National Library of Energy BETA

Sample records for nearby www pages

  1. http://www.em.doe.gov/Pages/groundwaterReport.aspx?plumeCode...

    Office of Environmental Management (EM)

    Record 992011 http:www.em.doe.govPagesgroundwaterReport.aspx?plumeCode175 Environmental Indicators (EIs) Groundwater Migration Under Control? Yes Confirmed by Lead...

  2. http://www.em.doe.gov/Pages/groundwaterReport.aspx?plumeCode=10

    Office of Environmental Management (EM)

    Energy Transport Corridors

    doe.gov/media/Myths_and_Facts.pdf http://www.doe.gov/media/Myths_and_Facts.pdf http://www.doe.gov/media/Myths_and_Facts.pdf (143.91 KB) More Documents & Publications Biofuels & Greenhouse Gas Emissions: Myths versus Facts Microsoft Word - 47C468D4-69BA-281F40.doc Biofuels & Greenhouse Gas Emissions: Myths versus Facts

    South Valley Responsible DOE Office: Office of Environmental Management Plume Name: South Valley Plume Remediation Contractor:

  3. Page comments

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

    with-serial-codes-on-login-nodesPageComment101 http:www.nersc.govuserssoftwarecompilersintel-fortran-c-and-cintel-bug-reportsintel-uses-very-old-version-of-libstdc-by-de...

  4. http://www.cemp.dri.edu/cemp/climate/

    National Nuclear Security Administration (NNSA)

    Go Page 1 of 1 Community Environmental Monitoring Program | CEMP - DOE 5152011 http:www.cemp.dri.educempclimate

  5. Page 11, Links

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

    11 of 11 Previous Page Links Information for Employees & In-Processing DOE Order 3792.3 - Drug-Free Federal Workplace Testing http://www.archives.gov/federal-register/codification/executive-order/12564.html Flexible Spending Accounts (FSA) https://www.fsafeds.com/fsafeds/index.asp Pay & Pay Scales http://www.opm.gov/a-z-index/ Benefits Facts on Leave Programs http://www.opm.gov/policy-data-oversight/pay-leave/leave-administration/ Health Benefits

  6. Property:Foaf/Page | Open Energy Information

    Open Energy Info (EERE)

    "FoafPage" Showing 25 pages using this property. (previous 25) (next 25) " "The Future of Geothermal Energy" and Its Challenges + http:www.geothermal-energy.orgpdf...

  7. Property:FacebookPage | Open Energy Information

    Open Energy Info (EERE)

    search Property Name FacebookPage Property Type URL Description The URL for a Facebook page. It should start with https:www.facebook.com Pages using the property...

  8. http://www.epa.gov/climateleaders/smallbiz/footprint.html

    National Nuclear Security Administration (NNSA)

    you Climate Leaders Page 1 of 2 How to Calculate your Carbon Footprint | Climate Leaders | US EPA 5252011 http:www.epa.govclimateleaderssmallbizfootprint.html collect data ...

  9. http://www

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

    Schematic showing generic flight plan for sampling fields of cumulus within the plume emanating from Oklahoma City Source: http://www.asp.bnl.gov/ASP_ST_mtg_pres_2006/10.26_Berkowitz_CHAPS.pdf

  10. Computing at SSRL Home Page

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

    contents you are looking for have moved. You will be redirected to the new location automatically in 5 seconds. Please bookmark the correct page at http://www-ssrl.slac.stanford.edu/content/staff-resources/computer-networking-group

  11. WWW media distribution via Hopwise reliable multicast

    SciTech Connect (OSTI)

    Donnelley, J.E.

    1994-12-01

    Repeated access to WWW pages currently makes inefficient use of available network bandwidth. A Distribution Point Model is proposed where large and relatively static sets of pages (e.g. magazines or other such media) are distributed via bulk multicast to LAN distribution points for local access. Some access control issues are discussed. Hopwise Reliable Multicast (HRM) is proposed to simplify reliable multicast of non real time bulk data between LANs. HRM uses TCP for reliability and flow control on a hop by hop basis throughout a multicast distribution tree created by today`s Internet MBone.

  12. http://www.clarkcountynv.gov/depts/daqem/Pages/default.aspx

    National Nuclear Security Administration (NNSA)

    with your stationary source permit application or a compliance issue? More Information Air Quality The Department of Air Quality and Environmental Management is the air...

  13. http://www.clarkcountynv.gov/depts/daqem/Pages/default.aspx

    National Nuclear Security Administration (NNSA)

    More Information Air Quality The Department of Air Quality and Environmental Management is the air pollution control agency for all of Clark County, Nevada. Established by the ...

  14. http://www.em.doe.gov/Pages/Transportation.aspx

    National Nuclear Security Administration (NNSA)

    regarding this site should be sent to EM Web Feedback You are here: EM Home > Packaging ... DC 20585 1-800-dial-DOE | f202-586-4403 Web Policies | No Fear Act | Site Map | Privacy ...

  15. http://www.sord.nv.doe.gov/meda_wind_roses_by_station_numbe.htm

    National Nuclear Security Administration (NNSA)

    Phone: Contact - (702) 295-1232 Fax - (702) 295-3068 http:www.sord.nv.doe.gov Report web page problems to: SORD Webmaster Page 1 of 2 SORD MEDA Wind Roses 5162011 http:...

  16. DATE: PAGE:

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

    PAGE: of NEPA COMPLIANCE OFFICER: 2015 Annual NEPA Planning Summary TYPE: STATUS: COST: NOIEAD: DRAFT: FINAL: DOCUMENT NUMBER & TITLE DESCRIPTION COMMENT TYPE: STATUS: COST:...

  17. DATE: PAGE:

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

    PAGE: of NEPA COMPLIANCE OFFICER: 2016 Annual NEPA Planning Summary TYPE: STATUS: COST: NOI/EAD: DRAFT: FINAL: DOCUMENT NUMBER & TITLE DESCRIPTION / COMMENT TYPE: STATUS: COST: NOI/EAD: DRAFT: FINAL: DOCUMENT NUMBER & TITLE DESCRIPTION / COMMENT TYPE: STATUS: COST: NOI/EAD: DRAFT: FINAL: DOCUMENT NUMBER & TITLE DESCRIPTION / COMMENT TYPE: STATUS: COST: NOI/EAD: DRAFT: FINAL: DOCUMENT NUMBER & TITLE DESCRIPTION / COMMENT TYPE: STATUS: COST: NOI/EAD: DRAFT: FINAL: DOCUMENT NUMBER

  18. WIPP Home Page Search

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

    Home Page Search Enter word(s) to search for on the WIPP Home Page: Search

  19. AMO Test page

    Broader source: Energy.gov [DOE]

    http://www.nrel.gov/docs/fy03osti/31919.pdfhttp://www1.eere.energy.gov/library/pdfs/itp/partnering_for_success.pdfhttp://www.eere.energy.gov/manufacturing/tech_deployment/pdfs/mtrmkt.pdfhttp://www...

  20. http://www.sord.nv.doe.gov/MEDAStationInfo-tng.htm

    National Nuclear Security Administration (NNSA)

    ... Phone: Contact - (702) 295-1232 Fax - (702) 295-3068 http:www.sord.nv.doe.gov Report web page problems to: SORD Webmaster Date Modified: 031208 ||Home | Privacy Policy | ...

  1. ARM - Front Page

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

    Page Front Page World's premier ground-based observations facility advancing climate change research A U.S. Department of Energy Office of Science user facility, providing data...

  2. Aprun MAN Page

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

    Aprun MAN Page Aprun MAN Page aprun -a arch -b -B -cc cpulist | keyword -cp cpuplacementfilename -d depth -D value -L nodelist -m sizeh|hs -n...

  3. Main Page Main Page: Find energy information and data. Share...

    Open Energy Info (EERE)

    Main Page Main Page: Find energy information and data. Share knowledge. Connect with people. energy datasets energy community Main Page energy information open data 0...

  4. 1. CONTRACT ID CODE PAGE OF PAGES

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

    CONTRACT ID CODE PAGE OF PAGES AMENDMENT OF SOLICITATION/MODIFICATION OF CONTRACT I1 1 1 3 2. AMvEND)MENfmODIFICATION NO. 3 EFFECT IVE DATE (M'D/)Y) 4 REQUISITION/PURCHASE REQ. NO 5.PROJECT NO. (If applicable, 240 See Block 16C 12EM000054 T 6. ISSUFD BY CODE 7. ADMINISTE'RED BY GIf aher than Item 6)1 CODE U.S. Department of Energy Office of River Protection P. 0. Box 450, MS 1-6-60 Richland, WA 99352 8 NAvM AND ADDRESS OF CONTRACTOR (No., wreel, county, Sltate and ZIP code) 9A. AMENDMENT OF

  5. NREL: Photovoltaics Research - Matthew Page

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

    Matt Page Senior Engineer Photo of Matt Page 303-384-6648 Matthew.Page@nrel.gov Matthew Page received his bachelor's degree in engineering physics from the Colorado School of Mines...

  6. Energy Efficiency -- Home Page

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

    If you are having trouble, call 202-586-8800 for help. Home >Energy Users EEnergy Efficiency Page Energy-Efficiency Measurement MEASUREMENT DISCUSSION: Measures and Policy Issues...

  7. CAMD Cleanroom Login Page

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

    Cleanroom Equipment Booking Page Microfabrication Home Please enter in your User ID and Password below. UserID Password Login Forgot your password?

  8. Page Under Construction | Department of Energy

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

    Page Under Construction Page Under Construction This page is currently under construction.

  9. http://www.em.doe.gov/Pages/groundwaterReport.aspx?plumeCode=16

    Office of Environmental Management (EM)

    Shiprock Responsible DOE Office: Office of Environmental Management Plume Name: Shiprock Remediation Contractor: S. M. Stoller Corporation Report Last Updated: 2009 Contaminants Halogenated VOCs/SVOCs Present? No Fuel Present? No Metals Present? Yes Metal Name Metal Concentration (ppb) Regulatory Driver Cleanup Requirement Mn 8300 No Se 530 Yes 0.05 U 2600 Yes 0.044 Isotopes Present? Yes Isotope Name Isotope Activity (pCi/l) Regulatory Driver Cleanup Requirement Sr 11000 No Explosives Present?

  10. http://www.em.doe.gov/Pages/groundwaterReport.aspx?plumeCode=16

    Office of Environmental Management (EM)

    Old North Continent Responsible DOE Office: Office of Legacy Management Plume Name: Slick Rock - Old North Continent Remediation Contractor: Unknown Report Last Updated: 2009 Contaminants Halogenated VOCs/SVOCs Present? No Fuel Present? No Metals Present? Yes Metal Name Metal Concentration (ppb) Regulatory Driver Cleanup Requirement Se 11.55 Yes 10 U 616.5 Yes 440 Isotopes Present? No Explosives Present? Yes Other Contaminants?No Tritium Present? No Nitrates Present? No Sulfates Present? No

  11. http://www.em.doe.gov/Pages/groundwaterReport.aspx?plumeCode=16

    Office of Environmental Management (EM)

    Union Carbide Responsible DOE Office: Office of Environmental Management Plume Name: Slick Rock - Union Carbide Remediation Contractor: Unknown Report Last Updated: 2009 Contaminants Halogenated VOCs/SVOCs Present? No Fuel Present? No Metals Present? Yes Metal Name Metal Concentration (ppb) Regulatory Driver Cleanup Requirement Se 2600 Yes 180 Mo 2200 Yes 100 U 111 Yes 44 Isotopes Present? No Explosives Present? Yes Other Contaminants?No Tritium Present? No Nitrates Present? Yes Concentration:

  12. http://www.em.doe.gov/Pages/groundwaterReport.aspx?plumeCode=17

    Office of Environmental Management (EM)

    Spook Responsible DOE Office: Office of Environmental Management Plume Name: Spook Remediation Contractor: Unknown Report Last Updated: 2009 Contaminants Halogenated VOCs/SVOCs Present? No Fuel Present? No Metals Present? Yes Metal Name Metal Concentration (ppb) Regulatory Driver Cleanup Requirement Cr (total) No Se 0 No U No Isotopes Present? Yes Isotope Name Isotope Activity (pCi/l) Regulatory Driver Cleanup Requirement other (provide names) Ra-226 No other (provide names) Ra-228 No Explosives

  13. http://www.em.doe.gov/Pages/groundwaterReport.aspx?plumeCode=17

    Office of Environmental Management (EM)

    Tuba City Responsible DOE Office: Office of Legacy Management Plume Name: Tuba City Remediation Contractor: Unknown Report Last Updated: 2009 Contaminants Halogenated VOCs/SVOCs Present? No Fuel Present? No Metals Present? Yes Metal Name Metal Concentration (ppb) Regulatory Driver Cleanup Requirement Se 50 Yes 10 Mo 300 Yes 100 U 250 Yes 44 Isotopes Present? No Explosives Present? Yes Other Contaminants?No Tritium Present? No Nitrates Present? Yes Concentration: 1000 (ppb) Regulatory Driver: Yes

  14. http://www.em.doe.gov/Pages/groundwaterReport.aspx?plumeCode=17

    Office of Environmental Management (EM)

    East Plume) Remediation Contractor: Unknown Report Last Updated: 2009 Contaminants Halogenated VOCs/SVOCs Present? No Fuel Present? No Metals Present? No Isotopes Present? No Explosives Present? No Explosive Name Explosive Concentration (ppb) Regulatory Driver Cleanup Requirement TNT (trinitrotoluene) 21 Yes 2.8 other (provide names) 2,4-DNT 200 Yes 0.11 other (provide names) 2,6-DNT 222 Yes 1.3 other (provide names) 1,3-DNB 0.16 Yes 1 Other Contaminants?No Tritium Present? No Nitrates Present?

