 March Theatre

Du, Jie


Tru-ly Clean - What Does It Mean?  

SciTech Connect

The evolution and genesis of the definition of transuranic waste (known as TRU) and its application to the cleanup criteria applied to soils contaminated with transuranics, specifically plutonium, has been a matter of discussion at contaminated sites in the United States and elsewhere. Cleanup decisions and the processes that led up to those decisions have varied at several plutonium contaminated sites within the United States and without the pacific region. The sites with radionuclide soil action levels include Bikini and Enewetak Atolls, Republic of the Marshall Islands; Johnston Atoll, Hawaii; the Hanford Site in Washington State; the Nevada Test Site; the Rocky Flats Environmental Technology Site in Colorado; the Chariot Site in north Alaska; and the Maralinga Site in Australia. The soil-action level developed for Rocky Flats by the U.S. Department of Energy, U.S. Environmental Protection Agency, and the Colorado Department of Public Health and Environment for plutonium is one of the higher soil-action levels approved by regulatory agencies that is considered protective for future use of land at a cleanup site. The Republic of the Marshall Islands has adopted a relatively conservative cleanup standard to accommodate the subsistence lifestyle of the islanders, while the Rocky Flats Environmental Technology Site has been transferred to the U.S. Department of the Interior to be used as a fish and wildlife refuge, a land use that resulted in a less conservative plutonium soil cleanup level. (authors)

Hopkins, A. [Fluor Hanford, Inc, Richland, WA (United States)



The effect of injection hole geometry on flat plate film cooling and heat transfer  

E-Print Network (OSTI)

to thermal ly protect a gas turb ine blade f r om the hot gases w i th in a gas turbine engine by inject ion of a coo l ing f lu id th rough discrete holes i n the surface of the blade. Tests were conducted on a flat p late us ing the f i lm cool ing... surface w i th coo l ing a ir c i rculated w i th in the hol low core of the turb ine b lade. External cool ing employs co ld a ir inject ion th rough holes on the outer surface of the turb ine blade produc ing a f i lm of a i r that protects...

Madsen, Eric Perry



LY294002 and LY303511 Sensitize Tumor Cells to Drug-Induced Apoptosis via Intracellular Hydrogen Peroxide Production Independent of the Phosphoinositide 3-Kinase-Akt Pathway  

Science Journals Connector (OSTI)

...oxygen species production, in particular hydrogen peroxide...intracellular H2O2 production and downstream...Materials and Methods Determination...Materials and Methods. The total...intracellular H2O2 production at a concentration...produces hydrogen peroxide...

Tze Wei Poh and Shazib Pervaiz



Mass-to-light ratio of Ly? emitters: implications of Ly? surveys at redshifts z= 5.7, 6.5, 7 and 8.8  

Science Journals Connector (OSTI)

......lifetime divided by the rest mass energy, M * c 2) and the total number...and high values being for the solar and zero metallicity, respectively...simple argument based upon energy conservation, we have shown...in the analysis. The most economical way to improve our model is......

Elizabeth R. Fernandez; Eiichiro Komatsu



A Historical Overview of Alcohol and Alcoholism  

Science Journals Connector (OSTI)

...Duane Miller Wei Li Univ. of Tennessee Health Science Ctr., Memphis, TN; the Ohio...Denver, CO Malignant melanoma is the most dangerous form of skin cancer, accounting for 75...of Pharmacy, University of Tennessee Health Science Center; and the Van Vleet Endowed...

Mark Keller



Ly49 Family Receptors Are Required for Cancer Immunosurveillance Mediated by Natural Killer Cells  

Science Journals Connector (OSTI)

...determined using an electronic caliper (Marathon) to measure the length and width. Mice...mug methylcholanthrene dissolved in corn oil. Mice were monitored weekly for tumor...determined using an electronic caliper (Marathon) to measure length and width. Sarcoma...

Megan M. Tu; Ahmad Bakur Mahmoud; Andrew Wight; Amelia Mottashed; Simon Bélanger; Mir Munir A. Rahim; Elias Abou-Samra; and Andrew P. Makrigiannis



Magnetic moment and plasma environment of HD 209458b as determined from Ly? observations  

Science Journals Connector (OSTI)

...We assume the atmosphere of HD 209458b...consistent with atmospheric models...by the shaded area. One can...shows the thermal atmospheric atoms. Fig...the estimated plasma parameters are from the...209458b at 150 MHz (19). Proximity...not support a larger magnetic moment that exceeds...

Kristina G. Kislyakova; Mats Holmström; Helmut Lammer; Petra Odert; Maxim L. Khodachenko



The scattering of Ly? radiation in the intergalactic medium: numerical methods and solutions  

Science Journals Connector (OSTI)

......temperature of hydrogen to the gas temperature. One method is based on...product of the production rate of Lyalpha...per neutral hydrogen atom and the...our numerical methods recover the...The photon production rate between......

Jonathan Higgins; Avery Meiksin



Molecular hydrogen in damped Ly? systems: clues to interstellar physics at high redshift  

Science Journals Connector (OSTI)

......radiation field. Because our method for SFR estimation is independent...consistency between the two methods is interesting to explore...cannot be estimated by our method. 5.2.3 Q 1232+082...star formation (and metal production) history (see also Pei Fall......

H. Hirashita; A. Ferrara




Office of Legacy Management (LM)

re3xf.H ROJECT TIM % HER M JWDlCTICd Cf M W.&f&t ff NIF, Ml TtE FKILIIY If0 LICWSES TO WRE ffiDliXClIVE tt%iML. IVJ R&w mm IS h-m. STTE SW MC&TED W P4DlOKTIVIN kmvi t+mi BkcTmam...


A measurement of galaxy halo mass from the surrounding H I Ly? absorption  

Science Journals Connector (OSTI)

......smaller minimum halo mass. Using a spectroscopic...for measuring halo mass is presented in Section...the 2D absorption maps from R12 in Section...II SNe, stellar winds, and asymptotic...The assumed initial mass function (IMF...particles are kicked at a velocity of 600s1. The mass......

Olivera Rakic; Joop Schaye; Charles C. Steidel; C. M. Booth; Claudio Dalla Vecchia; Gwen C. Rudie



Furfural Inhibits Growth by Limiting Sulfur Assimilation in Ethanologenic Escherichia coli Strain LY180  

Science Journals Connector (OSTI)

...more than twofold are shown, with red (green) indicating genes with increased (decreased...by 1.5-fold or greater are shown in green (negative sign assigned). All others...acid hydrolysates of lignocellulose with lime. Biotechnol. Prog. 17: 287-293...

Elliot N. Miller; Laura R. Jarboe; Peter C. Turner; Priti Pharkya; Lorraine P. Yomano; Sean W. York; David Nunn; K. T. Shanmugam; Lonnie O. Ingram



Magnetic moment and plasma environment of HD 209458b as determined from Ly? observations  

Science Journals Connector (OSTI)

...best fit equals {chi} 2 = 0.081 . Green, the same as red, but excluding broadening...exceeds ? Jup , as predicted by an energy flux scaling model (20, 21). In summary...Yang H. France K. Froning C. S. Green J. C. Stocke J. T. Osterman S...

Kristina G. Kislyakova; Mats Holmström; Helmut Lammer; Petra Odert; Maxim L. Khodachenko



Towards Extreme(ly) Usable Software: Exploring Tensions Between Usability and Agile Software Development  

E-Print Network (OSTI)

that draws from extreme programming (XP), a widely practiced agile software development process, and scenario that need to be addressed for agile software development methods and usability engineering practices to work with multidisciplinary system design--focusing specifically on agile software development and usability----by developing

McCrickard, Scott


Incompatibility of a comoving Ly-alpha forest with supernova-Ia luminosity distances  

E-Print Network (OSTI)

Recently Perlmutter et al. suggested a positive value of Einstein's cosmological constant Lambda on the basis of luminosity distances from type-Ia supernovae. However, Lambda world models had earlier been proposed by Hoell & Priester and Liebscher et al. on the basis of quasar absorption-line data. Employing more general repulsive fluids ("dark energy") encompassing the Lambda component we quantitatively compare both approaches with each other. Fitting the SN-data by a minimum-component model consisting of dark energy + dust yields a closed universe with a large amount of dust exceeding the baryonic content constrained by big-bang nucleosynthesis. The nature of the dark energy is hardly constrained. Only when enforcing a flat universe there is a clear tendency to a dark-energy Lambda fluid and the `canonical' value Omega_M = 0.3 for dust. Conversely, fitting the quasar-data by a minimum-component model yields a sharply defined, slightly closed model with a low dust density ruling out significant pressureless dark matter. The dark-energy component obtains an equation-of-state P = -0.96 epsilon close to that of a Lambda-fluid. Omega_M = 0.3 or a precisely flat spatial geometry are inconsistent with minimum-component models. It is found that quasar and supernova data sets cannot be reconciled with each other via (repulsive ideal fluid+dust+radiation)-world models. Compatibility could be reached by drastic expansion of the parameter space with at least two exotic fluids added to dust and radiation as world constituents. If considering such solutions as far-fetched one has to conclude that the quasar absorption line and the SN-Ia constraints are incompatible.

Jens Thomas; Hartmut Schulz


Note: This page contains sample records for the topic "vleet hol ly" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


The impact of The IGM on high-redshift Ly? emission lines  

Science Journals Connector (OSTI)

......background that accompanied the completion of reionization barely increased...frequency with nuH. For stars, the index beta is typically 4 to 5 and we...H ii-bubble size prior to the completion of reionization. We have shown......

Mark Dijkstra; Adam Lidz; J. Stuart B. Wyithe



Effect of radiative transfer on damped Ly? and Lyman limit systems in cosmological SPH simulations  

Science Journals Connector (OSTI)

......median points, and a straight power law does not necessarily...bracketed by our no-UVB run and optically thin run...lines are the SW and WW runs, respectively, in the...Pontzen et al. (2008, Gasoline SPH simulation) and Cen...result is close to the OTUV run. Although Tescari et......

Hidenobu Yajima; Jun-Hwan Choi; Kentaro Nagamine



DOI: 10.1002/cctc.201200311 Low-Temperature Chemoselective Gold-Surface-Mediated Hydrogenation of  

E-Print Network (OSTI)

.[9] Claus found that, in the production of allyl alco- hol from the hydrogenation of acrolein, gold

Henkelman, Graeme


List of Publications Thomas B. Schon  

E-Print Network (OSTI)

. Becker, G. Bleser, D. Stricker, C. Wohlleber, M. Felsberg, F. Gustafsson, J. Hol, T. B. Sch¨on, J

Schön, Thomas


Spherical harmonic modes of 5.5 post-Newtonian gravitational wave polarizations and associated factorized resummed waveforms for a particle in circular orbit around a Schwarzschild black hol  

E-Print Network (OSTI)

Recent breakthroughs in numerical relativity enable one to examine the validity of the post-Newtonian expansion in the late stages of inspiral. For the comparison between post-Newtonian (PN) expansion and numerical simulations, the waveforms in terms of the spin-weighted spherical harmonics are more useful than the plus and cross polarizations, which are used for data analysis of gravitational waves. Factorized resummed waveforms achieve better agreement with numerical results than the conventional Taylor expanded post-Newtonian waveforms. In this paper, we revisit the post-Newtonian expansion of gravitational waves for a test-particle of mass $\\m$ in circular orbit of radius $r_0$ around a Schwarzschild black hole of mass $M$ and derive the spherical harmonic components associated with the gravitational wave polarizations up to order $v^{11}$ beyond Newtonian. Using the more accurate $h_{\\ell m}$'s computed in this work, we provide the more complete set of associated $\\rho_{\\ell m}$'s and $\\delta_{\\ell m}$'s that form important bricks in the factorized resummation of waveforms with potential applications for the construction of further improved waveforms for prototypical compact binary sources in the future. We also provide ready-to-use expressions of the 5.5PN gravitational waves polarizations $h_+$ and $h_\\times$ in the test-particle limit for gravitational wave data analysis applications. Additionally, we provide closed analytical expressions for 2.5PN $h_{\\ell m}$, 2PN $\\rho_{\\ell m}$ and 3PN $\\delta_{\\ell m}$, for general multipolar orders $\\ell$ and $m$ in the test-particle limit. Finally, we also examine the implications of the present analysis for compact binary sources in Laser Interferometer Space Antenna.

Ryuichi Fujita; Bala R. Iyer



What Damped Ly-alpha Systems Tell Us About the Radial Distribution of Cold Gas at High Redshift  

E-Print Network (OSTI)

We investigate the properties of damped Lyman-alpha systems (DLAS) in semi-analytic models, focusing on whether the models can reproduce the kinematic properties of low-ionization metal lines described by Prochaska & Wolfe (1997b, 1998). We explore a variety of approaches for modelling the radial distribution of the cold neutral gas associated with the galaxies in our models, and find that our results are very sensitive to this ingredient. If we use an approach based on Fall & Efstathiou (1980), in which the sizes of the discs are determined by conservation of angular momentum, we find that the majority of the DLAS correspond to a single galactic disc. These models generically fail to reproduce the observed distribution of velocity widths. In alternative models in which the gas discs are considerably more extended, a significant fraction of DLAS arise from lines of sight intersecting multiple gas discs in a common halo. These models produce kinematics that fit the observational data, and also seem to agree well with the results of recent hydrodynamical simulations. Thus we conclude that Cold Dark Matter based models of galaxy formation can be reconciled with the kinematic data, but only at the expense of the standard assumption that DLAS are produced by rotationally supported gas discs whose sizes are determined by conservation of angular momentum. We suggest that the distribution of cold gas at high redshift may be dominated by another process, such as tidal streaming due to mergers.

Ariyeh H. Maller; Jason X. Prochaska; Rachel S. Somerville; Joel R. Primack



Damped Ly-alpha Systems in Semi-Analytic Models: Sensitivity to dynamics, disk properties, and cosmology  

E-Print Network (OSTI)

Previously we have shown that it is possible to account for the kinematic properties of damped Lyman alpha systems (DLAS) in the context of semi-analytic models. In these models, hierarchical structure formation is approximated by constructing a merger tree for each dark matter halo. A natural consequence is that every virialized halo may contain not only a central galaxy, but also a number of satellite galaxies as determined by its merging history. Thus the kinematics of the DLAS arise from the combined effects of the internal rotation of gas disks and the motions between gas disks within a common halo. Here we investigate the sensitivity of this model to some of the assumptions made previously, including the modeling of satellite dynamics, the scale height of the gas, and the cosmology.

Ariyeh H. Maller; Rachel S. Somerville; Jason X. Prochaska; Joel R. Primack



Polyamine Transporters and Polyamines Increase Furfural Tolerance during Xylose Fermentation with Ethanologenic Escherichia coli Strain LY180  

Science Journals Connector (OSTI)

...hemicellulose sugars into fuels and chemicals (9, 23...lignocellulosic biomass to fuels and chemicals. Annu...Liden. 2009. Metabolic effects of furaldehydes and impacts...and LO Ingram. 2000. Effects of Ca(OH)2 treatments...Skerker, JM , D Leon, MN Price, JS Mar, DR Tarjan...

Ryan D. Geddes; Xuan Wang; Lorraine P. Yomano; Elliot N. Miller; Huabao Zheng; Keelnatham T. Shanmugam; Lonnie O. Ingram



A Phase I Trial of LY2510924, a CXCR4 Peptide Antagonist, in Patients with Advanced Cancer  

Science Journals Connector (OSTI)

...Galsky, Mount Sinai School of Medicine, 10 East 102nd Street Tower Building, Second Floor Box 1128, New York, NY 10029. Phone...Table 2. Seven patients experienced a serious adverse event (SAE): grade 2 abdominal abscess (n = 1, 2.5 mg/day), grade...

Matthew D. Galsky; Nicholas J. Vogelzang; Paul Conkling; Eyas Raddad; John Polzer; Stephanie Roberson; John R. Stille; Mansoor Saleh; and Donald Thornton



Polyamine Transporters and Polyamines Increase Furfural Tolerance during Xylose Fermentation with Ethanologenic Escherichia coli Strain LY180  

Science Journals Connector (OSTI)

...PotABCD). Supplementing AM1 mineral salts medium with individual...cultures were grown in AM1 mineral salts medium (31). All media...RNA (Qiagen QuantiTect SYBR green RT-PCR kit). Primer sequences...hydrolysates of lignocellulose with lime. Biotechnol. Prog. 17 :287-293...

Ryan D. Geddes; Xuan Wang; Lorraine P. Yomano; Elliot N. Miller; Huabao Zheng; Keelnatham T. Shanmugam; Lonnie O. Ingram



9-1 VLSI Memo Series MTL Annual Research Report 2008 2007 07-2015 L.Y. Chen  

E-Print Network (OSTI)

08-2033 M. Straayer Noise Shaping Techniques for Analog and Time to Digital Converters Using Voltage 08-2038 H. Ma Electrochemical Impedance Spectroscopy using Adjustable Nanometer-Gap Electrodes 08

Reif, Rafael


Direct Numerical Simulation of the Flow in a Pebble Bed  

E-Print Network (OSTI)

,lelt),uvdyms(lx1,ly1,lz1,lelt), $ uvdzms(lx1,ly1,lz1,lelt),uwdxms(lx1,ly1,lz1,lelt), $ uwdyms(lx1,ly1,lz1,lelt),uwdzms(lx1,ly1,lz1,lelt), $ vwdxms(lx1,ly1,lz1,lelt),vwdyms(lx1,ly1,lz1,lelt), $ vwdzms(lx1,ly1,lz1,lelt),eps_uu(lx1...,ly1,lz1,lelt), $ eps_vv(lx1,ly1,lz1,lelt),eps_ww(lx1,ly1,lz1,lelt), $ eps_uv(lx1,ly1,lz1,lelt),eps_uw(lx1,ly1,lz1,lelt), $ eps_vw(lx1,ly1,lz1,lelt) common /production/ $ prd_uu(lx1,ly1,lz1,lelt),prd_vv(lx1,ly1,lz1,lelt...

Ward, Paul



Problem Solving with Tactics Masami Hagiya1, Hitoshi Tanaka1, Mitsuharu Yamamoto1, Shin-ya Nishizaki2  

E-Print Network (OSTI)

@math.s.chiba-u.ac.jp Abstract We implemented a solver for a puzzle called Picross under HOL, a tactic* *-based for implementing a logical variable under HOL. Our logical variables are insta* *ntiated according to more be implemented as a proof pro* *cedure that is applied to a problem Q and computes a solution a while proving

Hagiya, Masami


Research White Paper February 2007  

E-Print Network (OSTI)

. Chandaria, G. Thomas, B. Bartczak, K. Koeser, R. Koch, M. Becker, G. Bleser, D. Stricker, C. Wohlleber, M. Koeser, R. Koch, M. Becker, G. Bleser, D. Stricker, C. Wohlleber, M. Felsberg, F. Gustafsson, J. Hol, T3 , D. Stricker3 , C. Wohlleber3 , M. Felsberg4 , F. Gustafsson4 , J. Hol4 , T. B. Schön4 , J

Schön, Thomas


The natural killer cell receptor Ly-49A recognizes a peptide-induced conformational determinant on its major histocompatibility complex class I ligand  

Science Journals Connector (OSTI)

...molecules (14). Moreover, because mAb 34-5-8S is specific for a private epitope on H-2Dd, this result rules out a surreptitious effect from endog- enous H-2k class I molecules. The mAb 28-8-6 did not have any effect, even though it bound to...

M Orihuela; D H Margulies; W M Yokoyama



PotentialLy toxic elemetnsi-ntanganese \\\\ \\ r ' r \\ * , " A c . H 3n o . F 7 g 1 5 2 8 8 -. . . _ l \\ ' ( '  

E-Print Network (OSTI)

- . . . _ l \\ ' ( ' r- "--lililllllllllilllllllllillllilllii"-"" roclq'1rBsaf e-\\ ,n I Fefdman, Carol A. \\ r

Luther, Douglas S.


First-in-Human Dose Study of the Novel Transforming Growth Factor-? Receptor I Kinase Inhibitor LY2157299 Monohydrate in Patients with Advanced Cancer and Glioma  

Science Journals Connector (OSTI)

...del Rocio 12 Oncology, Johns Hopkins Kimmel Cancer Center 13 Brain Cancer Program, Johns Hopkins University 14 Lilly Research...echocardiography/Doppler imaging, serum troponin I and brain natriuretic peptide (BNP) levels. Anti-tumor activity was...

Jordi Rodon; Michael A. Carducci; Juan M. Sepulveda-Sanchez; Analia Azaro; Emiliano Calvo; Joan Seoane; Irene Brana; Elisabet Sicart; Ivelina Gueorguieva; Ann L Cleverly; N Sokalingum Pillay; Durisala Desaiah; Shawn T Estrem; Luis Paz-Ares; Matthias Holdoff; Jaishri Blakeley; Michael M Lahn; Jose Baselga


Filter Induced Bias in Ly{\\alpha} Emitter Surveys: A Comparison Between Standard and Tunable Filters. Gran Telescopio Canarias Preliminary Results  

E-Print Network (OSTI)

Lyman-alpha emitter (LAE) surveys have successfully used the excess in a narrow-band filter compared to a nearby broad-band image to find candidates. However, the odd spectral energy distribution (SED) of LAEs combined with the instrumental profile have important effects on the properties of the candidate samples extracted from these surveys. We investigate the effect of the bandpass width and the transmission profile of the narrow-band filters used for extracting LAE candidates at redshifts z ~ 6.5 through Monte Carlo simulations, and we present pilot observations to test the performance of tunable filters to find LAEs and other emission-line candidates. We compare the samples obtained using a narrow ideal-rectangular-filter, the Subaru NB921 narrow-band filter, and sweeping across a wavelength range using the ultra-narrow-band tunable filters of the instrument OSIRIS, installed at the 10.4m Gran Telescopio Canarias. We use this instrument for extracting LAE candidates from a small set of real observations. ...

de Diego, J A; Cepa, J; Bongiovanni, A; Verdugo, T; Sánchez-Portal, M; González-Serrano, J I



J U LY 1 , 2 0 0 6 / A N A LY T I C A L C H E M I S T R Y 4 2 4 7 2 0 0 6 A M E R I C A N C H E M I C A L S O C I E T Y Microparticles are used in a plethora  

E-Print Network (OSTI)

bifunctional microparticles called Janus particles, after the Roman god with two faces. The number of chemical in diameter, Doyle and col- leagues indicated that smaller particles of ~1-µm-diam could be created functionali- ties wasn't restricted to two. "To date, we've [fabricated] particles that have four

Doyle, Patrick S.


Problem Solving with Tactics Masami Hagiya 1 , Hitoshi Tanaka 1 , Mitsuharu Yamamoto 1 , Shinya Nishizaki 2  

E-Print Network (OSTI)

for this programming style, by which we implement a logical variable under HOL. Unlike ordinary logical variables, our be implemented as a proof procedure that is applied to a problem Q and computes a solution a and a proof of Q(a@math.s.chiba­u.ac.jp Abstract. We implemented a solver for a puzzle called Picross under HOL, a tactic­based theorem prover

Hagiya, Masami

Note: This page contains sample records for the topic "vleet hol ly" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
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We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


Problem Solving with Tactics Masami Hagiya 1 , Hitoshi Tanaka 1 , Mitsuharu Yamamoto 1 , Shinya Nishizaki 2  

E-Print Network (OSTI)

@math.s.chiba­u.ac.jp Abstract We implemented a solver for a puzzle called Picross under HOL, a tactic­based theorem prover. In the last step, we employed a technique for implementing a logical variable under HOL. Our logical variables can be implemented as a proof procedure that is applied to a problem Q and computes a solution a while

Hagiya, Masami


UMore Ph IA CR Report 7-8-10.pdf  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

PHASE IA ARCHAEOLOGICAL AND PHASE IA ARCHAEOLOGICAL AND ARCHITECTURAL HISTORY SURVEY FOR THE UMORE PARK RESEARCH WIND TURBINE PROJECT, DAKOTA COUNTY, MINNESOTA SHPO File No. Pending Client No. Pending The 106 Group Project No. 10-18 Submitted to: Barr Engineering Company 4700 West 77th Street Minneapolis, MN 55435-4803 Submitted by: The 106 Group Ltd. The Dacotah Building 370 Selby Avenue St. Paul, MN 55102 Principal Investigators: AnneKetz, M.A., RPA Greg Mathis, M.C.R.P. Report Authors: Mark Doperalski, B.S. Miranda Van Vleet, M.H.P July 2010 UMore Park Wind Turbine Project Phase IA Archaeological and Architectural History Survey Page i MANAGEMENT SUMMARY During May of 2010, The 106 Group Ltd. (106 Group) conducted a Phase IA archaeological and architectural history survey for the University of Minnesota Outreach, Research, and


Biosurfactant Activity for Enhanced Oil Recovery Final Report  

NLE Websites -- All DOE Office Websites (Extended Search)

Development of Microorganisms with Improved Transport and Development of Microorganisms with Improved Transport and Biosurfactant Activity for Enhanced Oil Recovery Final Report Report Start Date: June 1, 2002 Report End Date: August 31, 2005 M. J. McInerney, K.E. Duncan, N. Youssef, T. Fincher, S. K. Maudgalya, M. J. Folmsbee, R. Knapp, Randy R. Simpson, N. Ravi, and D. Nagle Date of Report: August 15, 2005 DE-FC-02NT15321 R 02 Department of Botany and Microbiology and Department of Petroleum Engineering University of Oklahoma 770 Van Vleet Oval Norman, OK 73019-0245 2 Disclaimer This report was prepared as an account of work sponsored by an agency of the United States Government. Neither the United States Government not any agency thereof, nor any of their employees, makes any warranty, expressed or implied, or


E-Print Network 3.0 - antineoplastic protocols Sample Search...  

NLE Websites -- All DOE Office Websites (Extended Search)

For LyP-1-conjugated LPs (LyP1LPs), LPs with maleimide groups were prepared... Acta Bioenerg, 812:55-65. 31. Mayer LD, Bally MB, Hope MJ, Cullis PR (1985) Uptake of...


Idaho – Sexual Orientation and Gender Identity Law and Documentation of Discrimination  

E-Print Network (OSTI)

Amend Sex Designation on Birth Certificates, http://bit.ly/that does not amend birth certificates to change gender

Sears, Brad



FIREBALL: The Faint Intergalactic medium Redshifted Emission Balloon --Overview and 1st Science Flight Results  

E-Print Network (OSTI)

Ly (1216Ã?), OVI (1033Ã?) and CIV (1549Ã?) are redshifted into the 1950-2250Ã? stratospheric balloon

Martin, Chris


Synapsid Burrows in the Lower Jurassic Navajo Sandstone, Utah  

E-Print Network (OSTI)

ite ctu ral an d s urf ici al m orp hol ogi es. 23 Type I Structures Architectural Morphology.—Type I comprise high-density, complex networks of interconnected Y- and T- branched, inclined ramps, horizontal to subhorizontal large...

Riese, David



Problem Solving with Tactics Masami Hagiya1, Hitoshi Tanaka1, Mitsuharu Yamamoto1,  

E-Print Network (OSTI)

@math.s.chiba-u.ac.jp Abstract We implemented a solver for a puzzle called Picross under HOL, a tactic problem and find an unknown solution. In the last step, we employed a technique for implementing. 1 Introduction Under a theorem prover, a solver of a problem can be implemented as a proof

Hagiya, Masami


The Mississippi Valley earthquakes of 1811 and 1812: Intesities, ground motion and magnitudes  

Science Journals Connector (OSTI)

...the same. m~ment. .. The Comet has been passingto the wesiward...of t~he boatmen a~ the landing, Wh(~ szpposed the bank...about the time o~ their landing , they saw,~hat the island...hol~, Anxfous to o~tain landing~ and dreading the high banks...

Otto W. Nuttli


Bridging the Gaps between eTransforming SMEs and SME -ICT Providers  

E-Print Network (OSTI)

of what eTransforming SMEs need based on their current technology and future business requirements. Keywords: SMEs, eTransformation, Information and Communication Technology, ICT providers 1 IntroductionBridging the Gaps between eTransforming SMEs and SME - ICT Providers Ana Hol1 and Athula Ginige1

Boyer, Edmond


Escape to ATP for Mizar Piotr Rudnicki  

E-Print Network (OSTI)

Escape to ATP for Mizar Piotr Rudnicki University of Alberta Edmonton, Alberta, Canada piotr ATP service is a new feature in the Mizar proof assistant. The functionality of the service is in many respects analogous to the Sledgehammer subsystem of Isabelle/HOL. The ATP service requires minimal user

Paris-Sud XI, Université de


Single-Walle 4. Single-Walled Carbon Nanotubes  

E-Print Network (OSTI)

applications, carbon nanotube research is ac- tively being pursued in diverse areas including energy storage105 Single-Walle 4. Single-Walled Carbon Nanotubes Sebastien Nanot, Nicholas A. Thompson, Ji Single-walled carbon nanotubes (SWCNTs) are hol- low, long cylinders with extremely large aspect ratios

Kono, Junichiro


Sustainable Energy Resources for Consumers (SERC) - Geothermal...  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

2011-11-03 09.59 Monitoring SERC TechnologiesGround Source Heat Pumps Page 1 of 22 Am Amy y Ho Hol ll la an nd de er r, , Da Dav vi id d P Pe et te er rs so on n Amy Hollander:...


An approach for lifetime reliability analysis using theorem proving  

Science Journals Connector (OSTI)

Recently proposed formal reliability analysis techniques have overcome the inaccuracies of traditional simulation based techniques but can only handle problems involving discrete random variables. In this paper, we extend the capabilities of existing ... Keywords: Failure rate, Formal methods, Fractile function, HOL, Hazard function, Lifetime analysis, Random variables, Reliability analysis, Statistical properties, Theorem proving

Naeem Abbasi; Osman Hasan; Sofiène Tahar




Science Journals Connector (OSTI)

......assume that our affine symplectic manifold X is connected. Assume for a moment that it is finite-dimensional. The way to pro- ceed in geometric quantization is to define, for each polarization, the Hilbert space H0 L2 (X; L) := L2 hol(X, L) of holomorphic......

Hessel Posthuma



Int. J. , Vol. x, No. x, xxxx 1 Modelling and Analysis of Service Parts Logistics Systems  

E-Print Network (OSTI)

Int. J. , Vol. x, No. x, xxxx 1 Modelling and Analysis of Service Parts Logistics Systems Fernando, the behaviour of the service parts logistics system (SPLS) is approximated with a modified M/G/1 HOL queuing policy. Keywords: Service parts logistics, optimisation, genetic algorithms, M/G/1 queuing model

Rossetti, Manuel D.


Assessing the frictional and baroclinic contributions to stratified wake formation: a parameter space study  

E-Print Network (OSTI)

The baroclinic and surface-frictional contributions to stratified wake formation are considered as a function of the non-dimensional height ( = Nho/U) and aspect-ratio ( = ho/L) of the barrier. Numerical simulations are computed for a wide range...

Smith, Jamie Brooke



ELSEVIER Surface Science 303 (lYY4) 206-230 ;,,.;_:_.y y .../. .' ..`,. :> .,  

E-Print Network (OSTI)

by means of the Fischer- Tropsch technique, and the steam reforming of natural gas to form so-called syngas. Representative examples are the ammonia synthesis via Haber-Bosch, the synthesis of alco- hols and hydrocarbons of products, and (7) diffusion of products from the surface. One typically treats these elementary reactions

Miller, William H.


Formalising the -calculus using Nominal Logic Jesper Bengtson and Joachim Parrow  

E-Print Network (OSTI)

of Information Technology, University of Uppsala, Sweden Abstract. We formalise the pi-calculus using the nominal an implementation in Isabelle/HOL. The purpose is to derive powerful induction rules for the semantics in order. This is a normal strategy for manual proofs about the pi-calculus, but that kind of hand waving has previously been

Flener, Pierre


Abstract The typing of single nucleotide polymorphisms (SNPs) located throughout the mitochondrial genome  

E-Print Network (OSTI)

to nuclear DNA testing in cases of extreme sample degradation, shed hairs, or where com- parisons between less power of discrimination than nuclear DNA. However, forensic mtDNA testing targets only a small maternal relatives are necessary (a gen- eral review of mtDNA forensic testing is given by Hol- land

Note: This page contains sample records for the topic "vleet hol ly" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


Regio-and Enantioselective Alkane Hydroxylation with Engineered Cytochromes P450 BM-3  

E-Print Network (OSTI)

-alco- hols.10 This enzyme does not accept larger alkanes. Soluble methane monooxygenase from the same cytochrome P450s that have been characterized are in general faster, soluble (i.e., not membrane-bound), more hydroxylation and, in some cases, even regioselective alkane hydroxylation. For example, the particulate methane

Arnold, Frances H.


J A N U A R Y 1 , 2 0 0 1 / A N A LY T I C A L C H E M I S T R Y 3 9 A p ro d u c t re v i e w  

E-Print Network (OSTI)

-probe microscopy imaging has led to various interrelated instruments. James P. Smith Scanning-probe microscopy (SPM and nanotechnological systems are founded in electrochemical processes. Thus, the full characterization of many processes requires topographic images and chemical information. One such approach is to combine electro

Kwak, Juhyoun


E-Print Network 3.0 - arab republic niger Sample Search Results  

NLE Websites -- All DOE Office Websites (Extended Search)

Summary: Dominican Republic ---- TP East Timor -Iu- EC Ecuador (Republic of) bIU- EG Egypt (Arab Republic of) ---- SV... Liberia (Republic of) ---- LY Libyan Arab Jamahiriya...


LI, W. K. W. Annual average abundance of heterotrophic bacteria ...  

Science Journals Connector (OSTI)

ern Indian Ocean: The southwest and northeast monsoon, .... Data for Synechococcus in the Indian ... ly for 6 yr over the deepest point of the basin (Li et al.


Central Washington University: 2014 Engineering Technologies, Safety & Construction Fair  

Energy.gov (U.S. Department of Energy (DOE))

Location: 400 E. University Way Ellensburg, WA 98926, SURC BallroomPOC: Heather BainWebsite: http://bit.ly/1pgOpN7


A potential role for intragenic miRNAs on their hosts' interactome  

E-Print Network (OSTI)

Merritt WM, Lin YG, Han LY, Kamat AA, Spannuth WA, Schmandt R, Urbauer D, Pennacchio LA, Cheng J-F, Nick

Hinske, Ludwig; Galante, Pedro AF; Kuo, Winston P; Ohno-Machado, Lucila



NCBECS C&E 1979  

U.S. Energy Information Administration (EIA) Indexed Site

9. Distribution of Commercial Buildings Supplied with Fuel Oil, by Number of Tanks, Tank CapaciLy, and Inventory, as of January 1, 1980 (Thousands of Buildings)...



E-Print Network (OSTI)

effect of future geothermal power plants. A detailed testgram for modeling geothermal power plants. Previous- ly,program for modeling geothermal power plants Interactive

Authors, Various



The Relationship between Economic Growth and HIV/AIDS in Southern Africa: A Review of the Literature  

E-Print Network (OSTI)

Justice Africa. Drezc;jean and Amartya Sen. 1989. HungtrandJ. 27(86): 577-582. Sen, Amartya. 1999. DeLY! lopmetlt as

Costa, Patricia R.



E-Print Network 3.0 - adipose derived stem Sample Search Results  

NLE Websites -- All DOE Office Websites (Extended Search)

and ob- L-4F-LY294002. Food intake, insulin, glucose adipocyte stem cells, p Source: Brand, Paul H. - Department of Physiology and Pharmacology, University of Toledo...


Author's personal copy The effect of surface topography on the lunar photoelectron sheath  

E-Print Network (OSTI)

and electrostatic dust transport Andrew R. Poppe a,e, , Marcus Piquette b , Alexandre Likhanskii c , Mihály Horányi

California at Berkeley, University of


Geophys. J. R. astr. SOC.(1984) 79, 893-910 Deep Schlumberger soundingand the crustal  

E-Print Network (OSTI)

& Lilley 1Y74; Cough, McElhinny & Lilley 1Y74: Lilley 1976;White & Polatajko lY78; White & Hopgood 1979

Constable, Steve



Science Journals Connector (OSTI)

weather forecasts, particularly since many HABs are strong- ly influenced by the weather ... sea-surface pigment concentration from satellite observa- tions.


Numerical Experiments on Soft X-ray Emission Optimization of Nitrogen Plasma in 3 kJ Plasma Focus SY-1 Using Modified Lee Model  

Science Journals Connector (OSTI)

The X-ray emission properties of nitrogen plasmas are numerically investigated using corona plasma equilibrium model. The X-ray emission intensities... ? , Ly ?

M. Akel; Sh. Al-Hawat; S. Lee




Science Journals Connector (OSTI)

Jun 5, 1988 ... enough bacterial biomass for the carbon iso- ... Combustion tubes were cooled slow- ly (4 h) to .... factor regulating bacterial biomass and pro-.



Black Engineering of the Year Awards and STEM Conference Career Fair  

Energy.gov (U.S. Department of Energy (DOE))

Location:  Washington Marriott Wardman Park, 2660 Woodley Road, NW, Washington, DC 20008Website Link:  http://bit.ly/1CbVvraPOC:  Dameone Ferguson (NNSA)


2009 Publications | Stanford Synchrotron Radiation Lightsource  

NLE Websites -- All DOE Office Websites (Extended Search)

09 Publications 09 Publications Journal Papers J. Abendroth, A. C. Kreger and W. G. J. Hol, "The Dimer Formed by the Periplasmic Domain of EpsL from the Type 2 Secretion System of Vibrio parahaemolyticus", J. Struct. Biol. 168, 313 (2009) doi: 10.1016/j.jsb.2009.07.022 J. Abendroth, D. D. Mitchell, K. V. Korotkov, T. L. Johnson, A. Kreger, M. Sandkvist and W. G. J. Hol, "The Three-dimensional Structure of the Cytoplasmic Domains of EpsF from the Type 2 Secretion System of Vibrio cholerae", J. Struct. Biol. 166, 303 (2009) doi: 10.1016/j.jsb.2009.03.009 V. Aguilar-Guerrero, R. J. Lobo-Lapidus and B. C. Gates, "Genesis of a Cerium Oxide Supported Gold Catalyst for CO Oxidation: Transformation of Mononuclear Gold Complexes into Clusters as Characterized by X-ray


Pion distribution amplitude from holographic QCD and the electromagnetic form factor F{sub {pi}}(Q{sup 2})  

SciTech Connect

The holographic QCD prediction for the pion distribution amplitude (DA) {phi}{sub hol}(u) is used to compute the pion spacelike electromagnetic form factor F{sub {pi}}(Q{sup 2}) within the QCD light-cone sum rule method. In calculations the pion's renormalon-based model twist-4 DA, as well as the asymptotic twist-4 DA are employed. Obtained theoretical predictions are compared with experimental data and with results of the holographic QCD.

Agaev, S. S.; Nobary, M. A. Gomshi [Institute for Physical Problems, Baku State University, Z. Khalilov Street 23, Az-1148 Baku (Azerbaijan); Department of Physics, Faculty of Science, Razi University, Kermanshah (Iran, Islamic Republic of)



Inhibition of Trichoderma reesei cellulase by cellobiose, glucose, ethanol and butanol  

E-Print Network (OSTI)

INHIBITION OF TRICHODERMA REESEI CELLULASE BY CELLOBIOSE, GLUCOSE, ETHANOL AND BUTANOL A Thesis by MONA BETH COGNATA Submitted to the Graduate College of Texas A&M University in partial fulfillment of the requirement for the degree... of MASTER OF SCIENCE December 1988 Major Subject: Chemical Engineering INHIBITION OF TRICHODERMA REESEI CELLULASE BY CELLOBIOSE, GLUCOSE, ETHANOL AND BUTANOL A Thesis by MONA BETH COGNATA Approved as to style and content by: Mark T. Hol a (Chair...

Cognata, Mona Beth



Individual User Behavior Leading Factor in Comfort Control  

E-Print Network (OSTI)

Conference for Enhanced Building Operations, Berlin, Germany, October 20-22, 2008 METHODS Integral Intelligent Process Control Integration between end-user and building is the ultimate in the intelligent building concept. ?Connecting? the end... deterministic hol i s ti c ESL-IC-08-10-46 Proceedings of the Eighth International Conference for Enhanced Building Operations, Berlin, Germany, October 20-22, 2008 Figure 4. Conceptual map comfort (van Schijndel 2007) The most important research...

Zeiler, W.; Boxem, G.; Van Houten, M. A.; Wortel, W.; Van Der Velden, J. A. J.; Kamphuis, R.; Hommelberg, M.; Broekhuizen, H.

Note: This page contains sample records for the topic "vleet hol ly" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
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to obtain the most current and comprehensive results.


Technische Universitat Munchen Institut fur Informatik  

E-Print Network (OSTI)

Technische Universit¨at M¨unchen Institut f¨ur Informatik Prof. Tobias Nipkow, Ph. D. SS 2005 4. 5 nat), k¨onnen wie folgt in Isabelle/HOL repr¨asentiert werden: datatype tree = Tip | Nd tree nat tree Definieren Sie eine Funktion consts set_of :: "tree nat set" die einen solchen bin¨aren Baum als Argument

Cengarle, María Victoria


Pennsylvanian ichthyoliths from the Shawnee Group of eastern Kansas  

E-Print Network (OSTI)

similarities. Many of the units lack conodonts but contain ichthyoliths. These samples include SB-1-6, SB- 1-7, KH-4-1, KH-4-2, Te-Sp-1, TCS-1-1 and TCS- 1-2. Samples SB-1-5B, Sn-1-2B, Sn-1-3, KH-4-3, Os-1-1B, Os-1-2A, Os-1-2B, Os-1-2C, Os-1-2D, and Os-1-2E... lack both conodonts and ichthyoliths. Samples T-1-6, Sn-1-1B, He-1-1, Ke-1-4, Ke-1-6, SB-1-4B, LB-1-2, LB-1-3A, LB-1-3D, EC-1-1I, JPS-1-2C, TCS-1-4, Hol-1-1, Hol-1-2A, and Hol- 1-2B contain conodonts but lack ichthyoliths; however, samples...

Tway, L. E.



Neural control of tuneable skin iridescence in squid  

Science Journals Connector (OSTI)

...the electrode rapidly backfilled with 3 per cent LY in 200 mM lithium chloride using a microfil needle. After 20 min, the LY dye...open patches (figure 3 a). Applying ACh in physiological excess (200 mM) did not recover these red phenotypes to a green...




SciTech Connect

We use the spatially resolved, multi-band photometry in the GOODS South field acquired by the CANDELS project to constrain the nature of candidate Lyman continuum (LyC) emitters at redshift z {approx} 3.7 identified using ultradeep imaging below the Lyman limit (1{sigma} limit of Almost-Equal-To 30 AB in a 2'' diameter aperture). In 19 candidates out of a sample of 20 with flux detected at >3{sigma} level, the light centroid of the candidate LyC emission is offset from that of the Lyman break galaxy (LBG) by up to 1.''5. We fit the spectral energy distribution of the LyC candidates to spectral population synthesis models to measure photometric redshifts and the stellar population parameters. We also discuss the differences in the UV colors between the LBG and the LyC candidates, and how to estimate the escape fraction of ionizing radiation (f{sub esc}) in cases, like in most of our galaxies, where the LyC emission is spatially offset from the host galaxy. In all but one case we conclude that the candidate LyC emission is most likely due to lower redshift interlopers. Based on these findings, we argue that the majority of similar measurements reported in the literature need further investigation before it can be firmly concluded that LyC emission is detected. Our only surviving LyC candidate is an LBG at z = 3.795, which shows the bluest (B - V) color among LBGs at similar redshift, a stellar mass of M {approx} 2 Multiplication-Sign 10{sup 9} M{sub Sun }, weak interstellar absorption lines, and a flat UV spectral slope with no Ly{alpha} in emission. We estimate its f{sub esc} to be in the range 25%-100%, depending on the dust and intergalactic attenuation.

Vanzella, Eros; Cristiani, Stefano; Nonino, Mario [INAF Osservatorio Astronomico di Trieste, Via G.B. Tiepolo 11, 34131 Trieste (Italy); Guo Yicheng; Giavalisco, Mauro [Department of Astronomy, University of Massachusetts, 710 North Pleasant Street, Amherst, MA 01003 (United States); Grazian, Andrea; Castellano, Marco; Fontana, Adriano; Giallongo, Emanuele; Pentericci, Laura; Galametz, Audrey [INAF Osservatorio Astronomico di Roma, Via Frascati 33, 00040 Monteporzio (RM) (Italy); Dickinson, Mark [National Optical Astronomy Observatory, P.O. Box 26732, Tucson, AZ 85726 (United States); Faber, S. M. [UCO/Lick Observatory, University of California, Santa Cruz, CA 95064 (United States); Ferguson, Henry C.; Grogin, Norman A.; Koekemoer, Anton M. [Space Telescope Science Institute, Baltimore, MD 21218 (United States); Newman, Jeffrey [Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, PA 15260 (United States); Siana, Brian D., E-mail: vanzella@oats.inaf.it [Department of Physics and Astronomy, University of California, Riverside, CA 92521 (United States)



A Machine-Assisted Proof of Gödel’s Incompleteness Theorems for the Theory of Hereditarily Finite Sets  

E-Print Network (OSTI)

be downloaded from an Internet archive.1§2. Background. These proofs were conducted using Isabelle/HOL, an interactive theorem prover (Nipkow et al., 2002). Therefore all proofs are conducted in a formal calculus: higher-order logic. Nevertheless... –392. Feferman, S., editor (1986). Kurt Go¨del: Collected Works, Volume I. Oxford University Press. Franze´n, T. (2005). Go¨del’s Theorem: An Incomplete Guide to Its Use and Abuse. A K Peters. Go¨del, K. (1931). U¨ber formal unentscheidbare Sa¨tze der Principia...

Paulson, Lawrence



A Morphometrical Analysis of Lymph Node Responses to Tumors of Different Immunogenicity  

Science Journals Connector (OSTI)

...N-acetyl-dihydrosphingosine; DAG, diacylglycerol; DETAPAC, diethylenetriamine pentaacetic acid; LED, light-emitting diode; LSM, low-serum medium; LY-R, L5178Y-R; PDT, photodynamic treatment; SAPK, stress-activated protein...

Cornelis J. H. van de Velde; Chris J. L. M. Meyer; Cees J. Cornelisse; Edo A. van der Velde; Luke M. van Putten; Albert Zwaveling



NEWS & NOTES Sooah Chae (DMA, `03 from the studio of Nancy Weems) per-  

E-Print Network (OSTI)

cello; Timothy Hester, piano Works by Debussy, Kodály, Brahms Monday, November 7, 7:00 pm 21st Annual Recital Hall Thursday, November 10, 8:30 pm Student Recital Nathan Cunningham, tuba (Studio of Mark Barton

Azevedo, Ricardo


E-Print Network 3.0 - aij projects methodology Sample Search...  

NLE Websites -- All DOE Office Websites (Extended Search)

is the algorithm most common- ly... . For example, the data can be collected over any set of lines, the projections do not have to be distributed Source: Cong, Jason "Jingsheng"...


Mass Adult Education: A Necessary Element in the Development of Socialism in Tanzania  

E-Print Network (OSTI)

on aduLt education in Tanzania. He is currentLy head of theof Adul-t Educators in Tanzania. A paper delivered at theAduLt Education in Tanzania-- A Handbook on Approaches,

Hall, Budd L.



September 20 Save Money on Home Energy Efficiency  

E-Print Network (OSTI)

September 20 Save Money on Home Energy Efficiency Evaluate home energy use and learn practical cost effective improvements. http://bit.ly/SaveEn October 25 When Mom & Dad Need Help Managing their Finances

Watson, Craig A.


Naval Support Activity (NSA) in Bethesda Employment Education Fair  

Energy.gov (U.S. Department of Energy (DOE))

Location: NSA Bethesda Fitness Center (Gymnasium, Bldg 17), 8901 Wisconsin Ave., Bethesda, MD 20889Attendees: Donna Friend (HC) and Rauland Sharp (HC)POC: Donna FriendWebsite: http://bit.ly/1yTjTNu


itcGill Radarl{eather 0bservatory _ llacdonald Campusof l'lcGiI I Unj verii tv  

E-Print Network (OSTI)

-p."Oi.t, D = _4/3, 5/3 for isouarsiro-ii"irl..ils=.espect_ iye'ly, in a two-dinnnsionalc"oii_ie.iion

Lovejoy, Shaun


Desalination, 48 (1983) l-16 Elsevier Science Publishers B.V., Amsterdam -Printed in The Netherlands  

E-Print Network (OSTI)

, S.B. McCRAY AND J.W. McCUTCHAN Chemical, Nuclear and Thermal Engineering Department, University instability, gas injection must be carried out continuous- ly. A six hour pre-injection period was required

Zachariah, Michael R.


American Recovery & Reinvestment Act Newsletter - Issue 28  

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

ulti- mately be sent to the WTP can be accurate- ly sampled. "We've clearly shown in our small scale mixing work that we can sample extreme waste particulates in a manner...


The thirteenth AAAI Mobile Robot Competition and Exhibition was once again collocated with  

E-Print Network (OSTI)

events. T he thirteenth AAAI Mobile Robot Com- petition and Exhibition was held last Ju- ly, Bruce Maxwell, Ashley Stroupe, Jennifer Casper, Adam Jacoff, Holly Yanco, and Magda Bugajska AI Magazine

Maxwell, Bruce



E-Print Network (OSTI)

square-free monomials m1,...,mr, set a[t] = (mt. 1,...,mt. r) for integers t ? 0. Lyubeznik [Ly1, Theorem 1 (i)] proved that the natural maps. Exti. R(R/a[t],R) ?? Hi.


Left globus pallidus abnormality in never-medicated patients with schizophrenia  

Science Journals Connector (OSTI)

...Natl. Acad. Sci. USA 84 (1987) 563 vantages in dichotic listening, dichotic shadowing, handed- ness, performance on psychometric...connections (32). Unfortunate- ly, the resolution of the imaging device used in this study does not permit us to distinguish between...

T S Early; E M Reiman; M E Raichle; E L Spitznagel



Microsoft Word - DOE_science_kits.docx  

NLE Websites -- All DOE Office Websites (Extended Search)

city from co ponding ma o sponsorin s for eleme nt of Energy Office Pilot Plant Mexico Opens r Middle ly 13, 2011 o learn abo bad Field Of e Waste Iso geologic re te...



E-Print Network (OSTI)

based solar energy commercialization project (Project SAGE).demonstra- tion projects in solar energy by Dr. Weingart offollowi7lY Solar Energy Devel~ opment ProJects: (i) OTEC sea

Authors, Various



HBCU College Festival sponsored by Alfred Street Baptist Church  

Energy.gov (U.S. Department of Energy (DOE))

Location: T.C. Williams High School, 3330 King St, Alexandria, VA 22302Attendees: Rauland Sharp (HC) and Dameone Ferguson (NNSA)POC: Chester Scott Website: http://bit.ly/1BARRqp

Note: This page contains sample records for the topic "vleet hol ly" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


E-Print Network 3.0 - absorption model analysis Sample Search...  

NLE Websites -- All DOE Office Websites (Extended Search)

to six stars with theoretical models for di11;erent assumed mass loss... the blue-side excess Ly11; absorption predicted by the four models of the 11; CenProxima Cen... ....



E-Print Network (OSTI)

lyFind the equation of the tangent line to the graph of g(.'13) : M at :1: : 4. ... {VIM population P, in thousands, of a small city is given by. 5015 where t is the time in


ENGLISH SUMMARY Breast cancer is the most common malignancy among women in the western world. The  

E-Print Network (OSTI)

with CXCR4. Secondly, the activation of CXCR3 and CXCR4 were measured with calcium influx assay to validate with LY294002, inhibited the CXCL11-induced MTLn3 cell invasion. The disruption of autocrine loop of CXCR3

van den Brink, Jeroen


Thermal Dosimetry and Temperature Measurements  

Science Journals Connector (OSTI)

...N-acetyl-dihydrosphingosine; DAG, diacylglycerol; DETAPAC, diethylenetriamine pentaacetic acid; LED, light-emitting diode; LSM, low-serum medium; LY-R, L5178Y-R; PDT, photodynamic treatment; SAPK, stress-activated protein...

D. A. Christensen



New HTLV-1 and HTLV-2 infections in rural population, in North of Gabon, Central Africa  

Science Journals Connector (OSTI)

The emergence of Human retroviruses, in Central Africa, may occur in contact with non human primates, during hunting and butchering. Recent studies described several cases of human infections with Human T-cell Ly...

Augustin Mouinga Ondeme; Rodrigue Bikangui; Ulrick Bisvigou; Paul Ngari…



DOE Secretary Steven Chu has selected the  

E-Print Network (OSTI)

the Bulletin DOE Secretary Steven Chu has selected the staff of the RHIC/ ATLAS Computing Facility of the ear- ly universe by collid- ing heavy ions such as gold -- and the ATLAS experiment, located

Johnson, Peter D.


E-Print Network 3.0 - annual cycle solar Sample Search Results  

NLE Websites -- All DOE Office Websites (Extended Search)

is clouds... Ch.2 Solar Energy to Earth and the Seasons The Solar System, Sun, and Earth Solar Energy: From... s 1 light-year (ly) 9.5 trillion km Light year is a unit of...


E-Print Network 3.0 - absorbing galaxies mrk Sample Search Results  

NLE Websites -- All DOE Office Websites (Extended Search)

nearby ( 2000-2500 km s-1 ) Ly-absorbers. The absorbers are located along the sight lines towards Markarian 817, Markarian 509 and VII Zwicky 118. The Summary: from 3.2107...


Hiring Our Heroes | Department of Energy  

Energy Savers (EERE)

Hiring Our Heroes Hiring Our Heroes November 14, 2014 10:00AM to 1:00PM EST Location: 1401 N. Wheeler, Portland, OR 97227 POC: Helen Bain Website: http:bit.ly1yQOmHR...


E-Print Network 3.0 - alternative high-z cosmic Sample Search...  

NLE Websites -- All DOE Office Websites (Extended Search)

5 > >> 1 StructureStructure in the Universein the Universe Summary: -rays Gaseous Cosmic Web - Baryonic gas traces the Cosmic Web: Ly forest neutral hydrogen gas, mostly at high...


Ceramide Generation in Response to Photodynamic Treatment of L5178Y Mouse Lymphoma Cells  

Science Journals Connector (OSTI)

...N-acetyl-dihydrosphingosine; DAG, diacylglycerol; DETAPAC, diethylenetriamine pentaacetic acid; LED, light-emitting diode; LSM, low-serum medium; LY-R, L5178Y-R; PDT, photodynamic treatment; SAPK, stress-activated protein...

Duska Separovic; Jin He; Nancy L. Oleinick



E-Print Network 3.0 - anticuerpos contra chlamydia Sample Search...  

NLE Websites -- All DOE Office Websites (Extended Search)

for Two New Insect-Associated Chlamydia of the Family Simkaniaceae MyLo Ly... the elementary and reticulate bodies of chlamydia (Costa HS, Westcot DM, Ullman DE, Rosell R, Brown...


Detection of Lyman-alpha emission from a DLA galaxy: Possible implications for a luminosity-metallicity relation at z = 2-3  

E-Print Network (OSTI)

In an ongoing programme to identify a sample of high z DLA galaxies we have found the long sought for case of a Ly-alpha emitter seen in the centre of a broad DLA trough. This is the predicted `textbook case' of an intervening DLA galaxy if DLA galaxies are small, but would not be expected if intervening high redshift DLA galaxies have large gaseous disks. The Ly-alpha flux is 5.4{+2}{-0.8} * 1e-17 ergs/s/cm2 similar to what has been found in previously known high z DLA galaxies. The impact parameter is found to be 0.3+-0.3 arcsec. This is smaller than what was found in previous cases but still consistent with random sight-lines through absorbers with mean impact parameter ~1 arcsec. Of the 24 DLAs targeted in the NICMOS imaging survey five have now been identified as Ly-alpha emitters. The DLA galaxies with detected Ly-alpha emission tend to have higher interstellar metallicities than those with undetected Ly-alpha emission. This is plausibly explained as a consequence of a positive correlation between the Ly-alpha line luminosities of the galaxies and their metallicities, although the present sample is too small for a definitive conclusion. The available observations of high-redshift DLA galaxies are also consistent with a negative correlation between Ly-alpha equivalent widths and metallicities, as seen in nearby star-forming galaxies and usually attributed to the preferential absorption of Ly-alpha photons by dust grains.

P. Moller; J. P. U. Fynbo; S. M. Fall



A Note on the Associative Law  

Science Journals Connector (OSTI)

......We have (4) ALx = EL{xB.eC)DF for all* of 0. Combining this with (3) and cancelling F, we get (6) Ly El^xB. eOD = EL(XB . vOD for all x, y of 0. Let x = b in (5),y where 6 is a solution of (xB eC) D = e. Then (6) LyE^ELto......

T. Evans



An Evaluation of the Impact of Surface Coatings on the Heat Transfer in High Temperature Ceramic Recuperators  

E-Print Network (OSTI)

COATINGS Engineering ceramics, particular ly SiC, are being investigated for use as high temperature heat exchanger materials. ORNL has conducted exposure test in real and simulated high tempera ture corrosive flue gases and these have... indicated that SiC ceramics are sucepti ble to flue gases containing sodium and potassium, compounds such as sulfates, carbonates and halides. ORNL is current ly investigating whether commercially available ceramic coatings could be from 1500 0...

Guerrero, P. S.; Rebello, W. J.; Federer, J. I.


On The Detection Of Ionizing Radiation Arising From Star-Forming Galaxies At Redshift z ~ 3-4 : Looking For Analogs Of "Stellar Reionizers"  

E-Print Network (OSTI)

We use the spatially-resolved, multi-band photometry in the GOODS South field acquired by the CANDELS project to constrain the nature of candidate Lyman continuum (LyC) emitters at redshift z~3.7 identified using ultra-deep imaging below the Lyman limit (1-sigma limit of ~30 AB in a 2" diameter aperture). In 18 candidates, out of a sample of 19 with flux detected at >3-sigma level, the light centroid of the candidate LyC emission is offset from that of the LBG by up to 1.5". We fit the SED of the LyC candidates to spectral population synthesis models to measure photometric redshifts and the stellar population parameters. We also discuss the differences in the UV colors between the LBG and the LyC candidates, and how to estimate the escape fraction of ionizing radiation (f_esc) in cases, like in most of our galaxies, where the LyC emission is spatially offset from the host galaxy. In all but one case we conclude that the candidate LyC emission is most likely due to lower redshift interlopers. Based on these fi...

Vanzella, Eros; Giavalisco, Mauro; Grazian, Andrea; Castellano, Marco; Cristiani, Stefano; Dickinson, Mark; Fontana, Adriano; Nonino, Mario; Giallongo, Emanuele; Pentericci, Laura; Galametz, Audrey; Faber, S M; Ferguson, Henry C; Grogin, Norman A; Koekemoer, Anton M; Newman, Jeffrey; Siana, Brian D



Systematic Survey of Extended Lyman-alpha Sources over z~3-5  

E-Print Network (OSTI)

Spatially extended Ly-alpha sources which are faint and compact in coninuum are candidates for extremely young galaxies (age of ~intermediate-band imaging data taken with the Suprime-Cam on the Subaru Telescope. Our survey covers a field of view of 33' * 25' and a redshift range of 3.24Ly-alpha flux of ~1e-17 ergs/cm^2/s. We identified 41 extended Ly-alpha sources. The redshift distribution of these sources shows that this kind of objects are common in the early universe over the surveyed redshift range. The identified objects have typical sizes of \\~10-15 kpc and luminosities of ~10^42 ergs/s. Follow-up spectroscopy made for 7 of the 41 objects showed that our sample suffers from little contamination. All 7 objects have large equivalent widths of Ly-alpha emission line, all but one exceeding 240A in the rest frame. The large equivalent widths suggest that their extended Ly-a...

Saitô, T; Okamura, S; Ouchi, M; Akiyama, M; Yoshida, M; Saito, Tomoki; Shimasaku, Kazuhiro; Okamura, Sadanori; Ouchi, Masami; Akiyama, Masayuki; Yoshida, Michitoshi



Coordinated UV-optical observations of quasars: the evolution of the Lyman absorption  

E-Print Network (OSTI)

The average flux decrement shortward the Ly$_{\\alpha}$ emission, due to the well-known ``forest'' of absorptions, has been measured in the spectra of 8 quasars. Quasi-simultaneous optical and IUE observations of the two low redshift quasars PKS 0637--75 (z=0.654) and MC 1104+16 (z=0.632) have been carried out, obtaining relatively high S/N, spectrophotometrically calibrated data on their energy distribution from the rest frame H$_{\\beta}$ to the Lyman continuum. Six more quasars in the redshift range 2.5-3.4 have been observed in the optical domain. For all the quasars the ``intrinsic'' continuum slope and normalization have been estimated longward the Ly$_{\\alpha}$ emission and extrapolated towards the Lyman continuum to measure the average depressions, which have been compared with the model statistics of the Ly$_{\\alpha}$ clouds. When all the known classes of absorbers are taken into account with plausible values for their equivalent width distribution and evolution, a good agreement is obtained with the observations. The results for the observed continuum decrement at $z \\sim 0.65$ are identical to those predicted by the evolution with redshift of the number of Ly$_{\\alpha}$ forest systems including the HST data and within $2\\sigma$ of the predicted value using the ``standard'' Ly$_{\\alpha}$ evolution (as determined only at high z).

S. Cristiani; E. Giallongo; L. M. Buson; C. Gouiffes; F. La Franca



A VLT colour image of the optical Einstein ring 0047-2808  

E-Print Network (OSTI)

The optical Einstein ring 0047-2808 was imaged by the VLT UT1 during the science verification programme. The ring is the image of a high-redshift z=3.595 star-forming galaxy, with strong Ly-alpha emission at 5589A, gravitationally lensed by a massive early-type galaxy at z=0.485. Relative to earlier NTT data the high signal-to-noise ratio of the VLT Ly-alpha narrow-band image allows much improved constraints to be placed on the surface-brightness profile of the source and on the mass, leading to a measured mass-to-light ratio of M/L(B)~13h for the deflector galaxy. We have combined the VLT B-band and Ly-alpha narrow-band images with a K-band image obtained at UKIRT to produce a deep colour image of the system.

S. J. Warren; G. F. Lewis; P. C. Hewett; P. Moller; P. Shaver; A. Iovino



A Lyman-alpha blob in the GOODS South field: evidence for cold accretion onto a dark matter halo  

E-Print Network (OSTI)

We report on the discovery of a z = 3.16 Lyman-alpha emitting blob in the GOODS South field. The blob has a total Ly-alpha luminosity of ~ 10^(43) erg s^(-1) and a diameter larger than 60 kpc. The available multi-wavelength data in the GOODS field consists of 13 bands from X-rays (Chandra) to infrared (Spitzer). Unlike other discovered Ly-alpha blobs, this blob shows no obvious continuum counter-part in any of the broad-bands. In particular, no optical counter-parts are found in the deep HST/ACS imaging available. For previously published blobs, AGN (Active Galactic Nuclei) or 'superwind' models have been found to provide the best match with the data. We here argue that the most probable origin of the extended Ly-alpha emission from the blob in the GOODS South field is cold accretion onto a dark matter halo.

Kim Nilsson; Johan P. U. Fynbo; Palle Moller; Jesper Sommer-Larsen; Cedric Ledoux


Note: This page contains sample records for the topic "vleet hol ly" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


Expansion and Collapse in the Cosmic Web  

Science Journals Connector (OSTI)

We study the kinematics of the gaseous cosmic web at high redshift using Ly? forest absorption in multiple QSO sight lines. Observations of the projected velocity shifts between Ly? absorbers common to the lines of sight to a gravitationally lensed QSO and three more widely separated QSO pairs are used to directly measure the expansion of the cosmic web in units of the Hubble velocity, as a function of redshift and spatial scale. The lines of sight used span a redshift range from about 2 to 4.5 and represent transverse scales from the subkiloparsec range to about 300 h physical kpc. Using a simple analytic model and a cosmological hydrodynamic simulation, we constrain the underlying three-dimensional distribution of expansion velocities from the observed line-of-sight distribution of velocity shear across the plane of the sky. The shape of the shear distribution and its width (14.9 km s-1 rms for a physical transverse separation of 61 h kpc at z = 2, 30.0 km s-1 for 261 h kpc at z = 3.6) are found to be in good agreement with the IGM undergoing large-scale motions dominated by the Hubble flow, making this one of the most direct observations possible of the expansion of the universe. However, modeling the Ly? clouds with a simple "expanding pancake" model, the average expansion velocity of the gaseous structures causing the Ly? forest in the lower redshift (z ~ 2) smaller separation (61 kpc) sample appears about 20% lower than the local Hubble expansion velocity. In order to understand the observed velocity distribution further we investigated the statistical distribution of expansion velocities in cosmological Ly? forest simulations. The mean expansion velocity in the (z ~ 2, separation ~ 60 kpc) simulation is indeed somewhat smaller than the Hubble velocity, as found in the real data. We interpret this finding as tentative evidence for some Ly? forest clouds breaking away from the Hubble flow and undergoing the early stages of gravitational collapse. However, the distribution of velocities is highly skewed, and the majority of Ly? forest clouds at all redshifts from 2 to 3.8 expand with super-Hubble velocities, typically about 5%-20% faster than the Hubble flow. This behavior is explained if most Ly? forest clouds in the column density range typically detectable are expanding filaments that stretch and drain into more massive nodes. The significant difference seen in the velocity distributions between the high- and low-redshift samples may conceivably reflect actual peculiar deceleration, the differences in spatial scale, or our selecting higher densities at lower redshift for a given detection threshold for Ly? forest lines. We also investigate the alternative possibility that the velocity structure of the general Ly? forest could have an entirely different, local origin, as expected if the Ly? forest were produced or at least significantly modified by galactic feedback, e.g., winds from star-forming galaxies at high redshift. However, we find no evidence that the observed distribution of velocity shear is significantly influenced by processes other than Hubble expansion and gravitational instability. To avoid overly disturbing the IGM, galactic winds may be old and/or limp by the time we observe them in the Ly? forest, or they may occupy only an insignificant volume fraction of the IGM. We briefly discuss the observational evidence usually presented in favor of an IGM afflicted by high-redshift extragalactic superwinds and find much of it ambiguous. During the hierarchical buildup of structure, galaxies are expected to spill parts of their interstellar medium and to heat and stir the IGM in ways that make it hard to disentangle this gravitational process from the effects of winds.

Michael Rauch; George D. Becker; Matteo Viel; Wallace L. W. Sargent; Alain Smette; Robert A. Simcoe; Thomas A. Barlow; Martin G. Haehnelt



GRB 000301C: a possible short/intermediate duration burst connected to a DLA system  

E-Print Network (OSTI)

We discuss two main aspects of the GRB 000301C afterglow (Fynbo et al. 2000, Jensen et al. 2000); its short duration and its possible connection with a Damped Ly-alpha Absorber (DLA). GRB 000301C falls in the short class of bursts, though it is consistent with belonging to the proposed intermediate class or the extreme short end of the distribution of long-duration GRBs. Based on two VLT spectra we estimate the HI column density to be Log(N(HI))=21.2+/-0.5. This is the first direct indication of a connection between GRB host galaxies and Damped Ly-alpha Absorbers.

J. Gorosabel; J. U. Fynbo; B. L. Jensen; P. Moller; H. Pedersen; J. Hjorth; M. I. Andersen; K. Hurley



Word Pro - Untitled1  

U.S. Energy Information Administration (EIA) Indexed Site

chemical compounds composed of chemical compounds composed of carbon, hydrogen, and oxygen. The series of molecules vary in chain length and are composed of a hydrocarbon plus a hydroxyl group: CH 3 -(CH 2 )n-OH (e.g., metha- nol, ethanol, and tertiary butyl alcohol). See Fuel Ethanol. Alternative Fuel: Alternative fuels, for transportation applications, include the following: methanol; denatured ethanol, and other alcohols; fuel mixtures contain- ing 85 percent or more by volume of methanol, denatured ethanol, and other alco- hols with motor gasoline or other fuels; natural gas; liquefied petroleum gas (propane); hydrogen; coal-derived liquid fuels; fuels (other than alcohol) derived from biological materials (biofuels such as soy diesel fuel); electricity (including electricity from solar energy); and "... any other fuel the Secretary determines, by


The electronic structure of arene tricarbonyl complexes of group 6 metals: ultraviolet photoelectron spectra and molecular orbital calculations, and the low-temperature X-ray crystal structure of hexamethylbenzene chromium tricarbonyl  

E-Print Network (OSTI)

okl, k=2n+1 hol, 1=2n+ 1 hko, h=2n+1 13. 622(1)A 13. 369(2)A 15. 162(3)A 2761. 2As 8 1. 43g cm s Enraf-Nonius CAD-4 Mo K (X = 0. 71073A) 21 cm 2. 0 to 2. 6 mm horizontal 2. 0 mm vertical Scan type Scan rate Scan width(') Maximum 2e.... Fischer in 1955. The 1973 Nobel prize in chemistry was shared by E. O. Fischer and G. Wilkinson for their pioneering work, performed separately, on "sandwhich" complexes such as (Bz)zCr (in this thesis Bz=benzene, Tmb=1, 3, 5-trimethylbenzene, and Hmb...

Byers, Brien Patrick



Lovers" Leap  

E-Print Network (OSTI)

and the actors who EnfemT- ?o mlw f"tert,a'n^nt hereJ ?s is purelv amatter of Pereona' view; "alternate r Ql^ANTUMyLFAP9niw L '" "^r W?rdS| ?nat if"?" This 2ine *? not call the stars ofSta^rtrr ^S-WJ * ?re than one would ca" Max von Svdow. Wil|em Defoe... anice straigh let Itaf 6 ?Ut there than ,here are of ,hese' after a]l Uve and t? ?? 'would'ike to ,ake ?his opportunity to thank several people for making this all possible(YouYe S k?d STeotalp0 ^^ hol?9rapnic sex is a,urn-?n: wnat abunch of perverts...

Multiple Contributors



Vol. 92 Concord, NH, Wednesday, November 6, 2013 No. 37 Weekly Market Bulletin  

E-Print Network (OSTI)

to recruit new members and future customers for the full-service cooperative grocery store the group plans sustainability. The cooperative- ly owned business "strives to serve the North Country of New HampshireVol. 92 Concord, NH, Wednesday, November 6, 2013 No. 37 Weekly Market Bulletin State of New

New Hampshire, University of


Biophysics of Bird Flight  

Science Journals Connector (OSTI)

...small field and can be disassembled for return to its base by trailer (6a). During the glide of the bird, the measuring sailplane...disclosed that the porpoise is complete-ly covered with a hydraulic skin 1/16 inch thick that is elastic and ducted. Kramer...

August Raspet



News & Notes The Trombone Choir, under the direction of Timothy  

E-Print Network (OSTI)

Bertman and Mark Barton, will be featured in the "Music at St. Martins Concert Series" on Sunday, April 18 Recital Hall Nien Ly, piano (Studio of Timothy Hester) Tuesday, April 13, 6:30 pm STUDENT RECITAL - Dudley STUDENT RECITAL - Dudley Recital Hall Brandon Pafford, piano (Studio of Timothy Hester) Saturday, April 17

Azevedo, Ricardo


Effects on milk protein yield of graded levels of lysine infused into the duodenum of dairy cows fed diets  

E-Print Network (OSTI)

Effects on milk protein yield of graded levels of lysine infused into the duodenum of dairy cows). In order to determine ly- sine requirements, graded levels of lysine (0, 15, 30, 45 g/d) were infused period (2 wk) they received a duo- denal infusion of one dose of lysine + 11 g of methionine and enough

Paris-Sud XI, Université de


Finding typical high redshift galaxies with the NOT  

E-Print Network (OSTI)

We present results from an ongoing search for galaxy counterparts of a subgroup of Quasar Absorption Line Systems called Damped Ly-alpha Absorbers (DLAs). DLAs have several characteristics that make them prime candidates for being the progenitors of typical present day galaxies.

J. U. Fynbo; P. Moller; B. Thomsen



"Ask Argonne" - Charlie Catlett, Computer Scientist, Part 2  

ScienceCinema (OSTI)

A few weeks back, computer scientist Charlie Catlett talked a bit about the work he does and invited questions from the public during Part 1 of his "Ask Argonne" video set (http://bit.ly/1joBtzk). In Part 2, he answers some of the questions that were submitted. Enjoy!

Catlett, Charlie



Released on receipt but intended for use  

E-Print Network (OSTI)

be possible t o produce a good-sized thundershower by mere- ly burning down a forest, or, if one preferred. The idea of generating rain by means of artificial vortices in the atmos- phere, produced (p3gardless the deposit of water an the out- side of an ice pitcher, proposed t o set up a barrier packed with ice


VOLUME 71, NUMBER 7 PHYSICAL REVIEW LETTERS 16 AUGUST 1993 Effects of Adsorption Site and Surface Stress on Ordered Structures of Oxygen Adsorbed on W(110)  

E-Print Network (OSTI)

Stress on Ordered Structures of Oxygen Adsorbed on W(110) K. E. Johnson, * R. J. Wilson, and S. Chiang: 68.35.Bs, 68.35.Rh, 68.60.Dv, 82.65.My Atomic scale ordering of adsorbates at surfaces strong- ly to elucidating the fundamen- tal physical origins of adsorbate ordering and phase diAerentiation. It is precisely

Chiang, Shirley


Project Summary Report 1781-S 1 The University of Texas at Austiny of Texas at Austiny of T  

E-Print Network (OSTI)

direct- ly affects the reliability of a test program in characterizing the properties of the materi- als and improve the effectiveness and efficiency of construction qual- ity control. The implementation of this research to collect infor- mation on current QC/QA practices among state DOTs and other agencies. It shows

Texas at Austin, University of


JOURNAL DE PHYSIQUE Colloque C4, supplment au n 4, Tome 40, avril 1979, page C4-181 Crystal-field effects in NdP-UP solid solution studied by neutron spectroscopy  

E-Print Network (OSTI)

for uranium ion as derived from the high-temperature susceptibi- lity results, indicates that the doublet F6 the mixed uranium-neodymium monophosphides. The boundary compounds NdP and UP have metal- lic conductivity and order antif erromagnetical- ly at 11 and 125 K respectively. Uranium and neody- mium ions

Boyer, Edmond


Network Planning Aspects of the HeliNet Telecommunications Architecture  

E-Print Network (OSTI)

Network Planning Aspects of the HeliNet Telecommunications Architecture Zs. Pándi*°, T. V. Do*, Cs. Király* *Department of Telecommunications, Budapest University of Technology and Economics Magyar Tudósok of a telecommunication infrastructure based on HAVE (High Altitude Very long Endurance) unmanned solar aerodynamic

Do, Tien Van


Lead in albacore: guide to lead pollution in Americans  

Science Journals Connector (OSTI)

...main-ly used in drilling oil wells, making paint and smoke...This value stands as a benchmark that correctly ori-ents scientific...on the basis of the lowest cost per analysis. The aca-demic...International Council for the Exploration of the Sea, 20 of 63 participating...

DM Settle; CC Patterson



Schedule-Dependent Synergy between the Heat Shock Protein 90 Inhibitor 17-(Dimethylaminoethylamino)-17-Demethoxygeldanamycin and Doxorubicin Restores Apoptosis to p53-Mutant Lymphoma Cell Lines  

Science Journals Connector (OSTI)

...with previously reported loss of pRb phosphorylation...differences in cell cycle distribution. WT p53 TK6 and OCI-Ly3...Schedule-dependent synergy between the heat shock protein 90 inhibitor...lymphoma cell lines. | Loss of p53 function impairs...examined the effect of the heat shock protein 90 (HSP90...

Ana I. Robles; Mollie H. Wright; Bheru Gandhi; Steven S. Feis; Christin L. Hanigan; Adrian Wiestner; and Lyuba Varticovski



Evolutionary Trends in Heteroptera. Part 1, Eggs, Architecture of the Shell, Gross Embryology and Eclosion. R. H. Cobben. Centre for Agricultural Publications and Documentation, Wageningen, The Netherlands, 1968. viii + 476 pp., illus. Dfl. 55. Laboratorium voor Entomologie, Wageningen, Mededeling No. 151. Also published as Agricultural Research Reports, No. 707  

Science Journals Connector (OSTI)

...so quick-ly to pick up the feel of research in France. ALISON JOLLY The Old Brewery House, Southover High Street, I,ewes...are so speculative, however, that the author may have been wise not to spend too much time on them. On the whole, the mass...

Richard Froeschner



Book Reviews  

Science Journals Connector (OSTI)

...liber-ty." The role of energy in the history of mankind is...question of whether we have enough energy re-sources on earth to support...also in-crease and their storage may eventual-ly tax our technological...a breakthrough in producing energy by nuclear fusion, but then...


Note: This page contains sample records for the topic "vleet hol ly" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


Expanded Program  

Science Journals Connector (OSTI)

...Health T-Helper: Automated support for protocol-directed...and laboratory simulation ofRNA evolution...system is evolving rapid-ly asJapanese...analytical methods in the rapid development of rDNA...advances in computer modeling. Saturday, AM...flight experiment to simulation: Muriel D. Ross...



RHIC Spin Program Goals of RHIC Spin Program  

E-Print Network (OSTI)

longitudinal polarization · polarized atomic hydrogen jet target Installed and commissioned during run 4 violating production of W± · Transverse spin: Transversity () & transverse spin effects with connections to orbital angular momentum (Ly) #12;5/11/2006 L.C.Bland, DOE Review of MEP 5 Methods to Address Spin


A Model of Optimal Portfolio Selection under Liquidity Risk and Price Impact  

E-Print Network (OSTI)

A Model of Optimal Portfolio Selection under Liquidity Risk and Price Impact Vathana LY VATH risky asset subject to liquidity risk and price impact. In this market, an investor may transfer funds between the two assets at any discrete time. Each purchase or sale policy decision affects the price

Paris-Sud XI, Université de



E-Print Network (OSTI)

basic Search (autocomplete) 10 Full Search 11 browsing Menus 12 PERFORMING aNaLySIS 12 Navigating Functions 13 Stock/Company Screening 14 analyzing a Company 15 analyzing an Index, bond or Currency 16 Ex sectors. It features company financials, market data spanning more than 20 years, charts, statistics

Banaji,. Murad


DOI: 10.1002/chem.200700480 Visible Light Induced Catalytic Water Reduction without an Electron Relay  

E-Print Network (OSTI)

cells to drive electrolysis,[1] semiconductor-based charge separation techniques,[2­4] thermochemical photosensitizer, thereby creating charge separation at the cost of reducing the systems free energy. Numerous systems where a photosensitizer is covalent- ly linked to a hydrogen evolving metal complex.[32­35] Aside

Bernhard, Stefan


Industrial Energy in Transition: A Petrochemical Perspective  

Science Journals Connector (OSTI)

...synthesis gas available is the following: 1) The need for medium Btu gas (more or less synonymous with synthesis gas) for...PUROX pro-cess, based on a unique, oxygen-fed slagging gasifier that has been extensive-ly shown in a pilot plant (yielding...

Ronald S. Wishart



BPRIDE&PROGRESS2012 By Nathan Bergstedt  

E-Print Network (OSTI)

gathered on the specific site picked for the SPRUCE Experiment, adding great- ly to the future data, and the potential feedback to the atmosphere could be big depending on what climate change we might expect Experimental Forest, pro- viding electricity to all the instruments. Because of the scale of


Direct Observation of Dynamical Bifurcation in a Superfluid Josephson Junction Supradeep Narayana and Yuki Sato  

E-Print Network (OSTI)

Direct Observation of Dynamical Bifurcation in a Superfluid Josephson Junction Supradeep Narayana Josephson junction. We excite the superfluid plasma resonance into a nonlinear regime by driving below.205302 PACS numbers: 67.25.dg, 07.60.Ly, 47.20.Ky, 85.25.Cp A superfluid Josephson junction is formed

Sato, Yuki


"Ask Argonne" - Charlie Catlett, Computer Scientist, Part 2  

SciTech Connect

A few weeks back, computer scientist Charlie Catlett talked a bit about the work he does and invited questions from the public during Part 1 of his "Ask Argonne" video set (http://bit.ly/1joBtzk). In Part 2, he answers some of the questions that were submitted. Enjoy!

Catlett, Charlie



Protest, Page 8 The Weather  

E-Print Network (OSTI)

meeting immediate- ly after the PlayFair and before the Residence Midway Sunday night. The meeting included midway coordinators Sherri E. Davidoff '03, Grace R. Kessenich '03, and Tyler J. Bronder '03's resi- dence midway was briefly imper- iled. The clashes have revealed deep fissures between students


Anthropogenic Chlorofluoromethanes in the Greenland and Norwegian Seas  

Science Journals Connector (OSTI)

...that are younger than the Bonneville shoreline (5). The scarps...year calculated for the Bonneville shore-line yields an age...Ed. (Federal Aviation Administration, Washington, D.C., 1980...moderate-ly high resolving power, show weak at-mospheric...




Leading Scientists Active in New Committee on Economics of Peace  

Science Journals Connector (OSTI)

...electricity for the fed-erally owned Bonneville Power Ad-ministration (the TVA of...this story (an anti-public-power man) does not seem to particular-ly...practitioner progranm, which the Administration wanted to hold at the present...



Theory and Applications of Categories, Vol. 20, No. 13, 2008, pp. 405-496. QUOTIENTS OF UNITAL A1 -CATEGORIES  

E-Print Network (OSTI)

words and phrases: A1 -categories, A1 -functors, A1 -transformations, 2-* *categories, 2-functors and Verdier [Ver77]. The second answer - a differential graded category D - is given by Drinfeld * *[Dri-construction type - is given by Ly* *ubashenko and Ovsienko [LO06]. This A1 -category is especially useful when

Chapman, Robin


Reusable Knowledge for Best Clinical Practices: Why We Have Difficulty Sharing And What We Can Do  

E-Print Network (OSTI)

Reusable Knowledge for Best Clinical Practices: Why We Have Difficulty Sharing And What We Can Do is the difficulty in creating shareable repositories of best practice knowledge. A host of proprietary systems makes it difficult to have a wide- ly accepted representation format. Different uses of knowledge and contextualized

Peleg, Mor


Pseudomonas fluorescens -A robust manufacturing platform  

E-Print Network (OSTI)

Pseudomonas fluorescens -A robust manufacturing platform Reprinted from July/August 2004 Speciality at efficient- ly transporting single chain antibodies and other mammalian-derived proteins. In addition production. Dowpharma, a contract manufacturing services unit of Dow Chemical, has developed a manufacturing

Lebendiker, Mario


Visualization of Turbulent Flame Fronts with Planar Laser-Induced Fluorescence  

Science Journals Connector (OSTI)

...TWO-DIMENSIONAL GAS CONCENTRATION MEASUREMENTS...flames at atmospheric pressure. More-over, the...carried out at constant pressure and the molecular...win-dows in the combustor. A simple fused...because ofthe often high and rapid-ly fluctuating...made it an ideal natural laboratory for the...




A procedure for determining contents of rabbit stomachs and its application to cottontails on the Gene Howe Wildlife Management Area in midwinter  

E-Print Network (OSTI)

~ Submitted to the Graduate Scbool of. toe Agricultural and t ecoanxcal College of 'fexas in partial fulfillment of tbe rec:uirements for tbe degree of ~TmR OF oGIMG~ . ny ly5U mAJOR SUiSJFG1 & HARCn mA5AGbiaL'8T LISRARY & 4 Nl COLLEGE OF TEXACO A dHv...

Davis, Charles A



Multiwavelength Thermal Emission  

E-Print Network (OSTI)

Multiwavelength Astronomy NASA #12;Thermal Emission #12;Thermal Emission Non-thermal p-p collisions Optical IR Radio/ Microwave sources of emission massive stars, WHIM, Ly many dust, cool objects-ray ~GeV Gamma-ray ~TeV sources of emission AGN, clusters, SNR, binaries, stars AGN (obscured), shocks

California at Santa Cruz, University of


Citation for attached reprint: Smith, M. L., S. B. Hedges, W. Buck, A. Hemphill, S. Inchaustegui, M. Ivie, D. Martina, M.  

E-Print Network (OSTI)

ecoregions. Mexico City: CEMEX. Note: This reprint was supplied by the publisher, with photos removed of the area of the hotspot in Mexico. Conservation action to counter the ongoing threats to the Mesoamerica. The Mesoamerica Hotspot also has within it a global- ly recognized model for the value of ecotourism as a for

Hedges, Blair


Mazama and Glacier Peak Pumice Glass: Uniformity of Refractive Index after Weathering  

Science Journals Connector (OSTI)

...combina-tions which has resulted in a group of morphologically similar weathering profiles...glass from poor-ly drained sites also fall within these limits. Thus it is evident...through-out most of the known areas of fall-out; all show refractive indices in...

Virginia C. Steen; Roald Fryxell


Note: This page contains sample records for the topic "vleet hol ly" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


Differences in germination and seedling establishment of alien and native Impatiens species  

E-Print Network (OSTI)

Differences in germination and seedling establishment of alien and native Impatiens species Rozdíly., Jarosík V. & Pysek P. (2009): Differences in germi- nation and seedling establishment of alien and native design. In this study seed and seedling traits of three congeneric alien species in Europe, differing

Kratochvíl, Lukas


Theoretical Surface Science Wintersemester 2007/08  

E-Print Network (OSTI)

. Introduction Surfaces · Processes on surfaces play an enormous- ly important technological role · Harmful processes: 1. Rust, corrosion 2. Wear · Advantageous processes: 1. Production of chemicals 2. Conversion) DFT surface band structure M F M 0 5 -10 -5 Energy(eV) Cu(111): Band gas and parabolic surface band

Pfeifer, Holger


Classical Mechanics (Prof. P. L. Read)  

E-Print Network (OSTI)

cancellation of internal torques #12;Moment of inertia tensor ! Lx Ly Lz " # $ $ $ % & ' ' ' = mi (ri 2 ( xi xi ) i ) ( mi xi yi i ) ( mi xizi i ) ( mi yi xi i ) mi (ri 2 ( yi yi ) i ) ( mi yizi i ) ( mizi xi i ) ( mizi yi i ) mi (ri 2 ( zizi ) i ) " # $ $ $ $ $ $ % & ' ' ' ' ' ' *x *y *z " # $ $ $ % & ' ' ' ! xi

Read, Peter L.


Industrial Energy in Transition: A Petrochemical Perspective  

Science Journals Connector (OSTI)

...available is the following: 1) The need for medium Btu gas (more or less synonymous with...limitation on shale oil production is not the size of the resource, but rather 10 FEBRUARY...based on a unique, oxygen-fed slagging gasifier that has been extensive-ly shown in...

Ronald S. Wishart



Mechanisms of transcriptional activation of estrogen responsive genes in breast cancer cells  

E-Print Network (OSTI)

(SRF) in gel mobility shift assays. Hormone-responsiveness of Egr-1 in MCF-7 cells was specifically inhibited by PD98059, a MAPKK inhibitor, but not by LY294002, an inhibitor of PI3-K. These results contrasted with the hormone-dependent activation...

Chen, Chien-Cheng



Increasing Crop Production Through More Controlled Photosynthesis  

Science Journals Connector (OSTI)

...harvested organ (such as the seed, root, or fruit) are related...converted to the glucose moiety as starch, a major storage product in...6-phosphate (G6P) and then to starch, or it can be exported from...plant such as the growing tip, seeds, roots, or other sinks. Alternative-ly...

James A. Bassham



Micellar structure from comparison of X-ray and neutron small-angle scattering  

E-Print Network (OSTI)

249 Micellar structure from comparison of X-ray and neutron small-angle scattering T. Zemb and P according to the method developed by Hayter and Penfold. Both X-ray and neutron scattering signals, or by a combination of both. It has been shown recent- ly [1, 2] that it is possible in neutron scattering studies

Boyer, Edmond


The mystery of spectral breaks: Lyman continuum absorption by photon-photon pair production in the Fermi GeV spectra of bright blazars  

E-Print Network (OSTI)

We reanalyze Fermi/LAT gamma-ray spectra of bright blazars with a higher photon statistics than in previous works and with new Pass 7 data representation. In the spectra of the brightest blazar 3C 454.3 and possibly of 4C +21.35 we detect breaks at 5 GeV (in the rest frame) associated with the photon-photon pair production absorption by He II Lyman continuum (LyC). We also detect confident breaks at 20 GeV associated with hydrogen LyC both in the individual spectra and in the stacked redshift-corrected spectrum of several bright blazars. The detected breaks in the stacked spectra univocally prove that they are associated with atomic ultraviolet emission features of the quasar broad-line region (BLR). The dominance of the absorption by hydrogen Ly complex over He II, rather small detected optical depth, and the break energy consistent with the head-on collisions with LyC photons imply that the gamma-ray emission site is located within the BLR, but most of the BLR emission comes from a flat disk-like structure ...