  15. http://www.em.doe.gov/Pages/groundwaterReport.aspx?plumeCode=17

    Office of Environmental Management (EM)

    Legacy Management Plume Name: Chemical Plant (Quarry) Remediation Contractor: SM Stoller Report Last Updated: 2009 Contaminants Halogenated VOCs/SVOCs Present? No Fuel Present? No Metals Present? Yes Metal Name Metal Concentration (ppb) Regulatory Driver Cleanup Requirement U 3486 Yes 30 Isotopes Present? No Explosives Present? Yes Explosive Name Explosive Concentration (ppb) Regulatory Driver Cleanup Requirement DNT (dinitrotoluene) 9.3 Yes 0.11 Other Contaminants?No Tritium Present? No

  16. http://www.em.doe.gov/Pages/groundwaterReport.aspx?plumeCode=17

    Office of Environmental Management (EM)

    VOC) Remediation Contractor: Unknown Report Last Updated: Unknown Contaminants Halogenated VOCs/SVOCs Present? Yes VOC Name Concentration (ppb) Regulatory Driver Cleanup Requirement TCE No Fuel Present? No Metals Present? No Isotopes Present? No Explosives Present? No Other Contaminants?No Tritium Present? No Nitrates Present? No Sulfates Present? No Hydrogeology Conduit Flow? Yes Multiple Units Affected? No Depth (feet): Avg Velocity (feet/year): Plume Information (no source) Source Plume

  17. http://www.em.doe.gov/Pages/groundwaterReport.aspx?plumeCode=17

    Office of Environmental Management (EM)

    West Plume) Remediation Contractor: SM Stoller Corp Report Last Updated: 2009 Contaminants Halogenated VOCs/SVOCs Present? Yes VOC Name Concentration (ppb) Regulatory Driver Cleanup Requirement TCE 763 Yes 5 Fuel Present? No Metals Present? Yes Metal Name Metal Concentration (ppb) Regulatory Driver Cleanup Requirement U 264 Yes 20 Isotopes Present? No Explosives Present? Yes Explosive Name Explosive Concentration (ppb) Regulatory Driver Cleanup Requirement DNT (dinitrotoluene) Yes 0.11 Other

  18. http://www.em.doe.gov/Pages/groundwaterReport.aspx?plumeCode...

    Office of Environmental Management (EM)

    Plume) Remediation Contractor: SM Stoller Corp Report Last Updated: 2009 Contaminants Halogenated VOCsSVOCs Present? Yes VOC Name Concentration (ppb) Regulatory Driver Cleanup...

  19. http://www.eia.doe.gov/cneaf/coal/page/coaldistrib/distable1...

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

    Glossary Home > Coal > Domestic and Foreign Distribution of U.S. Coal by Origin Domestic and Foreign Distribution of U.S. Coal by State of Origin Release Date: January 2006 Next...

  20. http://www.em.doe.gov/Pages/groundwaterReport.aspx?plumeCode...

    Office of Environmental Management (EM)

    Legacy Management Plume Name: Chemical Plant (Quarry) Remediation Contractor: SM Stoller ... by naturally occurring chemical reduction process and absorption onto aquifer materials. ...

  1. http://www.em.doe.gov/Pages/groundwaterReport.aspx?plumeCode...

    Office of Environmental Management (EM)

    Source Aquifer? No Does an Exit Strategy Exist? No Basis for Exit Strategy: No Response Environmental Indicators (EIs) Groundwater Migration Under Control? No Confirmed by Lead...

  2. Data Release Page

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

    Data Release Page This page provides links to data (histograms, error matrices, ntuples, etc.) released in association with MINERvA publications. MINERvA Collaboration, L. Aliaga, M. Kordosky, T. Golan et al,"Neutrino Flux Predictions for the NuMI Beam" hep-ex/1607.00704.[Data Release Page] MINERvA Collaboration, Z. Wang, C.M. Marshall et al.,"First Evidence of Coherent Production of K + in Neutrino Interactions on Carbon Nuclei"hep-ex/1606.08890. MINERvA Collaboration, C.M.

  3. PAGES_C211

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

    osti.gov The DOE public access tool for scholarly publications A portal to journal articles and accepted manuscripts resulting from DOE-funded research www.osti.govpages DOE...

  4. DOE PAGES Beta

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

    portal to journal articles and accepted manuscripts resulting from DOE-funded research DOE PAGES Beta is the DOE response to the February 2013 White House Office of Science and...

  5. Featured Topic Pages

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

    Featured Topic Pages * Renowned scientists, with information about the scientists' R&D results * Significant DOE research disciplines, with R&D results * Manhattan Project, including scientists and key events Laureates * Nobel Prize winners associated with DOE and predecessor agencies * Winners of the Enrico Fermi Award, a U.S. Presidential award Database * Selected documents about noteworthy R&D results * Documents and individual pages searchable by word or phrase * Tag cloud

  6. Energy.gov Page Types

    Broader source: Energy.gov [DOE]

    Learn about the standard page types available in the Energy.gov Drupal content management system. For information about other available page types, or to request a new kind of page type, contact...

  7. Item Not Found | DOE PAGES

    Office of Scientific and Technical Information (OSTI)

    requested, OSTI ID 1182424, is not available in this collection. If you followed a link to this page, that link is outdated or contains an error. Search DOE PAGES DOE PAGES Home

  8. Sample page | Open Energy Information

    Open Energy Info (EERE)

    Sample pages; Help pages; References Francis C. Monastero. 2002. An overview of industry-military cooperation in the development of power operations at the Coso...

  9. Aprun MAN Page

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

    aprun » Aprun MAN Page Aprun MAN Page aprun [-a arch ] [-b ] [-B] [-cc cpu_list | keyword ] [-cp cpu_placement_file_name ] [-d depth ] [-D value ] [-L node_list ] [-m size[h|hs] ] [-n pes ] [-N pes_per_node ][-F access mode ] [-q ] [-r cores][-S pes_per_numa_node ] [-sl list_of_numa_nodes ] [-sn numa_nodes_per_node ] [-ss ] [-T ] [-t sec ] executable [ arguments_for_executable ] IMPLEMENTATION Cray Linux Environment (CLE) DESCRIPTION To run an application on CNL compute nodes, use the

  10. Palm Physics Page

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

    Palm Physics Page ** We no longer support this website. This is a preliminary group of Palm applications/databases that are intended to serve the interests of atomic, nuclear and particle physics. Applications Periodic Table: Shareware version of the periodic table with basic chemical properties of the elements.(Download) Particle Data Book: From the Particle Data Group at LBL. (Download) Heavy Ion Fusion Calculator: Compute available energy, Coulomb energy, maximum angular momentum for compound

  11. PAGE Cover: Top Photo

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

    PAGE Cover: Top Photo Energy Sciences Building. Elevation of the recently completed Energy Sciences Building (ESB) project at Argonne National Laboratory in Lemont, Illinois. The ESB was a capital line-item project funded by the Science Laboratories Infrastructure program at a total cost of $96 million and was completed on August 6, 2014. The ESB project provided 173,000 gross square feet of interdisciplinary research and collaborative space to accommodate a range of physical sciences research

  12. Source: Greentech Media; http://www.greentechmedia.com/articles...

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

    Source: Greentech Media; http:www.greentechmedia.comarticlesreadchart-of-the-day- solyndra-edition...

  13. Create Page | Open Energy Information

    Open Energy Info (EERE)

    try using the search feature to see if the page or topic already exists. If so, feel free to add to or edit that page using the Edit or Edit With Form button at the top of the...

  14. THIS PAGE INTENTIONALLY LEFT BLANK

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

    THIS PAGE INTENTIONALLY LEFT BLANK i U.S. DEPARTMENT OF ENERGY CRITICAL MATERIALS STRATEGY DECEMBER 2011 ii THIS PAGE INTENTIONALLY LEFT BLANK iii TABLE OF CONTENTS FOREWORD ........................................................................................................................................................... 1 ACKNOWLEDGEMENTS .......................................................................................................................................... 2 EXECUTIVE

  15. Geothermal Technologies Office Home Page | Department of Energy

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

    Technologies Office Home Page Geothermal Technologies Office Home Page

  16. Final Meeting Summary Page 1

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

    ... administrative controls, worker training, industrial hygiene procedures, occupational medicine programs and oversight 2009-present" Final Meeting Summary Page 4 Health, Safety ...

  17. Web Page Error 404.1 Page Cannot be Found

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

    Us Media Center Contact Us Site Map The page you are looking for cannot be found. The Web site you are looking for is unavailable due to its identification configuration...

  18. Web Page Error 404.1 Page Cannot be Found

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

    ... About ORISE Safety Careers Working with Us Media Center Contact Us Site Map The page you are looking for cannot be found. The Web site you are looking for is unavailable due to its ...

  19. name SRSCRO description url http www srscro org namespaces oembed...

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

    description url http www srscro org namespaces oembed authentication routes namespace methods GET endpoints methods GET args context required false default view links self http...

  20. http://www.ars.usda.gov/research/publications/Publications.htm...

    National Nuclear Security Administration (NNSA)

    - Ed Wagner, Larry Tatarko, John Publications Publications Related National Programs Air Quality (203) Soil Resource Management (202) Page 1 of 2 ARS | Publication request:...

  1. SSRL Accelerator Phycics Home Page

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

    at.gif (15297 bytes) BeamOptics.gif (29047 bytes) ICFA2000t.gif (31362 bytes) Home Page LCLS Accelerator Physics at SSRL The field tha t can be covered by the Accelerator Physics...

  2. Tank Waste Committee Page 1

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

    ... He said the genesis of this cycle was in 2006 when C Farm demolition plans were approved ... Tank Waste Committee Page 9 Final Meeting Summary June 9, 2011 Chris said the pipeline ...

  3. Final Meeting Summary Page 1

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

    ... Grindstaff, DOE-ORP Ginger Wireman, Ecology Sharon Braswell, MSA Steve Pfaff, DOE-ORP Hillary Johnson, EnviroIssues Abby Chazanow, EnviroIssues Final Meeting Summary Page 16 Tank ...

  4. Help:User page | Open Energy Information

    Open Energy Info (EERE)

    User page Jump to: navigation, search A user page is a page about a wiki user; someone who registered on the wiki, and is (most probably) a contributor. If you have registered, you...

  5. SF30 Continuation Page, Block 14

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

    ... Page 9 of 12 Contract DE-AC27-08RV 14800 Modification 083 SF30 Continuation Page, Block 14 7. Update Section J, J-4 Performance Evaluation and Measurement Plan (PEMP), page ...

  6. ATVM 1-Page Summary | Department of Energy

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

    1-Page Summary ATVM 1-Page Summary ATVM 1-Page Summary Jan 2016.pdf (1.46 MB) More Documents & Publications ATVM Program Overview 2015 Advanced Technology Vehicles Manufacturing Loan Program DOE-LPO_Outreach_LPO-Overview_CSP

  7. Help:Protected pages | Open Energy Information

    Open Energy Info (EERE)

    only sysop users can protect a page in the first place, or unprotect the page to lift the restriction. There are several reasons why a particular page might be protected: On...

  8. Widget:CreatePage | Open Energy Information

    Open Energy Info (EERE)

    CreatePage Jump to: navigation, search This is a widget containing HTML for creating new pages Parameters none - This is an HTML form for creating a page. Usage...

  9. Template:PageMeta | Open Energy Information

    Open Energy Info (EERE)

    Jump to: navigation, search This is the PageMeta template. It is used to assign special meta properties to a page with the intent of increasing the page's LOD and SEO exposure....

  10. Help:Special pages | Open Energy Information

    Open Energy Info (EERE)

    pages Jump to: navigation, search Special pages are pages that are created by the software on demand. They are located in their own namespace Special: and are not editable...

  11. IP Kids Page | The Ames Laboratory

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

    belinblankStudentsinventia InventNow.org - World: http:www.inventnow.org American Intellectual Property Law Association: http:www.aipla.orgcommitteescommitteepages...

  12. EERE: Alternative Fuels Data Center Home Page

    Alternative Fuels and Advanced Vehicles Data Center [Office of Energy Efficiency and Renewable Energy (EERE)]

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Delicious Rank EERE: Alternative Fuels Data Center Home Page on Digg Find More places to share EERE: Alternative Fuels

  13. NewPage Demonstration-Scale Biorefinery

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

    in Wisconsin (NewPage Corporation in Wisconsin Rapids and Flambeau River Papers, LLC in Park Falls). NewPage and Flambeau River have demonstrated successful collaboration on...

  14. Household Vehicles Energy Use Cover Page

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

    Energy Use Cover Page Glossary Home > Households, Buildings & Industry >Transportation Surveys > Household Vehicles Energy Use Cover Page Contact Us * Feedback * PrivacySecurity *...