Stern, Boris E



BP and Hydrogen Pipelines DOE Hydrogen Pipeline Working Group Workshop  

E-Print Network (OSTI)

BP and Hydrogen Pipelines DOE Hydrogen Pipeline Working Group Workshop August 30-31, 2005 Gary P · UK partnership opened the first hydrogen demonstration refueling station · Two hydrogen pipelines l · " i i l i 2 i i ll i i l pl ifi i · 8" ly idl i i l s Hydrogen Pipelines Two nes, on y a brand


AB&C 12:34 PM Have you ever been faced with a problem in the lab or at  

E-Print Network (OSTI)

to change the world! 2 3 4 To SUBMIT AN IDEA you can Find us on facebook MCBI mHealth Challenge Go to this link: http://bit.ly/RgM5lN Send an email to mcbi@mcgill.ca Scan the QR code below OR OR The mHealth

Shoubridge, Eric


Detection of dark galaxies and circum-galactic filaments fluorescently illuminated by a quasar at z=2.4  

E-Print Network (OSTI)

A deep narrow-band survey for Ly-alpha emission carried out on the VLT-FORS2 has revealed 98 Ly-alpha candidates down to a flux limit of 4.e-18 erg/s/cm^2 in a volume of 5500 comoving Mpc^3 at z=2.4 centered on the hyperluminous quasar HE0109-3518. The properties of the detected sources in terms of their i) equivalent width distribution, ii) luminosity function, and iii) the average luminosity versus projected distance from the quasar, all suggest that a large fraction of these objects have been fluorescently "illuminated" by HE0109-3518. This conclusion is supported by comparison with detailed radiative transfer simulations of the effects of the quasar illumination. 18 objects have a rest-frame Equivalent Width (EW0) larger than 240A, the expected limit for Ly-alpha emission powered by Population II star formation and 12 sources among these do not have any continuum counterpart in a deep V-band imaging of the same field. For these, a stacking analysis indicates EW0>800A, effectively ruling out Ly-alpha power...

Cantalupo, Sebastiano; Haehnelt, Martin G



PLANETARY SURFACES AND ASTR/GEOL 5800 [1: introductory lecture  

E-Print Network (OSTI)

(25%), final (25%) and final group project & presentation (25%). · Homework due on Fridays (beginning Mars radar MESSENGER Mercury 2004- NASA Venus flyby Rosetta Comet 2004- ESA Deep Impact Comet 2005 NASA = 150 million km Nearest star (Proxima Centauri) is 4.2 LY=265,000 AU KB Me V E Ma Note log scales

Mojzsis, Stephen J.


Khesbn no. 61-62 - Autumn - Winter 1970-1971 - Journal  

E-Print Network (OSTI)

StJ't lyl! )t rrtvj s I'N lgh r'ltNT J.r," ltJt' srs N ,-t:l t? illt D ''ly rrs;t /l1"lgh,, rtfty'l .rJD]t: 1y,'1 IrR

Admin, LAYCC



Khesbn no. 45-46 - January 1967 - Journal  

E-Print Network (OSTI)

lybyDll, lls' ']D N lJ'h -}Jh lgh Dg'LD'! Yrll bDNEYll3 El;1lguir.tls ;il'':u -rNIrD l'r! lgh N llN ly:'rDy) ,lJrrly -

Admin, LAYCC



Khesbn no. 71-72 - April 1973 - Journal  

E-Print Network (OSTI)

I22O .uxn-lrl t. :"tt tr:lllN lgh bsnr Db$hyl r1 'J19 Frg 't' ItT 'l']N lyP D$T .D'lr lgh, lrlz''llytND '1y'lly' .D,

Admin, LAYCC



A Polynomial Translation of S4 into T and Contraction?Free Tableaux for S4  

Science Journals Connector (OSTI)

......to pro vide an alternativ e translation of K? in to K ? p olynomial in the size of the input? In fact? it su?ces to pro ceed as w e did in dealing with the con traction? elimination issue in S? ? namely? ?? P olynomial ly transform the input set......

Serenella Cerrito; Marta Cialdea Mayer



PRP5: a helicase-like protein required for mRNA splicing in yeast.  

Science Journals Connector (OSTI)


G Dalbadie-McFarland; J Abelson



Invasive Group B Streptococcal  

E-Print Network (OSTI)

. Ear- ly-onset disease (EOD) occurs within the first week. Late- onset disease (LOD) occurs after implemented in many countries, the incidence of EOD has declined to proportion of EOD and most cases of LOD (3­8). Different studies have suggested that most neonatal invasive

Paris-Sud XI, Université de


Using a drug-word Stroop task to differentiate recreational from dependent drug use  

E-Print Network (OSTI)

, Garavan H. A consistent attentional bias for drug-related material in active cocaine users across word and picture versions of the emotional Stroop task. Drug Alcohol Depend. 2006;81(3):251–257. 38. Franken IHA, Kroon LY, Wiers RW, Jansen A. Selective...

Smith, Dana G.; Ersche, Karen D.



How We Achieved a 41% Energy Reduction  

E-Print Network (OSTI)

nea~ly all moto~s in the 3 - 60 HP ~ange had a estimate this ~nning ~et~ofit p~og~am will save b~eak-even hou~s of ope~ation of less than 8,800 ove~ $2 million annnually. hours, or 1 full yea~ of continuous operation. -------_. __.. SIE"ENS LOUIS...

Maze, M. E.

Note: This page contains sample records for the topic "vleet hol ly" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


Semiconductor Alternating-Current Motor Drives and Energy Conservation  

Science Journals Connector (OSTI)

...required to avoid high heating losses in the motors...important user concerns-price, efficiency, and...been offered at a price thatjustified broad...direct-ly, causes motor heating, mechanical stress...000 barrels of oil equivalent per day...University, New Haven, Connecticut, and is currently...

D. J. BenDaniel; E. E. David Jr.



Further Investigations on Induction of Mammary Cancer in Mice by Isografts of Hypophyseal Tissue  

Science Journals Connector (OSTI)

...in dependently to select the positive reactors "name ly: (a) The conversion of the...644586452472328Exp.QROUPVWX strates the reliability of the selection method employed. Mammary...described above are unsuitable for a complete analysis, since this investigation was primarily...

L. M. Boot; O. Mühlbock; G. Röpcke; and W. van Ebbenhorst Tengbergen



124 Los Alamos Science Number 23 1995 Number 23 1995 Los Alamos Science 125  

E-Print Network (OSTI)

, reactor-produced pluto- nium in gram quantities was first fashioned into the pure metallic form needed- ly absorbed and never leave the body. The most reliable detection scheme is to measure the small, was instru- mental in the design and analysis of some of those experiments (see "The Plutonium Injection

Massey, Thomas N.


Decomposition of Fresh and Anaerobically Digested Plant Biomass in Soil1 K. K. MOORHEAD, D. A, GRAETZ, AND K. R. REDDY2  

E-Print Network (OSTI)

information deals with land ap- plication of anaerobically digested sewage sludge, and on- ly limited data such as plant biomass, sewage sludge, or animal wastes is used to generate CH4 and stabilized organic waste, or preferably utilized, in an environmentally safe manner. Disposal of the anaerobically digested sludge by land

Florida, University of


"Ask Argonne" - Robert Jacob, Climate Scientist, Part 2  

ScienceCinema (OSTI)

Previously, climate scientist Robert Jacob talked a bit about the work he does and invited questions from the public during Part 1 of his "Ask Argonne" video set (http://bit.ly/1aK6WDv). In Part 2, he answers some of the questions that were submitted.

Jacob, Robert



Circadian Variation of Tumor Blood Flow in Rat Subcutaneous Tumors and Its Alteration by Angiotensin II-induced Hypertension  

Science Journals Connector (OSTI)

...LY80 cells (n = 11). Tumor growth was divided into two stages, the first stage (/) (K = 0.1762.V - 1.4938. r = 0.9975, P < 0.001 ) and the second stage (//) ( Y= 0.0526* + 0.1160, r = 0.9956, P < 0.001). Bari, SD. measured...

Katsuyoshi Hori; Maroh Suzuki; Shigeru Tanda; Sachiko Saito; Mika Shinozaki; Qiu-Hang Zhang



Interpretation of Shape-Related Iconic Gestures in Virtual Environments  

E-Print Network (OSTI)

Interpretation of Shape-Related Iconic Gestures in Virtual Environments Timo Sowa and Ipke focused main- ly on deictic and emblematic gestures. Iconics, viewed as iconic signs in the sense idea towards a computational model of gesture semantics for iconic gestures. Based on an empirical

Wachsmut, Ipke


Over the past five years, analysts and policymakers have become increasingly interested in the "full  

E-Print Network (OSTI)

- ly. From the 1920s to the 1960s, major decisions about building and financing highways were left in the late 1960s, however, "a growing awareness of the human and environmental costs of roads, dams costs, such as air pollution costs, as well as private or market costs, such as the cost of vehicles

Murphy, James J.


Communicating climate change risks in a skeptical world John D. Sterman  

E-Print Network (OSTI)

Communicating climate change risks in a skeptical world John D. Sterman Received: 31 March 2011 Regulations"; http://bit.ly/etpa11. 1 The challenge of risk communication on climate change on Climate Change (IPCC) has been extraor- dinarily successful in the task of knowledge synthesis and risk

Edwards, Paul N.


Instrumental Requirements for Global Atmospheric Chemistry  

Science Journals Connector (OSTI)

...lower stratosphere-upper troposphere research generally. The Boeing Condor (27), for example, can fly for a few days continuous-ly...available, however. The drone aircraft mentioned above, the Boeing Condor, is capable of a continuous unattended flight of a few...

D. L. Albritton; F. C. Fehsenfeld; A. F. Tuck



Khesbn no. 61-62 - Autumn - Winter 1970-1971 - Journal  

E-Print Network (OSTI)

619 ,10 ,1970 It:yPyr bu'r ''ly ugi]l ilJlD sTg .b''''. -.1iu)ts;lyn'iN yplyr:7yr og.l ugi 'r! r Dly)D Tm .lnlr t)uyr:

Admin, LAYCC



Khesbn no. 98 - Autumn 1981 - Journal  

E-Print Network (OSTI)

ltJ'r{D yutt ly t? l'1lt 'fyl Ugi "l\\lsDu DIN ulri11yt,','fDn6 D't ltN -'syEo I)t bxnyl Ugi tg ltlj)tDyl u)! $] p:Nv

Admin, LAYCC



IEEE Technology and Society Magazine, Spring 2003 47 Jerome E. Dobson and Peter F. Fisher  

E-Print Network (OSTI)

in which one entity, the master, coercively or surreptitious- ly monitors and exerts control over simultaneously. Enhanced surveil- lance and control may be attained through complementary monitor- ing of functional indicators such as body temperature, heart rate, and perspiration. It is possible to monitor

Wright, Dawn Jeannine


,r;p==;;;:;i;j Proceedings, Canadian Society for Civil Engineering  

E-Print Network (OSTI)

on this comparison, a simplified and refined expression for prediction of crack spacing is proposed. The second, there are certain types of structures such as tanks, silos, and nuclear reactor containment structures, where tensile cracks can pose serious problems. All such structures are general- ly reinforced in two directions


Max Weber and the future of religion: liberation or the Iron Cage  

E-Print Network (OSTI)

mited) is shaped by economica1ly orient- ed social action under some criter1on (past, present, or potent1al) of ultimate values (Wertende Postulate) regardless of the nature of these ends. " Substant1ve rationa1ity directly orders action into patterns...

Dowdy, Thomas E.



Veterans Employment Forum | Department of Energy  

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

Employment Forum November 5, 2014 7:30AM to 9:30AM PST Location: 614 SW 11th Avenue, Portland, OR 97205, 2nd Floor Library Room POC: Heather Bain Website: http:bit.ly1t6XjaO...


12 Towards an Analytical Livelihoods Perspective in  

E-Print Network (OSTI)

, the Sustainable Livelihoods Approach/Framework (SLA or SLF) had emerged as a promising and challenging re-life' problems and opportunities of rural people. Accordingly, the SLF was part- ly perceived as a new `theory the framework. The out- come was that the SLF indeed helped to focus research on core livelihood issues

Richner, Heinz


Managing Insect Resistance to Bacillus thuringiensis Toxins  

Science Journals Connector (OSTI)

...adapt. Combinations of B.t. with other mortality...applied and transgenic B.t. toxins (Table 2...environmental-ly, and sociologically acceptable pest sup-pression tools...1103 (1987); D. A. Fischhoff et al., Bio/Technology5...330, 160 (1987). 8. B. C. Carlton, in Biotechnology...

William H. McGaughey; Mark E. Whalon


API5 Confers Tumoral Immune Escape through FGF2-Dependent Cell Survival Pathway  

Science Journals Connector (OSTI)

...antiapoptotic gene, apoptosis inhibitor 5 (API5), in the immune-resistant...and Methods Chemical kinase inhibitors LY294002 (Calbiochem Corp...siApi5- or siGFP-loaded chitosan nanoparticles (CNP) starting...Exposure to the proteasome inhibitor, MG 132, restored Bim levels...

Kyung Hee Noh; Seok-Ho Kim; Jin Hee Kim; Kwon-Ho Song; Young-Ho Lee; Tae Heung Kang; Hee Dong Han; Anil K. Sood; Joanne Ng; Kwanghee Kim; Chung Hee Sonn; Vinay Kumar; Cassian Yee; Kyung-Mi Lee; and Tae Woo Kim



Nitrated Cyclic GMP Modulates Guard Cell Signaling in Arabidopsis  

Science Journals Connector (OSTI)

...ODQ, a guanylate cyclase inhibitor, which suggests that an NO...Arabidopsis. Two guanylate cyclase inhibitors, ODQ and LY83583, prevented...response to UV-B, ABA, chitosan, and extracellular calmodulin...Supplemental Figure 1. Effect of Inhibitors on Stomatal Aperture. Supplemental...

Takahiro Joudoi; Yudai Shichiri; Nobuto Kamizono; Takaaki Akaike; Tomohiro Sawa; Jun Yoshitake; Naotaka Yamada; Sumio Iwai


Note: This page contains sample records for the topic "vleet hol ly" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.



E-Print Network (OSTI)

(vol) PE, filter and apply suction until reasonably dry. Air dry and store in a jar. Filter paper and jars (Virtis Model 23 and 200-ml blender jars), rotating evaporator with 250-ml flask, film to seal without vacuum. Apply vacuum, rinse brief- ly, and press down along edge of mat to ensure a good seal


Note: PMS 2725C HNI30 June 2012  

E-Print Network (OSTI)

. Pack corn into freezer containers, leaving ½ inch headspace. Seal, label, date and freeze the container. Tightly wrap ears individual- ly in moisture vapor-proof film and pack in plastic freezer bags. Seal. Fill jar to 1 inch from top with boiling hot cooking liquid. Remove air bubbles.Wipe jar rims. Adjust


Nepal's peace process and challenges ahead  

E-Print Network (OSTI)

Nepal's peace process and challenges ahead Context and policy connections When the Communist Party of Nepal (Maoist) [CPN(M)] and the Seven Party Alliance government signed the CPA on 21 November 2006 and the United Nations worked collective- ly to achieve peace and stability. The United Nations Mission in Nepal

Richner, Heinz


Appalachian Program: A Mechanism for a National Growth Policy?  

Science Journals Connector (OSTI)

...resigned last week after 1 /2 years as president...Stanford presidency on 1 December 1968. * BLACK...College has received a $1-million grant from the...which is current-ly 500. Meharry is the only predomi-nantly...allowed to claim a total rebate by adopting severance taxes...

Luther J. Carter



Effects of Water Velocity and Trash Rack Architecture on Juvenile Fish Passage and Interactions: A Simulation  

E-Print Network (OSTI)

species have experienced population declines due to modification of estuarine ecosystems. Fish screens (or for many urban, agricultural, and industrial activities (FAO and DVWK 1996). Current- ly, the Sacramento and San Joaquin rivers to spawn, and juveniles of these species move down these rivers to the ocean, where

Anderson, Todd


Swift-UVOT captures the earliest ultraviolet spectrum of a Gamma Ray Burst  

E-Print Network (OSTI)

We present the earliest ever ultraviolet spectrum of a gamma-ray burst (GRB) as observed with the Swift-UVOT. The spectrum of GRB 081203A was observed for 50 seconds with the UV grism starting 251 seconds after the Swift-BAT trigger when the GRB was of u ~13.4 mag and still rising to its peak optical brightness. The UV grism spectrum shows a damped Ly-alpha line, Ly-beta, and the Lyman continuum break at a redshift z = 2.05 +/- 0.01. A model fit to the Lyman absorption implies log N(HI) = 22.0 +/- 0.2 cm-2, which is typical for GRB host galaxies with damped Ly-alpha absorbers. This observation of GRB 081203A demonstrates that for GRBs brighter than v ~14 mag and with 0.5 < z < 3.5 the UVOT will be able to provide redshifts, and probe for damped Ly-alpha absorbers within 4-6 minutes from the time of the Swift-BAT trigger.

Kuin, N P M; Page, M J; Schady, P; Still, M; Breeveld, A A; De Pasquale, M; Brown, P J; Carter, M; James, C; Curran, P A; Cucciara, A; Gronwall, C; Holland, S T; Hoversten, E; Hunsberger, S; Kennedy, T; Koch, S; Lamoureux, H; Marshall, F E; Oates, S R; Parsons, A; Palmer, D; Roming, P; Smith, P J



To cite this version : Nesterenko, Alla and Alric, Isabelle and Violleau, Frdric and Silvestre,  

E-Print Network (OSTI)

-acylation Microencapsulation Spray-drying Biopolymer based microparticles were efficiently prepared from sunflower protein (SP) wall material and -tocopherol (T) active core using a spray-drying technique. Protein enzymatic in viscosity, whereas acylation did not significant- ly affect emulsion droplet size and viscosity

Boyer, Edmond


Achieving Full View Coverage with Randomly-Deployed Heterogeneous Camera Sensors  

E-Print Network (OSTI)

: {iceworld0324, xwang8}@sjtu.edu.cn Abstract--A brand-new concept about the coverage problem of camera sensor to be captured. It is specially significant for camera networks since image shot at the frontal viewpoint to this topic. The image or video provided by camera sensors great- ly enriches the information retrieved from

Wang, Xinbing



E-Print Network (OSTI)

SURVEY OF THE COLUMBIA RIVER AND ITS TRIBUTARIES - Part VIII SPECIAL SCIENTIFIC REPORT: FISHERIES Falls By Zell E. Parkhurst Fishery Research Biologist Special Scientific Report Fisheries No. 57 #12 for a distance of approximate- ly 600 miles to the impassable Augur Falls opposite the town of Jerome, Idaho


Embryos, polyps and medusae of the Early Cambrian scyphozoan Olivooides  

Science Journals Connector (OSTI)

...and medusae of the Early Cambrian scyphozoan Olivooides Xi-Ping Dong 1 2 John A. Cunningham 3 Stefan Bengtson 4 Ceri-Wyn...373-376. 32 Li, P , H Hua, LY Zhang, DD Zhang, XB Jin, and Z Liu. 2007 Lower Cambrian phosphatized Punctatus...



Burgess Shale Faunas and the Cambrian Explosion  

Science Journals Connector (OSTI)

...Ediacaran faunas, in contrast, are substantially younger. A recent U-Pb determination on zircons from a tuff that smothered an Edia-caran community in southeast Newfoundland provides an apparent-ly acceptable date of 565 Ma (5), and most of the other...




The 19 August 1976 Denizli, Turkey, earthquake: Evaluation of the strong motion accelerograph record  

Science Journals Connector (OSTI)

...ottonis, ~o. Hi~9=.~o,~o ~ F'oLy~to~W'Jl~'mognesla . 'Smyr o "sq~%it.d,~ , phio *PhiLome Lion eDia "~ TroLLe&~ . ]'E~esos , ....'~apamem I Loaalcela Samos Kotossat MiLetos Kibyra I I I I 2 3 Fia. 3. Historical...

Ref'an Can Ates; Nejat Bayülke


Morphology and Anatomy of Texas Persimmon (Diospyros texana Scheele).  

E-Print Network (OSTI)

and the two types of h;ilictid bees (Table 1). However, a num- ber of otlier insects were present which probal~ly are important for pollination. Consequently, Texas per- simmon may 11e either partially 01- entirely insect pol- linated. Fruit The fi...

Meyer, R. E.



Development of procedures for preparation of data for operational evaluation of the low level meteorological model  

E-Print Network (OSTI)

the course of tne current j aves tigation, yields the solar declination angle within. 0. 5 dcg. A root-mean-squsre error of approximately 0. 25 deg was found 6) cosiparrng empi rical ly determined values of the solar:lac lination angle with those given...

Burnett, Paul Taylor




Office of Legacy Management (LM)

p l o s i o n near R i f l e , Colorado, on 10 September lyGg by R. M. Hamilton, B. E. Smith and J. H. Healy Own-File R e w r t 1970 This r e p r t i s prelircinary and has n o t...


A&G Volume 55 Issue 4, Full Issue  

Science Journals Connector (OSTI)

......bit.ly/ UMdDy9 PROFILE:HAYLEY FLOOD A&G7k]kij(&'*Leb$++ 4.9...eXWdXkho$eh] Q&AHayleyFlood Hayley Flood, Coopers Technology College, winner...experiment [EVE] data from http://lasp. colorado.edu accessed 11 May 2013, courtesy......

A&G Volume 55 Issue 4; Full Issue



Secondary condenser Cooling water  

E-Print Network (OSTI)

Receiver Secondary condenser LC LC Reboiler TC PC Cooling water PC FCPC Condenser LC XC Throttling valve ¨ mx my l© ª y s § y m «¬ ly my wx l n® ® x np © ¯ Condenser Column Compressor Receiver Super-heater Decanter Secondary condenser Reboiler Throttling valve Expansion valve Cooling water

Skogestad, Sigurd


JOURNAL DE PHYSIQUE Colloque C3,supplmentau n03,Tome 46,mars 1985 page C3-223  

E-Print Network (OSTI)

rheology at theDarcyscale is expressed by a formulation using the grand resistance matrix. The time suspension can be reconstructed by elementary translations) contains only one particle. In most cases quantities can then be related to the main kinematic quantities by a "grand resistance matrix" which on- ly

Paris-Sud XI, Université de


Robustness of shortfall risk minimising strategies in the binomial model  

E-Print Network (OSTI)

units of the stock Sn. We shall always suppose our investment strategies to be self-financing, namely function `. In order to keep things simple, we restrict ourselves to t* *he case in which the market the non-risky asset is supposed (by considering forward prices) identical* *ly equal to 1, and the stock

Vargiolu, Tiziano


The Louis Stokes Alliance for Minority Participation programs support the establishment of comprehensive Alliances to  

E-Print Network (OSTI)

The Louis Stokes Alliance for Minority Participation programs support the establishment of comprehensive Alliances to increase the quantity and quality of students who successful- ly earn STEM. David Aragon and Dr. Renee Beeton External Evaluator: Dr. Rose Shaw #12;Colorado Alliance for Minority

Note: This page contains sample records for the topic "vleet hol ly" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.



E-Print Network (OSTI)

in Fig. 1A, and in Figs. 1B­1F in typical in-use setups measuring light-duty vehicles (LDV), heavy-duty trucks, locomotives, snow- mobiles, and airplanes respectively. The IR/UV light source and speed bar. In this article we discuss its application to the measurement of individual vehicle emissions remote- ly

Denver, University of



SciTech Connect

We present the results of rest-frame, UV slitless spectroscopic observations of a sample of 32 z {approx} 0.7 Lyman break galaxy (LBG) analogs in the COSMOS field. The spectroscopic search was performed with the Solar Blind Channel on the Hubble Space Telescope. We report the detection of leaking Lyman continuum (LyC) radiation from an active galactic nucleus-starburst composite. While we find no direct detections of LyC emission in the remainder of our sample, we achieve individual lower limits (3{sigma}) of the observed non-ionizing UV-to-LyC flux density ratios, f{sub {nu}} (1500 A)/f{sub {nu}}(830 A) of 20 to 204 (median of 73.5) and 378.7 for the stack. Assuming an intrinsic Lyman break of 3.4 and an intergalactic medium transmission of LyC photons along the line of sight to the galaxy of 85%, we report an upper limit for the relative escape fraction in individual galaxies of 0.02-0.19 and a stacked 3{sigma} upper limit of 0.01. We find no indication of a relative escape fraction near unity as seen in some LBGs at z {approx} 3. Our UV spectra achieve the deepest limits to date at any redshift for the escape fraction in individual sources. The contrast between these z {approx} 0.7 low escape fraction LBG analogs with z {approx} 3 LBGs suggests that either the processes conducive to high f{sub esc} are not being selected for in the z {approx}< 1 samples or the average escape fraction is decreasing from z {approx} 3 to z {approx} 1. We discuss possible mechanisms that could affect the escape of LyC photons.

Bridge, Carrie R.; Siana, Brian; Salvato, Mara; Rudie, Gwen C. [California Institute of Technology, 220-6, Pasadena, CA 91125 (United States); Teplitz, Harry I. [Infrared Processing and Analysis Center, MS 100-22, Caltech, Pasadena, CA 91125 (United States); Scarlata, Claudia; Colbert, James; Armus, Lee [Science Center, California Institute of Technology, 220-6, Pasadena, CA 91125 (United States); Conselice, Christopher J. [University of Nottingham, Nottingham, NG7 2RD (United Kingdom); Ferguson, Henry C.; Brown, Thomas M.; Giavalisco, Mauro [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States); De Mello, Duilia F. [Department of Physics, Catholic University of America, 620 Michigan Avenue, Washington, DC 20064 (United States); Gardner, Jonathan P., E-mail: bridge@astro.caltech.ed [Astrophysics Science Division, Observational Cosmology Laboratory, Code 665, Goddard Space Flight Center, Greenbelt, MD 20771 (United States)



A Group of Galaxies at Redshift 2.38  

E-Print Network (OSTI)

We report the discovery of a group of galaxies at redshift 2.38. We imaged about 10% of a claimed supercluster of QSO absorption-lines at z=2.38 (Francis & Hewett 1993). In this small field (2 arcmin radius) we detect two Ly-alpha emitting galaxies. The discovery of two such galaxies in our tiny field supports Francis & Hewett's interpretation of the absorption-line supercluster as a high redshift "Great Wall". One of the Ly-alpha galaxies lies 22 arcsec from a background QSO, and may be associated with a multi-component Ly-alpha absorption complex seen in the QSO spectrum. This galaxy has an extended (50kpc) lumpy Ly-alpha morphology, surrounding a compact IR-bright nucleus. The nucleus shows a pronounced break in its optical-UV colors at about 4000 A (rest-frame), consistent with a stellar population of mass about 7E11 solar masses, an age of more than 500 Myr, and little on-going star-formation. C IV emission is detected, suggesting that a concealed AGN is present. Extended H-alpha emission is also detected; the ratio of Ly-alpha flux to H-alpha is abnormally low (about 0.7), probable evidence for extended dust. This galaxy is surrounded by a number of very red (B-K>5) objects, some of which have colors suggesting that they too are at z=2.38. We hypothesize that this galaxy, its neighbors and a surrounding lumpy gas cloud may be a giant elliptical galaxy in the act of bottom-up formation.

Paul Francis; Bruce Woodgate; Steve Warren; Palle Moller; Marg Mazzolini; Andy Bunker; James Lowenthal; Ted Williams; Takeo Minezaki; Yukiyasu Kobayashi; Yuzuru Yoshii




Office of Legacy Management (LM)

.55 LyEnfant Plaro. S.W., Washingzon, D.C. 20024.2174, Telephone: (202) 488-6000 .55 LyEnfant Plaro. S.W., Washingzon, D.C. 20024.2174, Telephone: (202) 488-6000 7117-03.87.cdy.27 27 May 1987 Mr. 'Andrew Wallo, III, NE:23 Division of Facility & Site Decommissioning Projects U.S. Department of Energy Germantown, Maryland: 20545 Dear Mr. Wallo: I STATUS OF ACTIONS - FUSRAP SITE LIST Aerospace recently completed .a comprehensive review of sites listed in the FUSRAP Site Investigation and Remedial Action Summary Report, dated Uecember 31, 1986. The primary objectives of this review were to examine the status of each site identified in Sections II and III of the Reportwith respect to actions required to complete the Identification and Characterization Process; to provide,DFSD a current-status of these actions; and to identify



NLE Websites -- All DOE Office Websites (Extended Search)

distribution is unlimited; September 2013. distribution is unlimited; September 2013. Other requests shall be referred to NAVFAC EXWC or ESTCP. TECHNICAL REPORT TR-NAVFAC-EXWC-PW-1303 SEPTEMBER 2013 BUILDING INTEGRATED PHOTOVOLTAIC (PV) ROOFS FOR SUSTAINABILITY AND ENERGY EFFICIENCY Peter Ly, NAVFAC EXWC George Ban-Weiss, LBNL Nathan Finch, NAVFAC EXWC Craig Wray, LBNL Mark de Ogburn, NAVFAC Atlantic Woody Delp, LBNL Hashem Akbari, LBNL Scott Smaby, NAVFAC EXWC Ronnen Levinson, LBNL Bret Gean, NAVFAC EXWC SEI Group, Inc. 1 BUILDING INTEGRATED PHOTOVOLTAIC (BIPV) ROOFS FOR SUSTAINABILITY AND ENERGY EFFICIENCY Energy and Water ESTCP Number: EW-200813 September 2013 Peter Ly, NAVFAC EXWC George Ban-Weiss, LBNL Nathan Finch, NAVFAC EXWC Craig Wray, LBNL Mark de Ogburn, NAVFAC Atlantic



NLE Websites -- All DOE Office Websites (Extended Search)

8 results: 8 results: BibTex RIS RTF XML Sort by: Author Title Type [ Year (Desc) ] Filters: Author is George Ban-Weiss [Clear All Filters] 2013 Ly, Peter, George Ban-Weiss, Nathan Finch, Craig Wray, Mark de Ogburn, William W. Delp, Hashem Akbari, Scott Smaby, Ronnen Levinson, and Bret Gean. Building integrated photovoltaic (BIPV) roofs for sustainability and energy efficiency. Naval Facilities Engineering Command - Engineering and Expeditionary Warfare Center, 2013. Ban-Weiss, George, Craig P. Wray, William W. Delp, Peter Ly, Hashem Akbari, and Ronnen M. Levinson. "Electricity production and cooling energy savings from installation of a building-integrated photovoltaic roof on an office building." Energy and Buildings 56 (2013): 210-220. 2011 Sleiman, Mohamad, George Ban-Weiss, Haley E. Gilbert, David François, Paul


Paints and Painting Materials and Miscellaneous Analyses.  

E-Print Network (OSTI)

, B ry an . To m B at te ,B ry an . E . E . B ro ug he r, o f H ug he s S p ri n gs . 1.90 9, 38 0 83 1 fi6 1 49 1 04 .84 3.81 Sodium Chloride...................... Magnesium Chloride ............... 2.29 2.17 4... to m . A re m ar k ab ly pu re w at er . *Cacl2. 0.75. tCaClg. 3.55. JCaClg. 48.50. 968 T E X A S A G R IC U L T U R A L E X P E R IM E N T ST A T IO N . Table o f A na ly se s . Address...

Harrington, H. H.; Tilson, P. S.



Absorption Systems in the Spectrum of GRB 021004  

E-Print Network (OSTI)

We report on a 3600 s spectrum of GRB 021004 obtained with the Nordic Optical Telecope on La Palma 10.71 hours after the burst. We identify absorption lines from five systems at redshifts 1.3806, 1.6039, 2.2983, 2.3230, and 2.3292. In addition we find an emission line which, if due to Ly-alpha from the host galaxy, gives a redshift of 2.3351. The nearest absorber is blueshifted by 530 km/s with respect to this line, consistent with shifts seen in Damped Ly-alpha and Lyman-Break galaxies at similar redshifts. The emission line flux is 2.46+-0.50 x 10^-16 erg/s/cm^2. Some of the absorption systems are "line-locked", an effect often seen in QSO absorption systems believed to originate close to the QSO central engine.

P. Møller; J. P. U. Fynbo; J. Hjorth; B. Thomsen; M. P. Egholm; M. I. Andersen; J. Gorosabel; S. T. Holland; P. Jakobsson; B. L. Jensen; H. Pedersen; K. Pedersen; M. Weidinger



Detecting filaments at z=3  

E-Print Network (OSTI)

We present the detection of a filament of Ly-alpha emitting galaxies in front of the quasar Q1205-30 at z=3.04 based on deep narrow band imaging and follow-up spectroscopy obtained at the ESO NTT and VLT. We argue that Ly-alpha selection of high redshift galaxies with relatively modest amounts of observing time allows the detection and redshift measurement of galaxies with sufficiently high space densities that we can start to map out the large scale structure at z=2-3 directly. Even more interesting is it that a 3D map of the filaments will provide a new cosmological test for the value of the cosmological constant, Omega_Lambda.

J. P. U. Fynbo; P. Moller; B. Thomsen



The optical afterglow and host galaxy of GRB 000926  

E-Print Network (OSTI)

In this paper we illustrate with the case of GRB 000926 how Gamma Ray Bursts (GRBs) can be used as cosmological lighthouses to identify and study star forming galaxies at high redshifts. The optical afterglow of the burst was located with optical imaging at the Nordic Optical Telescope 20.7 hours after the burst. Rapid follow-up spectroscopy allowed the determination of the redshift of the burst and a measurement of the host galaxy HI-column density in front of the burst. With late-time narrow band Ly-alpha as well as broad band imaging, we have studied the emission from the host galaxy and found that it is a strong Ly-alpha emitter in a state of active star formation.

J. P. U. Fynbo; J. Gorosabel; P. Moller; J. Hjorth; M. I. Andersen; M. P. Egholm; B. L. Jensen; H. Pedersen; B. Thomsen; M. Weidinger



Rings and convolution algebras  

E-Print Network (OSTI)

convolution al ebra if the follow1ng properties hold: i) For every xcS and feF the function f defined by f(y) = f(xy) is x x an element of F. ii) For every xcS and LcL the funct1on f defined by fL(x) = L( f) is x an element of F. For notat1onal reasons we... introduce a new var1able y into the above equation by defining f (x) = Ly(f(xy)). L 1ii) For every L, Met the linear functional M*L on F defined by M*L(f) = Mx(Ly(f(xy))) 1s an element of L. M*L is called the convolution of M and L. It is easy to ver1fy...

Zeller, Mike



The relationship of the long bones of the thoracic and pelvic limbs as indicators of muscling in the beef carcass  

E-Print Network (OSTI)

!. +hot th. * tibia and femur ax"! c iv:r d by nun rou. muscl . and~ th ref'. . r ~ their 3. enpth 1? xrtr =m?ly !!ard to o. tinct 'r! ups 3, l?5 nrxi 6 shiv the hi "host d!?r e of r lationc'dp b tv ien n"tacarpui ond metatarsus l neth and caress...!. +hot th. * tibia and femur ax"! c iv:r d by nun rou. muscl . and~ th ref'. . r ~ their 3. enpth 1? xrtr =m?ly !!ard to o. tinct 'r! ups 3, l?5 nrxi 6 shiv the hi "host d!?r e of r lationc'dp b tv ien n"tacarpui ond metatarsus l neth and caress...

Orts, Frank A



Excitation wavelength dependence of water-window line emissions from boron-nitride laser-produced plasmas  

SciTech Connect

We investigated the effects of laser excitation wavelength on water-window emission lines of laser-produced boron-nitride plasmas. Plasmas are produced by focusing 1064 nm and harmonically generated 532 and 266 nm radiation from a Nd:YAG laser on BN target in vacuum. Soft x-ray emission lines in the water-window region are recorded using a grazing-incidence spectrograph. Filtered photodiodes are used to obtain complementary data for water-window emission intensity and angular dependence. Spectral emission intensity changes in nitrogen Ly-{alpha} and He-{alpha} are used to show how laser wavelength affects emission. Our results show that the relative intensity of spectral lines is laser wavelength dependent, with the ratio of Ly-{alpha} to He-{alpha} emission intensity decreasing as laser wavelength is shortened. Filtered photodiode measurements of angular dependence showed that 266 and 532 nm laser wavelengths produce uniform emission.

Crank, M.; Harilal, S. S.; Hassan, S. M.; Hassanein, A. [Center for Materials Under Extreme Environment, School of Nuclear Engineering, Purdue University, West Lafayette, Indiana 47907 (United States)



Heavy Elements in the Lyman-$?$\\ Forest: Abundances and Clustering at z=3  

E-Print Network (OSTI)

For the purpose of studying the properties of heavy-elements associated with the Lyman-$\\alpha$\\ forest, we observed the gravitational lens Q1422+2309. We used the HIRES instrument on the W.M. Keck telescope to obtain a high-resolution, very high signal-to-noise spectrum of this z=3.63 quasar; the spectrum covers wavelengths from below Lyman-$\\beta$\\ up to the C IV emission line. Consistent with previous estimates, we find that a moderate fraction of the Ly-$\\alpha$\\ forest clouds have been enriched with heavy elements at a level significantly below solar abundance. However, unlike the fairly uniform distribution of Ly-$\\alpha$\\ forest lines, we show that the C IV absorption lines are clustered on large velocity scales.

D. S. Womble; W. L. W. Sargent; R. S. Lyons



The Grape.  

E-Print Network (OSTI)

wine grape which grows well here. wV F 8 B {Rip. x Lab.).? G row th very w eak , shoots sm ooth , purp lish s tr ip ed ; leaves deep ly 3 -lobed , ja gged m arg in ed ; bunches m ed ium size, ob long , m odera te ly com pac t ; berries m ed... ium size, b la ck , m u sk y sw eet f la v o r ; seeds la rg e ; fo liage green and v igorous N ovem ber 6, 1896, bu t the vines are show ing m uch sign o f w eakness now . wV 5 ] U B c 8 {Lab. x Vin.).? Growrth medium, shoots green...

Price, R. H.; Ness, H.



High l state population in O sup 7+ produced in ion-solid collisions  

SciTech Connect

The high {ell}-state population of fast ions excited in ion-solid interactions is very different from {ell}-state populations produced under single collision conditions. A study of the population dynamics of electronic excitation and transport within the framework of a classical transport theory for O{sup 2+} (2 MeV/u) ions traversing carbon foils shows food agreement with experimental results from delayed photon emission spectroscopy. We investigate the dependence of the characteristic exponent for the power-law decay of delayed Ly{alpha} and Ly{beta} radiation on the initial n,{ell} distribution. From our simulations we find evidence that the very high {ell}-state populations produced in ion-solid collision are the consequence of a high-{ell} state diffusion under the influence of multiple inelastic and elastic collisions in the bulk of the solid. 15 refs., 4 figs.

Kemmler, J. (Centre Interdisciplinaire de Recherches avec les Ions Lourds, 14 - Caen (France)); Bourgdoerfer, J.; Reinhold, C.O. (Tennessee Univ., Knoxville, TN (United States) Oak Ridge National Lab., TN (United States))



Mycorrhizal fungi in roots of Texas crops  

E-Print Network (OSTI)

~h, 1 f d ' d with peanuts grown at Stephenville, Texas. In watermelon material, five different kinds of mycorrhiza1 ~ p ly d, ' 1 d' S h* G~ p G~t 11 'd, G. ~l d G. ~h, d p ' f S~ltt, S. Slf 1 d S. ~tfd . 1'h ~dl ' p 1 *1 f d ' h ll p t ~dl... ~h, 1 f d ' d with peanuts grown at Stephenville, Texas. In watermelon material, five different kinds of mycorrhiza1 ~ p ly d, ' 1 d' S h* G~ p G~t 11 'd, G. ~l d G. ~h, d p ' f S~ltt, S. Slf 1 d S. ~tfd . 1'h ~dl ' p 1 *1 f d ' h ll p t ~dl...

Yeh, May-Wei Mavix



Theoretical model for plasma expansion generated by hypervelocity impact  

SciTech Connect

The hypervelocity impact experiments of spherical LY12 aluminum projectile diameter of 6.4?mm on LY12 aluminum target thickness of 23?mm have been conducted using a two-stage light gas gun. The impact velocity of the projectile is 5.2, 5.7, and 6.3?km/s, respectively. The experimental results show that the plasma phase transition appears under the current experiment conditions, and the plasma expansion consists of accumulation, equilibrium, and attenuation. The plasma characteristic parameters decrease as the plasma expands outward and are proportional with the third power of the impact velocity, i.e., (T{sub e}, n{sub e})???v{sub p}{sup 3}. Based on the experimental results, a theoretical model on the plasma expansion is developed and the theoretical results are consistent with the experimental data.

Ju, Yuanyuan; Zhang, Qingming, E-mail: qmzhang@bit.edu.cn; Zhang, Dongjiang; Long, Renrong; Chen, Li; Huang, Fenglei [State Key Laboratory of Explosion Science and Technology, Beijing Institute of Technology, Beijing 100081 (China); Gong, Zizheng [National Key Laboratory of Science and Technology on Reliability and Environment Engineering, Beijing Institute of Spacecraft Environment Engineering, Beijing 100094 (China)



The social theories of Bertrand Russell  

E-Print Network (OSTI)

fozcaerly can not be denied: when the woman goes out to industrxel erx lilss ner husband, the cnildren spend most o" their day at chool, tb cconosn sx betwe? husb~ wrf e r= e?ormou ly ceaJNnsde 2 Once mo. e, lf toe relation or t?e sexc 1e ever to ttern... fozcaerly can not be denied: when the woman goes out to industrxel erx lilss ner husband, the cnildren spend most o" their day at chool, tb cconosn sx betwe? husb~ wrf e r= e?ormou ly ceaJNnsde 2 Once mo. e, lf toe relation or t?e sexc 1e ever to ttern...

Dameron, Alton Bernard



Two dimensionally space-resolved electron temperature measurement of fusion plasma by x-ray monochromatic imaging method  

SciTech Connect

Electron temperature distributions of laser created fusion plasma were measured by using toroidally bent Bragg crystals. A tiny amount of argon was seeded in deuterium fuel gas and monochromatic images of Ar{sup +17} (1{ital s}{minus}3{ital p}) Ly{beta} and Ar{sup +16} (1{ital s}{sup 2}{minus}1{ital s}3{ital p}) He{beta} lines were taken to provide temperature distribution of the compressed core from their intensity ratios. A fusion core created by laser-generated x rays in a micro-cavity showed the temperature structure corresponding to the illumination asymmetry caused by the cavity irradiation geometry. The experimental distribution of the line-ratio of Ly{beta} to He{beta} was compared with the postprocessed outputs from one dimensional simulation, assuming perfect spherical implosion, to discuss degradation of pellet implosion. {copyright} {ital 1996 American Institute of Physics.}

Fujita, K.; Nishimura, H.; Uschmann, I.; Foerster, E.; Takabe, H.; Kato, Y.; Nakai, S. [Institute of Laser Engineering, Osaka University, 2-6 Yamadaoka, Suita, Osaka 565 (Japan)


Note: This page contains sample records for the topic "vleet hol ly" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


Energy Value vs. Energy Cost: A Fundamental Concept of Economics Applied to Cogeneration  

E-Print Network (OSTI)

known as MESA (Modular Energy System Analyzer).* CONCLUSIONS Economic cogeneration by any reasonable def ini tion is a desirable practice. The effective application of principles and concepts that lead to minimum expenditure of resources... been very accurately calculated by the use of MESA. The value of the shaft power has been estab lished by the alternative option of pur chased elec tr ical energy at a known incremental cost. These examples do not aPl?ly universally to all steam...

Viar, W. L.



High Gradient Acceleration in a 17 GHz Photocathode RF Gun* S. C. Chen, J. Gonichon, 1;. C-L. Lin, R. J. Temkin, S. Trotz, B. G. Danly, and J. S. Wurtele  

E-Print Network (OSTI)

High Gradient Acceleration in a 17 GHz Photocathode RF Gun* S. C. Chen, J. Gonichon, 1;. C-L. Lin.icle acceleration at high mi- ccowave (RF) frequencies are under study at hIIT. The 17 GHz photocathode RF gun has, efforts have been made recent,ly t,o creat,e novel electron beam sources.[l] While existing RF guns

Wurtele, Jonathan


Gene organization and structure of the Streptomyces lividans gal operon.  

Science Journals Connector (OSTI)

...Leu Arg Arg RE Asp Akg no 820 840 860 TXC aoc GM ox GM oXcoX AcC ooX 7cATMM GCO GOX TXG...xa AIX; AOC OGG AAG Mat SBr Gly Ly 1080 1100 TM OX ox...1420 1440 M OX GM OX GMG GM (TT coX AM aOc GM TOC oX m ACAMV O AMC MT [yr Gly Glu...

C W Adams; J A Fornwald; F J Schmidt; M Rosenberg; M E Brawner



www.activemotif.comwww.activemotif.com Protein Purification  

E-Print Network (OSTI)

Storage Resuspension Buffer 45 ml 175 ml Room Temp. Buffer A 33 ml 125 ml Room Temp. Elution Buffer 11 ml. Resuspension Buffer 50 mM Tris, pH 8.0, 300 mM NaCl, and 10 mM Imidazole, 0.2% Triton X-100 2. Lysozyme 100 mg concentration of 0.2% to the Resuspension Buffer. This will help the ly

Lebendiker, Mario


Measures of the sentence intonation of read and spontaneous speech in American English  

E-Print Network (OSTI)

or toplines that gradually fall throughout he course of a sentence describe linguistical- ly salient aspects of the Fo contour. These claims differ from those of earlier studies like those of Armstrong and Ward (1926}, Trager and Smith {1951... Fo peaks to phenomena such as linguistic stress (e.g., Pierre- humbert, 1979}. The breath-group theory, like earlier theor- ies (e.g., Armstrong and Ward, 1926; Jones, 1932; Trager and Smith, 1951}, instead claims that the terminals are used...