  15. NewPage Corporation | Department of Energy

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

    NewPage Corporation NewPage Corporation Construct and operate a thermal gasification and gas-to-liquids plant. PDF icon newpagefactsheet040308.pdf More Documents & Publications ...

  16. http://www.epa.gov/climateleaders/smallbiz/footprint.html

    National Nuclear Security Administration (NNSA)

    What Do I Do Next? Join the Climate Leaders Small Business Network to set a goal, share ... 2010 Page 2 of 2 How to Calculate your Carbon Footprint | Climate Leaders | US EPA 514

  17. http://www.wrcc.dri.edu/summary/nvut.html

    National Nuclear Security Administration (NNSA)

    Select from the list to the left in such cases. Western Regional Climate Center, wrcc@dri.edu Big Ben Ranger Stn (COOP) Page 1 of 1 WRCC cgi generated image map 5162011 http:...

  18. http://www.cityofnorthlasvegas.com/departments/fire/fire.shtm

    National Nuclear Security Administration (NNSA)

    ... with Disabilities Act, an accessible version of content can be requested for this web page by clicking here, calling (800) 326-6868 for Telecommunications Device for the Deaf ...

  19. Property:NEPA SerialRegisterPage | Open Energy Information

    Open Energy Info (EERE)

    SerialRegisterPage Jump to: navigation, search Property Name NEPA SerialRegisterPage Property Type Page Description Serial Register Page files for NEPA Docs. Related Serial...

  20. Hanford Advisory Board Page 1

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

    Page 1 Final Meeting Summary November 1-2, 2012 FINAL MEETING SUMMARY HANFORD ADVISORY BOARD November 1-2, 2012 Richland, WA Topics in This Meeting Summary Executive Summary ...................................................................................................................................... 1 Welcome, Introductions, and Announcements ............................................................................................. 3 Tri-Party Agreement Agencies - Program

  1. pages)

    Energy Savers [EERE]

    origins.indd origins.indd origins.indd (6.28 MB) More Documents & Publications Fehner and Gosling, Origins of the Nevada Test Site Fehner and Gosling, Atmospheric Nuclear Weapons Testing, 1951-1963. Battlefield of the Cold War: The Nevada Test Site, Volume I NTS_History.indd

  2. pages)

    Energy Savers [EERE]

  3. Page

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

    Packaging and Transportation Packaging and Transportation Packaging and Transportation Radiological shipments are accomplished safely. Annually, about 400 million hazardous materials shipments occur in the United States by rail, air, sea, and land. Of these shipments, about three million are radiological shipments. Since Fiscal Year (FY) 2004, EM has completed over 150,000 shipments of radioactive material/waste. Please click here to see Office of Packaging and Transportation Fiscal Year 2012

  4. Page

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

    ... was turbulent, the bubble motion appears to quickly change the structure of the turbulence in major ways. ... A single-phase turbulent velocity profile is first generated by ...

  5. Page

    Gasoline and Diesel Fuel Update (EIA)

    ... Peru PE501 Loreto 34 0.3 PE502 Talara 32.7 0.1 PE505 High Cold Test 37.5 NA PE506 Bayovar 22.6 NA PE507 Low Cold Test 34.3 NA PE508 Carmen Central-5 20.7 NA PE509 Shiviyacu-23 20.8 ...

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

    ... 03 Orange, TX 04 Beaumont, TX (including Port Neches) 23 LAREDO, TEXAS 01 Brownsville-Cameron County (including Port Isabel) 02 Del Rio 03 Eagle Pass 04 Laredo 05 HildagoPharr 07 ...

  7. ARM - Low Bandwidth Data Page

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

    LinksLow Bandwidth Data Page Related Links ISDAC Home AAF Home AVP Aircraft Instrumentation, October 14-16, 2008 ARM Data Discovery Browse Data Post-Campaign Data Sets Flight Summary Table (PDF, 440K) ISDAC Wiki Mission Summary Journal Deployment Resources NSA Site ARM Data Plots Quick Links Experiment Planning ISDAC Proposal Abstract Full Proposal (pdf, 1,735K) Science Questions Science Overview Document for ISDAC (pdf, 525K) ISDAC Flight Planning Document (PDF, 216K) Collaborations Logistics

  8. http://www.wipp.ws/TeamWorks/truteamworks.htm

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

    2/04 Shipments expected this week: RFETS (13), SRS (6) A weekly e-newsletter for the Waste Isolation Pilot Plant team February 12, 2004 The Big Story SEGA and MEGA exemplify science@wipp Topics Characterization News Transportation News Disposal News Safety News Working Smart Announcements Tools Acronym List Back to Main Page WIPP Home Page Links Feedback Contact us with feedback or submit your e-mail address for updates. Click here to e-mail. WIPP Shipments (as of 02/12/04 at 9:24 a.m.)

  9. http://www.wipp.ws/TeamWorks/truteamworks.htm

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

    9/04 Shipments expected this week: SRS (6) A weekly e-newsletter for the Waste Isolation Pilot Plant team February 19, 2004 The Big Story WIPP public information meetings held Topics Characterization News Transportation News Disposal News Safety News Working Smart Announcements Tools Acronym List Back to Main Page WIPP Home Page Links Feedback Contact us with feedback or submit your e-mail address for updates. Click here to e-mail. WIPP Shipments (as of 02/19/04 at 6:55 a.m.) Shipments scheduled

  10. http://www.wipp.ws/TeamWorks/truteamworks.htm

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

    26/04 Shipments expected for the week of 02/22/04 through 2/28/04: Hanford (2), RFETS (11), SRS (6) A weekly e-newsletter for the Waste Isolation Pilot Plant team February 26, 2004 The Big Story WIPP impacts international Waste Management Symposium Topics Characterization News Transportation News Disposal News Safety News Working Smart Announcements Tools Acronym List Archives Back to Main Page WIPP Home Page Links Feedback Contact us with feedback or submit your e-mail address for updates.

  11. http://www.wipp.ws/TeamWorks/truteamworks.htm

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

    5/04 | Shipments expected for the week of 03/14/04 through 3/20/04: INEEL (4), Hanford (2), RFETS (11), SR A weekly e-newsletter for the Waste Isolation Pilot Plant team March 15, 2004 Topics Characterization News Transportation News Disposal News Safety News Working Smart Announcements Tools Acronym List Archives Back to Main Page WIPP Home Page Links Feedback Contact us with feedback or submit your e-mail address for updates. Click here to e-mail. WIPP Shipments (as of 03/15/04 at 8:59 a.m.)

  12. http://www.wipp.ws/TeamWorks/truteamworks.htm

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

    8/04 | Shipments expected for the week 3/21/04 through 3/27/04: Hanford (2), INEEL (3), RFETS (11), SRS A weekly e-newsletter for the Waste Isolation Pilot Plant team March 18, 2004 The Big Story WIPP personnel overcome evacuation order Topics Characterization News Transportation News Disposal News Safety News Working Smart Announcements Tools Acronym List Archives Back to Main Page WIPP Home Page Links Feedback Contact us with feedback or submit your e-mail address for updates. Click here to

  13. http://www.wipp.ws/TeamWorks/truteamworks.htm

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

    25/04 | Shipments expected for the week 3/28/04 through 4/3/04: INEEL (2), RFETS (11), SRS (6) A weekly e-newsletter for the Waste Isolation Pilot Plant team March 25, 2004 The Big Story AMWTP sends first shipment to WIPP Topics Characterization News Transportation News Disposal News Safety News Working Smart Announcements Tools Acronym List Archives Back to Main Page WIPP Home Page Links Feedback Contact us with feedback or submit your e-mail address for updates. Click here to e-mail. WIPP

  14. Cover Page of Household Vehicles Energy Use: Latest Data & Trends

    Gasoline and Diesel Fuel Update (EIA)

    Household Vehicles Energy Use Cover Page Cover Page of Household Vehicles Energy Use: Latest Data & Trends...

  15. Category:RecipePage | Open Energy Information

    Open Energy Info (EERE)

    in category "RecipePage" The following 10 pages are in this category, out of 10 total. K KeithPao M Mutton Rogan Josh MyRecipe P Pork R User:Rmckeel S Sambar Help:Sandbox...

  16. Page Electric Utility | Open Energy Information

    Open Energy Info (EERE)

    Page Electric Utility Jump to: navigation, search Name: Page Electric Utility Place: Arizona Phone Number: (928) 645-2419 Website: pageutility.com Outage Hotline: (928) 645-2419...

  17. Template:RecipePage | Open Energy Information

    Open Energy Info (EERE)

    RecipePage Jump to: navigation, search This is the "RecipePage" template. Description RecipeDescription - describing the recipe RecipeInstructions - steps to prepare Usage It...

  18. Search for: All records | DOE PAGES

    Office of Scientific and Technical Information (OSTI)

    Switch to Detail View for this search DOE PAGES Search Results Page 1 of 1 Search for: All records 8 results for: All records CreatorsAuthors contains: "Kioupakis, Emmanouil" ...

  19. Search for: All records | DOE PAGES

    Office of Scientific and Technical Information (OSTI)

    Switch to Detail View for this search DOE PAGES Search Results Page 1 of 1 Search for: All records 3 results for: All records CreatorsAuthors contains: "Bhattacharya, Anand" ...

  20. Export pages to RDF | Open Energy Information

    Open Energy Info (EERE)

    obtain data from a page in RDF format. To export pages, enter the titles in the text box below, one title per line. Export Retrieved from "http:en.openei.orgwiki...

  1. Search for: All records | DOE PAGES

    Office of Scientific and Technical Information (OSTI)

    Switch to Detail View for this search DOE PAGES Search Results Page 1 of 1 Search for: All records Author ORCID ID is 000000018654847X Sort by Relevance Sort by Date (newest...

  2. Search for: All records | DOE PAGES

    Office of Scientific and Technical Information (OSTI)

    Switch to Detail View for this search DOE PAGES Search Results Page 1 of 1 Search for: All records CreatorsAuthors contains: "Sharma, Anand" Sort by Relevance Sort by Date...

  3. OHA Archive Download Page | Department of Energy

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

    OHA Archive Download Page OHA Archive Download Page OHA FOIA Cases Archive File OHA Security Cases Archive File OHA Whistleblower Cases Archive File OHA EIA Cases Archive File OHA ...

  4. Neutrino CCQE Data Release Page

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

    Neutrino CCQE Data Release Page "Measurement of Muon Neutrino Quasi-Elastic Scattering on a Hydrocarbon Target at Ev ~ 3.5 GeV" Phys. Rev. Lett. 111 (2013) 022502, hep-ex/1305.2243 Data Ancillary data files for this result are given here, and supercede the ones originally associated with the arXiv entry: they have been updated with MINERvA's best estimate of the NuMI neutrino flux. The available data files have the following format: The columns are Q2 bins, first the 8 neutrino and

  5. Antineutrino CCQE Data Release Page

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

    Antineutrino CCQE Data Release Page "Measurement of Muon Antineutrino Quasi-Elastic Scattering on a Hydrocarbon Target at Ev ~ 3.5 GeV" Phys. Rev. Lett. 111 (2013) 022501, hep-ex/1305.2234 Data Ancillary data files for this result are given here, and supercede the ones originally associated with the arXiv entry: they have been updated with MINERvA's best estimate of the NuMI neutrino flux. The available data files have the following format: The columns are Q2 bins, first the 8 neutrino

  6. Microsoft Word - page_abstract

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

    7, at 3:00 pm "Probing Nuclear Structure beyond the Proton Drip Line" Prof. Robert Page Dept. of Physics, University of Liverpool, UK Understanding nuclei at the limits of existence is a major challenge in nuclear physics and impressive advances in addressing this issue are being achieved. At the limits of proton-rich nuclei, over 30 proton emitters have been discovered to date. This success has been made possible by exploiting recoil separators capable of isolating ephemeral species

  7. Coherent Pion data release page

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

    Coherent Pion data release page "Measurement of Coherent Production of π± in Neutrino and Anti-Neutrino Beams on Carbon from E_nu of 1.5 to 20 GeV" Phys. Rev. Lett. 113 (2014) 261802, hep-ex/1409.3835 Data Ancillary data files for this result are available on arXiv at http://arxiv.org/src/1409.3835/anc.< /li> Among the available data files are: Scale factors (obtained from background fits) applied to different GENIE 2.6.2 background sources. Fractional systematic uncertainties

  8. CC Kaon Data Release Page

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

    CC Kaon Data Release Page Measurement of Charged Current muon neutrino production of K+ Phys. Rev. D 94, 012002 and hep-ex/1604.03920 Data Ancillary data files for this result are available on arXiv at http://arxiv.org/src/1604.03920/anc Among the available data files are: Cross Sections with Uncertainties Flux Covariance Matrix Covariance Matrix of flux uncertainties Covariance Matrix of uncertainties OTHER than those coming from the flux Contact Information For information on use of this

  9. EM Launches Facebook Page | Department of Energy

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

    Launches Facebook Page EM Launches Facebook Page May 31, 2016 - 4:30pm Addthis EM Launches Facebook Page WASHINGTON, D.C. - EM has created its own Facebook page. Please like our page to keep up to date with EM's progress across the complex, as well as to learn more about the history of our sites, the work that we do, and our workforce. Keep an eye out for #TeardownTuesday, #WildlifeWednesday and #FlashbackFriday! EM is also on social media via our YouTube playlist and our Flickr account. Addthis

  10. http://www.energy.gov/print/6310.htm

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

    News Media Contact(s): Angela Hill, (202) 586-4940 For Immediate Release June 3, 2008 DOE Marks Milestone in Submitting Yucca Mountain License Application WASHINGTON, DC - The U.S. Department of Energy (DOE) today announced submittal of a license application (LA) to the U.S. Nuclear Regulatory Commission (NRC) seeking authorization to construct America's first repository for spent nuclear fuel and high-level radioactive waste at Yucca Mountain, Nevada. The 8,600 page application describes DOE's

  11. Help:Protecting and unprotecting pages | Open Energy Information

    Open Energy Info (EERE)

    pages Jump to: navigation, search Protecting and unprotecting pages is very straightforward, but these operations require sysop permissions. You can designate a page as a...