Lieberman, Phillip; Katz, William; Jongman, Allard; Zimmerman, Roger; Miller, Mark



Evaluation of massive hydraulic fracturing experiments in the Devonian Shales in Lincoln County, West Virginia  

E-Print Network (OSTI)

perfor- mance. The type curves that have been generated have qualitatively shown that the fractured wells are clear'ly more stimulated than the surrounding shot wells, Fracture treatment simulation indicates that treatments pumped in the MHF wells... Optimal Stimulation Design Per Zone Simulated Reservoir Properties Economic Production Forecasts 64 68 70 15 Economic Analysis Results Reservoir Case 72 LIST OF FIGURES FIGURES 10 12 13 15 16 17 MHF Well Location In Lincoln County, WV MHF...

Holgate, Karen Elaine



Spain's Earth Scientists and the Oil Spill  

E-Print Network (OSTI)

and a south to north slope current on the sea (1­11), the decision to move the vessel from about 43°N, 9.5°WSpain's Earth Scientists and the Oil Spill THE SPANISH COAST OF GALICIA IS CURRENT- ly subject to an oil spill that, given its spatial and temporal extent, could become one of the worst spills ever

Brown, James H.


A, Science Service Featura ? FIHY THE FEATHER ?  

E-Print Network (OSTI)

.ter. The cause is a hidden flash* A t h i r d form is llheat'l lightning, which i s the term applied t o are visible, a d is usu&ly explained as the reflection fron the hazsr air O f the lightning flashes of storns, American E%feteorolpgicalSociety, Describes: FOUR EIWDS OF LIGHTNING Lightning is popularly divided i n t o


Antigenic analysis of the genus Aeromonas  

E-Print Network (OSTI)

. The adsorbed serum was tested for homo- logous and hetrologous agglutinins using the above procedure. 18 CHAPTER IV RESULTS Biochemical Characteristics Selected biochemical tests were run on all of the type species of aeromonads in order to insure proper...: Antisera to particulate Antigens Cross adsorptions were performed with only those serological systems which showed reactions of sufficient titers. The data p ese ted in Table ly. Aliquots of A. ~1i uefacie s tise u we e adsorbed with the ella of A...

Rao, Vijaya Balusu



Indeterminism and predictability in economics  

E-Print Network (OSTI)

as an ideal foz ~ methodological purposes and erroneously concluded that they could eventually discover deterministic laws which would make possible prediction and control. The deterministic view which Newtonian ~ physics fostered has changed. Modern... and thc methodological problem of uncertainty were ~ ', ap?arer&tly made amenable to L'r e aiethods of science, As a cons qucnce, ' Lhe scient?fic comrs city came to b lieve that science could ultimat ly , ' . he c i r -''. ions rn Lhe fol] owing pages...

Barton, David Merritt



Thermodynamic and transport properties of self-assembled monolayers from molecular simulations  

E-Print Network (OSTI)

). ................................................................................................50 4.2 Pore size distribution of membranes as-received from manufacturer.120........ 52 4.3 Propane diffusivity as a function of the box lengths (Lx,Ly(? ))..................... 58 4.4 Propane/nitrogen selectivity as a function of propane...12 chains and diamonds represent membranes treated with C18 chains from Javaid et al.1............................................................................................66 4.6 Propane/nitrogen selectivity as a function of propane permeance...

Aydogmus, Turkan



Rangeland Drought Management for Texans: Toxic Range Plants  

E-Print Network (OSTI)

- ly alter grazing behavior. To minimize losses to toxic plants, producers should learn how to identify the toxic plants, use good graz- ing and livestock management practices, and take measures to control the plants when necessary. Know which plants... are toxic The first step in managing for toxic plants is being able to identify them. Ranchers must be able to: Identify plants that are toxic to livestock in their area Understand what makes them poisonous Recognize the symptoms produced when live...

Hart, Charles R.; Carpenter, Bruce B.



Khesbn no. 28 - Jaunary 1962 - Journal  

E-Print Network (OSTI)

ruu ytt1tr o$.r upynntgD ugi D$t,l ,jbrllt ll! EyrJ .i'tl'tNN) ''! y1 ]y:'N t'ly;ryr I'r ugi "yoog: .lyxyl Nli2D 'r'N .u ,? i.ir. 'l: ylyt:ttry; Ugi ('\\r3L. 7u! 'l,ti J'r biJ; rT

Admin, LAYCC



1. Off to East London! Will be tweeting again on Tuesday Oct 26th from Johannesburg.8:06 AM Oct 19th via web  

E-Print Network (OSTI)

th via web 2. Taking the new Gautrain to airport, very excited. I wish it ran later though. Late flight tomorrow night.7:59 AM Oct 19th via web 3. Orientation is our programme to introduce new foreign docs to SA ­ we manage the details! (http://bit.ly/8Z6BHJ)7:52 AM Oct 19th via web 4. Reviewing new

Plotkin, Joshua B.


Ecatepec Cogeneration Project, Mexico City. Final report. Export trade information  

SciTech Connect

;Table of Contents: Introduction; Task 1 - System Selection and Interconnection; Task 2 - Economic and Financial Analysis; Task 3 - Environmental Issues, Permits, and Compliance; Task 4 - Preliminary Engineering Scope Book; Task 5 - Criteria for and Selection of EPC Contractor; Task 6 - Implement Financing Plan/Prepare Offering Memorandum; Appendices (Invoice History; Capital Cost Estimates; SEMIP Application; Application Supplement List; Development Agreement; CFE/LyFC Pricing Methodology; EPC Bid Specifications and Drawings; Environmental Information for Permits).




Cotton Production under Traditional and Regulated Deficit Irrigation Schemes in Southwest Texas  

E-Print Network (OSTI)

It total irrigation amount of the TDI treatment Kc crop coefficient LEPA low energy precision application LY lint yield MANOVA multivariate analysis of variance vii P precipitation Pe effective precipitation PF profit pL lint... price pW water price rd deficit ratio dr average deficit ratio RDI regulated deficit irrigation ri irrigation efficiency TC total cost TDI traditional deficit irrigation Tr transpiration rate USDA United States Department...

Wen, Yujin



Individual based modeling of animal populations using object oriented simulation techniques: investigating the effects of bonding, predation and birth cover on white-tailed deer  

E-Print Network (OSTI)


German, Carl Duane



Environments of deposition and diagenesis of the Jurassic Upper Smackover Formation in the Lincoln Parish area, Louisiana  

E-Print Network (OSTI)

study area filled with fine to silty, well sortec, fining uvwards lithare. . ites, graded alterna . ins -rainstone-sandstone beds +s, voo ly sorted, skeletal-oncolite wackestones and vacks*ones, and calcareous silt:-. ones and shales. The sraded beds.... The Smackover interval is oolitic, pisolitic, intraclastic and oncolitic packstones to grainstones, with interbedded calcareous siltstones, litharenites and shales. The overlying Buckner is calcareous siltstones and shales interbedded with skeletal...

Palko, Gregory Jonathan



Are high-redshift DLA galxies Lyman-break galaxies?  

E-Print Network (OSTI)

We use deep HST STIS and NICMOS images of three spectroscopically confirmed galaxy counterparts of high-redshift damped Ly-alpha (DLA) absorbers (one of which is a new discovery) to test the hypothesis that high-redshift DLA galaxies are Lyman-break galaxies. If this hypothesis is correct the emission properties of DLA galaxies must lie within the range of emission properties measured for Lyman-break galaxies of similar absolute magnitude. This will be true regardless of selection biases in the sample of detected DLA galaxies. We test this prediction using several emission properties: half-light radius, radial profile (Sersic n parameter), optical-to-near-infrared colour, morphology, Ly alpha emission equivalent width, and Ly alpha emission velocity structure. In all cases the measured values for the DLA galaxies lie within the range measured for the population of Lyman-break galaxies. None of the measurements is in conflict with the prediction. We conclude that the measured emission properties of the three DLA galaxies studied here are consistent with the conjecture that high-redshift DLA galaxies are Lyman-break galaxies. We show that this result does not conflict with the observation that the few high-redshift DLA galaxies discovered are mostly fainter than spectroscopically confirmed L* Lyman-break galaxies.

P. Møller; S. J. Warren; S. M. Fall; J. U. Fynbo; P. Jakobsen



Intergalactic Medium Emission Observations with the Cosmic Web Imager. I. The Circum-QSO Medium of QSO 1549+19, and Evidence for a Filamentary Gas Inflow  

Science Journals Connector (OSTI)

The Palomar Cosmic Web Imager (PCWI), an integral field spectrograph designed to detect and map low surface brightness emission, has obtained imaging spectroscopic maps of Ly? from the circum-QSO medium (CQM) of QSO HS1549+19 at redshift z = 2.843. Extensive extended emission is detected from the CQM, consistent with fluorescent and pumped Ly? produced by the ionizing and Ly? continuum of the QSO. Many features present in PCWI spectral images match those detected in narrow-band images. Filamentary structures with narrow line profiles are detected in several cases as long as 250-400 kpc. One of these is centered at a velocity redshifted with respect to the systemic velocity, and displays a spatially collimated and kinematically cold line profile increasing in velocity width approaching the QSO. This suggests that the filament gas is infalling onto the QSO, perhaps in a cold accretion flow. Because of the strong ionizing flux, the neutral column density is low, typically , and the line center optical depth is also low (typically ?0 M gas = 12.5 ± 0.5) and the total (log M tot = 13.3 ± 0.5). We can also calculate a kinematic mass from the total line profile (2 ? 1013 M ?), which agrees with the mass estimated from the gas emission. The intensity-binned spectrum of the CQM shows a progression in kinematic properties consistent with heirarchical structure formation.

D. Christopher Martin; Daphne Chang; Matt Matuszewski; Patrick Morrissey; Shahin Rahman; Anna Moore; Charles C. Steidel


Note: This page contains sample records for the topic "vleet hol ly" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


Spectrally Resolved Intensities of Ultra-Dense Hot Aluminum Plasmas  

SciTech Connect

We present a first study of spectroscopic determination of electron temperature and density spatial profiles of aluminum K-shell line emission spectra from laser-shocked aluminum experiments performed at LULI. The radiation emitted by the aluminum plasma was dispersed with an ultra-high resolution spectrograph ({lambda}/{delta}{lambda}{approx_equal}6000). From the recorded films one can extract a set of time-integrated emission lineouts associated with the corresponding spatial region of the plasma. The observed spectra include the Ly{alpha}, He{beta}, He{gamma}, Ly{beta} and Ly{gamma} line emissions and their associated He- and Li-like satellites thus covering a photon energy range from 1700 eV to 2400 eV approximately. The data analysis rely on the ABAKO/RAPCAL computational package, which has been recently developed at the University of Las Palmas de Gran Canaria and takes into account non-equilibrium collisional-radiative atomic kinetics, Stark broadened line shapes and radiation transport calculations.

Gil, J. M.; Rodriguez, R.; Florido, R.; Rubiano, J. G.; Martel, P. [Departamento de Fisica, Universidad de Las Palmas de Gran Canaria, 35017 Las Palmas de Gran Canaria (Spain); Instituto de Fusion Nuclear, Universidad Politecnica de Madrid, 28006 Madrid (Spain); Minguez, E. [Instituto de Fusion Nuclear, Universidad Politecnica de Madrid, 28006 Madrid (Spain); Sauvan, P. [Departamento de Ingenieria Energetica, UNED, Madrid (Spain); Instituto de Fusion Nuclear, Universidad Politecnica de Madrid, 28006 Madrid (Spain); Angelo, P.; Dalimier, E. [Physique Atomique dans les Plasmas Denses, LULI, CNRS-CEA-Ecole Polytechnique-Universite Paris VI, 75252 Paris cedex 05 (France); Schott, R.; Mancini, R. [Department of Physics, University of Nevada, Reno, NV 89557 (United States)



Analysis of time-resolved argon line spectra from OMEGA direct-drive implosions  

SciTech Connect

We discuss the observation and data analysis of argon K-shell line spectra from argon-doped deuterium-filled OMEGA direct-drive implosion cores based on data recorded with two streaked crystal spectrometers. The targets were 870 {mu}m in diameter, 27 {mu}m wall thickness plastic shells filled with 20 atm of deuterium gas, and a tracer amount of argon for diagnostic purposes. The argon K-shell line spectrum is primarily emitted at the collapse of the implosion and its analysis provides a spectroscopic diagnostic of the core implosion conditions. The observed spectra includes the He{alpha}, Ly{alpha}, He{beta}, He{gamma}, Ly{beta}, and Ly{gamma} line emissions and their associated He- and Li-like satellites thus covering a broad photon energy range from 3100 to 4200 eV with a spectral resolution power of approximately 500. The data analysis relies on detailed atomic and spectral models that take into account nonequilibrium collisional-radiative atomic kinetics, Stark-broadened line shapes, and radiation transport calculations.

Florido, R.; Nagayama, T.; Mancini, R. C. [Department of Physics, University of Nevada, Reno, Nevada 89557 (United States); Tommasini, R. [Lawrence Livermore National Laboratory, Livermore, California 94550 (United States); Delettrez, J. A.; Regan, S. P.; Smalyuk, V. A. [Laboratory for Laser Energetics, University of Rochester, New York 14623 (United States); Rodriguez, R.; Gil, J. M. [Departamento de Fisica, Universidad de Las Palmas de Gran Canaria, 35017 Las Palmas de Gran Canaria (Spain)




SciTech Connect

We have obtained deep Hubble Space Telescope far-UV images of 15 starburst galaxies at z {approx} 1.3 in the GOODS fields to search for escaping Lyman continuum (LyC) photons. These are the deepest far-UV images (m{sub AB} = 28.7, 3{sigma}, 1'' diameter) over this large an area (4.83 arcmin{sup 2}) and provide some of the best escape fraction constraints for any galaxies at any redshift. We do not detect any individual galaxies, with 3{sigma} limits to the LyC ({approx}700 A) flux 50-149 times fainter (in f{sub {nu}}) than the rest-frame UV (1500 A) continuum fluxes. Correcting for the mean intergalactic medium (IGM) attenuation (factor {approx}2), as well as an intrinsic stellar Lyman break (factor {approx}3), these limits translate to relative escape fraction limits of f{sub esc,rel} < [0.03, 0.21]. The stacked limit is f{sub esc,rel}(3{sigma}) < 0.02. We use a Monte Carlo simulation to properly account for the expected distribution of line-of-sight IGM opacities. When including constraints from previous surveys at z {approx} 1.3 we find that, at the 95% confidence level, no more than 8% of star-forming galaxies at z {approx} 1.3 can have relative escape fractions greater than 0.50. Alternatively, if the majority of galaxies have low, but non-zero, escaping LyC, the escape fraction cannot be more than 0.04. In light of some evidence for strong LyC emission from UV-faint regions of Lyman break galaxies (LBGs) at z {approx} 3, we also stack sub-regions of our galaxies with different surface brightnesses and detect no significant LyC flux at the f{sub esc,rel} < 0.03 level. Both the stacked limits and the limits from the Monte Carlo simulation suggest that the average ionizing emissivity (relative to non-ionizing UV emissivity) at z {approx} 1.3 is significantly lower than has been observed in LBGs at z {approx} 3. If the ionizing emissivity of star-forming galaxies is in fact increasing with redshift, it would help to explain the high photoionization rates seen in the IGM at z>4 and reionization of the IGM at z>6.

Siana, Brian; Bridge, Carrie R. [California Institute of Technology, MS 249-17, Pasadena, CA 91125 (United States); Teplitz, Harry I.; Chary, Ranga-Ram; Colbert, James W.; Scarlata, Claudia [Spitzer Science Center, California Institute of Technology, 220-6, Pasadena, CA 91125 (United States); Ferguson, Henry C.; Brown, Thomas M. [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States); Giavalisco, Mauro [Department of Astronomy, University of Massachusetts, Amherst, MA 01003 (United States); Dickinson, Mark [National Optical Astronomy Observatory, 950 N. Cherry Avenue, Tucson, AZ 85719 (United States); De Mello, Duilia F. [Department of Physics, Catholic University of America, 620 Michigan Avenue, Washington, DC 20064 (United States); Conselice, Christopher J. [University of Nottingham, Nottingham, NG7 2RD (United Kingdom); Gardner, Jonathan P. [Astrophysics Science Division, Observational Cosmology Laboratory, Code 665, Goddard Space Flight Center, Greenbelt, MD 20771 (United States)




SciTech Connect

The spectral and temporal behavior of exoplanet host stars is a critical input to models of the chemistry and evolution of planetary atmospheres. Ultraviolet photons influence the atmospheric temperature profiles and production of potential biomarkers on Earth-like planets around these stars. At present, little observational or theoretical basis exists for understanding the ultraviolet spectra of M dwarfs, despite their critical importance to predicting and interpreting the spectra of potentially habitable planets as they are obtained in the coming decades. Using observations from the Hubble Space Telescope, we present a study of the UV radiation fields around nearby M dwarf planet hosts that covers both far-UV (FUV) and near-UV (NUV) wavelengths. The combined FUV+NUV spectra are publicly available in machine-readable format. We find that all six exoplanet host stars in our sample (GJ 581, GJ 876, GJ 436, GJ 832, GJ 667C, and GJ 1214) exhibit some level of chromospheric and transition region UV emission. No 'UV-quiet' M dwarfs are observed. The bright stellar Ly{alpha} emission lines are reconstructed, and we find that the Ly{alpha} line fluxes comprise {approx}37%-75% of the total 1150-3100 A flux from most M dwarfs; {approx}>10{sup 3} times the solar value. We develop an empirical scaling relation between Ly{alpha} and Mg II emission, to be used when interstellar H I attenuation precludes the direct observation of Ly{alpha}. The intrinsic unreddened flux ratio is F(Ly{alpha})/F(Mg II) = 10 {+-} 3. The F(FUV)/F(NUV) flux ratio, a driver for abiotic production of the suggested biomarkers O{sub 2} and O{sub 3}, is shown to be {approx}0.5-3 for all M dwarfs in our sample, >10{sup 3} times the solar ratio. For the four stars with moderate signal-to-noise Cosmic Origins Spectrograph time-resolved spectra, we find UV emission line variability with amplitudes of 50%-500% on 10{sup 2}-10{sup 3} s timescales. This effect should be taken into account in future UV transiting planet studies, including searches for O{sub 3} on Earth-like planets. Finally, we observe relatively bright H{sub 2} fluorescent emission from four of the M dwarf exoplanetary systems (GJ 581, GJ 876, GJ 436, and GJ 832). Additional modeling work is needed to differentiate between a stellar photospheric or possible exoplanetary origin for the hot (T(H{sub 2}) Almost-Equal-To 2000-4000 K) molecular gas observed in these objects.

France, Kevin; Froning, Cynthia S.; Stocke, John T.; Bushinsky, Rachel [Center for Astrophysics and Space Astronomy, University of Colorado, 389 UCB, Boulder, CO 80309 (United States)] [Center for Astrophysics and Space Astronomy, University of Colorado, 389 UCB, Boulder, CO 80309 (United States); Linsky, Jeffrey L. [JILA, University of Colorado and NIST, 440 UCB, Boulder, CO 80309 (United States)] [JILA, University of Colorado and NIST, 440 UCB, Boulder, CO 80309 (United States); Roberge, Aki [Exoplanets and Stellar Astrophysics Laboratory, NASA Goddard Space Flight Center, Greenbelt, MD 20771 (United States)] [Exoplanets and Stellar Astrophysics Laboratory, NASA Goddard Space Flight Center, Greenbelt, MD 20771 (United States); Tian, Feng [Center for Earth System Sciences, Tsinghua University, Beijing 100084 (China)] [Center for Earth System Sciences, Tsinghua University, Beijing 100084 (China); Desert, Jean-Michel [Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125 (United States)] [Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125 (United States); Mauas, Pablo; Vieytes, Mariela [Instituto de Astronomsica del Espacio (CONICET-UBA), C.C. 67 Sucursal 28, 1428 Buenos Aires (Argentina)] [Instituto de Astronomsica del Espacio (CONICET-UBA), C.C. 67 Sucursal 28, 1428 Buenos Aires (Argentina); Walkowicz, Lucianne M., E-mail: kevin.france@colorado.edu [Department of Astrophysical Sciences, Princeton University, Princeton, NJ 08544 (United States)



The Relationship Between Baryons and Dark Matter in Extended Galaxy Halos  

E-Print Network (OSTI)

The relationship between gas-rich galaxies and Ly-alpha absorbers is addressed in this paper in the context of the baryonic content of galaxy halos. Deep Arecibo HI observations are presented of two gas-rich spiral galaxies within 125 kpc projected distance of a Ly-alpha absorber at a similar velocity. The galaxies investigated are close to edge-on and the absorbers lie almost along their major axes, allowing for a comparison of the Ly-alpha absorber velocities with galactic rotation. This comparison is used to examine whether the absorbers are diffuse gas rotating with the galaxies' halos, outflow material from the galaxies, or intergalactic gas in the low redshift cosmic web. The results indicate that if the gas resides in the galaxies' halos it is not rotating with the system and possibly counter-rotating. In addition, simple geometry indicates the gas was not ejected from the galaxies and there are no gas-rich satellites detected down to 3.6 - 7.5 x 10^6 Msun, or remnants of satellites to 5-6 x 10^{18} cm^{-2}. The gas could potentially be infalling from large radii, but the velocities and distances are rather high compared to the high velocity clouds around the Milky Way. The most likely explanation is the galaxies and absorbers are not directly associated, despite the vicinity of the spiral galaxies to the absorbers (58-77 kpc from the HI edge). The spiral galaxies reside in a filament of intergalactic gas, and the gas detected by the absorber has not yet come into equilibrium with the galaxy. These results also indicate that the massive, extended dark matter halos of spiral galaxies do not commonly have an associated diffuse baryonic component at large radii.

M. E. Putman; J. L. Rosenberg; J. T. Stocke; R. McEntaffer



Camptothecin inhibits platelet-derived growth factor-BB-induced proliferation of rat aortic vascular smooth muscle cells through inhibition of PI3K/Akt signaling pathway  

SciTech Connect

The abnormal proliferation of vascular smooth muscle cells (VSMCs) in arterial wall is a major cause of vascular disorders such as atherosclerosis and restenosis after angioplasty. In this study, we investigated not only the inhibitory effects of camptothecin (CPT) on PDGF-BB-induced VSMC proliferation, but also its molecular mechanism of this inhibition. CPT significantly inhibited proliferation with IC50 value of 0.58 ?M and the DNA synthesis of PDGF-BB-stimulated VSMCs in a dose-dependent manner (0.5–2 ?M ) without any cytotoxicity. CPT induced the cell cycle arrest at G0/G1 phase. Also, CPT decreased the expressions of G0/G1-specific regulatory proteins including cyclin-dependent kinase (CDK)2, cyclin D1 and PCNA in PDGF-BB-stimulated VSMCs. Pre-incubation of VSMCs with CPT significantly inhibited PDGF-BB-induced Akt activation, whereas CPT did not affect PDGF-receptor beta phosphorylation, extracellular signal-regulated kinase (ERK) 1/2 phosphorylation and phospholipase C (PLC)-?1 phosphorylation in PDGF-BB signaling pathway. Our data showed that CPT pre-treatment inhibited VSMC proliferation, and that the inhibitory effect of CPT was enhanced by LY294002, a PI3K inhibitor, on PDGF-BB-induced VSMC proliferation. In addition, inhibiting the PI3K/Akt pathway by LY294002 significantly enhanced the suppression of PCNA expression and Akt activation by CPT. These results suggest that the anti-proliferative activity of CPT is mediated in part by downregulating the PI3K/Akt signaling pathway. - Highlights: ? CPT inhibits proliferation of PDGF-BB-induced VSMC without cytotoxicity. ? CPT arrests the cell cycle in G0/G1 phase by downregulation of cyclin D1 and CDK2. ? CPT significantly attenuates Akt phosphorylation in PDGF-BB signaling pathway. ? LY294002 enhanced the inhibitory effect of CPT on VSMC proliferation. ? Thus, CPT is mediated by downregulating the PI3K/Akt signaling pathway.

Park, Eun-Seok [Department of Applied Biochemistry, Division of Life Science, College of Health and Biomedical Science, Konkuk University, Chungju, Chungbuk (Korea, Republic of); Kang, Shin-il [College of Pharmacy Medical Research Center, Chungbuk National University, Cheongju (Korea, Republic of); Yoo, Kyu-dong [Hazardous Substances Analysis Division, Gwangju Regional Food and Drug Administration, Gwangju (Korea, Republic of); Lee, Mi-Yea [Department of Nursing Kyungbok University, Pocheon (Korea, Republic of); Yoo, Hwan-Soo; Hong, Jin-Tae [College of Pharmacy Medical Research Center, Chungbuk National University, Cheongju (Korea, Republic of); Shin, Hwa-Sup [Department of Applied Biochemistry, Division of Life Science, College of Health and Biomedical Science, Konkuk University, Chungju, Chungbuk (Korea, Republic of); Kim, Bokyung [Department of Physiology, Konkuk Medical School, Konkuk University, Chungju, Chungbuk (Korea, Republic of); Yun, Yeo-Pyo, E-mail: ypyun@chungbuk.ac.kr [College of Pharmacy Medical Research Center, Chungbuk National University, Cheongju (Korea, Republic of)



Metal enriched gaseous halos around distant radio galaxies: Clues to feedback in galaxy formation  

SciTech Connect

We present the results of an optical and near-IR spectroscopic study of giant nebular emission line halos associated with three z > 3 radio galaxies, 4C 41.17, 4C 60.07 and B2 0902+34. Previous deep narrow band Ly{alpha} imaging had revealed complex morphologies with sizes up to 100 kpc, possibly connected to outflows and AGN feedback from the central regions. The outer regions of these halos show quiet kinematics with typical velocity dispersions of a few hundred km s{sup -1}, and velocity shears that can mostly be interpreted as being due to rotation. The inner regions show shocked cocoons of gas closely associated with the radio lobes. These display disturbed kinematics and have expansion velocities and/or velocity dispersions >1000 km s{sup -1}. The core region is chemically evolved, and we also find spectroscopic evidence for the ejection of enriched material in 4C 41.17 up to a distance of {approx} 60 kpc along the radio-axis. The dynamical structures traced in the Ly{alpha} line are, in most cases, closely echoed in the Carbon and Oxygen lines. This shows that the Ly{alpha} line is produced in a highly clumped medium of small filling factor, and can therefore be used as a tracer of the dynamics of HzRGs. We conclude that these HzRGs are undergoing a final jet-induced phase of star formation with ejection of most of their interstellar medium before becoming 'red and dead' Elliptical galaxies.

Reuland, M; van Breugel, W; de Vries, W; Dopita, A; Dey, A; Miley, G; Rottgering, H; Venemans, B; Stanford, S A; Lacy, M; Spinrad, H; Dawson, S; Stern, D; Bunker, A



Dark energy and curvature from a future baryonic acoustic oscillation survey using the Lyman-? forest  

Science Journals Connector (OSTI)

We explore the requirements for a Lyman-? forest survey designed to measure the angular diameter distance and Hubble parameter at 2?z?4 using the standard ruler provided by baryonic acoustic oscillations (BAO). The goal would be to obtain a high enough density of sources to probe the three-dimensional density field on the scale of the BAO feature. A percent-level measurement in this redshift range can almost double the Dark Energy Task Force figure of merit, relative to the case with only a similar precision measurement at z?1, if the Universe is not assumed to be flat. This improvement is greater than the one obtained by doubling the size of the z?1 survey, with Planck and a weak Sloan Digital Sky Survey-like z=0.3 BAO measurement assumed in each case. Galaxy BAO surveys at z?1 may be able to make an effective Ly? forest measurement simultaneously at minimal added cost, because the required number density of quasars is relatively small. We discuss the constraining power as a function of area, magnitude limit (density of quasars), resolution, and signal-to-noise of the spectra. For example, a survey covering 2000 sq. deg. and achieving S/N=1.8 per Å at g=23 (?40??quasars per sq. deg.) with an R?250 spectrograph is sufficient to measure both the radial and transverse oscillation scales to 1.4% from the Ly? forest (or better, if fainter magnitudes and possibly Lyman-break galaxies can be used). At fixed integration time and in the sky-noise-dominated limit, a wider, noisier survey is generally more efficient; the only fundamental upper limit on noise being the need to identify a quasar and find a redshift. Because the Ly? forest is much closer to linear and generally better understood than galaxies, systematic errors are even less likely to be a problem.

Patrick McDonald and Daniel J. Eisenstein



Lyman Alpha Emitting Galaxies at 2 < z < 3: Towards a Calibrated Probe of Dark Energy  

SciTech Connect

The goal of this project was to establish the physical properties of Ly{alpha}#11;emitting galaxies from redshifts of 2 to 3 in order to better calibrate the use of LAEs as probes of the large scale structure of the universe for upcoming dark energy experiments, such as the Hobby Eberly Telescope Dark Energy Experiment (HETDEX). We have obtained narrow-band imaging of the Extended Chandra Deep Field South (ECDF-S) in two different narrow-band #12;filters centered at Ly{alpha}#11; at z=2.1 and 3.1. The resulting of samples of LAEs were used to determine the LAE luminosity function, equivalent width distribution and clustering properties (bias) of LAEs at these redshifts. While the results from the ECDF-S appear robust, they are based on a single field. To explore the effects of cosmic variance and galaxy environment on the physical properties of LAEs, we have also obtained narrow-band data at both redshifts (z = 2:1 and 3:1) in three additional #12;fields (SDSS 1030+-05, the Extended Hubble Deep Field South, and CW 1255+01). The narrow-band imaging data has been reduced and LAE catalogs are being generated. We have calculated preliminary luminosity functions, equivalent width distributions, and clustering properties. We have also obtained follow-up spectroscopy in the optical (using VLT/FORS) and in the near-infrared (using Magellan/MMIRS). Since individual LAEs have too little S/N to enable meaningful fits for stellar population parameters, our previous work has analyzed stacked Spectral Energy Distributions (SEDs). SED #12;fitting was performed on several subsets of LAEs selected by their rest-UV luminosity, UV spectral slope, Ly alpha luminosity, Equivalent Width, or rest-optical (IRAC) luminosity.

Caryl Gronwall



Argonne Lea Computing F A  

NLE Websites -- All DOE Office Websites (Extended Search)

Lea Lea Computing F A r g o n n e L e a d e r s h i p C o m p u t i n g FA c i l i t y 2 0 1 3 S c i e n c e H i g H l i g H t S Argonne leadership computing Facility C O N T E N T S About ALCF ...............................................................................................................................2 MirA...............................................................................................................................................3 SCienCe DireCtor'S MeSSAge ..........................................................................................4 ALLoCAtion ProgrAMS .......................................................................................................5 eArLy SCienCe ProgrAM ....................................................................................................



Office of Legacy Management (LM)

,:?' _. ,:?' _. .,. (p. z-3 ;: = 381 I!.0 MEMQRANDUM TO: FILE DATE +a& 7 -- -_ --------____ FROM: SUBJECT: SITE NAME: C ALTERNATE --------------'------------------------ OdYS NAME: -------------____-____ CITY: GOIS, STATE: -------- ----------------- c= OWNER(S) ------__ Past: c 36C~ Current: c, dfS --------- ----------- -------------------------- 'Owner contacted yes IJ no; if yes, date contacted_lySj 0 7 t(-zN/tr/y) TYPE OF OPERATION -----------______ 0 Research & Development 0 Production scale tasting 0 Pilot Scale 0 Bench Scale Process 0 Theoretical Studies 0 Sample SI Analysis cl Facility Type / /g n,-?;?=;;;i"g 0 Research Organization 0 Government Spons.ored Faci 1 i ty 0 Other ~~~~~~--__~~~--_----- fi Production c] DizsposalfStorage


O Ti-tE LOVE  

Office of Legacy Management (LM)

' ItqQtJulRl' IICt' O Ti-tE LOVE ~t?Al. . . At2D Al.CLkTED IChTTEtt~ . ' . . . : . ' . i I . . . . .mr TttE HOt\' ORAULE~ STANLEY FItZl:; SFCAKER ' . : ,J WE\J i' ORti STATE ASSH' rtrLY l r . . isay 29,.1980 Consultant to the Kew York ' , .' .I, " ..' . ,"' ! -. . . : . . . I.. . . . . ~. ,:- 9.. :. .' , * Ill . ,.. , ,i / All . ' %: : . : . . -. ;:. * :... . _ -. .' . . . I . ' J n' f armed. ?%c firtdingo and backup documentatiin embodied in thi preliminafy report compel the Task Yorao to call trprm ym; thr: . . I SpcnXer, to cwthorim crnd ompowcr the Assemly Sta?ding,CozmiCte I ' . : ,. . ..: .I' .,' :. .~.. ,:. :,-"'. ; ..d ::. . . .~~ ' .,' .' . : ' , ' ..,, -. . -. . . : : ? :. . . . .; *. . 1 ,.' .i. . . : \. .- :. " ' . . . c. : . I ! .'


Distributively generated near rings on the dihedral group of order eight  

E-Print Network (OSTI)

DISTRIBHvlri "LY GEZERKTED NEZR RINGS ON THE DIH ', DRAL GRODP OP ORDER EIGHT A Thesis INRy LING VILLHITE Submitted to the Gra~', . ate ' allege of Tezas jan& Rnid e'r, si!, y in Parti "1 fulfillment of the reGui rom nt fo- the eSree o MASTER... GP BC. E. ":lOE December le~70 Major Subject: llathematics DISTRIBUTIVELY GMWRA ED NEAR RINGE ON THE DIHED tAL GROUP OF ORDER EIGHT A Thesis NARY LYNN VILLHITE Approved as to st'yle and. content 'by: ax man. of Gom; i ee , member A &. ~;g...

Willhite, Mary Lynn



Particle dispersion within zonal jets in two-layer beta-plane turbulence  

E-Print Network (OSTI)

. were a, passive tracer. In eitlier case, liigh p. v. air from inside the polar vortex ivas ejected into lower latitudes, and thc vort&ix was eroded. Polvani and Plumb (1992) further classifie ivave-breaking using the Contour Dynamics method on a... decreases), a, parameter ivas needed that. allowed for relative comparisons of timescales in the two simulations. Thus, an Eulerian timescale was developed by examining thc cd&ly kinetic energies of the two cases. The eddy kinetic energy of a flow...

Roman, Jennifer Claire



Tal Shaya Issue 3  

E-Print Network (OSTI)

's current absence. . j -fpB W^ r r 21 "They enjoy the insultsi it keeps them on their toes." Chantal was glad that English idioms were becoming understand able to hen she pictured the two men spending time looking like ballet dancers. "And you...?but it was a close thing. Propped up on two dark pillows, chatting pleasant ly with several members of the crew gathered around the bed, she seemed every inch a queen. Except, perhaps, for the several inches surrounding her damaged left knee, the reason she...

Multiple Contributors



Engineering properties of shallow sediments in West Delta and South Pass Outer Continental Shelf Lease Areas, offshore Louisiana  

E-Print Network (OSTI)

, and sandy silt (WD024 1 WD028 ly WD029 1 WD029 2& WD029 3 1 1 These designations identify borehole locations. WD refers to West Delta OCS Lease Area, and SP refers to South Pass OCS Lease Area. The next three digits identify the number of the lease block... altering the linearity of the curve (Fig. 10). Since the curve was not deflected during consolidation as water content approached the plastic limit, the plastic limit does not appear to influence the minimum water content. It was noted that water content...

Helwick, Sterling J



The Salt Industry at Sterling, Kansas  

E-Print Network (OSTI)

. Exhaust stean of the engine plant is ad- mitted to the first evaporator and warms the "brine, then passes to the second and warns it lesD and condenses, causing a partial vacuum in the first where the brine then boils violent- ly. The vapor thus... and is condensed by a jet condenser, whereupon the third boils. Each evaporator has its own electric prop- eller stirrers and its own electric elevator to remove the salt. Nearly all the handling is done by electric conveyors until the salt is discharged...

Horner, Robert Messenger



Chemically Consistent Evolution of Galaxies on Cosmological Timescales and the DLA Galaxy Population  

E-Print Network (OSTI)

We describe the evolution of galaxies in a chemically consistent way accounting for the increasing initial metallicity of successive generations of stars. The enrichment of various types of model galaxies is compared with Damped Ly$\\alpha$ (= DLA) abundances over the redshift range from ${\\rm z \\sim 0}$ through ${\\rm z > 4.4}$. We discuss properties and composition of the galaxy population giving rise to DLA absorption. Beyond evolution of individual galaxies a change is found in the composition of DLA galaxy samples from high to low redshift. Spectrophotometric properties are predicted for optical identifications of DLA galaxies.

U. Fritze-v. Alvensleben; U. Lindner; C. S. Möller



Laboratory evaluation of selected fabrics for reinforcement of asphaltic concrete overlays  

E-Print Network (OSTI)

specimens to cyclic tensile loads. This testing was performed on the TTI Overlay Tester, a hydraul1cal ly powered apparatus des1gned to dupl1cate the thermally 1nduced contraction and expansion of roadway pavements. The testing scheme included plac1ng... the laboratory sample construction phase of th1s research. Thanks are also due to Mr. C. E. Fredericksen for his ass1stance 1n the electronic instrumen- tation and operation of the TTI Overlay Tester. Messrs. J. T. Labelle and P. B1lke are extended sincere...

Pickett, David L



Numerical Relaxation Approach for Solving the General Ginzburg-Landau Equations for Type-Ii Superconductors  

E-Print Network (OSTI)

PHYSICAL REVIEW B VOLUME 44, NUMBER 21 1 DECEMBER 1991-I Numerical relaxation approach for solving the general Ginzburg-Landau equations for type-II superconductors Z. D. Wang Texas Center for Superconductivity, Uniuersity ofHouston, Houston... in Fig. (1). This equation gives 11 920 Z. D. WANG AND C.-R. HU L [A (L,y, ) ?A (Oy;)]By; ?f [A (x,y, +, ) ?A?(x,y, )]dx=g(y, )6y, , where L?=?N~dx, I~ =N~dy, 6y,. =y, +,?y;, 4o =?hc/2e is the Aux quantum, and H (x,y) = V XA is the local mag- netic...

WANG, ZD; Hu, Chia-Ren.


Note: This page contains sample records for the topic "vleet hol ly" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


Electron-Transport Properties of Amorphous (Zr0.64ni0.36)1-Xalx Alloys  

E-Print Network (OSTI)

-4242 (Received 28 November 1988; revised manuscript received 16 March 1989) Measurements of the electrical resistivity p(T), thermopower S(T), and Hall coe%cient RH for a series of rapidly quenched Zr-Ni-Al alloys are reported for concentrations from x =0 to 0...-metal or ?metalloid amorphous alloys, the sign of RH can change from positive to negative as the concentration of the early transition metal is decreased. This is particular- ly well illustrated by measurements on amorphous Zr- based alloys, Zr-Cu, ' ' Zr-Ni, ' Zr...

BHATNAGAR, AK; PAN, R.; Naugle, Donald G.



Medical Professionalism in Society  

Science Journals Connector (OSTI)

...-dollar industry and those who seek greater government regulation. Physicians, feeling trapped between these camps, are turning to unionization and other tactics. In the first half of this century, medical professionalism was generally understood according to the structural–functional approach of Talcott... Today, at the dawn of a new century, genuine medical professionalism is in peril. Increasing-ly, physicians encounter perverse financial incentives, fierce market competition, and the erosion of patients' trust,1–7 yet most physicians are ill equipped to ...

Wynia M.K.Latham S.R.Kao A.C.Berg J.W.Emanuel L.L.



Response of Penaeus vannamei to dietary protein level, protein source and polyculture  

E-Print Network (OSTI)

). Within each feed series (2: I A; I: I = B), three formulated protein levels (22, 29 and 36% ) were mainta 1ned pr 1mar 1 ly by adjusting the percentages of rice bran and of the purified proteins (wheat gluten, alpha soy and vitamin-free casein... meal Fish solubles Rice bran Corn starch Alpha soy Wheat gluten Casein (vitamin-free) Alpha cellulose 2. 00 2. 00 2. 00 1. 50 1. 50 1. 50 2. 00 2. 00 2. 00 2. 00 2. 00 2. 00 22. 75 35. 00 36. 00 35. 00 35. 50 34. 50 12. 25 14, 40 25. 00 7. 20...

Smith, Linda Louise



Use of historic metabolic biotransformation data as a means of anticipating metabolic sites using MetaPrint2D and Bioclipse  

E-Print Network (OSTI)

in the second and third layers are labelled light and dark grey, respective- ly. Carlsson et al. BMC Bioinformatics 2010, 11:362 http://www.biomedcentral.com/1471-2105/11/362 Page 3 of 7 //For each fingerprint byte numberOfNonZeroEntries // All exist- ing atoms... advantage of new e-Science technologies, such as on-line (Web) services, high-performance computing, and networked databases. Equipped with an advanced provisioning system, it is very easy to publish updates for Bioclipse. This not only simplifies...

Carlsson, Lars; Spjuth, Ola; Adams, Sam; Glen, Robert C; Boyer, Scott



Aerodynamic effects in ink-jet printing on a moving web  

E-Print Network (OSTI)

Hsiao, W.-K., Hoath, S.D., Martin, G.D. and Hutchings, I.M., paper for NIP28 2012, 'Aerodynamic effects in ink-jet printing on a moving web' (accepted) Aerodynamic Effects in Ink-Jet Printing on a Moving Web Wen-Kai Hsiao, Stephen D Hoath... airflow and the wakes from the printed ink drops should be investigated as the primary source of aerodynamically-related print quality issues. Introduction The scope of commercial ink-jet printing has extended significant- ly in recent years. For new...

Hsiao, W.-K.; Hoath, S.D.; Martin, G.D.; Hutchings, I.M.



Expenses as a component of inventory cost  

E-Print Network (OSTI)

in de- termining inventoz'y cost such as fI rst-in, first-out, last- in, first-~ut, average, but does not give sufficient consi- derat1on to the pzoblem of what elemez ts of expense are propez ly included in the determination of 1nventory cost... in pz'oportion to the changes in operating levels ~ Semi- variable expenses are mez sly combinations of f1xed and vari- able elements in one expense classification, To emphasise the distinction between fixed and variable expense, it is appz...

Lott, Eugene H



The small firm enters international trade  

E-Print Network (OSTI)

the application of marketing procedures. This ', 'hos&s deals primarily with the factors which arc . iaq&ortant in t} e exporting of a product. It should be realized that most of these factors are also re. ievan* to ihc exporting of a service. The focus may...? ized, cormmmications have improved, and the population has become highly mobil=. Virtually all of the people are available as potential consumers, their buying character- istics have much in common, and they can be reached readi. ly by advertising...

Steelquist, Laura McDowell



Permian Foraminifera from Tunisia  

E-Print Network (OSTI)

in certain zones; Veibeekina, Neoschwagerina, and Sumatrina are present but rare. INTRODUCTION Several years ago Dr. CARL O. DUNBAR sent us a small piece of limestone from Djebel es Sotfinia, Tunisia, containing topotypes of Dun barula thieui C1RY. Still... club-shaped; large septal pores present, particular- ly along basal margins of septa, which number about 8 in 1st whorl, 8 in 2nd, 7 to 10 in 3rd, and 10 in 4th. Proloculus small, with outside diameter 101 to 140 p.. Tunnel low and not very wide, tunnel...

Skinner, J. W.; Wilde, G. L.



Kraith Collected Issue 3  

E-Print Network (OSTI)

the companionway. / / / '/ -.~.:-;~~-~ -+-~-=-,-=- ; -':: ~~ twt ? .p'i .t_., ~ :~'- ~.' .-:~- ... 6 The OBLIGATION/ ThROUGh TIme AN"b 'fSARS Jacqueline Lichtenberg & J. M. Winston K ra i t hili (1) The ruddy skyglow, overture to a Vulcan sunrise... the highest gallery access portal on the north side of the crystal. That was an honor he hadn't expected and he found strange ly that it awed him. For the first time, it hit him just what he'd donein Guardian Council. He let the feeling grow, nursing...