  12. Property:SpecPage | Open Energy Information

    Open Energy Info (EERE)

    uploads201412HydroLevel-Buoy.pdf + MHK ISDBInstrumentsAirMar 42183 Heading Sensor + http:www.airmartechnology.comuploadsbrochuresH2183.pdf + MHK ISDBInstruments...

  13. Color Page Charges | The Ames Laboratory

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

    Scientific and Technical Information Color Page Charges Color Page Charges Agreeing to pay color page charges is at the discretion of each individual Program at the Ames Laboratory. If a publisher charges for color and you need to have all or some of your figures printed in color, please have your program office prepare a purchase order, provide proper justification, and theywill have your Program Director sign it. You must obtain the Program Director's signature when requesting payment of

  14. Webtrends Archives by Fiscal Year - Topic Landing Pages | Department...

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

    topic landing pages by fiscal year. Topic Landing Pages FY10 (2.04 MB) Topic Landing Pages FY11 (2.02 MB) Topic Landing Pages FY12-FY13 (366.66 KB) More Documents & Publications ...

  15. Search for: All records | DOE PAGES

    Office of Scientific and Technical Information (OSTI)

    articles and manuscripts. When DOE PAGES moves beyond the "beta" period, it will offer distributed full-text access to all DOE-affiliated accepted manuscripts or articles...

  16. Microsoft Word - Cover Page - Exhibit 9

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

    Governors State Park Sanborn - Agric. Pres. Rest. Meeh, M.G. & T. Ellacoya State Park ... Pages Corner State Forest Blood - Agric. Pres. Rest. Lang Station State Forest ...

  17. Public Access Policy and Communications | DOE PAGES

    Office of Scientific and Technical Information (OSTI)

    DOE PAGES Public Access Policy and Communications Public Access Policy and Communications 72414 Department of Energy Public Access Plan DOE Public Access Plan 22213 White House ...

  18. Page, Arizona: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    Page, Arizona: Energy Resources Jump to: navigation, search Equivalent URI DBpedia Coordinates 36.9147222, -111.4558333 Show Map Loading map... "minzoom":false,"mappingservice...

  19. Video test page | National Nuclear Security Administration

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

    test page | National Nuclear Security Administration Facebook Twitter Youtube Flickr RSS People Mission Managing the Stockpile Preventing Proliferation Powering the Nuclear Navy...

  20. 11. CONTRACT ID CODE PAGE OF PAGES I AMENDMENT OF SOLICITATION...

    National Nuclear Security Administration (NNSA)

    11. CONTRACT ID CODE PAGE OF PAGES I AMENDMENT OF SOLICITATIONMODIFICATION OF CONTRACT 1 I 2. AMENDMENTIMODIFICATION NO. 258 6. ISSUED BY CODE 3. EFFECTIVE DATE See Block 16C ...

  1. THE GALEX NEARBY YOUNG-STAR SURVEY

    SciTech Connect (OSTI)

    Rodriguez, David R.; Faherty, Jacqueline K.; Zuckerman, B.; Kastner, Joel H.; Bessell, M. S.; Murphy, Simon J.

    2013-09-10

    We describe a method that exploits data from the Galaxy Evolution Explorer (GALEX) ultraviolet and Wide-field Infrared Survey Explorer and Two Micron All Sky Survey infrared source catalogs, combined with proper motions and empirical pre-main sequence isochrones, to identify candidate nearby, young, low-mass stars. Applying our method across the full GALEX-covered sky, we identify 2031 mostly M-type stars that, for an assumed age of 10 (100) Myr, all lie within {approx}150 ({approx}90) pc of Earth. The distribution of M spectral subclasses among these {approx}2000 candidate young stars peaks sharply in the range M3-M4; these subtypes constitute 50% of the sample, consistent with studies of the M star population in the immediate solar neighborhood. We focus on a subset of 58 of these candidate young M stars in the vicinity of the Tucana-Horologium association. Only 20 of these 58 candidates were detected in the ROSAT All-Sky X-ray Survey-reflecting the greater sensitivity of GALEX for the purposes of identifying active nearby, young stars, particularly for stars of type M4 and later. Based on statistical analysis of the kinematics and/or spectroscopic followup of these 58 M stars, we find that 50% (29 stars) indeed have properties consistent with Tuc-Hor membership, while 12 are potential new members of the Columba association, and 2 may be AB Dor moving group members. Hence, {approx}75% of our initial subsample of 58 candidates are likely members of young (age {approx} 10-40 Myr) stellar moving groups within 100 pc, verifying that the stellar color- and kinematics-based selection algorithms described here can be used to efficiently isolate nearby, young, low-mass objects from among the field star population. Future studies will focus on characterizing additional subsamples selected from among this list of candidate nearby, young M stars.

  2. Katharine Page-Atomic-level insights for better materials

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

    Katharine Page Katharine Page-Atomic-level insights for better materials Page's research supports materials' advances that could have wide-ranging impact, investigating, manipulating and manufacturing nano-particles. March 26, 2014 Katharine Page Katharine Page "Page advises young women to be unafraid of exploring new career options and to always ask questions and learn from others along the way." A Love for Science Impassioned by materials science, Katharine Page told her college

  3. Orbital masses of nearby luminous galaxies

    SciTech Connect (OSTI)

    Karachentsev, Igor D.; Kudrya, Yuri N. E-mail: yukudrya@gmail.com

    2014-09-01

    We use observational properties of galaxies accumulated in the Updated Nearby Galaxy Catalog to derive a dark matter mass of luminous galaxies via motions of their companions. The data on orbital-to-stellar mass ratio are presented for 15 luminous galaxies situated within 11 Mpc from us: the Milky Way, M31, M81, NGC 5128, IC342, NGC 253, NGC 4736, NGC 5236, NGC 6946, M101, NGC 4258, NGC 4594, NGC 3115, NGC 3627, and NGC 3368, as well as for a composite suite around other nearby galaxies of moderate and low luminosity. The typical ratio for these galaxies is M {sub orb}/M {sub *} = 31, corresponding to the mean local density of matter ? {sub m} = 0.09, i.e., one-third of the global cosmic density. This quantity seems to be rather an upper limit of dark matter density, since the peripheric population of the suites may suffer from the presence of fictitious unbound members. We note that the Milky Way and M31 halos have lower dimensions and lower stellar masses than those of the other 13 nearby luminous galaxies. However, the dark-to-stellar mass ratio for both the Milky Way and M31 is typical for other neighboring luminous galaxies. The distortion in the Hubble flow, observed around the Local Group and five other neighboring groups, yields their total masses within the radius of a zero velocity surface, R {sub 0}; these masses are slightly lower than the orbital and virial values. This difference may be due to the effect of dark energy producing a kind of 'mass defect' within R {sub 0}.

  4. Property:SoftwarePage | Open Energy Information

    Open Energy Info (EERE)

    scs900-site-controller-software + MHK ISDBSensors0.01" Rain Gauge (2m cable) Smart Sensor + http:www.onsetcomp.comproductssoftwarehoboware + MHK ISDBSensors0.2 mm...

  5. DOE Launches New Fraud Reporting Web Page

    Broader source: Energy.gov [DOE]

    The Department of Energy today launched a new Fraud Reporting web page to make it easier for members of the public to report suspected incidents of fraud, waste, and abuse, and to enable the...

  6. Search for: All records | DOE PAGES

    Office of Scientific and Technical Information (OSTI)

    Vran, Jean-Pierre" Name Name ORCID Search Authors Type: All Accepted Manuscript ... Page 1 of 1 Search for: All records CreatorsAuthors contains: "Vran, Jean-Pierre

  7. SC e-journals Help page

    Office of Scientific and Technical Information (OSTI)

    Need Help With Searching? 'Web of Science' Search: The Web of Science search link takes ... Detailed search information is provided on the Web of Science Help page. General Search ...

  8. Search for: All records | DOE PAGES

    Office of Scientific and Technical Information (OSTI)

    Li, Xuejin" Name Name ORCID Search Authors Type: All Accepted Manuscript Published Article ... Search Results Page 1 of 1 Search for: All records CreatorsAuthors contains: "Li, Xuejin

  9. Help:Talk pages | Open Energy Information

    Open Energy Info (EERE)

    a single word of it, and it doesn't mention the spider once -- User:Example|Bob Smith 18:07, 26 August 1991 (UTC) : No no. This page is talking about the "world wide...

  10. MINERvA PMG Meeting Web Page

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

    Meetings Main INjector ExpeRiment v-A DOE Status Review Documentation DOE Status Review Web Page (September 12, 2008) (all versions of documents there are as they were submitted...

  11. Health Safety and Environmental Protection Page 1

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

    Page 1 Final Meeting Summary March 10, 2011 FINAL MEETING SUMMARY HANFORD ADVISORY BOARD HEALTH, SAFETY AND ENVIRONMENTAL PROTECTION COMMITTEE March 10, 2011 Richland, WA Topics in this Meeting Summary Welcome and Introductions ............................................................................................................ 1 Beryllium ........................................................................................................................................ 1 Chemical

  12. Openei test page | Open Energy Information

    Open Energy Info (EERE)

    Openei test page Jump to: navigation, search Net value of PV generation under various rate structures and penetration levels for a(n) FullServiceRestaurant in Flagstaff,AZ (Salt...

  13. Www.deq.mt.gov/MFS/LawRules/Circular2 | Open Energy Information

    Open Energy Info (EERE)

    Www.deq.mt.govMFSLawRulesCircular2 Jump to: navigation, search OpenEI Reference LibraryAdd to library Reference: Www.deq.mt.govMFSLawRulesCircular2 Published Publisher Not...

  14. http://www.doe.gov/media/Myths_and_Facts.pdf | Department of...

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

    doe.govmediaMythsandFacts.pdf http:www.doe.govmediaMythsandFacts.pdf http:www.doe.govmediaMythsandFacts.pdf (143.91 KB) More Documents & Publications Biofuels & ...

  15. http://www.epa.gov/osw/hazard/tsd/pcbs/pubs/stordisp.htm

    National Nuclear Security Administration (NNSA)

    Your local yellow pages or state environmental agency may have a more in depth listing. EPA'S Where You Live web page links to many state environmental agencies. As of July 2010 ...

  16. NewPage Demonstration-Scale Biorefinery | Department of Energy

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

    NewPage Demonstration-Scale Biorefinery NewPage Demonstration-Scale Biorefinery The NewPage biorefinery will be added to an existing pulp and paper mill to create renewable ...

  17. Optimizing Web Pages for Search Engines | Department of Energy

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

    Web Writing » Optimizing Web Pages for Search Engines Optimizing Web Pages for Search Engines For search engine optimization (SEO), follow these best practices when writing content for Office of Energy Efficiency and Renewable Energy (EERE) websites and applications. Understand How Search Engines Work Search engines visit Web pages, index the words on those pages, and put the pages into a database. When a user does a search, the search engine compares the user's search terms against the pages

  18. Vermont State Lands Administration: Application Page | Open Energy...

    Open Energy Info (EERE)

    State Lands Administration: Application Page Jump to: navigation, search OpenEI Reference LibraryAdd to library Web Site: Vermont State Lands Administration: Application Page...

  19. Page County, Iowa: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    Energy Companies in Page County, Iowa BioProcess Algae Places in Page County, Iowa Blanchard, Iowa Braddyville, Iowa Clarinda, Iowa Coin, Iowa College Springs, Iowa Essex, Iowa...

  20. New Draft Page Change - Program and Project Management for the...

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

    Draft Page Change - Program and Project Management for the Acquisition of Capital Assets by Patricia Greeson The Page Change is a limited update to incorporate recent Secretarial...

  1. WWW Table of Radioactive Isotopes (TORI or ToI) from the Isotopes Project: Lawrence Berkeley National Laboratory - Lund University Collaboration

    DOE Data Explorer [Office of Scientific and Technical Information (OSTI)]

    Firestone, R. B. [LBNL; Ekstrom, L. P. [LUNDS Universitet; Chu, S. Y.F. [LBNL

    The handbook titled "Table of Isotopes" has long been a standard source of information for nuclear structure and decay data. This web page provides online access to the "Table of Isotopes" data. It provides specialized interfaces to search, including: 1) Radiation search - search for by energy range and/or parent properties; 2) Nuclide search - search for nuclides by A, Z, N, and/or half-life range; 3) Atomic data - search for X-rays and Auger electrons; 4) Periodic table interface to the nuclides; 5) Summary drawings for A=1-277 (PDF). This page also provides access to various other resources, including the WWW Table of Nuclear Structure where the user can interactively search adopted nuclear level and gamma-ray properties or display tables, level scheme ladder diagrams and nuclear charts.