Lichtenberg, Jacqueline; Multiple Contributors



Relationship of land-use patterns to quail habitat  

E-Print Network (OSTI)

were ground cherry (Physals sp. ), yellow wood sorrel (Oxalis dillenii), p lyp ' l~y) p p b ), 'ldb (~gh 1 ~1' ), d d d (~Gh 11' p. ) (1 bl 5). G d h y d y 11 d sorrel represented approximately 62X of the composition. No grass species were... 170. 1 28. 9 23. 1 22. 6 55. 3 Yaupon Indian Cherry Misc. 527 36 35 155. 6 22, 2 22. 2 Total 898 300. 0 598 200. 0 29 blackjack oak, eastern redcedar, and yaupon. Post oak was the most important species, with an importance value...

Grevstad, Gerald Oscar



Karyotypic variation in the Peromyscus boylii species group in western Mexico  

E-Print Network (OSTI)

de Caballo 49(1), 51(7) 52(14)% 53(11), 54(1) Oaxaca 4. Llano de las Flores 48(1), 50(3) 51(8), ** 52P(2), 54(1) P. b. ~1 5. Cerro San Felipe 6. Juquila 7. Suchixtepec Chihuahua 8. Santa Barbara Aguascalientes 9. Rincon de Romos 48(1) 50... of their geographic ranges in western Chihuahua and their karyotypic similarity suggest the possibility that they may represent a single species. Nevertheless, the karyotypic data suggest that P. il ' o 1o ly 11' d to P. p 1' th to other species in the P. ~bo lii...

Davis, Kathleen Marie



A comparison of thick film and thin film traffic stripes  

E-Print Network (OSTI)

paxemnt, is the asyhalt "bail~ or Isurfa~ssedcc stripe, This stripe is produced ly laying a binder layer of asphalt oec?nt and ooxering it vith a lager of cncifnrnXp graded aggregatei The strips, when eanstrueted vitb linestone aggregate, bas a rather... oonduoted researoh on ~te Pine CoId Asphalt" for sarhing pedestrian orossings. The binder used in their oonpound was a resinous residue obtained fron a prooess for the parifioatioa of lubrioating oD. It is nore transluoent than tbe albino bitussns...

Keese, Charles J



Studies on the lichen genus Xanthoparmelia (Vainio) Hale in Texas  

E-Print Network (OSTI)

. Pedernales Falls State Park. 6. 2 km east of Johnson City. Limestone, scrub oak woods. 28 October 1977. This area along the Pedernales River is a unique habitat. The south bank supports a rich lichen flora and the north bank is virtually bare of lichens... tai . W t 619766 1 pd t d X. ~t on wood in the Chisos Mountains. The limestones along the Rio Grande Mi dit ay t tatty PP td ~Xth li 9 6 t ad~pl 1 ?d ly ccai lly. M thpa li were found at the Pandale low water crossing of the Pecos River in Val...

Derstine, Kittie Sue



Utilization of artificial nesting cavities by wood ducks (Aix sponsa) in central Texas  

E-Print Network (OSTI)

lie study area, Brazos River study area. Measured densities were 89 trees per ha, 953 trees per ha, and 595 trees per ha, respectively , 28 INTRODUCTION The wood duck (Aix ~sonsa) is the only member of the subfamily Anatinae in North America... of the range. Prior studies on wood ducks have been carried out chief- ly east of the Nississippi River, several hundred miles east of central Texas. STUDY AREAS This study entailed observations of breeding wood ducks on three areas in central Texas (Fig...

Labuda, Stephen Edward



The magnesium nutrition of American upland and Egyptian cottons  

E-Print Network (OSTI)

. Magnesium n1trate, sulfate, and chloxide ax'e highly soluble in water and are read1ly leached from the soil ~ Albert and Armstrong (l) grew cotton plants in nutrient solutions containing two levels of magnesium and found that greater top and root gx... on maturity of cotton X the rate of growth was not afflicted by magnesium supply but symptoms of magnesium deficien)y were present in the foliage of the low magnesium plants ~ Schappelle, Armstrong and Hollis (52) studied the effect of high magnesium...

Helmy, Hussein



Roost dynamics and site fidelity of snow geese wintering in southeast Texas  

E-Print Network (OSTI)

on the Texas coast. 10 HIRRIS SASTROP 8AYOU 0 BASTROP BAY REFUGE BOUNDARY CHRISTMAS BAY SALT LAKE Q a p~ ga Fig. 2. Brazoria National Wildlife Refuge. S4+ 8p 4~O yyy py y Qlly eyo goo%. flOyD DOffo olVEyf eyo ~ly & yff Cpfy4~ Cyy Cyyp... Institute and State Oniversity Chair of Advisory Committee: Dr. R. Douglas Slack Roost dynamics and site fidelity of lesser snow geese (Chen caerulescens caerulescens) wintering in southeast Texas were investigated at Brazoria and San Bernard National...

Jennings, Ann Fortenberry



Cold fusion research  

Science Journals Connector (OSTI)

Cold fusion research ... Eugene Mallove (C&EN, Feb. 10, page 2) accuses Trevor Pinch and me of "arrogant misunderstanding of cold fusion research/' Casting his net further, he then accuses the scientific establishment and some science media of "arrogant dismissal" of a "new phenomenon of unparalleled signficance," because we regard it as "a priori impossible." ... The latter, at least, is untrue, as should be apparent to anyone who read even the first three pages of 'Too Hot to Handle," where I wrote, 'liven though intuitive[ ly we felt] that [cold fusion] was too far-fetched to be real, nonetheless it had to be checked." ...




The adsorption and desorption of picloram, trifluralin, and paraquat by ionic and nonionic exchange resins  

E-Print Network (OSTI)

!'i?i mi ried by r 1 nsing the ! reat- i ii res lies is i J. . h var Locis . -; 0 lvent s . Where l 1'ice cheer os exi. sted bct . veen Lhe r csin encl herbicide, small amounts of herbicide were adsorbed and where unlike charges were involved..., relatively l. arge amounts &&ere adsorbed. Also, where no cou- lo& rb ic 6 oz!. . er; z!!ere presenL on tin& part of 1 izc-. 1 e sizz 01 her bi& i de, rein&. i v ly 1 arge a!nount s were ads!? bc d. '1'he aniozzic resin (Cl -for&a) adsorbed 375, 0. 08...

McCall, Homer Gene



The Efficiency of Some Industrial Combinations in the United States  

E-Print Network (OSTI)

the total large producing areas to five, these last, while enormous­ ly productive ,give a very heavy,poor quality of oil. Very little of the product is refined,and consequently these fields may be ignored in a study of monopoly of finished product, (c...-Fail Pool. D. The Trust. 1. Origin. a. Standard Oil Trust. 8. Legal Defects. E. The Holding Company. 1. Origin. a. The New Jersey Law. 2. E, C. Knight Case. r , P. The Combination Movement of 1898a 1. Beginnings. a. Recovery from Panic "b. Large...

Hoyt, Homer



Differential of discounted present values of civilian versus military lifetime earnings  

E-Print Network (OSTI)

, the monthly strength figures varied significantly, thus no one month could be chosen as representative of the 1971 force strength. Sources; Department of Defense Annus. l Report For Fiscal Year 1968, Secretary of' Defense Department Repor*, Fiscal Year 1973.... 23 Department of Defense Annual Report for Fiscal Year 1968, Assuming the individual is in th: Army now, and in Vietnam, the probability of death du" to ground combat is 0. 02/9; in *he 44avy the chance of such a. hostile death is o?ly 0. 0129...

Phillips, Christian


Note: This page contains sample records for the topic "vleet hol ly" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


Failure of the Shockley-Haynes Mobility Experiment with organic semiconducting materials  

E-Print Network (OSTI)

of the teflon cylinder was 0. 20$ cm + 0. 00$ cm whioh was slight- ly smaller than the graphite rods used, This arrapgement provided an airtight seal to prevent the sublimation of iodine from the samples after pressing Small holes were drilled through...-iodine was lower than that reported, The upper limit of 3000 lb/i. n for the pressure used to 2 oompress the samples was dictated by the graphite rods used and the wall thickness of the teflon oylinders. Pressures above $000 lb/in oaused either the ends...

Boehme, Hollis Clyde



Chemical Abundances in High-Redshift Neutral Clouds  

E-Print Network (OSTI)

Neutral hydrogen clouds with high column density detected towards distant quasars are unique probes of elemental nucleosynthesis and chemical evolution in the low metallicity regime. They provide measurements for several elements at very early times which are unfeasible in other astrophysical environments. Comparison between refractory and non-refractory elements provides evidence for the presence of dust, and the recently measured Ar probes photoionization. A prominent characteristic is the dominance of a solar abundance pattern, which is somewhat unexpected at low metallicities. It is argued that this property and Nitrogen observations can be used to constrain the age of the Damped Ly_alpha systems and the epoch of star formation.

Paolo Molaro



Variations in the shape of the outer rise seaward of the central Aleutian trench: implications for the rheology of oceanic lithosphere  

E-Print Network (OSTI)

ss (4) the most successfu' model . o explain the varia. 'ors in the amplitude of zhe outs rise ' =- pa ? = ly elas, ic p a. e model wi h varyin?bending mcmen';. I'he pr dieted. va ue- of the dips o the subcucting plate r ted . cc nding momen.... of each mechanism Apparent lexural ri-id' ty as a function ci age of . . "e surface lead with data taken ro, a var ' e y cf' areas . The apparent ' lexural rig' dity is the f'lexural rigidity of th= elas . ic plate that mos . closely agrees...

Huang, Hong-Hsi



Morphological parameters of the barnacle, Balanus tintinnabulum antillensis, as indicators of physiological and environmental conditions  

E-Print Network (OSTI)

of microbial organisms which can cause corrosion within the system and necessitate the use of biocides. The biocide current. ly in use is acrolein which is a highly volatile, toxic and r'cacti ve substance (Middleditch and West 1979). Bioassay mortalities... of adult barnacles have been reported from a concentration of 0. 5 ppm acrolein (Walko and Smitl 1969). Butler (1965) reported a toxicity value for acrolein of 0. 055 opm EC * (96 h) for oysters (C'rnsa~s~e. vizniniua). 50 Pcrolein incorporated within...

Boland, Gregory Scott



Public Speaking 4-H Style  

E-Print Network (OSTI)

light- ly during the meal. Microphone Tips A microphone can be your best aid or your worst enemy. A mike does not guarantee quality. Do not use a mike unless it is necessary. When you boost your voice naturally, you also increase your energy level. Vocal... ?pumping? to project to the back row or to the most distant corner is what makes a speaker feel stronger and more in charge. If you choose to use a mike, adjust it to your height. The audience will wait; they have come to hear you. After you have adjusted...

Hall, Gayle



Use and productivity of resources in the corn producing area of Argentina  

E-Print Network (OSTI)

, soxeti. . . s called "topsoil. ". The B horizon referees to There is a nitroger an. 3 phosphorus shortage, ho!. e:er, calciun and pot-ssiu. . . :re sufficient x'or . rop require. -. ;eats. The 8 hor'zon starts bet!seen 30 and +g ce!xtizet rs; under th... considerable loss. Uplands, the . '. ost i. !portan. . " . om the agricultural !so" nt of v lee i. :do's's ax' because of 3. ex~ cover 80 per ce t of t3". e area. Low e good for grazlx!g especiai. ly ir su, . ?er th ir great hueidity , y 1'7 7. A g' roup...

Andruchowicz, Eugenio Waldemar



Performance Testing of Radiant Barriers (RB) with R11, R19, and R30 Cellulose and Rock Wool Insulation  

E-Print Network (OSTI)

lnvestlgated prevlously by ORNL, FSEC, and TVA. In each case, It was found that RBs, especially the RBR. do cause hlgher roof temperatures but that the Increase Is not large. In the worst case, ORNL found increases in roof temperatures of 10°F wlth the RBR... Attics Contalnlng Radlant Barrlers." Oak Ridge Natl onal Laboratory. Sponsored by the Department of Energy and TVA. ORNL/CON-200, July 1986. 5. Levins, W. P. and Karnitz, M. A.. "Heating Energy Measurement of Unoccupled Single-Faml ly Houses Wlth...

Hall, J. A.



Stress analysis by photoelasticity  

E-Print Network (OSTI)

temperature At 80'C Glyptal testa Phenol- formaldehyde Polystyrene Polystyrene Polystyrene Cdiulose nttrate Plate glass Acrylic resin Allyl dtglycol Geist tne 13 per cent aqueous solut ton Bakehte B1'-61 ? 893 Catahn-800 Marcon Fosterite... of the spherical wave surface, pro- vided it is at a considers'ole distance from the light source, is essentislLy plane ano. we tt'us nave a plane wave. line along which lignt energy flows from the source to some point on the wave front is a ray. I, ight...

Kothari, Mahesh A



Effects of pavement markings on vehicle paths in a dual left turn  

E-Print Network (OSTI)

of Highway and Public Transportation's Official Highway Travel Map (5). The intersection of Post Oak Boulevard and San Felipe is not included on the map; therefore, the approximate location has been circ 1 ed. Figures 5 and 5 ar e schematics... in Figure 7, on a copy of a map of Bryan/Col 1ege Station from the State Department of Highways and Public Transportation's Official Highway Travel Map (5). One of the three intersections was eliminated from analysis because it was a ful ly channelized T...

Simmons, Kathryn Fitzpatrick



New procedures for the estimation and analysis of animal-feed production functions  

E-Print Network (OSTI)

Agronomo Dnirersidad ;lacional de Buenos Aires Bepublica Argentina Directed by: Dr. 'i'~illiam G. Brown The o iginal objective of this tnesis was to con- duct a. feeding trial and analyze the results statistical- ly . nd economically using tradi... of my researcn pro- ject; Drs. Cli ~e B. Harston, Bollo ED ~ hrich~ and John T, Steele who provided valuable suggestions and aid in completing the thesis. Special thanks are due to Dr. ~~'illiam G, Brown, my thesis director in Argentina, whose...

Baldomero Pizarro, Jose



The Value of Different Phosphates for Various Texas Soils and Grasses, as Indicated by Pot Experiments.  

E-Print Network (OSTI)

. TEXAS 1 8 BULLETIN NO. 672, LTRAL EXPERIMENT STATION Several other p'nospha~ea at: UL IL~~LY ~ecome obtainable for use as ferti- lizers. Calcium metaphosphate is made by burning phosphorus and passing the conlbustion products into rock phosphate... at high temperature. De- fluorinated rock phosphate is made by fusing rock phosphate with silica and quenching the melt. In both of these processes, much of the fluorine in the rock phosphate is removed. Phosphoric acid in these two phosphates may have...

Fraps, G. S. (George Stronach); Fudge, J. F. (Joseph Franklin)



Tactics for managing the sorghum webworm in sorghum  

E-Print Network (OSTI)

. 53 30 24 22 20 E 0 18 16 E 0 tO V 0 L e Cl E X C Z 14 12 1 8 6 4 1 2 3 4 5 6 7 8 9 PBBICle t lghtAGSS il't llew] 54 Figure 11: Comparison of sorghum webworm larvae infesting sorghum with varying panicle characteristics... (May 1978) Johnny Ray Hobbs, B. S. , Texas A&M University Chairman of Advisory Committee: Dr . George L. Teetes Damaging populotion levels of the sorghum webworm, C 1 ~bi' ll R'1 y, 'd d by ly pl 1 g of sorghum. Sorghum planted by April 1...

Hobbs, Johnny Ray



Correlation of gravity anomalies and geology in the San Antonio region, Texas  

E-Print Network (OSTI)

? Bl;!nco, encl Gil- lc. spic cour?tie . It is bouncled b? latitudes 29 00 ' encl 30o 07 ' 30" ir], and long. ' tiides 98c' 22 ' 30" V and 98o '5 ' iri. C] ties w] thin i l?c. ai-ea are Sar. Ant, nio, Bocrrnc r Blat?co, anrlr dohnson Ci Ly (Irido...!le interior zoine of the Ouach J t a f ola bc J t biy liatkins (1962, p. 39) . l'recsnibrian and Paleozoic rocks of Lhi- lldllci up- lift hav been described by nu!nerous authors (Paige, 1912; Pliim~n. r, 1943; Sellarcls, Adkins, and Plumm. r. , 1932...

Gordon, Patrick Thomas



Lyman-alpha Forest Tomography of the z>2 Cosmic Web  

E-Print Network (OSTI)

The hydrogen Ly$\\alpha$ forest is an important probe of the $z>2$ Universe that is otherwise challenging to observe with galaxy redshift surveys, but this technique has traditionally been limited to 1D studies in front of bright quasars. However, by pushing to faint magnitudes ($g>23$) with 8-10m large telescopes it becomes possible to exploit the high area density of high-redshift star-forming galaxies to create 3D tomographic maps of large-scale structure in the foreground. I describe the first pilot observations using this technique, as well discuss future surveys and the resulting science possibilities for galaxy evolution and cosmology.

Lee, Khee-Gan



Aspects of the ecology and systematics of the lizards Coleonyx brevis and Coleonyx reticulatus (Lacertilia: Gekkonidae  

E-Print Network (OSTI)

Edward Dial, B. S. , Texas A&M University Chairman of Advisory Committee: Dr. James R. Dixon N 1 hi y d' f ~C1 1* ' ' 1 d ly- sis of the reproductive and thermal ecology, diet composition, and behavior of the species. Data on the thermal ecology, diet... and mensural data from each species were recorded and geographic variation in C. brevis was analyzed. The reproductive cycle of C. brevis involves cyclic gonadal development in males and females. Males emerge from hibernation with enlarged testes...

Dial, Benjamin Edward



The glans penes and bacula in Latin American taxa of the Peromyscus boylii group  

E-Print Network (OSTI)

of Committee) John W. Bickham (Member) Ira ee baum (M be Fred S. Hendr icks (Member) Davi J Schmidly (Head f Department May 1986 ABSTRACT The Glans Penes and Bacula in Latin American Taxa of th ~9~bi'' 8 p. (11 y 1986) Robert Dean Bradley, B. S...thtP. b. ~l*' y tb . l*ly related to other subspecies of P. ~bo lii as previously reported. Finally, results of the phenetic and phylogenetic analyses indicate that two distinct types of phalli are evident among taxa in the P. ~bo lii species group...

Bradley, Robert Dean



Nationalization of the oil industry in Iran 1951-1953: a study in cold war diplomacy  

E-Print Network (OSTI)

that this oil was their only national resource, and that they wanted. the full benefits of the revenue for themselves. After several oil crises, the Iranian parliament under the leader- ship of Dr. Mohammed. Mossadegh announced. the nationalization... by her ownersh1p of' the oil refinery and f1elds and because it threatened to cut off her huge revenue from oil sales. She was therefore the power primar1ly concerned. with a settlement. The United States and Russian reactions were more complex...

Qaim-Maqami, Linda Wills



Depositional environment and reservoir characteristics of the upper Frio sandstones, Willamar field, Willacy County, Texas  

E-Print Network (OSTI)

~ of my committee, Dr. 'Ihmm Tish and Dr. W. John Iee, for their review and constructive criticism of the manuscript. I wish to thank Mr. Bob Miles, Ms. Theresa Tiebeau, Mr. Richard Ogden, and Mr. Chuck ~ of Amoco Production company for providing... pravinoe. Ibe Rio ~ Embayment received sediment from the Gueydan Fluvial System which records the entry of a major river system trending subparallel to the axis of the embayment. ')he San Marcos Arch had two scurf of s~ ~ly. 'Ihe Choke ~Flatonia, Coastal...

Caram, Hector Luis



Santa Fe, New Mexico  

NLE Websites -- All DOE Office Websites (Extended Search)

Fe, New Mexico Fe, New Mexico May 29-31, 2013 Se q u e n c i n g , F i n i s h i n g , A n a ly s i s i n t h e F u t u r e M e e t i ng 8 t h A nn u a l 2013 SFAF Meeting Page 1 Contents Agenda Overview......................................... 3 May 29 th Agenda.................................. 11 Speaker Presentations (May 29 th ).................. 13 Meet and Greet Party w/ Food & Beverages... 39 Poster Session............................................ 41 May 30 th Agenda................................. 97 Speaker Presentations (May 30


Quantitative relationships between structure and reactivity of aliphatic esters  

E-Print Network (OSTI)

bnglneering -xpcrtuent station and fron the Robert A. belch IIosearoh Foundation. Introduat ion . ' ethos of ~lysis ~ 0 Quleul-. tion of;1~to Oonst nt, s : iste riel s ~ o ~ I. 'iyters ~ ~ ~ 16 lC 11, . i~::' . ' Crt ~d*iP' 1~&'" :~ppsrstus z&& rl...-tt'rdor Rotc Cansta, ts for . :. oetntas IIIc. Ceoond- rder ". :;te Const tots ". tr Identicr lly Jis tbstt ttttod stars 't 0 IV. Ct, t" an "ct. 'tyl stere V. . )c' o~ cot otcs z2 'tl, . &oto on fde. otic. . t ly Cisubctitttted . . coors . 1. mymificction...

Yager, Billy Joe


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T-Negative Issue 14  

E-Print Network (OSTI)

is probably inevitable, although the use of computer-aids and other adVances in educa tion may r..ave speeded up the p:l:'Ocess. According to Stephen Whitfield in The Making of Star Trek, filcC::>y had been a - generaljpractitioner until his decision... -2- T-Negative 14, March lY72, comes from Ruth Berman, 5620 Edgewater Boulevard Minneapolis Minnesota 55417. Reprint: Belated Brag Dept: The Portland Oregonian had a poem of mine, "Sea-going House," in the "Oregonian Verse" column, November 19...

Berman, Ruth; Hall, Anna Mary



E-Print Network (OSTI)

movements in the Third World where essential minerals are found and essential markets are located. The state bears the costs of policing the world while the capitalist class reaps the profits. The state must take sides. 69 Mid-American Review of Sociology... against those who mount effective opposition to the logics of capitalist growth-especially in the Third World. The various efforts to assassi­ nate Castro by the CIA in Cuba and to eliminate opposition to friend­ ly regimes are examples (Powers, 1979...

Young, T. R.



Application of digital filtering in the study of the geological structure under the LASA  

E-Print Network (OSTI)

n g 5 CL , ( 1 'I'& I l. ss 1. ss 3. 6) s. m n . :J' s. s. . s Figure 26. Noise spectrum of array sum, RT06. s '. Iu s 1. ' 0 I. l]i Y S'yl Figure 27. Noise spectrum of array sum, Soviet explosion. 49 noise spectrums show large.... 001 sec. These are unusuai ly large variations for separations of 200 km. 1'airborn (1966) computed the travel time anomalies ior a layered crustal model with dipping beds and a crustal model with a horizontal velocity gradient. He concluded...

Sonnad, Jagadeesh Ramanna



The effects of barley bran flour and barley oil on hypercholesterolemic men and women  

E-Print Network (OSTI)

% with some special strains of up to 16% (30) . Cellulose, hemicellulose, and lignin are the main constituents of the crude or insoluble fiber portion of barley. The crude fiber content of cov- ered barley is approximately 4-8% and only 2% or less in hull... and women in a 30-day intervention trial. All participants were instructed to follow the National Cholesterol Education Program (NCEP) step-one diet and were d ly 'g dto f th t t tg p*. G~t added 20 grams of cellulose fiber to their daily intake. mG2...

Robinson, Michael Clayton




NLE Websites -- All DOE Office Websites (Extended Search)

-10 -10 4934 DE91 000814 PHOTOCONDUCTIVITY OF ACTIVATED CARBONFIBERS ' Ko Kuriyama Mo S. ,Dresselhaus MIT ...... ' Cambridge, Massachusetts ' MASTEB ,_ ' _Yii:i" ' £31STRIBUTION OFIT_"IIS DoCUMEt"JT IS L I?',_'-:'_ , I)IS('I,AIMI,',R Work pt`rforlnt`(I iiil(|t`r lilt' llll._illl'_-'_Of lilt' I J,,H, I)t, pllrl- mt`ni of i,_nt`r_)' I),_' l,=lwrt`n_'t` I,Ivi.,rmort` Ntllhrn=ll l,ld_or=_- Ior,_'mldc,r _'onlrzlct mlml}t`r W-74(15-1,1N(;.4X, 'l'hi,_ doc'mm..||l t_'=l.,_ prt`p=lrt`d =Is ==_l=lt'v,,,|ml o1' work _ptm._(!rvd I_)' IIn =lp, t`|lC')' 01' lht` (ll|ilt`(l ,_tiHl's (;|_vt`rnn|t`nt. Nvilht, r lht` I Inilt`d ,Sl=dL, s (;o_'t`rl|u|el|l mir Iht` t ll|i_'t`r_lt.,,'of ('lllifl)r,fl_l mrr lilLY o1"II,.,Ir v|lll_l_|)'t`t`_, I|mkt`_ _lll)' ,_'_mrr_lnl); exprt`_ or i|npllt`d, or _l_sl|i|lt`_ _|,ly lel_=lllhd)lilly i_r r¢'sl)(m- _ihilll)'


Detection of a redshift 3.04 filament  

E-Print Network (OSTI)

The filamentary structure of the early universe has until now only been seen in numerical simulations. Despite this lack of direct observational evidence, the prediction of early filamentary structure formation in a Cold Dark Matter dominated universe has become a paradigm for our understanding of galaxy assembly at high redshifts. Clearly observational confirmation is required. Lyman Break galaxies are too rare to be used as tracers of filaments and we argue that to map out filaments in the high z universe, one will need to identify classes of objects fainter than those currently accessible via the Lyman Break technique. Objects selected via their Ly-alpha emission, and/or as DLA absorbers, populate the faintest accessible part of the high redshift galaxy luminosity function, and as such make up good candidates for objects which will map out high redshift filaments. Here we present the first direct detection of a filament (at z=3.04) mapped by those classes of objects. The observations are the deepest yet to have been done in Ly-alpha imaging at high redshift, and they reveal a single string of proto-galaxies spanning about 5 Mpc (20 Mpc comoving). Expanding the cosmological test proposed by Alcock & Paczynski (1979), we outline how observations of this type can be used to determine Omega_Lambda at z=3.

P. Moller; J. U. Fynbo



Excited states of exciton-polariton condensates in 2D and 1D harmonic traps  

Science Journals Connector (OSTI)

We present a theoretical description of Bogolyubov-type excitations of exciton-polariton Bose-Einstein condensates (BECs) in semiconductor microcavities. For a typical two-dimensional (2D) BEC we focus on two limiting cases, the weak- and strong-coupling regimes, where a perturbation theory and the Thomas-Fermi approximation, respectively, are valid. We calculate integrated scattering intensity spectra for probing the collective excitations of the condensate in both considered limits. Moreover, in relation to recent experiments on optical modulation allowing localization of condensates in a trap with well-controlled shape and dimensions, we study the quasi-one-dimensional (1D) motion of the BEC in microwires and report the corresponding Bogolyubov excitation spectrum. We show that in the 1D case the characteristic polariton-polariton interaction constant is expressed as g1=3?N/(2Ly) (? is the 2D polariton-polariton interaction parameter in the cavity, N the number of the particles, and Ly the wire cavity width). We reveal some interesting features for 2D and 1D Bogolyubov spectra for both repulsive (?>0) and attractive (?<0) interactions.

C. Trallero-Giner; M. V. Durnev; Y. Núñez Fernández; M. I. Vasilevskiy; V. López-Richard; A. Kavokin




SciTech Connect

The sky-averaged (global) 21 cm signal is a powerful probe of the intergalactic medium (IGM) prior to the completion of reionization. However, so far it has been unclear whether it will provide more than crude estimates of when the universe's first stars and black holes formed, even in the best case scenario in which the signal is accurately extracted from the foregrounds. In contrast to previous work, which has focused on predicting the 21 cm signatures of the first luminous objects, we investigate an arbitrary realization of the signal and attempt to translate its features to the physical properties of the IGM. Within a simplified global framework, the 21 cm signal yields quantitative constraints on the Ly? background intensity, net heat deposition, ionized fraction, and their time derivatives without invoking models for the astrophysical sources themselves. The 21 cm absorption signal is most easily interpreted, setting strong limits on the heating rate density of the universe with a measurement of its redshift alone, independent of the ionization history or details of the Ly? background evolution. In a companion paper, we extend these results, focusing on the confidence with which one can infer source emissivities from IGM properties.

Mirocha, Jordan; Harker, Geraint J. A.; Burns, Jack O., E-mail: jordan.mirocha@colorado.edu [Center for Astrophysics and Space Astronomy, University of Colorado, Campus Box 389, Boulder, CO 80309 (United States)



The Great Observatories Origins Deep Survey: Constraints on the Lyman Continuum Escape Fraction Distribution of Lyman--Break Galaxies at 3.4  

E-Print Network (OSTI)

We use ultra-deep ultraviolet VLT/VIMOS intermediate-band and VLT/FORS1 narrow-band imaging in the GOODS Southern field to derive limits on the distribution of the escape fraction (f_esc) of ionizing radiation for L >~ L*(z=3) Lyman Break Galaxies (LBGs) at redshift 3.4--4.5. Only one LBG, at redshift z=3.795, is detected in its Lyman continuum (LyC; S/N~5.5), the highest redshift galaxy currently known with a direct detection. Its ultraviolet morphology is quite compact (R_eff=0.8, kpc physical). Three out of seven AGN are also detected in their LyC, including one at redshift z=3.951 and z850 = 26.1. From stacked data (LBGs) we set an upper limit to the average f_esc in the range 5%--20%, depending on the how the data are selected (e.g., by magnitude and/or redshift). We undertake extensive Monte Carlo simulations that take into account intergalactic attenuation, stellar population synthesis models, dust extinction and photometric noise in order to explore the moments of the distribution of the escaping radi...

Vanzella, E; Inoue, A; Nonino, M; Fontanot, F; Cristiani, S; Grazian, A; Dickinson, M; Stern, D; Tozzi, P; Giallongo, E; Ferguson, H; Spinrad, H; Boutsia, K; Fontana, A; Rosati, P



Strong Emission-Line Galaxies at Low Redshift in the Field around the Quasar SDSSp J104433.04-012502.2  

E-Print Network (OSTI)

We discuss observational properties of strong emission-line galaxies at low redshift found by our deep imaging survey for high-redshift Ly alpha emitters. In our surveys, we used the narrowband filter, NB816 (lambda_center=8150A with FWHM = 120A), and the intermediate-band filter, IA827 (lambda_center = 8270A with FWHM = 340A). In this survey, 62 NB816-excess (> 0.9 mag) and 21 IA827-excess (> 0.8 mag) objects were found. Among them, we found 20 NB816-excess and 4 IA827-excess Ly alpha emitter candidates. Therefore, it turns out that 42 NB816-excess and 17 IA827-excess objects are strong emission-line objects at lower redshift. Since 4 objects in the two low-z samples are common, the total number of strong low-z emitters is 55. Applying our photometric redshift technique, we identify 7 H alpha emitters at z~0.24, 20 H beta-[OIII] ones at z~0.65, and 11 [OII] ones at z~1.19. However, we cannot determine reliable photometric redshifts of the remaining 17 emitters. The distributions of their rest frame equivalen...

Ajiki, M; Taniguchi, Y; Murayama, T; Nagao, T; Sasaki, S S; Sumiya, R; Morioka, T; Hatakeyama, Y; Yokouchi, A; Takahashi, M I; Koizumi, O; Ajiki, Masaru; Shioya, Yasuhiro; Taniguchi, Yoshiaki; Murayama, Takashi; Nagao, Tohru; Sasaki, Shunji S.; Sumiya, Ryoko; Morioka, Taichi; Hatakeyama, Yuichiro; Yokouchi, Asuka; Takahashi, Mari I.; Koizumi, Osamu



A Subaru Search for Lyman-Alpha Emitters at z=5.8 with an Intermediate-Band Filter  

E-Print Network (OSTI)

We present the results of a survey for Ly-alpha emitters at z ~ 5.8 using a new intermediate-band filter centered at lambda_c = 8275 AA with Delta-lambda_FWHM = 340 AA (i.e., the spectroscopic resolution is R ~ 23) with a combination with a traditional narrow-band centered at lambda_c = 8150 AA with Delta-lambda_FWHM = 120 AA (R ~ 68). Our observations were made with use of the Subaru Prime Focus Camera, Suprime-Cam, on the 8.2 m Subaru telescope in a sky area surrounding the high redshift quasar, SDSSp J104433.04-012522.2 at z=5.74, covering an effective sky area with ~ 720 arcmin^2. In this survey, we have found four Ly-alpha-emitter candidates from the intermediate-band image (z \\~ 5.8 with Delta z ~ 0.3). Combined with our previous results based on the NB816 imaging, we discuss the star formation activity in galaxies between z ~ 5.7 and z ~ 5.9.

Ajiki, M; Fujita, S S; Shioya, Y; Nagao, T; Murayama, T; Yamada, S F; Umeda, K; Sasaki, S S; Sumiya, R; Komiyama, Yu; Ajiki, Masaru; Taniguchi, Yoshiaki; Fujita, Shinobu S.; Shioya, Yasuhiro; Nagao, Tohru; Murayama, Takashi; Yamada, Sanae F.; Umeda, Kazuyoshi; Sasaki, Shunji S.; Sumiya, Ryoko; Komiyama, Yutaka



A Search for Lyman alpha Emitters at Redshift 3.7  

E-Print Network (OSTI)

We present the results of a survey for emission-line objects based on optical intermediate-band ($\\lambda_{\\rm c}$ = 5736 \\AA ~ and $\\Delta\\lambda$ = 280 \\AA) and broad-band ($B$, $V$, $R$, and $i^\\prime$) observations of the Subaru/XMM-Newton Deep Field on the 8.2 m Subaru telescope with the Subaru Prime Focus Camera, Suprime-Cam. All the data were obtained during the guaranteed time observations of the Suprime-Cam instrument. The intermediate-band image covered a sky area with 10\\minpoint62 $\\times 12\\minpoint40 \\approx 132$ arcmin$^2$ in the Subaru/XMM-Newton Deep Field (Ouchi et al.). Using this image, we have found 23 emission-line sources whose observed emission-line equivalent widths are greater than 250 \\AA. Their optical multicolor properties indicate that six emission-line sources are Ly$\\alpha$ emitters at $z \\approx$ 3.7 ($\\Delta z \\approx 0.22$). They are either intense starburst galaxies or active galactic nuclei like quasars at $z \\approx$ 3.7. Two more emission-line sources may also be Ly$\\alp...

Fujita, S S; Shioya, Y; Nagao, T; Murayama, T; Taniguchi, Y; Okamura, S; Ouchi, M; Shimasaku, K; Doi, M; Furusawa, H; Hamabe, M; Kimura, M; Komiyama, Yu; Miyazaki, M; Miyazaki, S; Nakata, F; Sekiguchi, M; Yagi, M; Yasuda, N; Matsuda, Y; Tamura, H; Hayashino, T; Kodaira, K; Karoji, H; Yamada, T; Ohta, K; Umemura, M; Fujita, Shinobu S.; Ajiki, Masaru; Shioya, Yasuhiro; Nagao, Tohru; Murayama, Takashi; Taniguchi, Yoshiaki; Okamura, Sadanori; Ouchi, Masami; Shimasaku, Kazuhiro; Doi, Mamoru; Furusawa, Hisanori; Hamabe, Masaru; Kimura, Masahiko; Komiyama, Yutaka; Miyazaki, Masayuki; Miyazaki, Satoshi; Nakata, Fumiaki; Sekiguchi, Maki; Yagi, Masafumi; Yasuda, Naoki; Matsuda, Yuichi; Tamura, Hajime; Hayashino, Tomoki; Kodaira, Keiichi; Karoji, Hiroshi; Yamada, Toru; Ohta, Kouji; Umemura, Masayuki



Kubo number and magnetic field line diffusion coefficient for anisotropic magnetic turbulence  

Science Journals Connector (OSTI)

The magnetic field line diffusion coefficients Dx and Dy are obtained by numerical simulations in the case that all the magnetic turbulence correlation lengths lx, ly, and lz are different. We find that the variety of numerical results can be organized in terms of the Kubo number, the definition of which is extended from R=(?B/B0)(l?/l?) to R=(?B/B0)(lz/lx), for lx>~ly. Here, l? (l?) is the correlation length along (perpendicular to) the average field B0=B0e^z. We have anomalous, non-Gaussian transport for R?0.1, in which case the mean square deviation scales nonlinearly with time. For R?1 we have several Gaussian regimes: an almost quasilinear regime for 0.1?R?1, an intermediate, transition regime for 1?R?10, and a percolative regime for R?10. An analytical form of the diffusion coefficient is proposed, Di=D(?Blz/B0lx)?(li/lx)?lx2/lz, which well describes the numerical simulation results in the quasilinear, intermediate, and percolative regimes.

P. Pommois; P. Veltri; G. Zimbardo



Nepali Aawaz Volume 1, Issue 6, 7-20 December 2005  

E-Print Network (OSTI)

fnfO{ ;'g;/L t/x/fsf] Ps lk;Lcf] af6 k|x/Ln] kqmfp u/]sf] 5 . pgn] cfkm' dfcf]jfbL ePsf] bfjL ub}{ Ps ;ftf cl3 b]vL 6]lnkmf]gaf6 /sd dfu ub}{ cfPsf lyP kqmfp k5L pgL t/sf/L tyf rf}kfo Aofkf/L ePsf] v'Ng cfPsf] 5 . g]skf dfcf]jfbLsf] gfd lnP/ o... ;/L ;j{;fwf/0fnfO{ wDsL lbb} rGbf p7fpg] lu/f]x ;lqmo x'g yfn]k5L dfcf]jfbLx?n] g} To:tf lu/f]xnfO{ vf]hL–vf]hL dfg{ yfn]sf 5g . g]skf dfcf]jfbL ;'g;/Ln] dfcf]jfbL ag]/ rGbf ;+sng ug]{ b'O{ / emfkfdf b'O{ hgfsf] ut jif{ xTof u/]sf lyP . Page 6 INGOS...

Shrestha, Kashish Das


The Energy Cascade from Warm Dark Matter Decays  

E-Print Network (OSTI)

We use a set of Monte Carlo simulations to follow the cascade produced by a primary electron of energy E_in in the intergalactic medium. We choose E_in=3-10 keV as expected from the decay of one of the most popular Warm Dark Matter (WDM) candidates, sterile neutrinos. Our simulation takes into account processes previously neglected such as free-free interactions with ions and recombinations and uses the best available cross sections for collisional ionizations and excitations with H and He and for electron-electron collisions. We precisely derive the fraction of the primary electron energy that heats the gas, ionizes atoms and produces line and continuum photons as a function of the ionization fraction. Handy fitting formulae for all the above energy depositions are provided. By keeping track of the individual photons we can distinguish between photons in the Ly-alpha resonance and those with energy E gas. This separation is important because a Ly-alpha background can heat or cool the gas depending on the nature of the photons, and can have effects on the 21 cm radiation emitted by neutral H, which will probably become detectable at z > 6 in the near future by the next generation radio interferometers.

M. Valdés; A. Ferrara



Effect of selected aldehydes on the growth and fermentation of ethanologenic Escherichia coli  

SciTech Connect

Bioethanol production from lignocellulosic raw-materials requires the hydrolysis of carbohydrate polymers into a fermentable syrup. During the hydrolysis of hemicellulose with dilute acid, a variety of toxic compounds are produced such as soluble aromatic aldehydes from lignin and furfural from pentose destruction. In this study, the authors have investigated the toxicity of representative aldehydes (furfural, 5-hydroxymethlyfurfural, 4-hydroxybenzaldehyde, syringaldehyde, and vanillin) as inhibitors of growth and ethanol production by ethanologenic derivatives of Escherichia coli B (strains K011 and LY01). Aromatic aldyhydes were at least twice as toxic as furfural of 5-hydroxymethylfurfural on a weight basis. The toxicities of all aldehydes (and ethanol) except furfural were additive when tested in binary combinations. In all cases, combinations with furfural were unexpectedly toxic. Although the potency of these aldehydes was directly related to hydrophobicity indicating a hydrophobic site of action, none caused sufficient membrane damage to allow the leakage of intracellular magnesium even when present at sixfold the concentrations required for growth inhibition. Of the aldehydes tested, only furfural strongly inhibited ethanol production in vitro. A comparison with published results for other microorganisms indicates that LY01 is equivalent or more resistant than other biocatalysts to the aldehydes examined in this study.

Zaldivar, J.; Ingram, L.O. [Univ. of Florida, Gainesville (United States). Dept. of Microbiology and Cell Science] [Univ. of Florida, Gainesville (United States). Dept. of Microbiology and Cell Science; Martinez, A. [Univ. of Florida, Gainesville (United States). Dept. of Microbiology and Cell Science] [Univ. of Florida, Gainesville (United States). Dept. of Microbiology and Cell Science; [Univ. Nacional Autonoma de Mexico (Mexico). Inst. de Biotecnologia



eCopy, Inc.  

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Tne -submitted manuscript has been authored Tne -submitted manuscript has been authored by a contractOr of the U. S. Government under contract No. W·31·109-ENG-38. Accordingly, the U. S. Government retains a nonexclusive, royalty·free license to publish or reproduce the published form of this contribution, or allow others to do so for U. S. Government purposes. I L8-162 1/91 Steering magnets and BPM's in the high energy transfer line. R. K. Koul Argonne N ational Laboratory This note contains the details concerning the steering magnets and the beam position monitors needed in the high energy transfer line. The computer code, written in "C" and used for the ray tracing of the positron particles was written 10ca1ly with the express pur- pose of handling this problem. However, the accuracy of the code was tested by calculating


BP and Hydrogen Pipelines  

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BP and Hydrogen Pipelines BP and Hydrogen Pipelines DOE Hydrogen Pipeline Working Group Workshop August 30-31, 2005 Gary P. Yoho, P.E. i l i * Green corporate philosophy and senior management commitment * Reduced greenhouse gas emissions nine years ahead of target * Alternatives to oil are a big part of BP' including natural gas, LNG, solar and hydrogen * Hydrogen Bus Project won Australia' prestigious environmental award * UK partnership opened the first hydrogen demonstration refueling station * Two hydrogen pipelines in Houston area BP Env ronmenta Comm tment s portfolio, s most BP' * li l " li i i * i l pl i i * Li l li l * " i i l i 2 i i ll i i l pl ifi i * 8" ly idl i i l s Hydrogen Pipelines Two nes, on y a brand new 12 ne s act ve Connect Houston area chem ca ant w th a ref nery nes come off a p



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D D AT E S O U T H W E S T E R N P O W E R A D M I N I S T R A T I O N S U P P L E M E N T A L E D I T I O N J U LY 1 3 , 2 0 0 6 PMA Partnership Implements New SCADA System at Springfield Operations Center Southwestern successfully installed its new Supervisory Control and Data Acquisition (SCADA) system at its Operations Center in Springfield, MO, on June 20, 2006. This new software, developed in cooperation with Western Area Power Administration (Western), essentially replaces the old Unix-based commercial system with a personal- computer-based SCADA and Automatic Generation Control (AGC) power control system. The new system provides additional functionality that meets recent requirements from the North American Electric Reliability Council for better alarming capabilities and situational awareness, and also



Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

71 71 2; W(A)-2011-067 ; CH-1639 General Electric Global Research Center (GE-GRC) requests an advance waiver of domestic and foreign patent rights for all subject inventions made under the above cooperative agreement for work entitled, "Model Based Optimal Sensor Network Design for Condition Monitoring in an IGCC Plant". The purpose of the cooperative agreement is to develop a systematic model-based approach for addressing the problem of optimal sensor placement (OSP) in a sensor network used for condition monitoring of key process equipment in an IGCC plant , namely, gasifier refractory lining and RSC fouling . This waiver is for inventions of GE-GRC on ly. The work under this cooperative agreement is expected to take place from August 20, 2010 through December 30, 2012, at a total cost of $1

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One West Third Street Tulsa Oklahoma  

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Conley Jennings Conley Jennings Lineman Springfield, MO Special thanks to: Marshall Boyken Mike Deihl Ruben Garcia Bethel Herrold William Hiller Beth Nielsen George Robbins Gary Swartzlander Cris Van Horn Rutha Williams Jan Woolverton U P D AT E S O U T H W E S T E R N P O W E R A D M I N I S T R A T I O N J U LY - S E P T E M B E R 2 0 0 5 Strategic Workshop Unites Hydropower Community At the invitation of the U.S. Army Corps of Engineers (Corps), Federal power customers joined representatives of the Corps, the Power Marketing Administrations, and national Federal power customer associations in Tulsa, Oklahoma, on August 9-10, 2005, for the second Hydropower Strategic Workshop. Nearly 100 people, including those involved in the daily operation of Corps hydropower projects and powerplants, managers and technical staff of Federal power customers, and


CEM: You Asked, We Answered | Department of Energy  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

CEM: You Asked, We Answered CEM: You Asked, We Answered CEM: You Asked, We Answered July 29, 2010 - 4:15pm Addthis John Schueler John Schueler Former New Media Specialist, Office of Public Affairs Last week, we invited you to submit your questions on the Clean Energy Ministerial (CEM) via E-mail, Facebook and Twitter. We received a diverse set of questions, which we presented to two of the key decision makers here at the Department of Energy, Assistant Secretary for Policy and International Affairs David Sandalow and Assistant Secretary for Energy Efficiency and Renewable Energy Cathy Zoi. jsalsman (via Twitter): What is @energy's position on http://3.ly/100by2030 (editor: links to a plan that claims that 100 percent of the world's energy, for all purposes, could be supplied by wind, water and solar resources, by as early as 2030 ) Is a 30%


Ronnen Levinson  

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Ronnen M. Levinson Ronnen M. Levinson Ronnen Levinson Windows and Envelope Materials Group Lawrence Berkeley National Laboratory 1 Cyclotron Road MS 90-2000 Berkeley CA 94720 Office Location: 90-2056H (510) 486-7494 RMLevinson@lbl.gov This publications database is an ongoing project, and not all Division publications are represented here yet. Publications 2013 Ban-Weiss, George, Craig P. Wray, William W. Delp, Peter Ly, Hashem Akbari, and Ronnen M. Levinson. "Electricity production and cooling energy savings from installation of a building-integrated photovoltaic roof on an office building." Energy and Buildings 56 (2013): 210-220. 2012 Levinson, Ronnen M.. The Case for Cool Roofs., 2012. Download: PDF (205.7 KB) 2011 Menon, Surabi, and Ronnen M. Levinson. Cool roofs and global cooling: a


Hanford Site Treating Record Amount of Contaminated Groundwater |  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Treating Record Amount of Contaminated Groundwater Treating Record Amount of Contaminated Groundwater Hanford Site Treating Record Amount of Contaminated Groundwater July 15, 2013 - 12:00pm Addthis Media Contacts Geoff Tyree, DOE (509) 376-4171 Geoffrey.Tyree@rl.doe.gov Tania Reyes, CHPRC (509) 373-6828 Tania_Reyes@rl.gov Department of Energy goal for fiscal year 2013 met early Note: Photos and graphics are available for downloading on our website link: http://ow.ly/mO5cT RICHLAND, Wash. - U.S. Department of Energy (DOE) contractor CH2M HILL Plateau Remediation Company (CH2M HILL) has exceeded this year's goal for treating 1.4 billion gallons of contaminated groundwater at the Hanford Site in Washington state. "In the last few years, DOE built three new groundwater treatment facilities, and now we are seeing the results," said Briant Charboneau,


Layout 1  

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32 32 0163-6804/11/$25.00 © 2011 IEEE INTRODUCTION A grid network is a collection of geographical- ly distributed resources, such as storage clus- ters, supercomputers, and scientific equipment, that are accessible to users over a network. Examples of e-Science grids include the Large Hadron Collider Computing Grid Project, the Biomedical Informatics Research Network, and the George E. Brown Network for Earthquake Engineering and Simulation. These networks typically deal with the trans- fer of large amounts of data in the terabytes and petabytes range. When the grid resources are connected by application-configurable optical paths (e.g., on an optical wavelength- routed network), the grid can be considered a LambdaGrid [1]. Optical wavelength-routed wavelength-divi-



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AECU - 785 AECU - 785 THE EFFECT OF ELECTRONIC PARAMAGNETISM ON NUCLEAR MAGNETIC RESONANCE FREQUENCIES IN METALS By C. H. Townes Conyers Herring W. D. Knig^it Columbia University Bell Telephone Laboratories Trinity College Tochnicai Information Division, ORE, Oak Ridgo, Tonnossoo J^ This document is FUBLK:LY RELEASABLF //> [\AAUMJ DISCLAIMER This report was prepared as an account of work sponsored by an agency of the United States Government. Neither the United States Government nor any agency Thereof, nor any of their employees, makes any warranty, express or implied, or assumes any legal liability or responsibility for the accuracy, completeness, or usefulness of any information, apparatus, product, or process disclosed, or represents that its use would not infringe privately


Building integrated photovoltaic (BIPV) roofs for sustainability and energy  

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integrated photovoltaic (BIPV) roofs for sustainability and energy integrated photovoltaic (BIPV) roofs for sustainability and energy efficiency Title Building integrated photovoltaic (BIPV) roofs for sustainability and energy efficiency Publication Type Report Year of Publication 2013 Authors Ly, Peter, George Ban-Weiss, Nathan Finch, Craig Wray, Mark de Ogburn, William W. Delp, Hashem Akbari, Scott Smaby, Ronnen Levinson, and Bret Gean Corporate Authors SEI Group Inc. Document Number ESTCP EW-200813 Pagination 156 pp. Date Published 09/2013 Publisher Naval Facilities Engineering Command - Engineering and Expeditionary Warfare Center Type Technical Report Report Number TR-NAVFAC-EXWC-PW-1303 Keywords Buildings Energy Efficiency, energy efficiency, Energy Usage, renewable energy, Renewable Energy: Policy & Programs Abstract


IGCC+S Financing  

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II II William G. Rosenberg, Dwight C. Alpern, Michael R. Walker Energy Technology Innovation Project a joint project of the Science, Technology and Public Policy Program and the Environment and Natural Resources Program Belfer Center for Science and International Affairs 2 0 0 4 - 0 8 J U LY 2 0 0 4 Deploying IGCC in this Decade with 3Party Covenant Financing VOLUME II William G. Rosenberg, Dwight C. Alpern, and Michael R. Walker Energy Technology Innovation Project a joint project of the Science, Technology and Public Policy Program and the Environment and Natural Resources Program Belfer Center for Science and International Affairs and Center for Business and Government John F. Kennedy School of Government Harvard University July 2004 Financing IGCC - 3Party Covenant ii



Office of Legacy Management (LM)

__, I,- __.j .^,, ~~.,l~, _I.x__ . ,,,,, ,_^_ ,,_xx,. ,~.__~_x -,-.. _1 ,.,., __, I,- __.j .^,, ~~.,l~, _I.x__ . ,,,,, ,_^_ ,,_xx,. ,~.__~_x -,-.. _1 ,.,., - I~ .c \ -- - g-' . @ ~--~Z~, Ls-u &. 0 -*,- hiK ,,-& b TO FILE ' = .-. r. AUG 2 9 1945 A~TPPHC~~~ METALS COPUDOP~TIO~ '* ~,ci~ly~1~~ 41 BROAD STREET (In duplicate) November 6, 1942 The District Engineer, u. s . Zngineer Office, Zanhattarn District, P. 0. 30x 4.2, Station P., i?C:: York, X.Y. Attention: Idajo- Thomas T. Crenshav:. Gentlemen: Classification Cancc!!A ZG? ;~yp~~ Follo~5.nS our conversation of yesterday, P;e here*oy confirm gi-ang you optior., vslid up to tine erd of Xcver.ssr 19LZ2, for the purchase cf: - :fbmm.I;1T,: _, ..I-- ASout 42 short tons of Sodi- Uranate Cranze, holding about 83-l/2$ of U30 ; packed in ooxes. . About 64 short tons of Sodium Uranate Yello:,



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CONSIDERATIONS IN THE DESIGN OF UNDULATORS CONSIDERATIONS IN THE DESIGN OF UNDULATORS L. C. Teng A. Relevant Radiation Formulas LS-66 July 28, 1986 (1) The midplane field in an undu1ator is given approximately by where y = s = t Bo = coordinate in coordinate in B (s) Y direction direction undu1ator period length peak field of gap of beam The orbit wiggles in the transverse direction x perpendicular to y and s, and is given by where d prime = Ts x' = 2;P cos (2~ t) - x~ cos (2~ ~) o Po = }- (rigidity, Bp = ~ p, of beam). o The deflection parameter K is defined by x' K max. wiggle angle 0 = ~ - radiation angle - l/y 2~po where Y is the particle energy in rest energy, mc 2 , units. A device '" with K > 10 for which the radiation spectrum is more-or-1ess continuous is


Newsletter (January 2010) SHR.pub  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Workshop Workshop Announce- 1 FPD Corner 2 CAP Corner 3 PMCDP Schedule 4 Question of the Month 5 Questions or Comments 5 P R O J E C T M A N A G E M E N T C A R E E R D E V E L O P M E N T P R O G R A M Pathways to Project Success J A N U A R Y 2 0 1 0 Cost: There is no registration fee. However, attendees are responsible for their own travel and lodging expenses. Registration: Registration is now open at http://bit.ly/83brzl and will close February 19, 2010. The Agenda is available at http://management.energy.gov/1771.htm. Both government and contractor executives and managers are invited to attend the March 9 & 10 workshop, although, due to meeting room space constraints, registration will be limited. PMCDP Course: The PMCDP Level 1, Course


VIA EMAIL Ms. Mariah Steele ENERGY STAR Program U.S. Environmental Protection Agency  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Peru1sylvania Avenue, NW Peru1sylvania Avenue, NW Room62023 Washington, DC 20460 Dear Ms. Steele: June 12, 2013 The U.S. Department of Energy ("DOE") selected a Fisher & Paykel Appliances ("F&P") residential clothes washer, model WA42T26GW1, for testing as part ofDOE's ENERGY STAR® Verification Testing Program. On March 18, 2013, DOE notified F&P that DOE testing showed the model did not meet the ENERGY STAR requirement for water factor ("WF") 1 or modified energy factor ("MEF"). 2 F&P replied to DOE on April 16, 2013, making two claims. First, F&P argued that DOE had impropel'ly tested the warm wash cycles on the relevant units because the tested model has a "uniformly distributed warm wash temperature selection/' as defined in section 1.17 of


SPEAR3 | A Brighter Source at SSRL  

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Pat Dehmer's Talk: Pat Dehmer's Talk: Almost precisely se ven years ago, the Office of Basic Energy Sciences commissioned the first review of its four light sources. The review was headed by Bob Birgeneau, who was then the Dean of Science at MIT. The committee members were among the most distinguished researchers in the country. However, very deliberately, only a fraction of them knew about the light sources. Some of the others were skeptics. A few were hostile, primari ly because of the large budgets associated with construction and operation of the light sources. We asked this committee ten questions. The first question, the most important question, was: "What has been the scientific impact of synchrotron radiation based research during the past decade, and what is it expected to be during the next decade?"



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Administration, Administration, like: Mike Deihl Administrator Tulsa, Oklahoma Special thanks to: Ladell Butts Scott Carpenter Dallas Cooper Linda Dunham Ruben Garcia Tom Green Janet Hagar Gregg Happle William Hiller Sean Long Stan Mason Linda Mummey Beth Nielsen Fritha Ohlson George Robbins Dave Sargent Aiden Smith Jane Thomas Mistie Yost U P D AT E S O U T H W E S T E R N P O W E R A D M I N I S T R A T I O N J U LY - S E P T E M B E R 2 0 0 7 Hilltop Helps Ease Transmission Woes The electricity is flowing a little easier in northern Arkansas these days, thanks to the August 2007 energization of an interconnection between Southwestern and Entergy Arkansas, Inc. (Entergy) near Silver Hill, Arkansas. Planning for the tie has been underway for over five years, with the goal of easing potential undervoltage and overload conditions, thus allowing increasing



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44 results: 44 results: BibTex RIS RTF XML Sort by: Author Title Type [ Year (Desc) ] Filters: Author is Ronnen M. Levinson [Clear All Filters] 2013 Ban-Weiss, George, Craig P. Wray, William W. Delp, Peter Ly, Hashem Akbari, and Ronnen M. Levinson. "Electricity production and cooling energy savings from installation of a building-integrated photovoltaic roof on an office building." Energy and Buildings 56 (2013): 210-220. 2012 Levinson, Ronnen M.. The Case for Cool Roofs., 2012. 2011 Menon, Surabi, and Ronnen M. Levinson. Cool roofs and global cooling: a response to Jacobson & Ten Hoeve (2011)., 2011. Sleiman, Mohamad, George Ban-Weiss, Haley E. Gilbert, David François, Paul Berdahl, Thomas W. Kirchstetter, Hugo Destaillats, and Ronnen M. Levinson. "Soiling of building envelope surfaces and its effect on solar


pac 2003 boundary3.ppt  

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5-yr program review May 13-14, 2003 5-yr program review May 13-14, 2003 Alcator Alcator C-Mod Divertor and Edge Physics program Presented by B. Lipschultz Relationship to other programs General program description Past 5 year highlights Transport Neutrals Impurities High heat flux & particle handling C-Mod 5-yr program review May 13-14, 2003 Alcator Alcator C-Mod C-Mod in relation to other tokamaks C-Mod operation overlaps that of other tokamaks in edge/divertor dimensionless parameters w/different dimensional parameters Some of the differences in edge & divertor dimensional parameters are Higher density (similar to ITER in divertor) Higher parallel heat flux (300-500 MW/m 2 , 3-5x other tokamaks, similar to ITER) Higher divertor opacity to Ly α (similar to ITER) Higher SOL plasma pressures (similar than ITER)


Hanford Site Treating Record Amount of Contaminated Groundwater |  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Hanford Site Treating Record Amount of Contaminated Groundwater Hanford Site Treating Record Amount of Contaminated Groundwater Hanford Site Treating Record Amount of Contaminated Groundwater July 15, 2013 - 12:00pm Addthis Media Contacts Geoff Tyree, DOE (509) 376-4171 Geoffrey.Tyree@rl.doe.gov Tania Reyes, CHPRC (509) 373-6828 Tania_Reyes@rl.gov Department of Energy goal for fiscal year 2013 met early Note: Photos and graphics are available for downloading on our website link: http://ow.ly/mO5cT RICHLAND, Wash. - U.S. Department of Energy (DOE) contractor CH2M HILL Plateau Remediation Company (CH2M HILL) has exceeded this year's goal for treating 1.4 billion gallons of contaminated groundwater at the Hanford Site in Washington state. "In the last few years, DOE built three new groundwater treatment facilities, and now we are seeing the results," said Briant Charboneau,


October 21, 2003, Board Public Meeting Presentations - DOE Independent Safety Oversight  

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HEARING HEARING Office of Independent Oversight and Performance Assurance October 21,2003 1 Office of Independent Oversight 1 and Performance Assurance 1 h.?s=- Role of Independent Oversight l Direct Report to the Secretary of Energy l Oversight for both NNSA and ESE l DOE's Corporate Oversight Entity l Provides Independent Performance-Based Evaluations Ytl l Well-Established Inspection Processes Office of Independent Oversight and Performance Assurance OA's Technical Competence l Dedicated Team of Experienced Inspectors l Extensive Managerial and Technical Expertise l Technical Qualification Program and External Certifications Office of Independent Oversight and Performance Assurance ? Some Key Inspection Focus Areas i l ISM Programs LY.W 0 Safety Systems


Manufacturing Perspective  

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EOT_RT_Sub_Template.ppt | 1/6/2009 | 1 EOT_RT_Sub_Template.ppt | 1/6/2009 | 1 BOEING is a trademark of Boeing Management Company. Copyright © 2009 Boeing. All rights reserved. Compressed Hydrogen Storage Workshop Manufacturing Perspective Karl M. Nelson (karl.m.nelson@boeing.com) Boeing Research & Technology Engineering, Operations & Technology | Boeing Research & Technology Materials & Fabrication Technology EOT_RT_Sub_Template.ppt | 1/12/2009 | Structural Tech 2 Copyright © 2009 Boeing. All rights reserved. DOE Hydrogen Program Development of Advanced Manufacturing Technologies for Low Cost Hydrogen Storage Vessels Mark Leavitt, Alex Ly Quantum Fuel Systems Technologies Worldwide Inc. Karl Nelson, Brice Johnson The Boeing Company Ken Johnson, Kyle Alvine, Stan Pitman, Michael Dahl, Daryl Brown


Lamp Divisions  

Office of Legacy Management (LM)

--- --- /A;; i :' r%i;in~house ilEc;' i:Z3:~cra:ion Lamp Divisions , _.. (I +i. 0 :,,,rg. . I . . -= i?e p/q! qe)-' &se pw E.rcale?l iev, Je!sey 07m March 20, 1 gs? ::r . J. A. Jones I ti. 5. Muclear Regulatory Commission .> = ..- haterials Licensing Branch -s - ,.I, - - Division of Fuel Cycle and hateri al Safety LY. , $2 - _ . ' -' . 3 _- - Yeshington, C. C. 2@555 - :_ :--, =-- -- .-?J -.: y...., : :- 7 Dear Mr. Jones : y-- --, ? . *I 2=15 2 r; X -P The following is our final report of the decontamination efZor?s takz in our Bui Iding 7 basement and wi 11 also serve to update our report i& November 12, 1980. As stated in NRC' s report of December 22, 1983, two closeout inspect ions were conducted by your King of Prussia off i ce on November 21 and December 2,

Note: This page contains sample records for the topic "vleet hol ly" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.



Office of Legacy Management (LM)

10256-MS 10256-MS Los Alamos National Laboratory is operated by the University of California for the United States Department of Energy under contract W-7405-ENG-36. Radiological Survey and Evaluation of the Fallout Area fom the Trinity Test: Chupadera Mesa and White Sands Misile Range, New Mexco - ~ ~S1S' :ts rV T Los Alamos National Laboratory Ly© /.aU U UwHjm ©,Los Alamos, New Mexico 87545 An Affirmative Action/Equal Opportunity Employer Prepared by Kathy Derouin, Group HSE-8 DISCLAIMER This report was prepared as an account of work sponsored by an agency of the United States Government. Neither the United States Government nor any agency thereof, nor any of their employees, makes any warranty, express or implied, or assumes any legal liability or responsibility for the accuracy, completeness,


A shipping plan for bulk petroleum products by sea-going tankers  

E-Print Network (OSTI)

(. 01; 1 ?I 0 st '. ii i 0 '. 0 i. gbt 01 uolltc e 0 1!i 1(!i Ly has 1&ci il (' !( !tlst ccl SL sotto po inL in i t s cr&!it 0) I&1 0 I, . P. 'I&(obl &i& iS ii(I jt!' Lcd . . ' 'g t(1011 'Oiuc, thc' pcoilp, 1 ti( Lh so(le 1&(& 1 ! (Pl!it c&i, 'll.... (gy us inc t&&o d I?! ts, ny nc &bcr up Lo &nd 1?eluding 1295 ccn be rcprcuc?Lcd in L&sc 36. ) The. ro&& n; &&c XJPj jpn spccii I&. s I h&t all Lh &uutri &. - in i his ro&& coL'respond co Lhe n r& quir -mont for: product p ?t dc; I inai &ou jj (base...

Boyd, David George



Red Rice Research and Control.  

E-Print Network (OSTI)

s cu l t iva ted white r i c e , Oryza sativa L. Red r i c e crosses read i ly .- with white r i c e and i s very s i m i l a r t o it i n appearance. The main morpho- logical d i f ferences t h a t d i s t ingu i sh it from white r i c... l e s i n white r i c e . Since these characters can be t r ans fe r red by crossing, new red r i c e types can and do appear. Red r i c e i s undesirable because: 1. Red r i c e p l a n t s compete with cu l t iva ted r i c e...

Baker, John B.; Baldwin, Ford L.; Bourgeois, W.J.; Cox, Clodis H.; Craigmiles, Julian P.; Dishman, William D.; Eastin, E. Ford; Helpert, Charles W.; Hill, Lewis C.; Huey, Bobby A.; Klosterboer, Arlen D.; Sonnier, Earl A.



Kh trng khn cp nc ung Trong nhng thi k ri ren, cc s y t a phng c th khuyn co ngi dn dng nc thn  

E-Print Network (OSTI)

nc cho gia ình bn, bn vn có th tìm c s lng gii hn dùng bng cách ly nc ra t bình nc nóng, hay là tan nc ni ó. Thuc kh trùng ít hiu nghim nu nc c. Cn phi lc nc c qua nhng khn sch hoc yên cho lng xung, và không b r sét. Có hai phng pháp kh trùng thông dng và hiu qu nu lng nc ít. Phng pháp th nht là Ðun


Sedimentology and stratigraphy of the Miocene to Pliocene Mona Reef Complex and its relation with relative sea-level fluctuations  

E-Print Network (OSTI)

or a ce rv ic or ni s PJ , E SC EP li- L Pl e M Pl e B 5- 30 m B R -F R L 2. A cr op or a pa lm at a PP , C I EP li- L Pl e M Pl e B 1- 5m R C L 3. A cr op or a pa na m en si s E M io -E Pl e B FR E 4. A cr op... sh al lo w -d ep th L 24 . P or ite s w ay la nd i U V L O l- E Pl e L O l M sh al lo w -d ep th B R -F R E 25 . S co ly m ia PC L M io -E Pl e M do w n 10 0m D R a nd W L 26 . S te ph an oc oe ni a du nc an i L...

Rodriguez Delgado, Alejandra Maria



The hypergeometric functions and their confluent forms  

E-Print Network (OSTI)

of an Ordinary Point Z. I'he, latur&: of the Solution in t&uo . leighborhoou of a Singularity l:uci&s' Conditions 4. The Solution for l. urge Values of S. Totally pvc&hs& nn &:, quot io?s 6. The Analytic Continuation of &F'1(a, b;c;z) 7. The Confluent..., + + ~ +, 0 I z who tficr cO?v&. r cnt or?&! t ~ I S Saiu tO asyr ptotical ly I'c&' rc&&0?t I j&c f u?ct iun f ( z) in I j!o . Cctor 8 I wrzt to:1 8 = 02 ~ f(z) J + + + ~ ' l if' f j&r every fixe&1 positive intej&ral ? li&: z (t(z) - (a...

Doyle, Jack Ellsworth



The osteology of Bufo woodhousi, with comparison to Bufo terrestris  

E-Print Network (OSTI)

. UP FikTR'VQXt ~ Oa ~ 4'is' ~ 1 ~ 4 ~ ~ aa 4 ~ ' ~te isa:4 44 , 68 gPVjMATXO GP PXAL' XXa ~ ~ ~ ~ i ~ ~ ~ ~ aa ~ eie ~ ~ 44 ~ 4 ~ o' ~ 411 ~ 1st 'PO KK4'aTZQH 'QP. , PCS X 4 ~ ~ 4 4 ~ 4 a ~ ' ~ 4 4 4 ~ i 4 4' s ~ ~ 1 ~ i1 ta'4 14 4 4 i ~ ' AT/N 4j.... gg~ (p1. 76) ss coaaeoteg frees Sage+, ets eke ~ieger, . (M9lL) ~bo chs onLy Qx~icm ~ bo %ho snthox ef Vis, -~ of ~o ~lie - +~g cacI~~~g-. ~ ~ ) (p1. ZQ~ ~. gQ- sng 43). ? ciai?sy ~ Qo g~ge ~ontancv (~ en@ %OX) offices ~e, ~csea of the ~an ana...

Baldauf, Richard John



Genome sequence of the moderately thermophilic halophile Flexistipes sinusarabici strain (MAS10T)  

SciTech Connect

Flexistipes sinusarabici Fiala et al. 2000 is the type species of the genus Flexistipes in the fami- ly Deferribacteraceae. The species is of interest because of its isolated phylogenetic location in a genomically under-characterized region of the tree of life, and because of its origin from a multiply extreme environment; the Atlantis Deep brines of the Red Sea, where it had to struggle with high temperatures, high salinity, and a high concentrations of heavy metals. This is the fourth completed genome sequence to be published of a type strain of the family Deferribacteraceae. The 2,526,590 bp long genome with its 2,346 protein-coding and 53 RNA genes is a part of the Genomic Encyclopedia of Bacteria and Archaea project.

Lapidus, Alla L. [U.S. Department of Energy, Joint Genome Institute; Chertkov, Olga [Los Alamos National Laboratory (LANL); Nolan, Matt [U.S. Department of Energy, Joint Genome Institute; Lucas, Susan [U.S. Department of Energy, Joint Genome Institute; Hammon, Nancy [U.S. Department of Energy, Joint Genome Institute; Deshpande, Shweta [U.S. Department of Energy, Joint Genome Institute; Cheng, Jan-Fang [U.S. Department of Energy, Joint Genome Institute; Tapia, Roxanne [Los Alamos National Laboratory (LANL); Han, Cliff [Los Alamos National Laboratory (LANL); Goodwin, Lynne A. [Los Alamos National Laboratory (LANL); Pitluck, Sam [U.S. Department of Energy, Joint Genome Institute; Liolios, Konstantinos [U.S. Department of Energy, Joint Genome Institute; Pagani, Ioanna [U.S. Department of Energy, Joint Genome Institute; Ivanova, N [U.S. Department of Energy, Joint Genome Institute; Huntemann, Marcel [U.S. Department of Energy, Joint Genome Institute; Mavromatis, K [U.S. Department of Energy, Joint Genome Institute; Mikhailova, Natalia [U.S. Department of Energy, Joint Genome Institute; Pati, Amrita [U.S. Department of Energy, Joint Genome Institute; Chen, Amy [U.S. Department of Energy, Joint Genome Institute; Palaniappan, Krishna [U.S. Department of Energy, Joint Genome Institute; Land, Miriam L [ORNL; Hauser, Loren John [ORNL; Brambilla, Evelyne-Marie [DSMZ - German Collection of Microorganisms and Cell Cultures GmbH, Braunschweig, Germany; Rohde, Manfred [HZI - Helmholtz Centre for Infection Research, Braunschweig, Germany; Abt, Birte [DSMZ - German Collection of Microorganisms and Cell Cultures GmbH, Braunschweig, Germany; Spring, Stefan [DSMZ - German Collection of Microorganisms and Cell Cultures GmbH, Braunschweig, Germany; Goker, Markus [DSMZ - German Collection of Microorganisms and Cell Cultures GmbH, Braunschweig, Germany; Bristow, James [U.S. Department of Energy, Joint Genome Institute; Eisen, Jonathan [U.S. Department of Energy, Joint Genome Institute; Markowitz, Victor [U.S. Department of Energy, Joint Genome Institute; Hugenholtz, Philip [U.S. Department of Energy, Joint Genome Institute; Kyrpides, Nikos C [U.S. Department of Energy, Joint Genome Institute; Klenk, Hans-Peter [DSMZ - German Collection of Microorganisms and Cell Cultures GmbH, Braunschweig, Germany; Woyke, Tanja [U.S. Department of Energy, Joint Genome Institute



Some effects of magnetic blowouts on arc interruption  

E-Print Network (OSTI)

z;i 2Lv +2r' - 2L' 8 LS 8 2L -2Lx +2r -2L (L-x)y~Pr' sin L -rs rL -rx ree, ~. O. ~ A 3'e'er Inte, : e' e lal and 18), Gi nn a~-'. Co. , Du' ten. EVALUATION OF SECOND INTEGRAL -x a ~r-z (H+zx+Ex ) J = -(25L+Y) K=M If the tri... . 390 . 320 1. 550 . '710 . 570 . l. )20 -350 1290 ~ 1340 7e, 612 65 I 4. 92 336 i 362 276 3o 2 5t APPENDIX II EVALUATION OF INTEGRALS EVALUATION OF FIRST INTEGRAL = L -2Lv +v where a ~ r -L v s. +bv +cv Iv I. dv 1 sin -2v 42L L sin...

Benish, Joe



Net energy for production of feed mixtures containing various levels of cottonseed hulls and coastal bermudagrass hay  

E-Print Network (OSTI)

!'er 16&]966) I3zeT(s'1! 2d I' f. lect r I !, cve1 o Cotto'i. ee ' Hu]! I r v!1s on Dai ly Yr'crl In I ai:u (d!i . 13 t o 0c tone 10 & 19r&6) Br. e&r le, Te;ras ?5 fir:eac ariel Cl aclraLic Ile irr . sion for id!e Ef tc;!ts of travel of li &ur&hage re...!ci sc o&1s 'or tji. 6 f -;!! s of (oas! r!I Be& ai!d; . ass Bay I rvel or! Inc. gy 6 . i! Cos Treat&!, ent Gi oiips (du e 13 ? Ceto! er . ' 6. 1966 ? Ber v' i Le) . B5 IC! I&i!se!r e&nr! Clued&cetic Renre. , sions fo" tlie Eff acts of Cot& t...

Mark, William Howard



Operational factorization of the linear second-order differential equation with variable coefficients  

E-Print Network (OSTI)

" ? ' + 2 2 3 x x x The expansion of Equation (I-4) is as follows. (. D + f (x) ] R) + g (x) j y = [ D + f (x) 3 L y' t g (x) y ) = D I. y ' + g (x) y J + f (x) Ly ' + g (x) y) = y" +g(x) y' + g'(x) y + f(x) y' + f (x) g (x) y . Collecting terms, we... terms gives (a + 4a) x + (2a+4b) x + (b ? a) = -4x 2 2 2 2 Therefore, a = -2, b = + J2 i, where i = J-l, and our solution is either g=-Zx+ jci or g = -2x - J 2i Note that the particular solutions in the above example are complex. The equation has...

Austin, Larry Morton



Diffuse Neutrino Intensity from the Inner Jets of Active Galactic Nuclei: Impacts of External Photon Fields and the Blazar Sequence  

E-Print Network (OSTI)

We study high-energy neutrino production in the inner jets of radio-loud active galactic nuclei (AGN), taking into account effects of external photon fields and the blazar sequence. We show that the resulting diffuse neutrino intensity is dominated by quasar-hosted blazars, in particular, flat spectrum radio quasars, and that PeV neutrino production due to photohadronic interactions with broadline radiation is unavoidable if the inner jets of blazars are cosmic-ray sources. The resulting neutrino spectrum has a cutoff feature around PeV energies since the main target photons are Ly$\\alpha$ emission. Because of infrared photons provided by the dust torus, neutrino spectra above PeV energies are too hard to be consistent with the IceCube data unless the proton spectral index is steeper than 2.5, or the maximum proton energy is $\\lesssim100$ PeV. Thus, although the cumulative background can be as high as $E_\

Murase, Kohta; Dermer, Charles D



Geology of the Pontotoc North-Northwest area San Saba County, Texas  

E-Print Network (OSTI)

zo 'Ogg'Ot", eg By sqdeg~otld etlS yo ayevs aqua, 6uyddsm tran pyB uz so pesn mes gyp' 'gp xeq6aaog pa~ap 8y-H88 B&g&&s po 908 GGT Pue 89-H88 Se'F&es ? 001 K6 pu- '9L 89 'l'Y 9 stlde&6O&+M ~ d". m ayboyoa6 ycuts e'. l ea&emT ~ pass. oBTB OSCst...i) a6pfxa pun 'sauxea 'pnoXO ~q (TX6T)?fed 9o uoygeezog ufegunog dey yeuy6yxo a~ uzoxg pauygapax semi Cpu&N 0%8*-FI II QV li N X 9 BIIZ 'uu7%$ usg 6 xacgi18'g Quogsalufg u'f Qgunog der 'uoT6ax ouegg -oxd pue sxagy~~ e poo6 Exalt axe spues Ezoqo...

Chauvin, Aaron Lawrence



BioDoser: Improved dose-estimation software for biological radiation dosimetry  

Science Journals Connector (OSTI)

This paper introduces a software program that was developed with the aims to improve the efficiency and veracity of calibration curve fitting and data processing in radiation biological dosimetry and other biological experiments, and which is termed BioDoser. BioDoser uses least squares and loop testing of monotonicity method and algorithm of non-uniformed confidence interval. In addition, this program enables integration of multiple different biomarkers typically used in biological dosimetry. These include partial body exposure, minimum number of cells to be analyzed, G function correction modules that are helpful in dose estimation when using chromosome aberration frequencies, micronucleus rate, comet assay and other biological methods. The software is freely available at http://bit.ly/kKBSNR.

Hong Wang; Qiang Liu; Dandan Wan; Jian Xiang; Liqing Du; Yan Wang; Jia Cao; Yue Fu; Feiyue Fan; Markus Hecker



The World of Dark Shadows Issue 6  

E-Print Network (OSTI)

it to t!w f.!mall screen. Th~ showing was '-1&:16 at 10:30 PM NST. Il'ho I)~ly qU0s";ion is, what took so long? ' It ·is thu rare movie that J1l!:sn't shown up on TV within three yellrs ot baving been made. ' . Evl>3 :t;i.rst TV Bhowin~ was plaguod... the commercial. The beginniors 01: t~w SC(;tDfJ whore Carolyn wns stakad ",as shoWl'l, but not the end. Cut ::lso ~10ra scenes from tdvery death following that - Julia Hoftmun, E~.::':)t ;Jtokes, Bogar Collins - as well a.part of the transtoroatic,j,'l of Bv...

Multiple Contributors




SciTech Connect

Although the baryons in the intergalactic medium (IGM) trace dark matter fluctuations on megaparsec scales, on smaller scales ?100 kpc, fluctuations are suppressed because the finite temperature gas is pressure supported against gravity, analogous to the classical Jeans argument. This Jeans filtering scale, which quantifies the small-scale structure of the IGM, has fundamental cosmological implications. First, it provides a thermal record of heat injected by ultraviolet photons during cosmic reionization events, and thus constrains the thermal and reionization history of the universe. Second, the Jeans scale determines the clumpiness of the IGM, a critical ingredient in models of cosmic reionization. Third, it sets the minimum mass scale for gravitational collapse from the IGM, and hence plays a pivotal role in galaxy formation. Unfortunately, it is extremely challenging to measure the Jeans scale via the standard technique of analyzing purely longitudinal Ly? forest spectra, because the thermal Doppler broadening of absorption lines along the line-of-sight, is highly degenerate with Jeans smoothing. In this work, we show that the Jeans filtering scale can be directly measured by characterizing the coherence of correlated Ly? forest absorption in close quasar pairs, with separations small enough ?100 kpc to resolve it. We present a novel technique for this purpose, based on the probability density function (PDF) of phase angle differences of homologous longitudinal Fourier modes in close quasar pair spectra. A Bayesian formalism is introduced based on the phase angle PDF, and Markov Chain Monte Carlo techniques are used to characterize the precision of a hypothetical Jeans scale measurement, and explore degeneracies with other thermal parameters governing the IGM. A semi-analytical model of the Ly? forest is used to generate a large grid (500) of thermal models from a dark matter only simulation. Our full parameter study indicates that a realistic sample of only 20 close quasar pair spectra can pinpoint the Jeans scale to ? 5% precision, independent of the amplitude T{sub 0} and slope ? of the temperature-density relation of the IGM T=T{sub 0}(?/ ?-bar ){sup ?-1}. This exquisite sensitivity arises because even long-wavelength one-dimensional Fourier modes ?10 Mpc, i.e., two orders of magnitude larger than the Jeans scale, are nevertheless dominated by projected small-scale three-dimensional (3D) power. Hence phase angle differences between all modes of quasar pair spectra actually probe the shape of the 3D power spectrum on scales comparable to the pair separation. We show that this new method for measuring the Jeans scale is unbiased and is insensitive to a battery of systematics that typically plague Ly? forest measurements, such as continuum fitting errors, imprecise knowledge of the noise level and/or spectral resolution, and metal-line absorption.

Rorai, Alberto; Hennawi, Joseph F. [Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg (Germany); White, Martin [Department of Astronomy, University of California at Berkeley, 601 Campbell Hall, Berkeley, CA 94720-3411 (United States)



Opacity and gradients in aluminum wire array z-pinch implosions on the Z pulsed power facility  

SciTech Connect

Aluminum wire array z pinches imploded on the Z generator are an extremely bright source of 1–2?keV radiation, with close to 400?kJ radiated at photon energies >1?keV and more than 50?kJ radiated in a single line (Al Ly-?). Opacity plays a critical role in the dynamics and K-shell radiation efficiency of these pinches. Where significant structure is present in the stagnated pinch this acts to reduce the effective opacity of the system as demonstrated by direct analysis of spectra. Analysis of time-integrated broadband spectra (0.8–25?keV) indicates electron temperatures ranging from a few 100?eV to a few keV are present, indicative of substantial temperature gradients.

Ampleford, D. J., E-mail: damplef@sandia.gov; Hansen, S. B.; Jennings, C. A.; Jones, B.; Coverdale, C. A.; Harvey-Thompson, A. J.; Rochau, G. A.; Dunham, G.; Moore, N. W.; Harding, E. C.; Cuneo, M. E. [Sandia National Laboratories, Albuquerque, New Mexico 87185 (United States)] [Sandia National Laboratories, Albuquerque, New Mexico 87185 (United States); Chong, Y.-K.; Clark, R. W.; Ouart, N.; Thornhill, J. W.; Giuliani, J.; Apruzese, J. P. [Naval Research Laboratory, Washington, DC 20375 (United States)] [Naval Research Laboratory, Washington, DC 20375 (United States)



FHBS calculation of ionized electron angular and energy distribution following the p+H collision at 20 keV  

E-Print Network (OSTI)

the following Schr? equa- tion ( D2 1r ) c(r) = E c(r): (2.6) The solution to the 1s ground state wave function is j0 >= 2e r Y0;0: (2.7) 11 There are two solutions for a scattering state with momentum k, namely c(+)k (r) = ep=2kG(1 i=k)e ik rF(i=k;1;ikr +ik r... l0 and m0 in Eq. (2.38), thus = ?? l=0 Z ? 0 Cl rl eikr F(l +1+in;2l +2; 2ikr) il(2l +1) jl(Qr) ( 1)l 2e r p4p r2dr( 1)l (4p) 2 (2l +1)2 ?m= lY lm(Q)Ylm(k): (2.42) De ne integral Il(k;Q) = Z ? 0 rl eikr F(l +1+in...

Fu, Jun



Plasma-wall interaction studies with optimized laser-produced jets  

SciTech Connect

The production of the laser-produced plasma jets at burnt-through low-Z foils was optimized by using three-frame interferometry. When striking secondary targets, these jets of energetic particles represent an efficient tool for the investigation of transient phenomena at surfaces of the plasma-exposed solids. Two sets of precisely measured x-ray spectroscopic data demonstrate diagnostic potential of the collimated jets in the plasma-wall interaction studies: Blue Doppler shifts of the Al jet self-emission visualize ion deceleration in the near-wall region. Local depressions found in Al Ly{gamma} profiles emitted from Al/Si(PMMA) targets indicate charge exchange between the Al XIII and fully stripped C ions.

Renner, O.; Krousky, E.; Smid, M. [Institute of Physics ASCR, 18221 Prague (Czech Republic); Pisarczyk, T.; Chodukowski, T.; Kalinowska, Z. [Institute of Plasma Physics and Laser Microfusion, 01-497 Warsaw (Poland); Pisarczyk, P. [Warsaw University of Technology, ICS, 00-665 Warsaw (Poland); Ullschmied, J. [Institute of Plasma Physics ASCR, 18200 Prague 8 (Czech Republic); Dalimier, E. [Sorbonne Universites, Pierre et Marie Curie, UMR 7605, LULI, 75252 Paris (France)



A study of factors affecting seed set in the hermaphroditic cucumber, Cucumis sativus L.  

E-Print Network (OSTI)

! a(ion (P) indical cd by seed-set Cfroct of !he year (Y) on seed yi&ld from po)lination methods (P) pollinated at. "(a) T ; (ni T2, and (c) r, . 29 Comparison ot number of fruit sot from polli. -. ations 'I I th da. !time high 'temper ture 'ny... in obtaining good scud yiel-. is fro!n horm. phrcdltos ~ Han. i ool. linations often a!crt cr coc!i?in few ", eels. ir'-" I: mili. often sc':!1 thout pol. . i!!ilia'll b!i. usu ' . ly co!1, '1 In no gcod s -aci Several fact. rs merit con" ic!aration as uossl...

Biegert, Carolyn Mae


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they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


Availability of Nitrous Nitrogen to Plants.  

E-Print Network (OSTI)

V, .=DL ULL LI~C a~ailability 01 ILILKLL~: IIILIU~~I~ LU curn, l~aa, 8011 31LY3 1 27.3 .53 .I447 1 I 1 5: 1250 .I349 ic nitrogen ( 37.P' 1 -59 1 .2195 ru.. nv / 36.6 .57 1 .2086 I -2141 1 .O7b/ I 1. gm. nitrous nitrogen 30.2 1 .64 1 .I933 1... .12 -.01 ' .09 V1 -- I w 01 ---- I ------ el M - 1 --O6 X * ---- ------ U1 $ !z - --- i d $ --- - I -20 2 Y * F - I M 4 M .34 I --- .20 M .14 5 nitrogen --- --- -.02 .14 -.48 -.01 -12 .18 .OS...

Fraps, G. S. (George Stronach); Sterges, A. J.



The World of Dark Shadows Issue 31  

E-Print Network (OSTI)

The World 01 llltfiK ~llltDaW~ 31 ~. 1 ~ I ­ ~ I ..\\ I I •~ J \\ .. ~ ! 1(18" !! ~ \\ 1 \\ U ;: 0 ~ I ' c " o'q~~\\ '0 l ~~ ", 9 I I r I - I ~ ( -;,­ ~l~ ~ . I ( ~"'"VW" " ) J!. d,.", .'\\ _C]~I ~ ~ ~ /';".!.t ~0-. THE WORLD OF DARK.... * JONATHAN FRID Address; SHAOOIICON 5I X - JULY 3, 1982 Transcription by Mar ia Barbosa Th e co nve,\\t.i.on 6Jm-lLoom L<.IU 6.dted t o c.a.pa.c.i.ty . Th e. Ilwn 06 the 6aM eon­ veJt,~.i.n9 ely l...ah each othM .i.6 6.liente.d a.6 tile doubt...

Multiple Contributors



Offstage Enterprise  

E-Print Network (OSTI)

S impossible not to fee:L ' J;~spect for the astonishing power gi't,h?!,y J';'emote alien mind. . ...... . , ."?~ce:Pt :perhaps foI' ,Mp.rie'f ' who ?.s9E:)med ::l;D..Glined to belieiTs' that demands fi-:or(Mr spopk were de,sJ.glle~ ?solE?:LY? ;f,o m~k\\3...:.:all, these: che9k-s. ",e.1 :r.;:erm:ming there ~ s jw~t;-tP.8 time ... -:: It f d be different if he was hqma...'1 ar..d prepared to accept that you can t t do eleven things at once~ let alone l-rh~t yoy.' .re meant to be.?l.oing; and it's SO hot in here...

David, Glen



A survey of selected aspects of health conditions and services in Texas, 1948  

E-Print Network (OSTI)

5. 98 Aa'chez' . ' 48 S, VSV V. QV hxsstxeng ' 18 -' ' 2, 298 8. 18 Ataseosm 181 29, 618 9. 94 Austtn 149 14, 631 19. 18 ssk'key V, QVS 8. 89 Qendex a 62 4, 384 14. 14 sastxoy 238 19, 561 12. 21 Qaylox 48 6~ 849 V. 15 Bee 215 1V, 91V 11.... 88 gloll, 491 V4, 1V2 6. 81 fhesex' 4, 43V 488, 959 8. 94 Slsneo ' 2V 8 J VV 1 V, 16 Sordlen ly199 . QQ Bosque 182 11 pV82 11. 29 BO44e 4M~ 81, VVV 6. 96 Bxesoa'lo 2QV 46, 382 8. 49 BF @sos 393 38, 284 V. SS Mewstex VQ V, 2VS 9. 61 Bx...

Haynes, Lemuel Lee



Partial Statement of Social Ethics for High Schools  

E-Print Network (OSTI)

to go in t h i s book. Another volume could we l l be wri t ten , po int ing out the agreements and d i s ­ agreements o f our present moral standards with C h r i s t i a n i t y . There i s much in what Socrates sa id , that most s i n s are caused... f requent ly pro tec t the physic ian. There are many complaints that are incurab le , and a l l that can be done i s to make the su f ferer comfort ­ a b l e . In case of cancer , the sore may be dressed and kept c l ean , and a pleasant p lace...

Wilson, Matthew Hale



UV pumping of hyperfine transitions in the light elements, with application to 21-cm hydrogen and 92-cm deuterium lines from the early universe  

E-Print Network (OSTI)

We present new analytic calculations of the coupling between ultraviolet resonance photons and the population of the hyperfine states in the light elements (H, D, He3+) which include several previously neglected physical processes. Among these are the backreaction of resonant scattering on the pumping radiation, the scattering of Ly_beta photons and the effect of local departure from pure Hubble flow. The application of the new treatment to the redshifted hydrogen 21 and deuterium 92 cm lines from the high-redshift universe results in an amplitude correction of up to an order of magnitude. We further show that the standard assumption that ultraviolet pumping drives the spin temperature towards the kinetic temperature does not hold for deuterium, whose spin temperature is generally negative.

Leonid Chuzhoy; Paul R. Shapiro



Laser heating of solid matter by light pressure-driven shocks  

SciTech Connect

Heating by irradiation of a solid surface in vacuum with 5 x 10{sup 20} W cm{sup -2}, 0.8 ps, 1.05 {micro}m wavelength laser light is studied by x-ray spectroscopy of the K-shell emission from thin layers of Ni, Mo and V. A surface layer is heated to {approx} 5 keV with an axial temperature gradient of 0.6 {micro}m scale length. Images of Ni Ly{sub {alpha}} show the hot region has a {approx} 25 {micro}m diameter, much smaller than {approx} 70 {micro}m region of K{sub {alpha}} emission. 2D particle-in-cell (PIC) simulations suggest that the surface heating is due to a light pressure driven shock.