  2. PAGES_thumbnail.jpg | OSTI, US Dept of Energy Office of Scientific and

    Office of Scientific and Technical Information (OSTI)

    Technical Information PAGES_thumbnail

  3. 2008 report transmittal letter page | Department of Energy

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

    8 report transmittal letter page 2008 report transmittal letter page 2008 report transmittal letter page 2008 report transmittal letter page (23.53 KB) More Documents & Publications FY_2010_REPORTING_INSTRUCTIONS_TRANSMITTAL_8-26-10-Horn.pdf Savannah River Site - Tank 48 Transmittal Letter of SRS Tank 48 Review Recommendations: Draft 2008 Section 999 Annual Plan

  4. Katharine Page: Atomic-level insights for better materials

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

    Katharine Page: Atomic-level insights for better materials Alumni Link: Opportunities, News and Resources for Former Employees Latest Issue:September 2015 all issues All Issues » submit Katharine Page: Atomic-level insights for better materials Page's research supports materials' advances that could have wide-ranging impact, investigating, manipulating and manufacturing nano-particles. May 1, 2014 Katherine Page Katherine Page Contact Linda Anderman Email A Love for Science Impassioned by

  5. How To Setup EA Landing Page As Default Home Page For Google Chrome |

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

    Department of Energy Google Chrome How To Setup EA Landing Page As Default Home Page For Google Chrome STEP 1: In Chrome enter the URL http://energy.gov/iea. Once the EA site loads, go to the Customize and Control Google Chrome button in the far right of the top menu (the icon looks like a page with multiple horizontal lines on it). STEP 1: In Chrome enter the URL http://energy.gov/iea. Once the EA site loads, go to the Customize and Control Google Chrome button in the far right of the top

  6. How To Setup EHSS Landing Page As Default Home Page For Google Chrome |

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

    Department of Energy Google Chrome How To Setup EHSS Landing Page As Default Home Page For Google Chrome STEP 1: In Chrome enter the URL http://energy.gov/ehss. Once the EHSS site loads, go to the Customize and Control Google Chrome button in the far right of the top menu (the icon looks like a page with multiple horizontal lines on it). STEP 1: In Chrome enter the URL http://energy.gov/ehss. Once the EHSS site loads, go to the Customize and Control Google Chrome button in the far right of

  7. http://www.nmenv.state.nm.us/hwb/hwb_facil.html

    National Nuclear Security Administration (NNSA)

    Statutes & Regulations Notifiers LANL Order Documents Contact Us Hazardous Waste Facilities This Web Page provides links to public notices and information on New Mexico hazardous ...

  8. Page 1, About DOE-ID

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

    1 of 11 Previous Page About the U.S. Department of Energy, Idaho Operations Office (DOE-ID) As a new employee of the Department of Energy (DOE), you are entering a Cabinet-Level Executive Branch Agency with a long history of achievement. The Idaho Operations Office (DOE-ID)/INL mission is to develop and deliver cost-effective solutions to both fundamental and advanced challenges in nuclear energy and other energy resources, national security, and environmental management. The Department's

  9. Page 10, Security Forms and Information

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

    10 of 11 Previous Page Security Forms and Information Building Access and DOE Badges Employees entering DOE facilities must have either a DOE photo identification Security Badge or a DOE Temporary Badge. Either badge must be displayed above the waist in plain view at all times while in DOE facilities. Employees must present said badges to Protective Force personnel for inspection prior to entry into the facilities. You should have been provided instruction by email regarding training that must

  10. Page 4, Federal Employees Health Benefits (FEHB)

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

    4 of 11 Previous Page Federal Employees Health Benefits (FEHB) Initial Election Period As a new employee, you have 60 days from your date of appointment to make an election for the health benefits program. Your completed Health Benefits Election Form, SF-2809, must be submitted to your servicing Human Resources Office in a timely manner. If you fail to make an election within the required deadline, you are considered to have declined coverage. You will not have another opportunity to enroll

  11. Office of Health, Safety and Security: Page Not Found

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

    Health, Safety and Security SEARCH TOOLS HOME ABOUT US FUNCTIONS RESOURCES NEWSFEEDS VIDEOS EVENTS warning icon Page Not Found Sorry, the page you are looking for can't be found! The page you are looking for might have been removed, has had its name changed, or is temporarily unavailable. Please try the following: If you typed the page address in the Address bar, make sure that it is spelled correctly. Try seeking the required page from our home page. Use the Back button to try another link.

  12. Help:Deleting a page | Open Energy Information

    Open Energy Info (EERE)

    helpfully redirect to the information. See Help:Redirects The page is out-of-date -- Re-word sentences to be in the past tense, to make the page an historical record....

  13. Help:Moving a page | Open Energy Information

    Open Energy Info (EERE)

    (renaming) a page means giving it another name. This is done by using "Move" tab at the top. Then simply enter the new name and click "Move page". Normally you would want to leave...

  14. New User Facilities Web Page Highlights Work at National Laboratories...

    Office of Environmental Management (EM)

    User Facilities Web Page Highlights Work at National Laboratories New User Facilities Web Page Highlights Work at National Laboratories January 15, 2014 - 12:00am Addthis The User ...

  15. Object Classification at the Nearby Supernova Factory (Journal...

    Office of Scientific and Technical Information (OSTI)

    Nearby Supernova Factory Citation Details In-Document ... Report Number(s): LBNL-696E TRN: US200815%%72 DOE Contract Number: DE-AC02-05CH11231 Resource Type: Journal Article ...

  16. Webtrends Archives by Fiscal Year — EERE Home Page

    Broader source: Energy.gov [DOE]

    From the EERE Web Statistics Archive: Corporate sites, Webtrends archives for the EERE home page by fiscal year.

  17. Webtrends Archives by Fiscal Year — Topic Landing Pages

    Broader source: Energy.gov [DOE]

    From the EERE Web Statistics Archive: Corporate sites, Webtrends archives for the topic landing pages by fiscal year.

  18. PIA - PAGE (Performance and Accountability for Grants in Energy System

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

    Corporate Planning System (CPS) | Department of Energy PAGE (Performance and Accountability for Grants in Energy System Corporate Planning System (CPS) PIA - PAGE (Performance and Accountability for Grants in Energy System Corporate Planning System (CPS) PIA - PAGE (Performance and Accountability for Grants in Energy System Corporate Planning System (CPS) PIA - PAGE (Performance and Accountability for Grants in Energy System Corporate Planning System (CPS) (3 MB) More Documents &

  19. Newsletters Data Backcheck Page | Jefferson Lab

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

    Newsletters Data Backcheck Page sort descending Wed, 2012-08-01 12:54 On Target August 2012 August 2012 The U.S. Department of Energy's Thomas Jefferson National Accelerator Facility Bright Future for Energizing Electrons: 12 GeV Cryomodule Test a Success Crab_1.jpg A C100 cryomodule is prepared to be lowered into the accelerator tunnel by Dave Bigelow (left) for installation, as John Hogan looks on. In the wee hours of May 18, the last crew to run the 6 GeV CEBAF accelerator caught a glimpse of

  20. Nuclear Target Ratios data release page

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

    Nuclear Target Ratios data release page "Measurement of ratios of muon neutrino charged-current cross sections on C, Fe, and Pb to CH at neutrino energies 2-20 GeV" Phys. Rev. Lett. 112 (2014) 231801, hep-ex/1403.2103. Data Anciliary files for this result can be found at http://arxiv.org/src/1403.2103v4/anc Anciliary Files include: Cross section ratios as a function of Bjorken x Cross Section ratio as a function of neutrino energy Target Masses used in the experiment Neutrino Flux used

  1. Electron Neutrino CCQE Data Release Page

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

    Electron Neutrino CCQE Data Release Page Measurement of electron neutrino quasielastic and quasielastic-like scattering on hydrocarbon at ⟨Eν⟩ = 3.6 GeV Phys. Rev. Lett. 116, 081802 (2016) and hep-ex/1509.05729 Data Ancillary files for this result are available at http://arxiv.org/src/1509.05729v6/anc The available data files are: Cross Section as a function of Electron Angle Cross Section as a function of Electron Energy Cross Section as a function of Q2 Covariance Matrix as a function of

  2. Page 6, The Thrift Savings Plan (TSP)

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

    6 of 11 Previous Page Thrift Savings Plan (TSP) The Thrift Savings Plan (TSP) is a voluntary retirement savings and investment plan for federal employees. The best way to assure that your retirement income meets your needs is to start investing in the Thrift Savings Plan at the beginning of your Federal service, and to continue to do so throughout your career. The agency will set up a Thrift Savings Plan account for you and will automatically contribute an amount equal to 1% of your basic pay

  3. Page 7, A Family-Friendly Workplace

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

    7 of 11 Previous Page A Family-Friendly Workplace The Department of Energy (DOE) takes its commitment to recruiting, retaining, and motivating a highly skilled, diverse, and productive workforce very seriously. Our objective is to be the employer of choice in the public sector. The U.S. Department of Energy is the Top-Ranked Cabinet-Level Agency for employee satisfaction and engagement according to the 2005 Best Places to Work in the Federal Government Rankings. Below is a summary of additional

  4. Energy.gov Content Management System Page Types

    Broader source: Energy.gov [DOE]

    For Office of Energy Efficiency and Renewable Energy (EERE) websites, learn about the standard page types available in the Energy.gov Drupal content management system (CMS). For information about other available page types, or to request a new kind of page type, contact the Site Coordinators.

  5. AMENDMENT OF SOLICITATION/MODIFICATION OF CONTRACT 1. CONTRACT ID CODE PAGE OF PAGES

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

    AMENDMENT OF SOLICITATION/MODIFICATION OF CONTRACT 1. CONTRACT ID CODE PAGE OF PAGES 1 20 2. AMENDMENT/MODIFICATION NO. A001 3. EFFECTIVE DATE See Block 16C 4. REQUISITION/PURCHASE REQ. NO. 5. PROJECT NO. (If applicable) 6. ISSUED BY CODE 7. ADMINISTERED BY (If other than Item 6) CODE U.S. Department of Energy National Energy Technology Laboratory PO Box 880, 3610 Collins Ferry Road Morgantown, WV 26507-0880 Attn: Amanda Lopez 8. NAME AND ADDRESS OF CONTRACTOR (No., street, county, State, and

  6. AMENDMENT OF SOLICITATION/MODIFICATION OF CONTRACT 1.CONTRACT ID CODE PAGE OF PAGES

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

    CONTRACT ID CODE PAGE OF PAGES T 1 1 13 2 AMENDIMENT/MODIFICATION NO 3. EFFECTIVE DATE 4 -REGUISITION/PURCHASE RED. NO 5. PROJECT NO. (If epplicable) 032 04/14/2011 11EM002244 6 ISSUED BY CODE 00603 7 ADMINISTERED BY (Iftherthan temrt6) CODE J00603 Office of River Protection Office of River Protection U.S. Department of Energy U.S. Department of Energy Office of River Protection office of River Protection P.O. Box 450 P.O. Box 450 Richland WA 99352 Richland WA 99352 8 NAME AND ADDRESS OF

  7. AMENDMENT OF SOLICITATION/MODIFICATION OF CONTRACT 11. CONTRACT ID CODE 1 PAGE OF PAGES

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

    1 PAGE OF PAGES 1 I 2 2. AMENDMENTIMODIFICATION NO. 3. EFFECTIVE DATE 4. REQUISITIONIPURCHASE REO. NO. 15. PROJECT NO. (If applicable) 352 See Block 16C 12SC001876 Item 3 6. ISSUED BY CODE 00518 7. ADMINISTERED BY (If other than Item 6) CODE 100518 Oak Ridge Oak Ridge U.S. Department of Energy U.S. Department of Energy P.O. Box 2001 P.O. Box 2001 Oak Ridge TN 37831 Oak Ridge TN 37831 8. NAME AND ADDRESS OF CONTRACTOR (No .* stteet. county. Stete and ZIP Coda) (X) 9A. AMENDMENT OF SOLICITATION

  8. AMENDMENT OF SOLICITATIONIMODIFICATION OF CONTRACT I CONTRACT ID CODE PAGE OF PAGES

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

    I CONTRACT ID CODE PAGE OF PAGES 1 14 2. AMENDMENT/MODIFICATION NO. 3 EFFECTIVE DATE 4. REQUISITION/PURCHASE RED. NO 5. PRtOJECT NO. (if pplicable) 186 See Block 16CL 6. ISSUED BY CODE j 0603 7. ADMINISTERED BY (If other than Item 6) CODE 00603 office of River Protection Office of River Protection U.S. Department of Energy U.S. Department of Energy office of River Protection office of River Protection P.O. Box 450 P.O. Box 450 Richland WA 99352 MS: H6-60 Richland WA 99352 6. NAME AND ADDRESS OF