Akli, K; Hansen, S B; Kemp, A J; Freeman, R R; Beg, F N; Clark, D; Chen, S; Hey, D; Highbarger, K; Giraldez, E; Green, J; Gregori, G; Lancaster, K; Ma, T; MacKinnon, A J; Norreys, P A; Patel, N; Patel, P; Shearer, C; Stephens, R B; Stoeckl, C; Storm, M; Theobald, W; Van Woerkom, L; Weber, R; Key, M H




NLE Websites -- All DOE Office Websites (Extended Search)

66 results: 66 results: BibTex RIS RTF XML Sort by: Author Title Type [ Year (Desc) ] Filters: Author is Craig P. Wray [Clear All Filters] 2013 Rapp, Vi H., Albert Pastor-Perez, Brett C. Singer, and Craig P. Wray. Predicting Backdrafting and Spillage for Natural-Draft Gas Combustion Appliances: Validating VENT-II., 2013. Ban-Weiss, George, Craig P. Wray, William W. Delp, Peter Ly, Hashem Akbari, and Ronnen M. Levinson. "Electricity production and cooling energy savings from installation of a building-integrated photovoltaic roof on an office building." Energy and Buildings 56 (2013): 210-220. J. Chris Stratton, and Craig P. Wray. Procedures and Standards for Residential Ventilation System Commissioning: An Annotated Bibliography., 2013. 2012 J. Chris Stratton, William J. N. Turner, Craig P. Wray, and Iain S. Walker.



Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

NEPACOMPUANCESURVEY NEPACOMPUANCESURVEY Project lnfonnatlon Project Title: Geothermal Technologies Program Date: 7/26/10 DOE Code: 6730.020.61041 Contractor Code: 8067-447 Project Lead: Ly1e Johnson Project Overview The work to be done is the installation of a sump in Little Teapot Creek from which water for the cooling loop 1. Brief project description pnclude anything that could impact the at the ~F can be withdrawn. The work will consis of burying a section of 8 foot diameter galvanized steel environment] culvert in the creek to produce a sump for the suction of a pump. The culvert will be set vertically to the bed rock or to a maximum depth of 8 fee~ which ever is less. The permit for withdrawal of the water has already 2. Legal location been received



Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

DATE: DATE: May 21,2008 SUBJECT: Fonnat of Petition for Advance Waiver of Patent Rights The attached document sets forth the fonnat to be used by field patent counsel for a Petition for an Advance Waiver of Patent Rights under 10 CFR 784. ~ Ja ' ,. ~ " " j ", .., lY CQ i -.-- Paul A GotiIi b Assistant General Counsel for Technology Transfer and Intellectual Property 1 * Printed with soy ink on recycled paper UNITED STATES DEPARTMENT OF ENERGY PETITION FOR ADVANCE WAIVER OF PATENT RIGHTS UNDER 10 C.F.R. PART 784 DOE WAIVER NO. (To be supplied by DOE) Notice: If you need help in completin9..1hisform. contact t~atent Counsel assisting the activity that is issuing your award or the Assistant General Counsel for Technology Transfer and Intellectual Property in the Office of General Counsel in DOE Headauarters. Visit: www.gc.energy.gov/documents/lntellectual Property (IP) Service



SciTech Connect

The effect of environment on the circumgalactic medium (CGM) is investigated through a comparison of Ly{alpha} absorption line data in the Virgo Cluster and the field. This Letter uses the first systematic survey of background QSOs in and around the Virgo Cluster and large existing surveys of galaxies at low redshift. While previous studies found denser gas (higher equivalent width) closer to a galaxy (lower impact parameter), this correlation disappears in the Virgo environment. In addition, the covering fraction of the CGM is lower in the cluster environment than in the circumcluster environment and field. The results indicate that the CGM is suppressed for cluster galaxies while galaxies in the circumcluster environment have abundant CGM. The truncation of the CGM may result in the quenching of star formation through starvation. Our results also show that CGM surveys must consider the role of environment.

Yoon, Joo Heon; Putman, Mary E., E-mail: jhyoon@astro.columbia.edu [Department of Astronomy, Columbia University, New York, NY 10027 (United States)



One Among You  

E-Print Network (OSTI)

. and stepped out into the co ?? ido.s of the Ente.p.ise. Within the week, the Ente.p.ise ente.ed Quad.ant No.th. The new secu.ity ensign had settled into ship .outine well enough. Secu.ity chief D'Lo ?? aine La.zen had appa.ently found a kind.ed spi.... The newlyweds, Yo-Ma 2ito and Elizabeth 2ito Cfo!"me!"ly McC!"aggins) st!"olled hand in hand th!"ough the co!"!"ido!"s of the Ente!"p!"ise, giggling like kids and mu!"mu!"ing sweet nothings into each othe!"'s ea!"s. "Can't you two find some place bette!" foro...

Alain, Alinda



A determination of the heats of combustion of the five-carbon fatty acids and their methyl and ethyl esters  

E-Print Network (OSTI)

'srr Ins~ Ce?c ~c Dl? 30? Tbe bstwLs sodAL 1Need wss ohtwixlsd frccc ths Q?S? Wool? Bar? of ghsnclalPds? Tbs hest ef ~tdocc wss giwRl se g6?QQ shs? kja/g? cocos (weighed in wceccs) er QLg eaL/g? essa (in @sees)? 3 oslorie? 0?wg$840 sbs, +? 'ei ~ r...LLd bs ~aied fer tbs fi~carhc?L aCCLds?ad the baste of vaoorisat4os of tbs ether Lsaee4e ac@de ae4hsated a4 their ~g, xdn4s The bs?te of vsyorhwQ. oe o' ths sands a4 2~ C? wars estiaated ly a?S~ 4R? k", ~? ~4lcsi55, ccsd '~ ~ . -? AIL' %7? Q? ~ +sad...

Gilby, Ralph F



The acoustic environment of a Gulf Stream cyclonic ring  

E-Print Network (OSTI)

). The SS curves have a normal succession of strong convergence and shadow zones that are usually present for a near-surface source in deep water. In the near field, transmission loss reaches 88 db at a distance of 5 km from the source and decreases 8..., and the receiver is at 260 m. 70 go cn /Oo C) I I I I I I I I I ll I ly II I J i I G CQ ~ //o /30 2O m qO SO CO 7G '80 PG /GG //G /A /JG R'0 /Sd /2 //G /ZG DI STili', CE (km} 57 Fig. 18 Transmission loss versus range for sound...

Owens, George Edward



Deep imaging of Q2112+059: A bright host galaxy but no DLA absorber  

E-Print Network (OSTI)

In a ongoing programme aimed at studying galaxy counterparts of Damped Ly-alpha Absorbers (DLAs) we have obtained high resolution deep I-band imaging data of the field around the z_em = 0.457 BAL QSO Q2112+059. In the literature this QSO is listed to have a candidate DLA at z_abs = 0.2039 along the line of sight. After subtraction of the QSO Point Spread Function (PSF) we detect a galaxy centred on the position of Q2112+059. To help answer whether this galaxy is the DLA or the QSO host galaxy we retrieved a GHRS spectrum of Q2112+059 from the HST-archive. This spectrum shows that there is no Ly-alpha absorption line at z_abs = 0.2039. This fact in combination with the perfect alignment on the sky of the galaxy and Q2112+059 lead us to the conclusion that the galaxy must be the host galaxy of Q2112+059. The host galaxy of Q2112+059 is bright (M_I^obs = -23.6), and has a radial profile well fitted by a {\\it modified Hubble + de Vaucouleurs} profile with R_c = 0.5 kpc and R_e = 3.6 kpc. Our results are well in line with the conclusion of earlier work done at lower redshifts, that bright low redshift QSOs preferentially reside in luminous, elliptical galaxies. The host of Q2112+059 is however, despite it's brightness, very compact when compared to early type galaxies at lower redshifts.

J. U. Fynbo; P. Moller; B. Thomsen



Active Galactic Nuclei in the CNOC2 Field Galaxy Redshift Survey  

E-Print Network (OSTI)

We present a sample of 47 confirmed and 14 candidate Active Galactic Nuclei (AGN) discovered in the Canadian Network for Observational Cosmology field galaxy redshift survey (CNOC2). The sample consists of 38 objects identified from broad emission lines, 8 from narrow [NeV] emission, and 15 candidates from FeII or MgII absorption lines, one of which has been confirmed as a broad-line AGN via infrared spectroscopy. Redshifts of these AGN range from z=0.27 to z=4.67, and the average absolute magnitude is M_B=-22.25. No color selection criteria were involved in selecting this spectroscopically discovered sample. The sample is also unbiased against objects with luminous host galaxies since the spectroscopy preferentially targeted extended objects. Simple color-color diagram selection criteria can recover 81+-6% of the CNOC2 AGN, but several of the most unusual objects would be missing from such a color-selected sample. In the subsample with broad emission lines, the average equivalent widths for MgII and CIII] agree with the predictions of previous studies of the Baldwin effect. However, the average equivalent widths for CIV and Ly-alpha are smaller than predicted by previous studies of the Baldwin effect at lower redshift. This may imply that the slopes of the CIV and Ly-alpha Baldwin effects evolve with redshift, steepening with cosmic time. The broad emission line AGN also show a higher incidence of associated MgII and CIV absorption than in most previous surveys. This may arise from strong absorption being anti-correlated with optical luminosity or becoming less frequent with cosmic time, or possibly because our selection method is not biased against objects with resolved spatial structure or reddened by dust associated with the absorbing gas. (Abridged)

Patrick B. Hall; H. K. C. Yee; Huan Lin; Simon L. Morris; David R. Patton; Marcin Sawicki; Charles W. Shepherd; Gregory D. Wirth; R. G. Carlberg; Richard Elston



Thermal Fatigue of Polycrystalline Copper in CLIC Accelerating Structures: Surface Roughening and Hardening as a Function of Grain Orientation  

E-Print Network (OSTI)

The ac­cel­er­at­ing struc­tures of CLIC will be sub­mit­ted to 2 x 1010 ther­mal-me­chan­i­cal fa­tigue cy­cles, aris­ing from Radio Fre­quen­cy (RF) in­duced eddy cur­rents, caus­ing local su­per­fi­cial cyclic heat­ing. In order to as­sess the ef­fects of su­per­fi­cial fa­tigue, high tem­per­a­ture an­nealed OFE Cop­per sam­ples were ther­mal­ly fa­tigued with the help of pulsed laser ir­ra­di­a­tion. They un­der­went post­mortem Elec­tron Backscat­tered Diffrac­tion (EBSD) mea­sure­ments and?hard­ness ob­ser­va­tions. Pre­vi­ous work has con­firmed that sur­face rough­en­ing de­pends on the ori­en­ta­tion of near-sur­face grains*,**. It is clear­ly ob­served that, through ther­mal cy­cling, the in­crease of hard­ness of a crys­tal­lo­graph­ic di­rec­tion is re­lat­ed to the amount of sur­face rough­en­ing in­duced by fa­tigue. Near-sur­face grains, ori­ent­ed [1 0 0] with re­spect to the sur­face, ex­hibit­ing ver...

Aicheler, M



Constraints on (Omega_m,Omega_Lambda) using distributions of inclination angles for high redshift filaments  

E-Print Network (OSTI)

In this paper we present a scale free method to determine the cosmological parameters (Omega_m, Omega_Lambda). The method is based on the requirement of isotropy of the distribution of orientations of cosmological filaments. The current structure formation paradigm predicts that the first structures to form are voids and filaments, causing a web-like structure of the matter distribution at high redshifts. Recent observational evidence suggests that the threads, or filaments, of the cosmic web most easily are mapped in Ly-alpha emission. We describe how such a 3D map can be used to constrain the cosmological parameters in a way which, contrary to most other cosmological tests, does not require the use of a standard rod or a standard candle. We perform detailed simulations in order to define the optimal survey parameters for the definition of an observing programme aimed to address this test, and to investigate how statistical and observational errors will influence the results. We conclude that observations should target filaments of comoving size 15-50 Mpc in the redshift range 2-4, and that each filament must be defined by at least four Ly-alpha emitters. Detection of 20 filaments will be sufficient to obtain a result, while 50 filaments will make it possible to place significant new constraints on the values of Omega_m and Omega_Lambda permitted by the current supernova observations. In a future paper we study how robust these conclusions are to systematic velocities in the survey box.

M. Weidinger; P. Moller; J. P. U. Fynbo; B. Thomsen; M. P. Egholm



Osseointegration of chitosan coated porous titanium alloy implant by reactive oxygen species-mediated activation of the PI3K/AKT pathway under diabetic conditions  

Science Journals Connector (OSTI)

Abstract Chitosan coated porous titanium alloy implant (CTI) is demonstrated a promising approach to improve osseointegration capacity of pure porous titanium alloy implant (TI). Since chitosan has been demonstrated to exhibit antioxidant activity, we propose CTI may ameliorate the ROS overproduction, thus reverse the poor osseointegration under diabetic conditions, and investigate the underlying mechanisms. Primary rat osteoblasts incubated on the TI and the CTI were subjected to normal serum (NS), diabetic serum (DS), DS + NAC (a potent ROS inhibitor) and DS + LY294002 (a PI3K/AKT-specific inhibitor). In vivo study was performed on diabetic sheep implanted with TI or CTI into the bone defects on crista iliaca. Results showed that diabetes-induced ROS overproduction led to osteoblast dysfunction and apoptosis, concomitant with the inhibition of AKT in osteoblasts on the TI substrate. While CTI stimulated AKT phosphorylation through ROS attenuation, thus reversed osteoblast dysfunction evidenced by improved osteoblast adhesion, increased proliferation and ALP activity, and decreased cytotoxicity and apoptotic rate, which exerted same effect to NAC treatment on the TI. These effects were further confirmed by the improved osseointegration within the CTI in vivo evidenced by Micro-CT and histological examinations. In addition, the aforementioned promotive effects afforded by CTI were abolished by blocking PI3K/AKT pathway with addition of LY294002. These results demonstrate that the chitosan coating markedly ameliorates diabetes-induced impaired bio-performance of TI via ROS-mediated reactivation of PI3K/AKT pathway, which elicits a new surface functionalization strategy for better clinical performance of titanium implant in diabetic patients.

Xiang Li; Xiang-Yu Ma; Ya-Fei Feng; Zhen-Sheng Ma; Jian Wang; Tian-Cheng Ma; Wei Qi; Wei Lei; Lin Wang



PC1643+4631A,B: The Lyman-Alpha Forest at the Edge of Coherence  

E-Print Network (OSTI)

This is the first measurement and detection of coherence in the intergalactic medium (IGM) at substantially high redshift (z~3.8) and on large physical scales (~2.5 h^-1 Mpc). We perform the measurement by presenting new observations from Keck LRIS of the high redshift quasar pair PC 1643+4631A, B and their Ly-alpha absorber coincidences. This experiment extends multiple sightline quasar absorber studies to higher redshift, higher opacity, larger transverse separation, and into a regime where coherence across the IGM becomes weak and difficult to detect. We fit 222 discrete Ly-alpha absorbers to sightline A and 211 to sightline B. Relative to a Monte Carlo pairing test (using symmetric, nearest neighbor matching) the data exhibit a 4sigma excess of pairs at low velocity splitting (coherence on transverse scales of ~2.5 h^-1 Mpc. We use spectra extracted from an SPH simulation to analyze symmetric pair matching, transmission distributions as a function of redshift and compute zero-lag cross-correlations to compare with the quasar pair data. The simulations agree with the data with the same strength (~4sigma) at similarly low velocity splitting above random chance pairings. In cross-correlation tests, the simulations agree when the mean flux (as a function of redshift) is assumed to follow the prescription given by Kirkman et al. (2005). While the detection of flux correlation (measured through coincident absorbers and cross-correlation amplitude) is only marginally significant, the agreement between data and simulations is encouraging for future work in which even better quality data will provide the best insight into the overarching structure of the IGM and its understanding as shown by SPH simulations.

Caitlin M. Casey; Christopher D. Impey; Catherine E. Petry; Andrew R. Marble; Romeel Dave


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SciTech Connect

We have used the Cosmic Origins Spectrograph (COS) to obtain far-UV spectra of three closely spaced QSO sight lines that probe the circumgalactic medium (CGM) of an edge-on spiral galaxy, ESO 157-49, at impact parameters of 74 and 93 h {sup -1} {sub 70} kpc near its major axis and 172 h {sup -1} {sub 70} kpc along its minor axis. H I Ly{alpha} absorption is detected at the galaxy redshift in the spectra of all three QSOs, and metal lines of Si III, Si IV, and C IV are detected along the two major-axis sight lines. Photoionization models of these clouds suggest metallicities close to the galaxy metallicity, cloud sizes of {approx}1 kpc, and gas masses of {approx}10{sup 4} M {sub Sun }. Given the high covering factor of these clouds, ESO 157-49 could harbor {approx}2 Multiplication-Sign 10{sup 9} M {sub Sun} of warm CGM gas. We detect no metals in the sight line that probes the galaxy along its minor axis, but gas at the galaxy metallicity would not have detectable metal absorption with ionization conditions similar to the major-axis clouds. The kinematics of the major-axis clouds favor these being portions of a 'galactic fountain' of recycled gas, while two of the three minor-axis clouds are constrained geometrically to be outflowing gas. In addition, one of our QSO sight lines probes a second more distant spiral, ESO 157-50, along its major axis at an impact parameter of 88 h {sup -1} {sub 70} kpc. Strong H I Ly{alpha} and C IV absorption only are detected in the QSO spectrum at the redshift of ESO 157-50.

Keeney, Brian A.; Stocke, John T.; Danforth, Charles W.; Shull, J. Michael; Green, James C. [Center for Astrophysics and Space Astronomy, Department of Astrophysical and Planetary Sciences, University of Colorado, 389 UCB, Boulder, CO 80309 (United States)] [Center for Astrophysics and Space Astronomy, Department of Astrophysical and Planetary Sciences, University of Colorado, 389 UCB, Boulder, CO 80309 (United States); Rosenberg, Jessica L. [Department of Physics and Astronomy, George Mason University, Fairfax, VA 22030 (United States)] [Department of Physics and Astronomy, George Mason University, Fairfax, VA 22030 (United States); Ryan-Weber, Emma V. [Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Mail H30, P.O. Box 218, Hawthorn, 3122 VIC (Australia)] [Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Mail H30, P.O. Box 218, Hawthorn, 3122 VIC (Australia); Savage, Blair D., E-mail: brian.keeney@colorado.edu [Department of Astronomy, University of Wisconsin-Madison, 5534 Sterling Hall, 475 North Charter Street, Madison, WI 53706 (United States)




SciTech Connect

We present a composite spectrum of 60 long duration gamma-ray burst (GRB) afterglows with redshifts in the range 0.35 < z < 6.7 observed with low-resolution optical spectra. The composite spectrum covers the wavelength range 700-6600 A in the rest frame and has a mean signal-to-noise ratio of 150 per 1 A pixel and reaches a maximum of {approx}300 in the range 2500-3500 A. Equivalent widths are measured from metal absorption lines from the Ly{alpha} line to {approx}5200 A, and associated metal and hydrogen lines are identified between the Lyman break and Ly{alpha} line. The average transmission within the Lyman forest is consistent with that found along quasar lines of sight. We find a temporal variation in fine-structure lines when dividing the sample into bursts observed within 2 hr from their trigger and those observed later. Other lines in the predominantly neutral gas show variations too, but this is most likely a random effect caused by weighting of individual strong absorption lines and which mimics a temporal variation. Bursts characterized with high- or low-prompt GRB energy release produce afterglows with similar absorption line strengths, and likewise for bursts with bright or faint optical afterglows. Bursts defined as dark from their optical to X-ray spectral index have stronger absorption lines relative to the optically bright bursts. The composite spectrum has strong Ca II and Mg II absorption lines as commonly found in dusty galaxies, however, we find no evidence for dust or a significant molecular content based on the non-detection of diffuse interstellar bands. Compared to starburst galaxy spectra, the GRB composite has much stronger fine-structure lines, while metal absorption lines are weaker.

Christensen, L. [Excellence Cluster Universe, Technische Universitaet Muenchen, Bolzmanstrasse 2, 85748 Garching (Germany); Fynbo, J. P. U. [Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 30, 2100 Copenhagen Oe (Denmark); Prochaska, J. X. [Department of Astronomy and Astrophysics, UCO/Lick Observatory, University of California, 1156 High Street, Santa Cruz, CA 95064 (United States); Thoene, C. C.; De Ugarte Postigo, A. [INAF - Osservatorio Astronomico di Brera, via E. Bianchi 46, 23807, Merate (Italy); Jakobsson, P., E-mail: lise.christensen@ph.tum.de [Centre for Astrophysics and Cosmology, Science Institute, University of Iceland, Dunhagi 5, IS-107 Reykjavik (Iceland)




SciTech Connect

In active galactic nucleus spectra, a series of Fe II multiplets form a pseudo-continuum that extends from the ultraviolet to the near-infrared (NIR). This emission is believed to originate in the broad-line region, and it has been known for a long time that pure photoionization fails to reproduce it in the most extreme cases, as does the collisional excitation alone. The most recent models by Sigut and Pradhan include details of the Fe II ion microphysics and cover a wide range in the ionization parameter log U{sub ion} = (- 3.0 {yields} -1.3) and density log n{sub H} = (9.6 {yields} 12.6). With the aid of such models and a spectral synthesis approach, we studied for the first time in detail the NIR emission of I Zw 1. The main goals were to confirm the role played by Ly{alpha} fluorescence mechanisms in the production of the Fe II spectrum and to construct the first semi-empirical NIR Fe II template that best represents this emission, consequently allowing its clean subtraction in other sources. A good overall match between the observed Fe II+Mg II features with those predicted by the best-fitted model was obtained, corroborating the Ly{alpha} fluorescence as a key process to understand the Fe II spectrum. The best model was fine-tuned by applying a deconvolution method to the observed Fe II+Mg II spectrum. This derived semi-empirical template was then fitted to the spectrum of Ark 564, showing that it nicely reproduced its observed Fe II+Mg II emission. Our work extends the current set of available Fe II templates into the NIR region.

Garcia-Rissmann, A.; Rodriguez-Ardila, A. [Laboratorio Nacional de Astrofisica, Rua Estados Unidos 154, 37504-364 Itajuba, MG (Brazil); Sigut, T. A. A. [University of Western Ontario, London, Ontario N6A 3K7 (Canada); Pradhan, A. K., E-mail: arissmann@lna.br [4055 McPherson Laboratory, Ohio State University, 140 W. 18th Ave., Columbus, OH 43210-1173 (United States)




SciTech Connect

Observations of very distant galaxies probe both the formation and evolution of galaxies, and also the nature of the sources responsible for reionizing the intergalactic medium (IGM). Here, we study the physical characteristics of galaxies at 6.3 < z {<=} 8.6, selected from deep near-infrared imaging with the Wide Field Camera 3 (WFC3) on board the Hubble Space Telescope. We investigate the rest-frame ultraviolet (UV) colors, stellar masses, ages, metallicities, and dust extinction of this galaxy sample. Accounting for the photometric scatter using simulations, galaxies at z{approx} 7 have bluer UV colors compared to typical local starburst galaxies at >4{sigma} confidence. Although the blue colors of galaxies at these redshifts necessitate young ages (<100 Myr), low or zero dust attenuation, and low metallicities, these are explicable by normal (albeit unreddened) stellar populations, with no evidence for near-zero metallicities and/or top-heavy initial mass functions. Most of these galaxies are undetected in deep Spitzer Infrared Array Camera imaging. However, the age of the universe at these redshifts limits the amount of stellar mass in late-type populations, and the WFC3 photometry implies galaxy stellar masses {approx}10{sup 8}-10{sup 9} M{sub sun} for Salpeter initial mass functions to a limiting magnitude of M{sub 1500} {approx} -18. The masses of 'characteristic' (L*) z > 7 galaxies are smaller than those of L* Lyman break galaxies at lower redshifts, and are comparable to less evolved galaxies selected on the basis of their Ly{alpha} emission at 3 < z < 6, implying that the 6.3 < z {<=} 8.6 galaxies are the progenitors of more evolved galaxies at lower redshifts. We estimate that Ly{alpha} emission is able to contribute to the observed WFC3 colors of galaxies at these redshifts, with an estimated typical line flux of {approx} 10{sup -18} erg s{sup -1} cm{sup -2}, roughly a factor of 4 below currently planned surveys. The integrated UV specific luminosity for the detected galaxies at z {approx} 7 and z {approx} 8 is within factors of a few of that required to reionize the IGM assuming low clumping factors, even with no correction for luminosity incompleteness. This implies that in order to reionize the universe, galaxies at these redshifts have a high ({approx}50%) escape fraction of Lyman continuum photons, possibly substantiated by the very blue colors of this population.

Finkelstein, Steven L.; Papovich, Casey [George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, Department of Physics and Astronomy, Texas A and M University, 4242 TAMU, College Station, TX 77843 (United States); Giavalisco, Mauro [University of Massachusetts, 710 North Pleasant Street, Amherst, MA 01003 (United States); Reddy, Naveen A.; Dickinson, Mark [National Optical Astronomy Observatory, 950 North Cherry Avenue, Tucson, AZ 85719 (United States); Ferguson, Henry C.; Koekemoer, Anton M., E-mail: stevenf@physics.tamu.ed [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States)



Cosmological parameters sigma_8, the baryon density, and the UV background intensity from a calibrated measurement of H I Lyman-alpha absorption at z = 1.9  

E-Print Network (OSTI)

We identify a concordant model for the intergalactic medium (IGM) at redshift z=1.9 that uses popular values for cosmological and astrophysical parameters and accounts for all baryons with an uncertainty of 6%. We have measured the amount of absorption, DA, in the Ly-alpha forest at redshift 1.9 in spectra of 77 QSO from the Kast spectrograph. We calibrated the continuum fits with realistic artificial spectra, and we found that averaged over all 77 QSOs the mean continuum level is within 1-2% of the correct value. Absorption from all lines in the Ly-alpha forest at z=1.9 removes DA=15.1 +/- 0.7% of the flux between 1070 and 1170 (rest) Angstroms. This is the first measurement using many QSOs at this z, and the first calibrated measurement at any redshift. Metal lines absorb 2.3 +/- 0.5%, and LLS absorb 1.0 +/- 0.4% leaving 11.8 +/- 1.0% from the lower density bulk of the IGM. Averaging over Delta z=0.1 or 154 Mpc, the dispersion is 6.1 +/- 0.3% including LLS and metal lines, or 3.9 (+0.5, -0.7)% for the lower density IGM alone, consistent with the usual description of large scale structure. LLS and metal lines are major contributors to the variation in the mean flux, and they make the flux field significantly non-Gaussian. We find that a hydrodynamic simulation on a 1024 cubed grid in a 75.7 Mpc box reproduces the observed DA from the low density IGM with parameters values H_o=71 km/s/Mpc, Omega_Lambda=0.73, Omega_m=0.27, Omega_b=0.044, sigma_8=0.9 and a UV background that has an ionization rate that is 1.08 +/- 0.08 times the prediction by Madau, Haardt & Rees (1999).

David Tytler; David Kirkman; John M. O'Meara; Nao Suzuki; Adam Orin; Dan Lubin; Pascal Paschos; Tridivesh Jena; Wen-Ching Lin; Michael L. Norman




SciTech Connect

We present a survey for low-ionization metal absorption line systems toward 17 QSOs at redshifts z{sub em} = 5.8-6.4. Nine of our objects were observed at high resolution with either Keck/HIRES or Magellan/MIKE, and the remainder at moderate resolution with Keck/ESI. The survey spans 5.3 < z{sub abs} < 6.4 and has a path length interval {Delta}X = 39.5 or {Delta}z = 8.0. In total we detect ten systems, five of which are new discoveries. The line-of-sight number density, l(X) = 0.25{sup +0.21}{sub -0.13} (95% confidence), is consistent with the combined number density at z {approx} 3 of damped Ly{alpha} systems (DLAs) and sub-DLAs, which comprise the main population of low-ionization systems at lower redshifts. This apparent lack of evolution may occur because low-ionization systems are hosted by lower-mass halos at higher redshifts, or because the mean cross section of low-ionization gas at a given halo mass increases with redshift due to the higher densities and lower ionizing background. The roughly constant number density notably contrasts with the sharp decline at z > 5.3 in the number density of highly ionized systems traced by C IV. The low-ionization systems at z {approx} 6 span a similar range of velocity widths as lower-redshift sub-DLAs but have significantly weaker lines at a given width. This may imply that the mass-metallicity relation of the host galaxies evolves toward lower metallicities at higher redshifts. These systems lack strong Si IV and C IV, which are common among lower-redshift DLAs and sub-DLAs. This is consistent, however, with a similar decrease in the metallicity of the low- and high-ionization phases, and does not necessarily indicate a lack of nearby, highly ionized gas. The high number density of low-ionization systems at z {approx} 6 suggests that we may be detecting galaxies below the current limits of i-dropout and Ly{alpha} emission galaxy surveys. These systems may therefore be the first direct probes of the 'typical' galaxies responsible for hydrogen reionization.

Becker, George D.; Calverley, Alexander P. [Kavli Institute for Cosmology and Institute of Astronomy, Madingley Road, Cambridge, CB3 0HA (United Kingdom); Sargent, Wallace L. W. [Palomar Observatory, California Institute of Technology, Pasadena, CA 91125 (United States); Rauch, Michael, E-mail: gdb@ast.cam.ac.uk, E-mail: acalver@ast.cam.ac.uk, E-mail: wws@astro.caltech.edu, E-mail: mr@obs.carnegiescience.edu [Carnegie Observatories, 813 Santa Barbara Street, Pasadena, CA 91101 (United States)



Verde iPad app | Open Energy Information  

Open Energy Info (EERE)

iPad app iPad app Jump to: navigation, search Tool Summary LAUNCH TOOL Name: Verde iPad app Agency/Company /Organization: Verde Sustainable Solutions, L3C Sector: Energy Focus Area: Energy Efficiency Phase: Create Early Successes Topics: GHG inventory Resource Type: Application prototype User Interface: Mobile Device Website: www.verdel3c.com Country: United States Locality: all Web Application Link: bit.ly/wuHQ1S Cost: Paid UN Region: Northern America Coordinates: 37.09024°, -95.712891° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":37.09024,"lon":-95.712891,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}



Office of Legacy Management (LM)

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3/13/05 - 03/19/05: 3/13/05 - 03/19/05: Hanford - 2 INL - 6 RFETS - 17 SRS - 4 (subject to change) total shipments received as of 03/09/05: 3,415 Disposal Waste disposed as of 03/09/05: 4,337 standard waste boxes 1,356 ten-drum overpacks 60,833 waste drums 27,031 cubic meters Operations: First on, last out A "TRU-ly" unique waste story ... TRU TeamWorks is a biweekly e-newsletter for the Waste Isolation Pilot Plant team D E P A R T M E N T O F E N E R G Y U N I T E D S T A T E S O F A M E R I C A Acronym List Archives Links WIPP Home Page Contact us with or submit your e-mail address for updates. feedback Tools Feedback By the Numbers Operations: Lab down under Unused areas in WIPP mine will soon be put to good use ... Working Smart: Submissions wanted


One West Third Street Tulsa, Oklahoma  

NLE Websites -- All DOE Office Websites (Extended Search)

Jane Thomas Jane Thomas Supply Technician Tulsa, Oklahoma Special thanks to: SWPA Marshall Boyken Kenny Broadaway Mike Dawson Scott Holland Beth Nielsen Margaret Skidmore Randy Staponski Gary Swartzlander Ron Szatmary Steve Wall Jon Worthington CNI/Bearskin Ashley Butler Vicki Clarke Ruben Garcia William Hiller Kathy O'Neal KC District Corps George Boban Andre Vasseur Tulsa District Corps Dan Brueggenjohann Little Rock District Corps Lee Beverly U P DAT E S O U T H W E S T E R N P O W E R A D M I N I S T R A T I O N J U LY - D E C E M B E R 2 0 1 0 continued on page 7 The Stockton Powerplant in Missouri is back online after an extended outage caused when a blade section sheared off of the project's only turbine in February 2009. The nearly five-ton section of blade was reattached in early August 2010 after related repairs had been



Office of Legacy Management (LM)

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Flim3.l Elaenbud  

Office of Legacy Management (LM)

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Office of Legacy Management (LM)

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I I LI I L I  

Office of Legacy Management (LM)

LI LI - I L I 1 II C c - ORNL/RASA-9618 OAK RlDGE NATlONAl. LA8ORATORY Results of the Independent Radiological Verification Survey at B&T Metals, 425 West Town Street, Columbus, Ohio (cooolv) M . E. Murray V. P. Patania C. A. Johnson M N M E D *wD OPEbM~ B V WUCNEEDllW?ME IWiARCH CoRpoRAng FoRTHEwITf@%tATeB ltEpAAMwTmBMeR(Ly ORNL-27 (34el ~~- L._~ This report has been reproduced directly from the best available copy. Avaiiable to DOE and DOE contractors from the Office of Scientific and Technical information, P.O. Box 62, Oak Ridge, TN 3783 1; prices available from (615) 576-8301, FlS 626-8401. Available to the public from the National Technical Information Service, U.S. Department of Commerce, 5285 Port Royal Rd., Springfield, VA 22161. This report was prepared as an account of work sponsored by an agency of the


BWXT Pantex, LLC Route 726, Mt. Athos Road  

National Nuclear Security Administration (NNSA)

Sol-lClTATlONlMODlFlCATlON OF CONTRACT I Sol-lClTATlONlMODlFlCATlON OF CONTRACT I I . CONTRACT ID CODE PAGE I OF P PAGES 9B. DATED (SEE E M 11) 2. AMENDMENTIMODIFICATION NO. MI01 Offers must acknowledge receipt of this amendment prior to the hour and date specifmd in the solicitation as mended, by one of the following methods: (a) By completing Items 8 and 15, and returning - coples of the amendment; @) By acknowledging r d p t of this amendment on each copy of the offer submitted; or (c) By seperate letter or telegram whlch includes a refer- to the solicitation and mendmmt numbers. FAILURE OF YOUR ACKNOWLEDGMENT TO BE RECEIVED AT THE PLACE DESIGNATED FOR THE RECEIPT OF OFFERS PRIOR TO THE HOUR AND DATE SPECIFIED MAY RESULT IN REJECTION OF YOUR OFFER. If by virtus of this msndment you desire to change an offer drem-ly submitted, such change



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2 2 T he ORNL Distrib- uted Active Archive Center (DAAC) is a NA- SA-sponsored source f o r b i o g e o ch e m i c a l a n d e c o l o g i c a l d a t a and services useful in environmental research. The ORNL DAAC cur- r e n t ly a rch i ve s a n d distributes nearly 900 products categorized as Field Campaign, Land Validation, Regional and Global, or Model Archive. Please visit us online at http://daac.ornl.gov for a comprehensive de- scription of data, services, and tools available from the ORNL DAAC. Cur- rent and past news can be found at http://daac. ornl.gov/news.shtml. http://www.nasa.gov * New Model Re-leased * NACP Data sets released * BIGFOOT Meteoro- logical data set. * 24 LBA data sets released * NASA Customer Survey Contents: National Aeronautics and Space Administration



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. 1.1 I . COO-30.72-25 11 t 1 Hadronic Form Factors in Asymptotically Free Field Theories David J. Gross and S.B. Treiman Joseph Henry Labor atorie s of Physics -NOTICE- Pri nce ton Uni ver sit y 1 1 This repor t was prep ared as an acco unt of work 1 Pri nce ton , New Jer sey 1 spons ored by the Unite d State s Gove rnme nt. Neith er 1 1 the Un ited Sta tes nor the Un ited Sta tes Ato mic Ene rgy I 08 54 0 1 j Comm issi on, nor any of thei r empl oyee s, nor any of I the ir con trac tors , sub con trac tors , or the ir em plo yee s, 111 »tti' R'111 wou ld not infr inge priv ate ly own ed righ ts. 1 - .3 ABSTRACT The breakdown of Bjorken scaling in asymptotically free gauge theories of the strong interactions is explored for its implications on the large q2 behavior of nucleon form factors.


Energy Information Administration / Annual Energy Outlook 2011  

Gasoline and Diesel Fuel Update (EIA)

7 7 Table A13. Natural Gas Supply, Disposition, and Prices (Trillion Cubic Feet per Year, Unless Otherwise Noted) Supply, Disposition, and Prices Reference Case Annual Grow th 2009-2035 (percent) 2008 2009 2015 2020 2025 2030 2035 Production Dry Gas Production 1 . . . . . . . . . . . . . . . . . . . . 20.29 20.96 22.10 23.02 23.64 24.71 26.10 0.8% Supplemental Natural Gas 2 . . . . . . . . . . . . . . 0.06 0.06 0.06 0.06 0.06 0.06 0.06 -0.0% Net Imp orts . . . . . . . . . . . . . . . . . . . . . . . . . . . 2.98 2.64 2.78 2.13 1.30 0.97 0.32 -7.8% Pipeline 3 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 2.68 2.23 2.42 1.62 0.97 0.83 0.18 -9.3% Liquefied Natural Gas . . . . . . . . . . . . . . . . . . . 0.30 0.41 0.36 0.51 0.34 0.14 0.14 -4.1% Total Supp ly . . . . . . . . . . . . . . . . . . . . . . . . . . . 23.33 23.66 24.94 25.21 25.00 25.74 26.48 0.4% Consumption by Sector Residential . . . . . . . . . . . . . . . . . . . . . . . . . . . 4.87 4.75 4.80 4.84



Office of Legacy Management (LM)

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The hydrodynamics of relict cosmological H?i i regions: impact of the IGM  

Science Journals Connector (OSTI)

Discrete sources of photoionizing radiation present at the time the intergalactic medium is largely neutral will create expanding H?i i regions. A source which turns off or dims quickly enough will not be able to maintain the advance of its ionization front indefinitely. The high pressure of the relict H?i i region will then drive a shock into the cold neutral ambient medium. We discuss the hydrodynamical evolution of relict cosmological H?i i regions generated at redshifts z?5–15. A thin shell of shocked material develops around the H?i i region. The peculiar velocity of the shell is typically 10–20 km s? 1. The dense shell may cool and fragment into objects with baryonic masses as high as 106–108 M ? and column densities of order 101 9 cm? 2. These values are independent of the nature of the photoionizing source. They are set only by the density of the IGM the sound speed of 104 K gas and the age of the shell. The shock propagation ceases once the filling factor of the H?i i regions reaches unity and the IGM is photoionized. The clouds formed may account for the Ly? forest seen in the spectra of high redshift QSOs. Gravitationally bound fragments may be candidates for blue?excess galaxies at high redshift.

Avery Meiksin; Piero Madau


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BDOS: An open-ended, basic disk operating system for a Nova/Diablo system  

E-Print Network (OSTI)

J 4 V 4 CL Cl I ?C 0 0 CL 4J I Cl 4J I LI CC Ll Cl cC Cl Ctl 0 O CC OO 0 CQ c O O Z Ctt I- Q V tY O Ctl JC Q O O CIJ IX'. cC Ctl Cl ttl Y ~ 2 CLI M M M c 0 Vl 0 Z M H OVM M r4 O Y M N OK JV 20 IJ0 4JQ HO 0 -0... f LJ 4J LJ I- VJ Z24J 4J43 H LJCJY ?Y I Q. 0 K CC C ?Y ?Y 43 0 HO 2 lY M ?4 ID CQ 2 2 Z U 43 cl Q- 43 3- 0 Z H 2 ?Y cC 0 4J I 4 43 CJ X C?l 4' o o 0 0 43 O l4 Vj C?l LO ?OMC3 lO ?O HM ?O h4 H VJ OJ Y Y ?Ll 2 tO 0 0 OJY?OY Ol...

Koontz, Joseph Patrick



The role of filament activation in a solar eruption  

E-Print Network (OSTI)

Observations show that the mutual relationship between filament eruptions and solar flares cannot be described in terms of an unique scenario. In some cases, the eruption of a filament appears to trigger a flare, while in others the observations are more consistent with magnetic reconnection that produces both the flare observational signatures (e.g., ribbons, plasma jets, post-flare loops, etc.) and later the destabilization and eruption of a filament. We study an event which occurred in NOAA 8471, where a flare and the activation of (at least) two filaments were observed on 28 February 1999. By using imaging data acquired in the 1216, 1600, 171 and 195 \\AA\\ TRACE channels and by BBSO in the continnum and in H$\\alpha$, a morphological study of the event is carried out. Using TRACE 1216 and 1600 \\AA\\ data, an estimate of the "pure" Ly$\\alpha$ power is obtained. The extrapolation of the magnetic field lines is done using the SOHO/MDI magnetograms and assuming a potential field. The potential magnetic field ext...

da Costa, Fatima Rubio; Fletcher, Lyndsay; Romano, Paolo; Labrosse, Nicolas



Preliminary consideration of selected chemical and oceanographic factors influential in the formation of the alumino-silicate fraction of some recent sediments  

E-Print Network (OSTI)


Whitehouse, Ulysses Grant



VLT identification of the optical afterglow of the gamma-ray burst GRB 000131 at z=4.50  

E-Print Network (OSTI)

We report the discovery of the gamma-ray burst GRB 000131 and its optical afterglow. The optical identification was made with the VLT 84 hours after the burst following a BATSE detection and an Inter Planetary Network localization. GRB 000131 was a bright, long-duration GRB, with an apparent precursor signal 62 s prior to trigger. The afterglow was detected in ESO VLT, NTT, and DK1.54m follow-up observations. Broad-band and spectroscopic observations of the spectral energy distribution reveals a sharp break at optical wavelengths which is interpreted as a Ly-alpha absorption edge at 6700 A. This places GRB 000131 at a redshift of 4.500 +/- 0.015. The inferred isotropic energy release in gamma rays alone was approximately 10^54 erg (depending on the assumed cosmology). The rapid power-law decay of the afterglow (index alpha=2.25, similar to bursts with a prior break in the lightcurve), however, indicates collimated outflow, which relaxes the energy requirements by a factor of < 200. The afterglow of GRB 000131 is the first to be identified with an 8-m class telescope.

M. I. Andersen; J. Hjorth; H. Pedersen; B. L. Jensen; L. K. Hunt; J. Gorosabel; P. Moller; J. Fynbo; R. M. Kippen; B. Thomsen; L. F. Olsen; L. Christensen; M. Vestergaard; N. Masetti; E. Palazzi; K. Hurley; T. Cline; L. Kaper; A. O. Jaunsen



Synthesis of Densely Functionalized Cyclopropanes via Diastereoselective Nucleophilic Additions to in Situ Generated Cyclopropenes  

E-Print Network (OSTI)

been isolated from the saccoglossan mollusc Elysia crispate8. Eglumetad 4 (LY 354740) is a highly potent agonist selective for group II (mGluR2/3) receptors (EC50 = 5.1 and 24.3 nM at Scheme 1 O O OHOFFF Cl HHCHEMBL475027 5O OO HOFumarranol 1 O... R2 OHH R2R1 H OHcat = NHSO2ArNHSO2ArR1 , R2 = Ph, PhCH2CH2, TrtOCH3, HAr = Ph, o-O2N-C6H4, m-O2N-C6H4, p-O2N-C6H48 9 1071 - 99 %66 - 82 %ee Ph OH MePh OH MePh OHO B OMe2NOC CONMe2Bu2.2 equiv Zn(CHIMe)21.1 equiv >95% ee > 50 : 111 12 13a 13bPh OH Ph...

Ryabchuk, Pavel



The VIMOS Ultra-Deep Survey (VUDS): IGM transmission towards galaxies with 2.5  

E-Print Network (OSTI)

(arXiv abridged abstract) The observed UV rest-frame spectra of distant galaxies are the result of their intrinsic emission combined with absorption along the line of sight produced by the inter-galactic medium (IGM). Here we analyse the evolution of the mean IGM transmission Tr(Ly_alpha) and its dispersion along the line of sight for 2127 galaxies with 2.5= 4 compared to results from QSOs, but a degeneracy between dust extinction and IGM prevents to draw firm conclusions if the internal dust extinction for star-forming galaxies at z>4 takes a mean value significantly in excess of E(B-V)>0.15. Most importantly, we find a large dispersion of IGM transmission along the lines of sight towards distant galaxies with 68% of the distribution within 10 to 17% of the median value in delta z=0.5 bins, similar to what is found on the LOS towards QSOs. We demonstrate the importance of taking into account this large range of IGM transmission when selecting high redshift galaxies based on their colour properties (e.g. LBG ...

Thomas, R; Cassata, V Le Brun P; Garilli, B; Lemaux, B C; Maccagni, D; Pentericci, L; Tasca, L A M; Zamorani, G; Zucca, E; Amorin, R; Bardelli, S; Cassarà, L; Castellano, M; Cimatti, A; Cucciati, O; Durkalec, A; Fontana, A; Giavalisco, M; Grazian, A; Hathi, N P; Ilbert, O; Paltani, S; Ribeiro, B; Schaerer, D; Scodeggio, M; Sommariva, V; Talia, M; Tresse, L; Vanzella, E; Vergani, D; Capak, P; Charlot, S; Contini, T; Cuby, J G; de la Torre, S; Dunlop, J; Fotopoulou, S; Koekemoer, A; López-Sanjuan, C; Mellier, Y; Pforr, J; Salvato, M; Scoville, N; Taniguchi, Y; Wang, P W



An Intermediate-band imaging survey for high-redshift Lyman Alpha Emitters: The Mahoroba-11  

E-Print Network (OSTI)

We present results of our intermediate-band optical imaging survey for high-$z$ Ly$\\alpha$ emitters (LAEs) using the prime focus camera, Suprime-Cam, on the 8.2m Subaru Telescope. In our survey, we use eleven filters; four broad-band filters ($B$, $R_{\\rm c}$, $i^\\prime$, and $z^\\prime$) and seven intermediate-band filters covering from 500 nm to 720 nm; we call this imaging program as the Mahoroba-11. The seven intermediate-band filters are selected from the IA filter series that is the Suprime-Cam intermediate-band filter system whose spectral resolution is $R = 23$. Our survey has been made in a $34^\\prime \\times 27^\\prime$ sky area in the Subaru XMM Newton Deep Survey field. We have found 409 IA-excess objects that provide us a large photometric sample of strong emission-line objects. Applying the photometric redshift method to this sample, we obtained a new sample of 198 LAE candidates at $3 42.67$ between $z \\sim 3$ and 5.

Yamada, S F; Sumiya, R; Umeda, K; Shioya, Y; Ajiki, M; Nagao, T; Murayama, T; Taniguchi, Y; Yamada, Sanae F.; Sasaki, Shunji S.; Sumiya, Ryoko; Umeda, Kazuyoshi; Shioya, Yasuhiro; Ajiki, Masaru; Nagao, Tohru; Murayama, Takashi; Taniguchi, Yoshiaki



A photometric survey for Lyalpha-HeII dual emitters: Searching for Population III stars in high-redshift galaxies  

E-Print Network (OSTI)

We present a new photometric search for high-z galaxies hosting Population III (PopIII) stars based on deep intermediate-band imaging observations obtained in the Subaru Deep Field (SDF), by using Suprime-Cam on the Subaru Telescope. By combining our new data with the existing broad-band and narrow-band data, we searched for galaxies which emit strongly both in Ly_alpha and in HeII 1640 (``dual emitters'') that are promising candidates for PopIII-hosting galaxies, at 3.93 2 Msun/yr was found by our photometric search in 4.03 x 10^5 Mpc^3 in the SDF. This result disfavors low feedback models for PopIII star clusters, and implies an upper-limit of the PopIII SFR density of SFRD_PopIII < 5 x 10^-6 Msun/yr/Mpc^3. This new selection method to search for PopIII-hosting galaxies should be useful in future narrow-band surveys to achieve the first observational detection of PopIII-hosting galaxies at high redshifts.

Nagao, Tohru; Maiolino, Roberto; Grady, Celestine; Kashikawa, Nobunari; Ly, Chun; Malkan, Matthew; Motohara, Kentaro; Murayama, Takashi; Schaerer, Daniel; Shioya, Yasuhiro; Taniguchi, Yoshiaki




SciTech Connect

The attenuation of high-energy gamma-ray spectrum due to the electron-positron pair production against the extragalactic background light (EBL) provides an indirect method to measure the EBL of the universe. We use the measurements of the absorption features of the gamma-rays from blazars as seen by the Fermi Gamma-ray Space Telescope to explore the EBL flux density and constrain the EBL spectrum, star formation rate density (SFRD), and photon escape fraction from galaxies out to z = 6. Our results are basically consistent with the existing determinations of the quantities. We find a larger photon escape fraction at high redshifts, especially at z = 3, compared to the result from recent Ly{alpha} measurements. Our SFRD result is consistent with the data from both gamma-ray burst and ultraviolet (UV) observations in the 1{sigma} level. However, the average SFRD we obtain at z {approx}> 3 matches the gamma-ray data better than the UV data. Thus our SFRD result at z {approx}> 6 favors the fact that star formation alone is sufficiently high enough to reionize the universe.

Gong Yan; Cooray, Asantha [Department of Physics and Astronomy, University of California, Irvine, CA 92697 (United States)



The Hamburg/SAO survey for low metallicity blue compact/HII-galaxies (HSS-LM). I. The first list of 46 strong-lined galaxies  

E-Print Network (OSTI)

We present the description and the first results of a new project devoted to the search for extremely metal-deficient blue compact/HII-galaxies (BCGs) and to the creation of a well selected large BCG sample with strong emission lines. Such galaxies should be suitable for reliable determination of their oxygen abundance through the measurement of the faint [OIII]4363A line. The goals of the project are two-fold: a) to discover a significant number of new extremely metal-poor galaxies (Z = 0 deg. and b^ii = 100 A). The remaining five lower excitation ELGs include three BCGs, and two galaxies classified as SBN (Starburst Nucleus) and DANS (Dwarf Amorphous Nucleus Starburst). One object is identified as a quasar with a strong Ly_alpha emission line near 5000 A (z~3). We provide a list with coordinates, measured radial velocities, B-magnitudes, equivalent widths EW([OIII]5007) and EW(H_beta) and for the 46 strong-lined BCGs the derived oxygen abundances 12+log(O/H). The abundances range between 7.42 and 8.4 (corresponding to metallicities between 1/30 and 1/3 Zo). The sample contains four galaxies with Z < 1/20 Zo, of which three are new discoveries.

A. V. Ugryumov; D. Engels; S. A. Pustilnik; A. Y. Kniazev; A. G. Pramskij; H. J. Hagen



A memory-efficient algorithm to obtain splicing graphs and de novo expression estimates from de Bruijn graphs of RNA-Seq data  

E-Print Network (OSTI)

tp ro ce ss in g al g or it h m , O as es an d Tr an s- A B yS S us in g si x p ub lic ly av ai la b le lib ra ri es ov er d if fe re n t va lu es of k -m er co ve ra g e cu to ff c . p os tp ro ce ss k _ c in it ia l no de s la rg es t ta ng le la rg... es t SC C sp lic in g gr ap hs m ax le ng th N 50 > 1- no de gr ap hs m ax no de s av g no de s SN Ps to ta l hi ts un iq ue hi ts > 1- hi t gr ap hs m ax hi ts ti m e (m in s) m em or y (G B) 35 _3 22 76 14 17 85 45 88 09 4 75 36 7 10 53 9 54 4 20 48...

Sze, Sing-Hoi; Tarone, Aaron M



MnSOD marks cord blood late outgrowth endothelial cells and accompanies robust resistance to oxidative stress  

SciTech Connect

Cord blood is source of colony-forming progenitors to vascular endothelial cells for potential use in cell therapies. These cells-called blood late outgrowth endothelial cells (OECs)-have undergone endothelial differentiation, but appear to still possess functional properties different from mature endothelial cells. A large-scale comparative proteomics screen of cord blood OECs versus human vein endothelial cells (HUVECs) using two-dimensional gel electrophoresis and mass spectrometry identified specific expression of manganese superoxide dismutase (MnSOD), a key antioxidant enzyme expressed in the mitochondria, in OECs but not in HUVECs. Immunoblotting verified significant MnSOD levels in all OEC isolates tested and maintained throughout passaging. Endothelial function and cell survival/proliferation assays in the presence of high cytotoxic doses of the superoxide generator compound LY83583 showed OECs profoundly better protected against oxidative stress than HUVECs. Such cytoprotective levels of MnSOD cells could give therapeutic cell transplants a survival advantage in necrotic or ischemic conditions.

Cai Hao [Department of Obstetrics, University Hospital Zurich (Switzerland); Gehrig, Peter [Functional Genomics Center Zurich, University of Zurich, Swiss Federal Institute of Technology, Zurich (Switzerland); Scott, Thomas M. [Functional Genomics Center Zurich, University of Zurich, Swiss Federal Institute of Technology, Zurich (Switzerland); Zimmermann, Roland [Department of Obstetrics, University Hospital Zurich (Switzerland); Schlapbach, Ralph [Functional Genomics Center Zurich, University of Zurich, Swiss Federal Institute of Technology, Zurich (Switzerland); Zisch, Andreas H. [Department of Obstetrics, University Hospital Zurich (Switzerland) and Center for Integrative Human Physiology, University of Zurich, Zurich (Switzerland)]. E-mail: andreas.zisch@usz.ch



Neutral chlorine and molecular hydrogen at high redshift  

E-Print Network (OSTI)

Chlorine and molecular hydrogen are known to be tightly linked together in the cold phase of the local interstellar medium through rapid chemical reactions. We present here the first systematic study of this relation at high redshifts using H$_2$-bearing damped Ly$\\alpha$ systems (DLAs) detected along quasar lines of sight. Using high-resolution spectroscopic data from VLT/UVES and Keck/HIRES, we report the detection of Cl$\\,$I in 9 DLAs (including 5 new detections) out of 18 high-$z$ DLAs with $N($H$_2) \\ge 10^{17.3}\\,$cm$^{-2}$ (including a new H$_2$ detection at $z=3.09145$ towards J$\\,$2100$-$0641) and present upper limits for the remaining 9 systems. We find a $\\sim$5$\\,\\sigma$ correlation between $N$(Cl$\\,$I) and $N$(H$_2$) with only $\\sim$0.2$\\,$dex dispersion over the range 18.1$\\,<\\,$log$\\,N$(H$_2$)$\\,<\\,$20.1, thus probing column densities 10 times lower those seen towards nearby stars, roughly following the relation $N$(Cl$\\,$I$) \\approx 1.5\\times10^{-6} \\times N($H$_2)$. This relation betwee...

Balashev, S A; Klimenko, V V; Petitjean, P; Srianand, R; Ledoux, C; Ivanchik, A V; Varshalovich, D A



D-branes and Azumaya/matrix noncommutative differential geometry,II: Azumaya/matrix supermanifolds and differentiable maps therefrom -- with a view toward dynamical fermionic D-branes in string theory  

E-Print Network (OSTI)

In this Part II of D(11), we introduce new objects: super-$C^k$-schemes and Azumaya super-$C^k$-manifolds with a fundamental module (or, synonymously, matrix super-$C^k$-manifolds with a fundamental module), and extend the study in D(11.1) ([L-Y3], arXiv:1406.0929 [math.DG]) to define the notion of `differentiable maps from an Azumaya/matrix supermanifold with a fundamental module to a real manifold or supermanifold'. This allows us to introduce the notion of `fermionic D-branes' in two different styles, one parallels Ramond-Neveu-Schwarz fermionic string and the other Green-Schwarz fermionic string. A more detailed discussion on the Higgs mechanism on dynamical D-branes in our setting, taking maps from the D-brane world-volume to the space-time in question and/or sections of the Chan-Paton bundle on the D-brane world-volume as Higgs fields, is also given for the first time in the D-project. Finally note that mathematically string theory begins with the notion of a differentiable map from a string world-sheet...

Liu, Chien-Hao



The Radiated Energy Budget of Chromospheric Plasma in a Major Solar Flare Deduced From Multi-Wavelength Observations  

E-Print Network (OSTI)

This paper presents measurements of the energy radiated by the lower solar atmosphere, at optical, UV, and EUV wavelengths, during an X-class solar flare (SOL2011-02-15T01:56) in response to an injection of energy assumed to be in the form of nonthermal electrons. Hard X-ray observations from RHESSI were used to track the evolution of the parameters of the nonthermal electron distribution to reveal the total power contained in flare accelerated electrons. By integrating over the duration of the impulsive phase, the total energy contained in the nonthermal electrons was found to be $>2\\times10^{31}$ erg. The response of the lower solar atmosphere was measured in the free-bound EUV continua of H I (Lyman), He I, and He II, plus the emission lines of He II at 304\\AA\\ and H I (Ly$\\alpha$) at 1216\\AA\\ by SDO/EVE, the UV continua at 1600\\AA\\ and 1700\\AA\\ by SDO/AIA, and the WL continuum at 4504\\AA, 5550\\AA, and 6684\\AA, along with the Ca II H line at 3968\\AA\\ using Hinode/SOT. The summed energy detected by these in...

Milligan, Ryan O; Dennis, Brian R; Hudson, Hugh S; Fletcher, Lyndsay; Allred, Joel C; Chamberlin, Phillip C; Ireland, Jack; Mathioudakis, Mihalis; Keenan, Francis P



The Ultimate Law of Social Evolution  

E-Print Network (OSTI)

0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 O 0 0 0 0 0 0 0 0 0 0 0 0 0 THE ULTIf'ATE LAW OF SOCIAL E7GLUTI0?-T. I n de termin ing the u n d e r l y i n g force? o f the s o c i a l organism, t h e o r i s t s and s c i e n t i... s t s have become i n v o l v e d i n q u e r i e s exceed ing ly p r o ­ b l e m a t i c a l . One r e l i e s upon B c e r t a i n c o n d i t i o n o f f a c t s andvo i rcumstan- ces to f i x and e s t a b l i s h what hp deems the on lv p o s s i b l e...

Overlander, Jacob Alphaeus



The X-ray eclipse geometry of CAL 87  

E-Print Network (OSTI)

We explore XMM-{\\it Newton} observations of the eclipsing super-soft X-ray source CAL~87 in order to map the accretion structures of the system. { Indirect imaging techniques were applied in X-ray light curves to provide eclipse maps}. The surface brightness distribution exhibits an extended and symmetric emission, { and from the hardest X-rays is revealed a feature that is likely due to a bright spot}. A rate of $\\dot{P} = (+6\\pm2) \\times 10^{-10}$ for changes in the orbital period of the system was derived from the eclipses. There is no significant variation of the emission lines even during eclipses, arguing that the lines are formed in an extended region. The continuum emission dominates the decrease in flux which is observed during eclipses. The O\\,{\\small VIII} Ly$\\alpha$ line reveals a broadening velocity { which is} estimated in 365$^{+65}_{-69}$ km\\,s$^{-1}$ (at 1$\\sigma$) and marginal evidence for asymmetry in its profile, and sometimes shows evidence of double-peaked emission. Together, the results...

Ribeiro, T; Borges,; W, B



Determination of the Central Mass in Active Galactic Nuclei Using Cross-Correlation Lags and Velocity Dispersions  

E-Print Network (OSTI)

We here estimate the mass M of the central object in five active galactic nuclei (AGNs), using the most recent reverberation data obtained by the AGN Watch Consortium. The cross-correlation function (CCF) centroids of the broad Ly-alpha 1216 and C IV 1549 lines are used to estimate the size of the broad-line region (BLR) in these sources. We calculate the velocity dispersions of these lines in the root mean square (rms) spectra and then use our results to estimate M. We argue that our technique of calculating the velocity dispersion should work in the general case of an arbitrary line profile, unlike methods that depend on the measurement of the full-width at half-maximum (FWHM) of the broad line. We also show that our results agree with the FWHM method in the limit of a normal (Gaussian) line profile. The masses calculated here are considerably smaller than those calculated with the previous generation of reverberation data.

Michael J. Fromerth; Fulvio Melia



Metallicity and Physical Conditions in the Magellanic Bridge  

E-Print Network (OSTI)

We present a new analysis of the diffuse gas in the Magellanic Bridge (RA>3h) based on HST/STIS E140M and FUSE spectra of 2 early-type stars lying within the Bridge and a QSO behind it. We derive the column densities of HI (from Ly\\alpha), NI, OI, ArI, SiII, SII, and FeII of the gas in the Bridge. Using the atomic species, we determine the first gas-phase metallicity of the Magellanic Bridge, [Z/H]=-1.02+/-0.07 toward one sightline, and -1.7H]Bridge gas along our three lines of sight is ~70-90% ionized, despite high HI columns, logN(HI)=19.6-20.1. Possible sources for the ongoing ionization are certainly the hot stars within the Bridge, hot gas (revealed by OVI absorption), and leaking photons from the SMC and LMC. From the analysis of CII*, we deduce that the overall density of the Bridge must be low (<0.03-0.1 cm^-3). We argue that our findings combined with other recent observational results should motivate new models of the evolution of the SMC-LMC-Galaxy system.

N. Lehner; J. C. Howk; F. P. Keenan; J. V. Smoker



Metallicity and Physical Conditions in the Magellanic Bridge  

Science Journals Connector (OSTI)

We present a new analysis of the diffuse gas in the Magellanic Bridge (R.A. 3h) based on HST STIS E140M and FUSE spectra of two early-type stars lying within the Bridge and a QSO behind it. We derive the column densities of the H I (from Ly?), N I, O I, Ar I, Si II, S II, and Fe II of the gas in the Bridge. Using the atomic species, we determine the first gas-phase metallicity of the Magellanic Bridge, -->[Z/H] = ? 1.02 ± 0.07 toward one sight line and -->-1.7 Z/H] N(H I), we show that the Bridge gas along our three lines of sight is ~70%-90% ionized, despite high H I columns, --> log N(H I) 19.6 ? 20.1. Possible sources for the ongoing ionization are certainly the hot stars within the Bridge, hot gas (revealed by O VI absorption), and leaking photons from the SMC and LMC. From the analysis of C II*, we deduce that the overall density of the Bridge must be low (?3). We argue that our findings combined with other recent observational results should motivate new models of the evolution of the SMC-LMC-Galaxy system.

N. Lehner; J. C. Howk; F. P. Keenan; J. V. Smoker


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Distribution of Si, Fe, and Ni in the Intracluster Medium of the Coma Cluster  

E-Print Network (OSTI)

We studied the distributions of Si, Fe, and Ni in the intracluster medium (ICM) of the Coma cluster, one of the largest clusters in the nearby universe, using XMM-Newton data up to 0.5 r180 and Suzaku data of the central region up to 0.16 r180. Using the flux ratios of Ly alpha of H-like Si and 7.8 keV blend to K alpha of He-like Fe, the abundance ratios of Si to Fe and Ni to Fe of the ICM were derived using APEC model v2.0.1. The Si/Fe ratio in the ICM of the Coma cluster shows no radial gradient. The emission weighted averages of the Si/Fe ratio in the ICM within 0.0--0.2 r180, 0.2--0.5 r180, and 0.0--0.5 r180 are 0.97 +- 0.11, 1.05 +- 0.36 and 0.99 +- 0.13, respectively, in solar units using the solar abundance of Lodders (2003). These values are close to those of smaller clusters and groups of galaxies. Using the Suzaku data of the central region, the derived Ni/Fe ratio of the ICM is 0.6--1.5 in solar units, according to the same solar abundance table. The systematic difference in the derived abundance r...

Matsushita, Kyoko; Sakuma, Eri; Sato, Kosuke



Spatially Resolved X-ray Spectroscopy of Vela Shrapnel A  

E-Print Network (OSTI)

We present the detailed X-ray spectroscopy of Vela shrapnel A with the XMM-Newton satellite. Vela shrapnel A is one of several protrusions identified as bullets from Vela supernova explosion. The XMM-Newton image shows that shrapnel A consists of a bright knot and a faint trailing wake. We extracted spectra from various regions, finding a prominent Si Ly$_\\alpha$ emission line in all the spectra. All the spectra are well represented by the non-equilibrium ionization (NEI) model. The abundances are estimated to be O$\\sim$0.3, Ne$\\sim$0.9, Mg$\\sim$0.8, Si$\\sim$3, Fe$\\sim$0.8 times their solar values. The non-solar abundance ratio between O and Si indicates that shrapnel A originates from a deep layer of a progenitor star. We found that the relative abundances between heavy elements are almost uniform in shrapnel A, which suggests that the ejecta from supernova explosion are well mixed with swept-up interstellar medium.

S. Katsuda; H. Tsunemi



Evolution of the 21 cm signal throughout cosmic history  

E-Print Network (OSTI)

The potential use of the redshifted 21 cm line from neutral hydrogen for probing the epoch of reionization is motivating the construction of several low-frequency interferometers. There is also much interest in the possibility of constraining the initial conditions from inflation and the nature of the dark matter and dark energy by probing the power-spectrum of density perturbations in three dimensions and on smaller scales than probed by the microwave background anisotropies. Theoretical understanding of the 21 cm signal has been fragmented into different regimes of physical interest. In this paper, we make the first attempt to describe the full redshift evolution of the 21 cm signal between 0neutral fraction, as well as the Lyman alpha flux, and allow for a post-reionization signal from damped Ly alpha systems. Our comprehensive analysis provides a useful foundation for optimizing the design of future arrays whose goal is to separate the particle physics from the astrophysics, either by probing the peculiar velocity distortion of the 21 cm power spectrum, or by extending the 21 cm horizon to z > 25 before the first galaxies had formed, or to z < 6 when the residual pockets of hydrogen trace large scale structure.

Jonathan R. Pritchard; Abraham Loeb




SciTech Connect

The far-ultraviolet spectrum of the Bright Star (B8 III) in 47 Tuc (NGC 104) shows a remarkable pattern: it is well fit by local thermodynamic equilibrium models at wavelengths longer than Ly{beta}, but at shorter wavelengths it is fainter than the models by a factor of two. A spectrum of this star obtained with the Far Ultraviolet Spectroscopic Explorer shows broad absorption troughs with sharp edges at 995 and 1010 A and a deep absorption feature at 1072 A; none of which are predicted by the models. We find that these features are caused by resonances in the photoionization cross sections of the first and second excited states of atomic nitrogen (2s {sup 2} 2p {sup 3} {sup 2} D {sup 0} and {sup 2} P {sup 0}). Using cross sections from the Opacity Project, we can reproduce these features, but only if we use the cross sections at their full resolution, rather than the resonance-averaged cross sections usually employed to model stellar atmospheres. These resonances are strongest in stellar atmospheres with enhanced nitrogen and depleted carbon abundances, a pattern typical of post-asymptotic giant branch stars.

Dixon, William V.; Chayer, Pierre, E-mail: dixon@stsci.edu, E-mail: chayer@stsci.edu [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States)



Project Lyman: Quantifying 11 Gyrs of Metagalactic Ionizing Background Evolution  

E-Print Network (OSTI)

The timing and duration of the reionization epoch is crucial to the emergence and evolution of structure in the universe. The relative roles that star-forming galaxies, active galactic nuclei and quasars play in contributing to the metagalactic ionizing background across cosmic time remains uncertain. Deep quasar counts provide insights into their role, but the potentially crucial contribution from star-formation is highly uncertain due to our poor understanding of the processes that allow ionizing radiation to escape into the intergalactic medium (IGM). The fraction of ionizing photons that escape from star-forming galaxies is a fundamental free parameter used in models to "fine-tune" the timing and duration of the reionization epoch that occurred somewhere between 13.4 and 12.7 Gyrs ago (redshifts between 12 > z > 6). However, direct observation of Lyman continuum (LyC) photons emitted below the rest frame \\ion{H}{1} ionization edge at 912 \\AA\\ is increasingly improbable at redshifts z > 3, due to the stead...

McCandliss, Stephan R; Bergvall, Nils; Bianchi, Luciana; Bridge, Carrie; Bogosavljevic, Milan; Cohen, Seth H; Deharveng, Jean-Michel; Dixon, W Van Dyke; Ferguson, Harry; Friedman, Peter; Hayes, Matthew; Howk, J Christopher; Inoue, Akio; Iwata, Ikuru; Kaiser, Mary Elizabeth; Kriss, Gerard; Kruk, Jeffrey; Kutyrev, Alexander S; Leitherer, Claus; Meurer, Gerhardt R; Prochaska, Jason X; Sonneborn, George; Stiavelli, Massimo; Teplitz, Harry I; Windhorst, Rogier A



Nepali Aawaz Volume 1, Issue 5, 23 November - 6 December 2005  

E-Print Network (OSTI)

]kfnLx¿ xªsª hfg] u/]sf lyP . nfdf] ;do xªsªdf sfd ubf{ cfkm\\ gf] cfly{s x}l;ot g} ablnPsf] atfpg] ;flGtnf gofF lgodn] w]/} g]kfnL dlxnfsf] /f]huf/ vf]l;Psf] atfpFl5g\\ . elG5g\\, æxªsªd} sfd ul//x]sf dlxnf sfdbf/ x¿n] t sfd kfp~h]n ug{ kfpF5g\\ g} t/ gof... . t/, ljut s]xL dlxgfb]lv xªsª cWofudg ljefun] lagf sf/0f eL;f /f]s]sf] 5 . t/, eL;f lsg aGb eof] eg]/ g t ;/sf/ rf;f] lnG5 g t Joj;foLx¿ g} . ;a}sf] df/ dlxnfnfO{ . 8Da/s[i0f >]i7 lnP/ 8f]d]l:6s x]Nk/sf] ¿kdf ToxfF w]/} g]kfnL uPsfdf dlxnfx...

Shrestha, Kashish Das


Nepali Aawaz Volume 1, Issue 15, 7 June 2006  

E-Print Network (OSTI)

during the movement. Funds for the injured Diaspora Nepali Aawaz | June 07.2006 #24; g]kfn ls/ft /fO{ P;f]l;P;g ckm o'P;P sf] cfof]hgfdf d] @! , @))^ sf lbg Go'of]s{df ls/f+t /fO{ x?sf] kj{ r08Lgfr eJo ?kdf ;DkGg eof] . Go'of]s{sf] SjLG; af]/f] a... |Lh kfs{ / HofS;g xfO6df ul/ b'O r/0fdf ul/Psf] pSt sfo{s|ddf ljleGg jStfx?n] dGtJo z[esfdgf cfbfg k|bfg k|z+;f kq ljt/0f ug{' ePsf] lyof] . pSt kj{df ls/ft /fO{ x? dfq g eP/ cGo w]/} g]kfnLx?n] klg dgf]/+hg lnPsf lyP . sfo{s|dsf k|d'v cltly Unf...

Shrestha, Kashish Das


A Star-Forming Shock Front in Radio Galaxy 4C+41.17 Resolved with Laser-Assisted Adaptive Optics Spectroscopy  

E-Print Network (OSTI)

Near-infrared integral-field spectroscopy of redshifted [O III], H-beta and optical continuum emission from z=3.8 radio galaxy 4C+41.17 is presented, obtained with the laser-guide-star adaptive optics facility on the Gemini North telescope. Employing a specialized dithering technique, a spatial resolution of 0.10 arcsec or 0.7 kpc is achieved in each spectral element, with velocity resolution of ~70 km/s. Spectra similar to local starbursts are found for bright knots coincident in archival Hubble Space Telescope (HST) restframe-ultraviolet images, which also allows a key line diagnostic to be mapped together with new kinematic information. There emerges a clearer picture of the nebular emission associated with the jet in 8.3 GHz and 15 GHz Very Large Array maps, closely tied to a Ly-alpha-bright shell-shaped structure seen with HST. This supports a previous interpretation of that arc tracing a bow shock, inducing 10^10-11 M_solar star-formation regions that comprise the clumpy broadband optical/ultraviolet mo...

Steinbring, Eric



An Expression of Cultural Change: Invisible Converts to Protestantism Among Highland Guatemala Mayas  

E-Print Network (OSTI)

s t an t , a n d the r e m a i n i n g 87 per cent Ca tho l ic . Of the p resen t gene ra t ion ' s g r a n d p a r e n t s , on ly a b o u t 3 p e r cen t were Pro tes tan t . Th i s r ecen t and r ap id ra te of c o n v e r s i o n is associa ted w i t h a...AN EXPRESSION OF CULTURAL CHANGE: INVISIBLE CONVERTS TO PROTESTANTISM AMONG HIGHLAND GUATEMALA MAYAS Li l i ana R . G o l d i n a n d B r e n t M e t z State U n i v e r s i t y of N e w Y o r k , A l b a n y T h e process of re l ig ious...

Goldin, Liliana R.; Metz, Brent



Engineering internship at Brown & Root, Incorporated: a report  

E-Print Network (OSTI)

Section. This section is responsible for designing and selecting oyN DLJOE GW&J mu Cy q?q tCOmlLy gf AngT OEm lL:O &LOEmS:f 1ymCL::L:f Ommx:f L,7J1&LYOf WYS :>Jxx: YLCL::WyU Om 1ymS7CL W 1ymS7CON rEJ: yL:1mY:JlJxJOU JYCx7SL: OEL SL:JcY WYS SL.Lxm1&LYO mu...JYLLyJYcf xxJ: yL:1mY:JlJxJOJL: WyL Om &W>L 1ym;LCO W::JcY&LYO:f Om CmmySJYWOL OEm Mmy>f Om &W>L umxxmMq71 CmyyL:1mYSLYCLf WYS Om ELx1 MJOE OEL WS&JYJ:OyWOJ.L WCOJ.JOJL:N Fym;LCO hYcJYLLy: tYL Fym;LCO hYcJYLLy :Em7xS LjJ:O umy LWCE mu OELN OEyLL :LCOJmY:N r...

Gannaway, Randall Joe, 1952-



Measurements of Martin-Puplett Interferometer Limitations using Blackbody Source  

SciTech Connect

Frequency domain measurements with Martin-Puplett interferometer is one of a few techniques capable of bunch length measurements at the level of ~ 100 fs. As the bunch length becomes shorter, it is important to know and be able to measure the limitations of the instrument in terms of shortest measurable bunch length. In this paper we describe an experiment using a blackbody source with the modified Martin-Puplett interferometer that is routine- ly used for bunch length measurements at the JLab FEL, as a way to estimate the shortest, measurable bunch length. The limitation comes from high frequency cut-off of the wire-grid polarizer currently used and is estimated to be 50 fs RMS. The measurements are made with the same Golay cell detector that is used for beam measure- ments. We demonstrate that, even though the blackbody source is many orders of magnitude less bright than the coherent transition or synchrotron radiation, it can be used for the measurements and gives a very good signal to noise ratio in combination with lock-in detection. We also compare the measurements made in air and in vacuum to characterize the very strong effect of the atmospheric absorption.

Evtushenko, Pavel E. [JLAB; Klopf, John M. [JLAB



The Eighth Data Release of the Sloan Digital Sky Survey: First Data from SDSS-III  

SciTech Connect

The Sloan Digital Sky Survey (SDSS) started a new phase in August 2008, with new instrumentation and new surveys focused on Galactic structure and chemical evolution, measurements of the baryon oscillation feature in the clustering of galaxies and the quasar Ly{alpha} forest, and a radial velocity search for planets around {approx}8000 stars. This paper describes the first data release of SDSS-III (and the eighth counting from the beginning of the SDSS). The release includes 5-band imaging of roughly 5200 deg{sup 2} in the Southern Galactic Cap, bringing the total footprint of the SDSS imaging to 14,555 deg{sup 2}, or over a third of the Celestial Sphere. All the imaging data have been reprocessed with an improved sky-subtraction algorithm and a final, self-consistent recalibration and flat-field determination. This release also includes all data from the second phase of the Sloan Extension for Galactic Understanding and Evolution (SEGUE-2), consisting of spectroscopy of approximately 118,000 stars at both high and low Galactic latitudes. All the more than half a million stellar spectra obtained with the SDSS spectrograph have been reprocessed through an improved stellar parameters pipeline, which has better determination of metallicity for high metallicity stars.

Aihara, Hiroaki; /Tokyo U.; Prieto, Carlos Allende; /Laguna U., Tenerife; An, Deokkeun; /Ewha Women's U., Seoul; Anderson, Scott F.; /Washington U., Seattle, Astron. Dept.; Aubourg, Eric; /APC, Paris /DAPNIA, Saclay; Balbinot, Eduardo; /Rio Grande do Sul U. /Rio de Janeiro Observ.; Beers, Timothy C.; /Michigan State U.; Berlind, Andreas A.; /Vanderbilt U.; Bickerton, Steven J.; /Princeton U.; Bizyaev, Dmitry; /Apache Point Observ.; Blanton, Michael R.; /New York U., CCPP /Penn State U.




SciTech Connect

We report the detection of a strong H I 21 cm absorption system at z = 0.5344, as well as a candidate system at z = 0.3389, in the sight line toward the z = 2.64 quasar MG J0414+0534. This, in addition to the absorption at the host redshift and the other two intervening absorbers, takes the total to four (possibly five). The previous maximum number of 21 cm absorbers detected along a single sight line is two and so we suspect that this number of gas-rich absorbers is in some way related to the very red color of the background source. Despite this, no molecular gas (through OH absorption) has yet been detected at any of the 21 cm redshifts, although, from the population of 21 cm absorbers as a whole, there is evidence for a weak correlation between the atomic line strength and the optical-near-infrared color. In either case, the fact that so many gas-rich galaxies (likely to be damped Ly{alpha} absorption systems) have been found along a single sight line toward a highly obscured source may have far-reaching implications for the population of faint galaxies not detected in optical surveys, a possibility which could be addressed through future wide-field absorption line surveys with the Square Kilometer Array.

Tanna, A.; Webb, J. K. [School of Physics, University of New South Wales, Sydney, NSW 2052 (Australia); Curran, S. J. [Sydney Institute for Astronomy, School of Physics, University of Sydney, NSW 2006 (Australia); Whiting, M. T. [CSIRO Astronomy and Space Science, P.O. Box 76, Epping, NSW 1710 (Australia); Bignell, C., E-mail: sjc@physics.usyd.edu.au [National Radio Astronomy Observatory, P.O. Box 2, Rt. 28/92 Green Bank, WV 24944-0002 (United States)



The Properties of Lyman Alpha Nebulae: Gas Kinematics from Non-resonant Lines  

E-Print Network (OSTI)

[Abridged] With VLT/X-shooter, we obtain optical and NIR spectra of six Ly-alpha blobs at z~2.3. Using three measures --- the velocity offset between the Lya line and the non-resonant [OIII] or H-alpha line (Dv_Lya), the offset of stacked interstellar metal absorption lines, and the spectrally-resolved [OIII] line profile --- we study the kinematics of gas along the line of sight to galaxies within each blob center. These three indicators generally agree in velocity and direction, and are consistent with a simple picture in which the gas is stationary or slowly outflowing at a few hundred km/s from the embedded galaxies. The absence of stronger outflows is not a projection effect: the covering fraction for our sample is limited to winds of up to ~1000km/s. The Dv_Lya offsets here are smaller than typical of LBGs, but similar to those of compact LAEs. The latter suggests that outflow speed cannot be a...

Yang, Yujin; Jahnke, Knud; Davé, Romeel



Cosmological implications of baryon acoustic oscillation (BAO) measurements  

E-Print Network (OSTI)

We derive constraints on cosmological parameters and tests of dark energy models from the combination of baryon acoustic oscillation (BAO) measurements with cosmic microwave background (CMB) and Type Ia supernova (SN) data. We take advantage of high-precision BAO measurements from galaxy clustering and the Ly-alpha forest (LyaF) in the BOSS survey of SDSS-III. BAO data alone yield a high confidence detection of dark energy, and in combination with the CMB angular acoustic scale they further imply a nearly flat universe. Combining BAO and SN data into an "inverse distance ladder" yields a 1.7% measurement of $H_0=67.3 \\pm1.1$ km/s/Mpc. This measurement assumes standard pre-recombination physics but is insensitive to assumptions about dark energy or space curvature, so agreement with CMB-based estimates that assume a flat LCDM cosmology is an important corroboration of this minimal cosmological model. For open LCDM, our BAO+SN+CMB combination yields $\\Omega_m=0.301 \\pm 0.008$ and curvature $\\Omega_k=-0.003 \\pm ...

Aubourg, Éric; Bautista, Julian E; Beutler, Florian; Bhardwaj, Vaishali; Bizyaev, Dmitry; Blanton, Michael; Blomqvist, Michael; Bolton, Adam S; Bovy, Jo; Brewington, Howard; Brinkmann, J; Brownstein, Joel R; Burden, Angela; Busca, Nicolás G; Carithers, William; Chuang, Chia-Hsun; Comparat, Johan; Cuesta, Antonio J; Dawson, Kyle S; Delubac, Timothée; Eisenstein, Daniel J; Font-Ribera, Andreu; Ge, Jian; Goff, J -M Le; Gontcho, Satya Gontcho A; Gott, J Richard; Gunn, James E; Guo, Hong; Guy, Julien; Hamilton, Jean-Christophe; Ho, Shirley; Honscheid, Klaus; Howlett, Cullan; Kirkby, David; Kitaura, Francisco S; Kneib, Jean-Paul; Lee, Khee-Gan; Long, Dan; Lupton, Robert H; Magaña, Mariana Vargas; Malanushenko, Viktor; Malanushenko, Elena; Manera, Marc; Maraston, Claudia; Margala, Daniel; McBride, Cameron K; Miralda-Escudé, Jordi; Myers, Adam D; Nichol, Robert C; Noterdaeme, Pasquier; Nuza, Sebastián E; Olmstead, Matthew D; Oravetz, Daniel; Pâris, Isabelle; Padmanabhan, Nikhil; Palanque-Delabrouille, Nathalie; Pan, Kaike; Pellejero-Ibanez, Marcos; Percival, Will J; Petitjean, Patrick; Pieri, Matthew M; Prada, Francisco; Reid, Beth; Roe, Natalie A; Ross, Ashley J; Ross, Nicholas P; Rossi, Graziano; Rubiño-Martín, Jose Alberto; Sánchez, Ariel G; Samushia, Lado; Santos, Ricardo Tanausú Génova; Scóccola, Claudia G; Schlegel, David J; Schneider, Donald P; Seo, Hee-Jong; Sheldon, Erin; Simmons, Audrey; Skibba, Ramin A; Slosar, Anže; Strauss, Michael A; Thomas, Daniel; Tinker, Jeremy L; Tojeiro, Rita; Vazquez, Jose Alberto; Viel, Matteo; Wake, David A; Weaver, Benjamin A; Weinberg, David H; Wood-Vasey, W M; Yèche, Christophe; Zehavi, Idit; Zhao, Gong-Bo




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Third Street Tulsa, Oklahoma 74103-3502 918-595-6600 Fax 918-595-6656 www.swpa.gov The UPDATE is published by and for customers, retirees, and employees of Southwestern Power Administration like: Dudley Steele Electrician Jonesboro Maintenance Unit Special thanks to: Marshall Boyken Miya Boyken Mike Denny Ruben Garcia Gary Gregory William Hiller Rick Jones Darlene Low Jim McDonald Jerry Murr Beth Nielsen Rutha Williams Mistie Yost U P D AT E S O U T H W E S T E R N P O W E R A D M I N I S T R A T I O N J U LY - S E P T E M B E R 2 0 0 6 Gore Crew Utilizes More Horsepower Deep in a canyon in the Ozark National Forest this past summer, the Gore Maintenance Office discovered a stand of trees growing dangerously tall under a Southwestern transmission line. Tree-clearing outside the right-of-way by another entity's contractor


Electricity production and cooling energy savings from installation of a  

NLE Websites -- All DOE Office Websites (Extended Search)

production and cooling energy savings from installation of a production and cooling energy savings from installation of a building-integrated photovoltaic roof on an office building Title Electricity production and cooling energy savings from installation of a building-integrated photovoltaic roof on an office building Publication Type Journal Article Year of Publication 2013 Authors Ban-Weiss, George, Craig P. Wray, William W. Delp, Peter Ly, Hashem Akbari, and Ronnen M. Levinson Journal Energy and Buildings Volume 56 Pagination 210 - 220 ISSN 0378-7788 Keywords Advanced Technology Demonstration, building design, Building heat transfer, cool roof, energy efficiency, Energy Performance of Buildings, energy savings, Energy Usage, energy use, Heat Island Abstract Reflective roofs can reduce demand for air conditioning and warming of the atmosphere. Roofs can also host photovoltaic (PV) modules that convert sunlight to electricity. In this study we assess the effects of installing a building integrated photovoltaic (BIPV) roof on an office building in Yuma, AZ. The system consists of thin film PV laminated to a white membrane, which lies above a layer of insulation. The solar absorptance of the roof decreased to 0.38 from 0.75 after installation of the BIPV, lowering summertime daily mean roof upper surface temperatures by about 5 °C. Summertime daily heat influx through the roof deck fell to ±0.1 kWh/m2from 0.3-1.0 kWh/m2. However, summertime daily heat flux from the ventilated attic into the conditioned space was minimally affected by the BIPV, suggesting that the roof was decoupled from the conditioned space. Daily PV energy production was about 25% of building electrical energy use in the summer. For this building the primary benefit of the BIPV appeared to be its capacity to generate electricity and not its ability to reduce heat flows into the building. Building energy simulations were used to estimate the cooling energy savings and heating energy penalties for more typical buildings.



SciTech Connect

We report the discovery of a protocluster at z {approx} 6 containing at least eight cluster member galaxies with spectroscopic confirmations in the wide-field image of the Subaru Deep Field (SDF). The overdensity of the protocluster is significant at the 6{sigma} level, based on the surface number density of i'-dropout galaxies. The overdense region covers {approx}6' Multiplication-Sign 6' (14 Mpc Multiplication-Sign 14 Mpc in comoving units at z = 6) and includes 30 i'-dropout galaxies. Follow-up spectroscopy revealed that 15 of these are real z {approx} 6 galaxies (5.7 < z < 6.3). Of these 15, 8 are clustering in a narrow redshift range ({Delta}z < 0.05 centered at z = 6.01), corresponding to a seven-fold increase in number density over the average in redshift space. We found no significant difference in the observed properties, such as Ly{alpha} luminosities and UV continuum magnitudes, between the eight protocluster members and the seven non-members. The velocity dispersion of the eight protocluster members is 647 {+-} 124 km s{sup -1}, which is about three times higher than that predicted by the standard cold dark matter model. This discrepancy could be attributed to the distinguishing three-dimensional distribution of the eight protocluster members. We discuss two possible explanations for this discrepancy: either the protocluster is already mature, with old galaxies at the center, or it is still immature and composed of three subgroups merging to become a larger cluster. In either case, this concentration of z = 6.01 galaxies in the SDF may be one of the first sites of formation of a galaxy cluster in the universe.

Toshikawa, Jun; Kashikawa, Nobunari; Shibuya, Takatoshi; Ishizaki, Yoshifumi [Department of Astronomy, School of Science, Graduate University for Advanced Studies, Mitaka, Tokyo 181-8588 (Japan); Ota, Kazuaki; Nagao, Tohru [Department of Astronomy, Graduate School of Science, Kyoto University, Sakyo-ku, Kyoto 606-8502 (Japan); Morokuma, Tomoki; Motohara, Kentaro [Institute of Astronomy, University of Tokyo, Mitaka, Tokyo 181-0015 (Japan); Hayashi, Masao [Optical and Infrared Astronomy Division, National Astronomical Observatory, Mitaka, Tokyo 181-8588 (Japan); Jiang, Linhua; Egami, Eiichi [Steward Observatory, University of Arizona, 933 North Chery Avenue, Tucson, AZ 85721 (United States); Malkan, Matthew A. [Department of Physics and Astronomy, University of California, Los Angeles, CA 90095-1547 (United States); Shimasaku, Kazuhiro, E-mail: jun.toshikawa@nao.ac.jp [Department of Astronomy, University of Tokyo, Hongo, Tokyo 113-0033 (Japan)



Properties of solar polar coronal plumes constrained by Ultraviolet Coronagraph Spectrometer data  

E-Print Network (OSTI)

We investigate the plasma dynamics (outflow speed and turbulence) inside polar plumes. We compare line profiles (mainly of \\ion{O}{6}) observed by the UVCS instrument on SOHO at the minimum of solar cycle 22-23 with model calculations. We consider Maxwellian velocity distributions with different widths in plume and inter-plume regions. Electron densities are assumed to be enhanced in plumes and to approach inter-plume values with increasing height. Different combinations of the outflow and turbulence velocity in the plume regions are considered. We compute line profiles and total intensities of the \\ion{H}{1} Ly$\\alpha$ and the \\ion{O}{6} doublets. The observed profile shapes and intensities are reproduced best by a small solar wind speed at low altitudes in plumes that increases with height to reach ambient inter-plume values above roughly 3-4 $R_\\sun$ combined with a similar variation of the width of the velocity distribution of the scattering atoms/ions. We also find that plumes very close to the pole give narrow profiles at heights above 2.5 $R_\\sun$, which are not observed. This suggests a tendency for plumes to be located away from the pole. We find that the inclusion of plumes in the model computations provides an improved correspondence with the observations and confirms previous results showing that published UVCS observations in polar coronal holes can be roughly reproduced without the need for large temperature anisotropy. The latitude distributions of plumes and magnetic flux distributions are studied by analyzing data from different instruments on SOHO and with SOLIS.

N. -E. Raouafi; J. W. Harvey; S. K. Solanki