  9. AMENDMENT OF SOUCITATIONIMODIFICATION OF CONTRACT 1. CONTRACT ID CODE PAGE OF PAGES

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

    1. CONTRACT ID CODE PAGE OF PAGES II 11 9 2. AMEN DMENTIMODIFICATION NO. 3. EFFECTIVE DATE 4. REOUISITIONIPURCHASE REQ. NO. 5. PROJECT NO. (If elpicable) 169 See Block 16C 12EM0020631 6. ISSUED BY CODE 00603 7. ADMINISTERED BY (If otherthan Item 6) CODE 100603 Office of River Protection Office of River Protection U.S. Department of Energy U.S. Department of Energy Office of River Protection Office of River Protection P.O. Box 450 P.O. Box 450 Richland WA 99352 MS: H6-60

  10. How To Setup EA Landing Page As Default Home Page For Internet Explorer |

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

    Department of Energy Internet Explorer How To Setup EA Landing Page As Default Home Page For Internet Explorer STEP 1: In Internet Explorer enter the URL http://energy.gov/iea/. Once the EA site loads, click on the Home (Alt + M) drop-down list (highlighted with the red arrow and box). STEP 1: In Internet Explorer enter the URL http://energy.gov/iea/. Once the EA site loads, click on the Home (Alt + M) drop-down list (highlighted with the red arrow and box). STEP 2: Choose “Add or

  11. How To Setup EHSS Landing Page As Default Home Page For Internet Explorer |

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

    Department of Energy Internet Explorer How To Setup EHSS Landing Page As Default Home Page For Internet Explorer STEP 1: In Internet Explorer enter the URL http://energy.gov/ehss/. Once the EHSS site loads, click on the Home (Alt + M) drop-down list (highlighted with the red arrow and box). STEP 1: In Internet Explorer enter the URL http://energy.gov/ehss/. Once the EHSS site loads, click on the Home (Alt + M) drop-down list (highlighted with the red arrow and box). STEP 2: Choose “Add

  12. 1,CONTRACT ID CODE PAGE OF PAGES AMENDMENT OF SOLICITATION/MODIFICATION

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

    1 1 (10.63 MB) More Documents & Publications Microsoft Word - GJPPGPracticesDraft.doc Updated Section H Greening Clauses DOE Purchase Card Policy

    ,CONTRACT ID CODE PAGE OF PAGES AMENDMENT OF SOLICITATION/MODIFICATION OF CONTRACT I 11 3 2. AMENDMENT/MODIFICATION NO. 3. EFFECTIVE DATE (M D Y) 4. REQUISITION/PURCHASE REQ. NO. 5. PROJECT NO, (If applicable) 221 See Block 16C 11 EM0026551 6. ISSUED BY CODE 7. ADMINISTERED BY (If other than Item 6) CODE U.S. Department of Energy Office of

  13. 11. CONTRACT ID CODE PAGE OF PAGES I AMENDMENT OF SOLICITATION/MODIFICATION OF CONTRACT

    National Nuclear Security Administration (NNSA)

    11. CONTRACT ID CODE PAGE OF PAGES I AMENDMENT OF SOLICITATION/MODIFICATION OF CONTRACT 1 I 2. AMENDMENTIMODIFICATION NO. 258 6. ISSUED BY CODE 3. EFFECTIVE DATE See Block 16C 05008 4. REQUISITION/PURCHASE REQ. NO. 7. ADMINISTERED BY (If other than Item 6) 15. PROJECT NO. (If applicable) CODE 1 0 5 0 0 8 NNSA/Oakridge Site Office NNSA/Oakridge Site Office U.S. Department of Energy U. S. Department of Energy NNSA/Y-12 Site Office NNSA/Y-12 Site Office P.O. Box 2050 P.O. Box 2050 Building 9704-2

  14. http://www.regulations.gov/#!documentDetail;D=EERE-2014-BT-STD...

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

    www.regulations.govdocumentDetail;DEERE-2014-BT-STD-0031-0002 EERE-2014-BT-STD-0031-0002 spreadsheet Sheet "Summary Switching" - Before ME1 19421032v.1 http:...

  15. https://www.jlab.org/integrated-rss en Jefferson Lab to Test...

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

    integrated-rss en Jefferson Lab to Test its Tornado Warning Siren at 10:30 a.m. on Friday, Dec. 4 https:www.jlab.orgnewsreleasesjefferson-lab-test-its-tornado-warning-siren-10...

  16. http://www.regulations.gov/#!documentDetail;D=EERE-2014-BT-STD-0031-0002

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

    www.regulations.gov/#!documentDetail;D=EERE-2014-BT-STD-0031-0002 EERE-2014-BT-STD-0031-0002 spreadsheet Sheet "Summary Switching" - Before ME1 19421032v.1 http://www.regulations.gov/#!documentDetail;D=EERE-2014-BT-STD-0031-0002 EERE-2014-BT-STD-0031-0002 spreadsheet Sheet "Summary Switching" - Available for download now ME1 19421032v.1

  17. http://www.epa.gov/ttn/chief/ap42/index.html

    National Nuclear Security Administration (NNSA)

    This is current through the Fifth Edition, Supplement C of AP 42. For sections and chapters added after November 1997, see the chapter web pages below. Introduction Introduction to ...

  18. http://www1.eere.energy.gov/financing/solicitations_detail.html

    National Nuclear Security Administration (NNSA)

    Printable Version EERE Financial Opportunities Home | EERE Home | U.S. Department of Energy Webmaster | Web Site Policies | Security & Privacy | USA.gov Page 1 of 1 EERE Financial ...

  19. http://www.leg.state.nv.us/nac/nac-445a.html

    National Nuclear Security Administration (NNSA)

    ... (d) The results of deviation checks conducted on a well which is constructed by drilling a pilot hole and enlarging that hole by reaming or other methods. Page 340 of 343 ...

  20. Page 5, Federal Employees' Group Life Insurance (FEGLI)

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

    5 of 11 Previous Page Federal Employees' Group Life Insurance (FEGLI) Initial Enrollment Period All Employees in eligible positions are automatically enrolled in Basic Life...

  1. Attachment 3 b. Part A Page 1 of 6

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

    Attachment 3 b. Part A Page 1 of 6 Section A - General Terms and Conditions ................................................................................................ 2 A.1. Purpose .................................................................................................................................................. 2 A.2. Authority ............................................................................................................................................... 2

  2. Attachment 3.a. Part A Page 1 of 6

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

    A Page 1 of 6 Section A - General Terms and Conditions ................................................................................................ 2 A.1. Purpose .................................................................................................................................................. 2 A.2. Authority ............................................................................................................................................... 2 A.3. Part A Identifier

  3. EIA-22M, Monthly Biodiesel Production Survey Page 1

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

    22M, Monthly Biodiesel Production Survey Page 1 Instructions for the EIA-22M Monthly Biodiesel, Biojet, Biokerosene, and Renewable Diesel Report General Information Questions If...

  4. Getting on the same page: Performance Excellence | Y-12 National...

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

    the same page: Performance Excellence Posted: July 16, 2015 - 5:47pm CNS Strategic Goals, Core Values and Daily Absolutes Lately, Morgan Smith, Chief Operating Officer for...

  5. Burkina Faso-Partnership for Action on Green Economy (PAGE) ...

    Open Energy Info (EERE)

    Want, which recognizes the green economy as a vehicle for sustainable development and poverty eradication. PAGE will support 30 countries over the next seven years in building...

  6. Senegal-Partnership for Action on Green Economy (PAGE) | Open...

    Open Energy Info (EERE)

    Want, which recognizes the green economy as a vehicle for sustainable development and poverty eradication. PAGE will support 30 countries over the next seven years in building...

  7. Mauritius-Partnership for Action on Green Economy (PAGE) | Open...

    Open Energy Info (EERE)

    Want, which recognizes the green economy as a vehicle for sustainable development and poverty eradication. PAGE will support 30 countries over the next seven years in building...

  8. Microsoft PowerPoint - Congressional+Request+Ccover+pages.ppt...

    Energy Savers [EERE]

    ... and is covered by the terms described in the Appendix T ... Page 77 * The Cruise Missile Warhead program will enter into ... efforts in radiological search training, and provide ...

  9. Paramagnetic Spin Seebeck Effect (Journal Article) | DOE PAGES

    Office of Scientific and Technical Information (OSTI)

    DOE PAGES Search Results Publisher's Accepted Manuscript: Paramagnetic Spin Seebeck Effect Title: Paramagnetic Spin Seebeck Effect Authors: Wu, Stephen M. ; Pearson, John E. ; ...

  10. New User Facilities Web Page Highlights Work at National Laboratories

    Office of Energy Efficiency and Renewable Energy (EERE)

    The Bioenergy Technologies Office (BETO) recently added a Web page titled, "User Facilities," to highlight the work at BETO-supported national laboratories.

  11. Optimizing TLB entries for mixed page size storage in contiguous memory

    DOE Patents [OSTI]

    Chen, Dong; Gara, Alan; Giampapa, Mark E.; Heidelberger, Philip; Kriegel, Jon K.; Ohmacht, Martin; Steinmacher-Burow, Burkhard

    2013-04-30

    A system and method for accessing memory are provided. The system comprises a lookup buffer for storing one or more page table entries, wherein each of the one or more page table entries comprises at least a virtual page number and a physical page number; a logic circuit for receiving a virtual address from said processor, said logic circuit for matching the virtual address to the virtual page number in one of the page table entries to select the physical page number in the same page table entry, said page table entry having one or more bits set to exclude a memory range from a page.

  12. http://www.wdol.gov/wdol/scafiles/std/05-2439.txt?v=15

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

    5) was first posted on www.wdol.gov on 08/05/2014 ************************************************************************************ REGISTER OF WAGE DETERMINATIONS UNDER | U.S. DEPARTMENT OF LABOR THE SERVICE CONTRACT ACT | EMPLOYMENT STANDARDS ADMINISTRATION By direction of the Secretary of Labor | WAGE AND HOUR DIVISION | WASHINGTON D.C. 20210 | | | | Wage Determination No.: 2005-2439 Diane C. Koplewski Division of | Revision No.: 15 Director Wage Determinations| Date Of Revision:

  13. http://www.wdol.gov/wdol/scafiles/std/15-5233.txt?v=3

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

    15-5233 (Rev.-3) was first posted on www.wdol.gov on 01/19/2016 ************************************************************************************ REGISTER OF WAGE DETERMINATIONS UNDER | U.S. DEPARTMENT OF LABOR THE SERVICE CONTRACT ACT | EMPLOYMENT STANDARDS ADMINISTRATION By direction of the Secretary of Labor | WAGE AND HOUR DIVISION | WASHINGTON D.C. 20210 | | | | Wage Determination No.: 2015-5233 Daniel W. Simms Division of | Revision No.: 3 Director Wage Determinations| Date Of Revision:

  14. Buildings and Energy in the 1980's -- Index Page

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

    Manager Phone: (202) 586-7237 Fax: (202) 586-0018 URL: http:www.eia.govemeurecs1f.html If you are having any technical problems with this site, please contact the EIA...

  15. Stellar and gaseous nuclear disks observed in nearby (U)LIRGs...

    Office of Scientific and Technical Information (OSTI)

    Stellar and gaseous nuclear disks observed in nearby (U)LIRGs Citation Details In-Document Search Title: Stellar and gaseous nuclear disks observed in nearby (U)LIRGs We present ...

  16. http://www.phmsa.dot.gov/portal/site/PHMSA/menuitem.ebdc7a8a7e3

    National Nuclear Security Administration (NNSA)

    Library Careers | Contact Us | No Fear | Privacy Policy | FOIA | Accessibility | FAQs | Web Policies | Site Map | Download Acrobat Page 2 of 2 PHMSA - Library - Ten Year Hazardous ...

  17. Event Planning Page Updated! | OpenEI Community

    Open Energy Info (EERE)

    Event Planning Page Updated Home > Groups > Linked Open Data Workshop in Washington, D.C. Jweers's picture Submitted by Jweers(88) Contributor 27 September, 2012 - 18:38 I updated...

  18. Added Public Promotional Page! | OpenEI Community

    Open Energy Info (EERE)

    Added Public Promotional Page Home > Groups > Linked Open Data Workshop in Washington, D.C. Jweers's picture Submitted by Jweers(88) Contributor 27 September, 2012 - 18:10 Event...

  19. Mongolia-Partnership for Action on Green Economy (PAGE) | Open...

    Open Energy Info (EERE)

    years of the partnership, PAGE will focus on seven pilot countries, yet to be named, and scale up this support to a total of 30 countries by 2020. The first global conference on...

  20. Heap/stack guard pages using a wakeup unit

    SciTech Connect (OSTI)

    Gooding, Thomas M; Satterfield, David L; Steinmacher-Burow, Burkhard

    2014-04-29

    A method and system for providing a memory access check on a processor including the steps of detecting accesses to a memory device including level-1 cache using a wakeup unit. The method includes invalidating level-1 cache ranges corresponding to a guard page, and configuring a plurality of wakeup address compare (WAC) registers to allow access to selected WAC registers. The method selects one of the plurality of WAC registers, and sets up a WAC register related to the guard page. The method configures the wakeup unit to interrupt on access of the selected WAC register. The method detects access of the memory device using the wakeup unit when a guard page is violated. The method generates an interrupt to the core using the wakeup unit, and determines the source of the interrupt. The method detects the activated WAC registers assigned to the violated guard page, and initiates a response.

  1. Help:Starting a new page | Open Energy Information

    Open Energy Info (EERE)

    else) creates a link to an article that doesn't exist yet, the link will be coloured red, like this. Clicking a red link will take you to the edit page for the new article....

  2. Air Permit Program Information Page | Open Energy Information

    Open Energy Info (EERE)

    LibraryAdd to library Web Site: Air Permit Program Information Page Author Division of Air Quality Published Publisher Not Provided, Date Not Provided DOI Not Provided Check for...

  3. What Do You Think of the Redesigned EERE Home Page?

    Broader source: Energy.gov [DOE]

    On Monday, Andrea pointed you to the redesigned EERE home page. While this blog usually focuses on resources from EnergySavers.gov and other sites that are specifically for consumers, we know that...

  4. Health Safety and Environmental Protection Committee Page 1

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

    Page 1 Final Meeting Summary March 8, 2012 FINAL MEETING SUMMARY HANFORD ADVISORY BOARD HEALTH, SAFETY AND ENVIRONMENTAL PROTECTION COMMITTEE March 8, 2012 Richland, WA Topics in this Meeting Summary Welcome & Introductions ............................................................................................................................. 1 2012 Priority and Strategic Planning

  5. Health Safety and Environmental Protection Committee Page 1

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

    Committee Page 1 Final Meeting Summary May 10, 2011 FINAL MEETING SUMMARY HANFORD ADVISORY BOARD HEALTH, SAFETY AND ENVIRONMENTAL PROTECTION COMMITTEE May 10, 2011 Richland, WA Topics in this Meeting Summary Welcome and Introductions ............................................................................................................ 1 Committee Business........................................................................................................................ 8

  6. The MicroBooNE Project - Home Page

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

    posted in the MicroBooNE DocDB, private access user-name is reviewer, password on request. ... Password access to these pages is necessary, user-name is reviewer, password on request. ...

  7. Contract No. DE-AC27-01RV14136 Modification No. M023 SF-30 Continuation Page(s)

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

    M023 SF-30 Continuation Page(s) Page 2 of 6 Block 13C Continuation: This supplemental agreement is entered into pursuant to authority of: A. Section I, Clause I.82, FAR 52.243-2 Changes - Cost-Reimbursement (AUG 1987) - Alternate III (APR 1984) B. Mutual agreement Block 14 Continuation: A. Purpose of the Modification: 1. Under Section C, Statement of Work, Table C.5-1.1, Deliverables: Modify Contract Due Date for Items 2.5, 2.6, 2.7, 4.1, & 7.3, and modify Action Required for Items 4.1 and

  8. New Manhattan Project Resource Page Launched | Department of Energy

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

    Manhattan Project Resource Page Launched New Manhattan Project Resource Page Launched July 16, 2013 - 5:48pm Addthis General Leslie Groves and J. Robert Oppenheimer are pictured here at the Trinity Test site in New Mexico, 1945. General Leslie Groves and J. Robert Oppenheimer are pictured here at the Trinity Test site in New Mexico, 1945. Terry Fehner Terry Fehner Historian, Federal Preservation Officer Andrew Weston-Dawkes Andrew Weston-Dawkes Director, Office of Classification What are the key

  9. Response to several FOIA requests - Renewable Energy pages 4001 - 4250 |

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

    Department of Energy Energy pages 4001 - 4250 Response to several FOIA requests - Renewable Energy pages 4001 - 4250 Response to several FOIA requests - Renewable Energy. nepdg_4001_4250.pdf R.eport Statement/Recommendation Background Pros/Cons discussion Response to several FOIA requests - Renewable Energy.. (5.64 MB) More Documents & Publications Response to several FOIA requests - Renewable Energy. Response to several FOIA requests - Renewable Energy.

  10. HANFORD TANK CLEANUP UPDATE MAY 2009 [VISIT US AT WWW.WRPSTOC.COM OR WWW.HANFORD.GOV/ORP/ FOR MORE INFORMATION

    SciTech Connect (OSTI)

    HOLLOWAY JN

    2009-05-03

    Retrieval of waste from single-shell tank C-110 resumed in January making it the first waste retrieval operation for WRPS since taking over Hanford's Tank Operations Contract last October. Now, with approximately 90 percent of the waste removed, WRPS believes that modified sluicing has reached the limits of the technology to remove any further waste and is preparing documentation for use in decision making about any future retrieval actions. Tank C-110 is located in C Fann near the center of the Hanford Site. It is a 530,000 gallon tank, built in 1946, and held approximately 126,000 gallons of sludge and other radioactive and chemical waste materials when retrieval resumed. Modified sluicing technology uses liquid waste from a nearby double-shell tank to break up, dissolve and mobilize the solid material so it can be pumped. Because of the variety of waste fon11S, sluicing is often not able to remove all of the waste. The remaining waste will next be sampled for analysis, and results will be used to guide decisions regarding future actions. Work is moving rapidly in preparation to retrieve waste from a second single-shell tank this summer and transfer it to safer double-shell tank storage. Construction activities necessary to retrieve waste from Tank C-104, a 530,000 gallon tank built in 1943, are approximately 60 percent complete as WRPS maintains its focus on reducing the risk posed by Hanford's aging single-shell waste tanks. C-104 is one of Hanford's oldest radioactive and chemical waste storage tanks, containing approximately 263,000 gallons of wet sludge with a top layer that is dry and powdery. This will be the largest sludge volume retrieval ever attempted using modified sluicing technology. Modified sluicing uses high pressure water or liquid radioactive waste sprayed from nozzles above the waste. The liquid dissolves and/or mobilizes the waste so it can be pumped. In addition to other challenges, tank C-104 contains a significant amount of plutonium and

  11. Page Not Found | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    Page Not Found Page Not Found Contact Information Office of Science U.S. Department of Energy 1000 Independence Ave., SW Washington, DC 20585 P: (202) 586-5430 The page that you...

  12. Poster - DOE PAGES Beta | OSTI, US Dept of Energy, Office of...

    Office of Scientific and Technical Information (OSTI)

    PAGES Beta Document Files and References Available Downloads for this Document: applicationpdf icon Poster DOE PAGES Beta Last updated on Thursday 04 June

  13. DOE Pages XML Data Services Manual | OSTI, US Dept of Energy Office of

    Office of Scientific and Technical Information (OSTI)

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  14. PAGES AMENDMENT OF SOLICITATION/MODIFICATION OF CONTRACT

    National Nuclear Security Administration (NNSA)

    1 PAGE 1 OF 2 PAGES AMENDMENT OF SOLICITATION/MODIFICATION OF CONTRACT 2. AMENDMENTIMODIFICATION NO. 13. EFFECTIVE DATE M186 October 15, 2009 4. REQUISITION/PURCHASE I 5. PROJECT NO. (If applicable) REQ. NO. 6. ISSUED BY CODE U.S. Department of Energy National Nuclear Security Administration Service Center Property and M&O Contract Support Department P.O. Box 5400 Albuquerque, NM 87185-5400 7. ADMINISTERED BY (If other than Item 6) CODE U.S. Department of Energy National Nuclear Security

  15. 1. CON'I'AC'r ID CODE PAGE OF PAGES AMENDMENT OF SOLICITATIONIMODIFICATION OF CONTRACT II 11 3

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    CON'I'AC'r ID CODE PAGE OF PAGES AMENDMENT OF SOLICITATIONIMODIFICATION OF CONTRACT II 11 3 2. AMENDMENT/MODIFICATION NO. 3. EFFECTIVE DATE (M/D.'F) 4. REQUISITION/PURCHASE RE-Q. NO. S. PROJECT1 NO. t7fapplieoble) 27See Block 16C 12EM001839 6. ISUED13Y ODE7. ADMINISTER.ED BY (If uI/wr ius /tem 6) CODE U.S. Department of Energy Office or River Protection P. 0. Box 450, MS 146-60 Richland, WA 99352 1. NAME AND ADDRESS OF CONTRACTOR (No.,stree, county State and Z11' code) 9A, AMENDMEN f

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    Ap5,sval 2700042 1. CONTRACT ID CODE PAGE OF PAGES AMENDMENT OF SOLICITATION/MODIFICATION OF CONTRACT I11 5 2. AMENDMENT/MOOIFICATION NO. 3. EFFECTIVE DATE 4. REQUISITION/PURCHASE REQ. NO.5 PROJECT NO. (If applicable) A077 See 16C 06-08RL-14383.O1 1 6. ISSUED BY CODE 7. ADMINISTERED BY (If other than Item 6) CODEJ US. Department of Energy Same as item 6. Richland Operations Office DOE Contracting POC: Richard Stimmrrel P. 0. Box 550, MSIN A7-80 (509) 376-2882 Richland, WA 99352 8 NAME AND

  17. Health Safety and Environmental Protection Committee Page 1

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    Page 1 Final Meeting Summary January 13, 2011 FINAL MEETING SUMMARY HANFORD ADVISORY BOARD Health Safety and Environmental Protection Committee Meeting January 13, 2011 Richland, WA Topics in this Meeting Summary Welcome and Introductions ............................................................................................................ 1 Integrated Safety Management System (ISMS) ............................................................................. 1 Beryllium

  18. Health, Safety and Environmental Protection Committee Page 1

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    Safety and Environmental Protection Committee Page 1 Final Meeting Summary April 19, 2012 FINAL MEETING SUMMARY HANFORD ADVISORY BOARD HEALTH, SAFETY AND ENVIRONMENTAL PROTECTION COMMITTEE April 19, 2012 Richland, WA Topics in this Meeting Summary Welcome & Introductions ............................................................................................................................. 1 Status Briefing on Asbestos

  19. High Statistics Study of Nearby Type 1a Supernovae. QUEST Camera...

    Office of Scientific and Technical Information (OSTI)

    Statistics Study of Nearby Type 1a Supernovae. QUEST Camera Short Term Maintenance: Final Technical Report Baltay, Charles 79 ASTRONOMY AND ASTROPHYSICS Study of Type 1a Supernovae...

  20. High Statistics Study of Nearby Type 1a Supernovae. QUEST Camera...

    Office of Scientific and Technical Information (OSTI)

    QUEST Camera Short Term Maintenance: Final Technical Report Citation Details In-Document Search Title: High Statistics Study of Nearby Type 1a Supernovae. QUEST Camera Short Term ...

  1. DUSTY WINDS: EXTRAPLANAR POLYCYCLIC AROMATIC HYDROCARBON FEATURES OF NEARBY GALAXIES

    SciTech Connect (OSTI)

    McCormick, Alexander; Veilleux, Sylvain; Rupke, David S. N. E-mail: veilleux@astro.umd.edu

    2013-09-10

    Recent observations have shown the presence of dust and molecular material in galactic winds, but relatively little is known about the distribution of these outflow components. To shed some light on this issue, we have used IRAC images from the Spitzer Space Telescope archive to investigate polycyclic aromatic hydrocarbon (PAH) emission from a sample of 16 local galaxies with known winds. Our focus on nearby sources (median distance 8.6 Mpc) has revealed detailed PAH structure in the winds and allowed us to measure extraplanar PAH emission. We have identified extraplanar PAH features on scales of {approx}0.8-6.0 kpc. We find a nearly linear correlation between the amount of extraplanar PAH emission and the total infrared flux, a proxy for star formation activity in the disk. Our results also indicate a correlation between the height of extraplanar PAH emission and star formation rate surface density, which supports the idea of a surface density threshold on the energy or momentum injection rate for producing detectable extraplanar wind material.

  2. Interaction between Cassiopeia A and nearby molecular clouds

    SciTech Connect (OSTI)

    Kilpatrick, C. D.; Bieging, J. H.; Rieke, G. H.

    2014-12-01

    We present spectroscopy of the supernova remnant Cassiopeia A (Cas A) observed at infrared wavelengths from 10 to 40 ?m with the Spitzer Space Telescope and at millimeter wavelengths in {sup 12}CO and {sup 13}CO J =2-1 (230 and 220 GHz) with the Heinrich Hertz Submillimeter Telescope. The IR spectra demonstrate high-velocity features toward a molecular cloud coincident with a region of bright radio continuum emission along the northern shock front of Cas A. The millimeter observations indicate that CO emission is broadened by a factor of two in some clouds toward Cas A, particularly to the south and west. We believe that these features trace interactions between the Cas A shock front and nearby molecular clouds. In addition, some of the molecular clouds that exhibit broadening in CO lie 1'-2' away from the furthest extent of the supernova remnant shock front. We propose that this material may be accelerated by ejecta with velocity significantly larger than the observed free-expansion velocity of the Cas A shock front. These observations may trace cloud interactions with fast-moving outflows such as the bipolar outflow along the southwest to northeast axis of the Cas A supernova remnant, as well as fast-moving knots seen emerging in other directions.

  3. Supernova Discoveries from the Nearby Supernova Factory (SNfactory)

    DOE Data Explorer [Office of Scientific and Technical Information (OSTI)]

    SNfactory International Collaboration,

    The Nearby Supernova Factory is an experiment designed to collect data on more Type Ia supernovae than have ever been studied in a single project before, and in so doing, to answer some fundamental questions about the nature of the universe. Type Ia supernovae are extraordinarily bright, remarkably uniform objects which make excellent "standard candles" for measuring the expansion rate of the universe. However, such stellar explosions are very rare, occurring only a couple of times per millenium in a typical galaxy, and remaining bright enough to detect only for a few weeks. Previous studies of Type Ia supernovae led to the discovery of the mysterious "dark energy" that is causing the universe to expand at an accelerating rate. To reduce the statistical uncertainties in previous experimental data, extensive spectral and photometric monitoring of more Type Ia supernovae is required. The SNfactory collaboration has built an automated system consisting of specialized software and custom-built hardware that systematically searches the sky for new supernovae, screens potential candidates, then performs multiple spectral and photometric observations on each supernova. These observations are stored in a database to be made available to supernova researchers world-wide for further study and analysis [copied from http://snfactory.lbl.gov/snf/snf-about.html]. Users must register and agree to the open access honor system. Finding charts are in FITS format and may not be accessible through normal browser settings.

  4. NREL: Dynamic Maps, GIS Data, and Analysis Tools Home Page

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

    The Dynamic Maps, Geographic Information System (GIS) Data and Analysis Tools website provides maps, data and tools for renewable energy resources that determine which energy technologies are viable solutions in domestic and international regions. MapSearch - While this site contains detailed information and quality data, if you want to search for the latest and most up-to-date maps created by NREL, please visit our MapSearch: http://www.nrel.gov/gis/mapsearch/ Renewable Energy Technical

  5. Contract Number DE-AC27-08RV14800 Continuation Page, Modification 138

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    Contract Number DE-AC27-08RV14800 Continuation Page, Modification 138 Attachment 1 DE-AC27-08RV14800, MODIFICATION 138 Replacement Pages (Total: One Hundred Twenty-Five (125) including this Cover Page) * Section H, Pages H-4 and H-24 * Section J, Table of Contents, Page J-1 * Section J, Attachment J.2, Pages J.2-4 thru J.2-7 and J.2.9 * Section J, Attachment J.10, Pages J.10-1 thru J.10-20 * Section J, Attachment J.13, Pages J.13-1 thru J.13-29 * Section J, Attachment J.14, Pages J.14-1 thru

  6. COTNAINSET REFERENCE NO. OF DOCUMENT BEING CONTINUED PAGE OF

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    COTNAINSET REFERENCE NO. OF DOCUMENT BEING CONTINUED PAGE OF NAME OF OFFEROR OR CONTRACTOR D-M039/071-0522 5 See Schedule ITE N. SPPESSERICS UANTITY UNIT UNIT PRICE AMOUNT (A) (B) (C) (D) (E) (F) Small Business Administration 965502193 NORTH WIND SOLUTIONS Attn: JADE SIDDOWAY 1425 HIGHAM STREET IDAHO FALLS ID 834021513 2085570857 IGF: :OT: :IGF Base - The Purpose of this Contract is to provide for for Technical, Environmental, and Programt Management Support Services- SBA Reference

  7. Office of Scientific and Technical Information DOE PAGES (Beta) Portal

    Office of Scientific and Technical Information (OSTI)

    Offers Public Access to Scholarly Scientific Publications Resulting from DOE Research Funding | OSTI, US Dept of Energy Office of Scientific and Technical Information Office of Scientific and Technical Information DOE PAGES (Beta) Portal Offers Public Access to Scholarly Scientific Publications Resulting from DOE Research Funding Get a printer-friendly version Recent Presentations Office of Scientific and Technical Information DOE PAGESBeta Portal Offers Public Access to Scholarly Scientific

  8. Recoiling supermassive black holes: a search in the nearby universe

    SciTech Connect (OSTI)

    Lena, D.; Robinson, A.; Axon, D. J.; Merritt, D.; Marconi, A.; Capetti, A.; Batcheldor, D.

    2014-11-10

    The coalescence of a binary black hole can be accompanied by a large gravitational recoil due to anisotropic emission of gravitational waves. A recoiling supermassive black hole (SBH) can subsequently undergo long-lived oscillations in the potential well of its host galaxy, suggesting that offset SBHs may be common in the cores of massive ellipticals. We have analyzed Hubble Space Telescope archival images of 14 nearby core ellipticals, finding evidence for small (? 10 pc) displacements between the active galactic nucleus (AGN; the location of the SBH) and the center of the galaxy (the mean photocenter) in 10 of them. Excluding objects that may be affected by large-scale isophotal asymmetries, we consider six galaxies to have detected displacements, including M87, where a displacement was previously reported by Batcheldor et al. In individual objects, these displacements can be attributed to residual gravitational recoil oscillations following a major or minor merger within the last few gigayears. For plausible merger rates, however, there is a high probability of larger displacements than those observed, if SBH coalescence took place in these galaxies. Remarkably, the AGN-photocenter displacements are approximately aligned with the radio source axis in four of the six galaxies with displacements, including three of the four having relatively powerful kiloparsec-scale jets. This suggests intrinsic asymmetries in radio jet power as a possible displacement mechanism, although approximate alignments are also expected for gravitational recoil. Orbital motion in SBH binaries and interactions with massive perturbers can produce the observed displacement amplitudes but do not offer a ready explanation for the alignments.

  9. DIRECT DETECTIONS OF YOUNG STARS IN NEARBY ELLIPTICAL GALAXIES

    SciTech Connect (OSTI)

    Ford, H. Alyson; Bregman, Joel N.

    2013-06-20

    Small amounts of star formation in elliptical galaxies are suggested by several results: surprisingly young ages from optical line indices, cooling X-ray gas, and mid-infrared dust emission. Such star formation has previously been difficult to directly detect, but using ultraviolet Hubble Space Telescope Wide Field Camera 3 imaging, we have identified individual young stars and star clusters in four nearby ellipticals. Ongoing star formation is detected in all galaxies, including three ellipticals that have previously exhibited potential signposts of star-forming conditions (NGC 4636, NGC 4697, and NGC 4374), as well as the typical ''red and dead'' NGC 3379. The current star formation in our closest targets, where we are most complete, is between 2.0 and 9.8 Multiplication-Sign 10{sup -5} M{sub Sun} yr{sup -1}. The star formation history was roughly constant from 0.5 to 1.5 Gyr (at (3-5) Multiplication-Sign 10{sup -4} M{sub Sun} yr{sup -1}), but decreased by a factor of several in the past 0.3 Gyr. Most star clusters have a mass between 10{sup 2} and 10{sup 4} M{sub Sun }. The specific star formation rates of {approx}10{sup -16} yr{sup -1} (at the present day) or {approx}10{sup -14} yr{sup -1} (when averaging over the past Gyr) imply that a fraction 10{sup -8} of the stellar mass is younger than 100 Myr and 10{sup -5} is younger than 1 Gyr, quantifying the level of frosting of recent star formation over the otherwise passive stellar population. There is no obvious correlation between either the presence or spatial distribution of postulated star formation indicators and the star formation we detect.

  10. Contract Number DE-AC27-08RV14800 Continuation Page, Modification 371

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

    Contract Number DE-AC27-08RV14800 Continuation Page, Modification 371 Attachment DE-AC27-08RV14800, MODIFICATION 371 Replacement Pages (Total: 19 including this Cover Page) * Section C, Statement of Work, pages C-11, C-18, C-45 thru C-47, C-49, C-54, C-56 and C-64 * Section J.2, Requirement Sources and Implementing Documents, pages J.2-2 thru J.2-4 * Section J.9, Special Financial Institution Account Agreement For Use With The Payments Cleared Financing Arrangement, pages J.9-1 thru J.9-5 *

  11. AMENDMENT OF SOLIr ATI ON/MODIFI CATION OF CONTRACT 1. CONTRACT ID CODE PAGE OF PAGES

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

    SOLIr ATI ON/MODIFI CATION OF CONTRACT 1. CONTRACT ID CODE PAGE OF PAGES 2 AMENDMENT/lIVDDIFICATiON NC 3. EFFECTIVE DATE [4 REDUISITION/PURCHASE REC NO IE PR3JECT NC (if applicable) 09 ISoe Bloo , 16- - ISee Soheoule S ISSUED D> CODE 7 ~ ADMINISTERED BY (if otnertrian ItemS CO DE Of fice of Ri-.er PoDLecOLODn office of Riv'er P-oCQ-ec-.iQ .S. Cet:F O<men of E-nerov,, I.S. Deparo:merio c-' Enrgv P.O. Box 4'5C 0 ... Box 45C .io ao 1 31 W YS: (-876 B. NAME AND ADDRESS CF CONTRACTOR (No seve

  12. Notice of Intent to Develop a Page Change to DOE O 413.3B, Program...

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

    a Page Change to DOE O 413.3B, Program and Project Management for the Acquisition of Capital Assets by Diane Johnson The Page Change is a limited update to incorporate recent...

  13. Microfluidic device having an immobilized pH gradient and page...

    Office of Scientific and Technical Information (OSTI)

    pH gradient and page gels for protein separation and analysis Citation Details In-Document Search Title: Microfluidic device having an immobilized pH gradient and page gels ...

  14. STIP 2.0 Static Content for Front Page Body | OSTI, US Dept of...

    Office of Scientific and Technical Information (OSTI)

    Static Content for Front Page Body STIP 2.0 Static Content for Front Page Body My Profile Create Review OSTI.Gov Newsletter - April-May 2016 Issue 15 OSTIblog: Thorium - An ...

  15. Why did someone delete the Utility Rate Database Page? | OpenEI...

    Open Energy Info (EERE)

    Why did someone delete the Utility Rate Database Page? Home > Groups > Utility Rate Can someone fix this? I can't access the Utility Rate Database Page It looks like someone...

  16. Page | OSTI, US Dept of Energy Office of Scientific and Technical...

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

    Page AN241.1 Web Services Available Downloads: AN241.1web service0.pdf PDF icon AN241.1web service0.pdf Tags: 2013 announcement evansd Page STIP Sub Site Legacy Node IDs: ...

  17. ScienceLive chat page: on the future of fusion research | Princeton Plasma

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

    Physics Lab ScienceLive chat page: on the future of fusion research American Fusion News Category: U.S. Universities Link: ScienceLive chat page: on the future of fusion research

  18. Top 10 Most Popular Energy Savers Web Pages of 2011 | Department...

    Energy Savers [EERE]

    Top 10 Most Popular Energy Savers Web Pages of 2011 Top 10 Most Popular Energy Savers Web Pages of 2011 December 27, 2011 - 9:08am Addthis Chris Stewart Senior Communicator at ...

  19. Scripts and Dynamic Pages on Websites Outside of the Energy.gov Drupal Environment

    Broader source: Energy.gov [DOE]

    This page describes the requirements for developing scripts and dynamic pages on EERE websites outside of Energy.gov. The use of scripting allows the creation of dynamic websites that allow user...

  20. Microfluidic device having an immobilized pH gradient and page...

    Office of Scientific and Technical Information (OSTI)

    and page gels for protein separation and analysis Title: Microfluidic device having an immobilized pH gradient and page gels for protein separation and analysis Disclosed is a ...

  1. Top 10 Most Popular Energy Savers Web Pages of 2011 | Department...

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

    Here's a look at the past year's 10 most popular Web pages: 10. Demand (Tankless or ... This Web page contains an overview of the federal tax credits for energy efficiency that ...

  2. New Draft Page Change - Program and Project Management for the Acquisition of Capital Assets

    Broader source: Directives, Delegations, and Requirements [Office of Management (MA)]

    The Page Change is a limited update to incorporate recent Secretarial policies and issues raised by external stakeholders.

  3. DOE - NNSA/NFO -- Photo Library Details page

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

    Photo Details NNSA/NFO Language Options U.S. DOE/NNSA - Nevada Field Office Instructions: Click the photograph number or name link below the thumbnail to view the full size image Photograph details are listed on the right Refer to the Viewing Instructions and FAQs for technical help Unable to display this Web Part. To troubleshoot the problem, open this Web page in a Windows SharePoint Services-compatible HTML editor such as Microsoft Office SharePoint Designer. If the problem persists, contact

  4. Page 9, Department of Energy Substance Abuse Testing Program

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    9 of 11 Previous Page DOE Substance Abuse Testing Program Executive Order 12564, Drug-Free Federal Workplace, states in part that "the use of illegal drugs or the use of legal drugs illegally by Federal employees impairs the efficiency of Federal Agencies, jeopardizes public health and safety, and violates the public trust." Substance abuse increases the burden on other employees who do not use illegal drugs and also is an economic problem due to lost productivity in the workplace,

  5. Cimon, Engstrom, Mattson, Pollet, Vanni, Suyama Page 1 of 3

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

    2014 RAP Committee: Draft Advice re: 100-N Draft A, v.2 Cimon, Engstrom, Mattson, Pollet, Vanni, Suyama Page 1 of 3 Draft Advice re: Proposed Plan for Remediation of the 100-NR-1 and 100-NR-2 Operable Units (DOE/RL-2012-68, Draft A) Background The 100-N area is the last of the 100 Area, River Corridor, RI/FS and Proposed Plans for submittal. The 100-N area consists of two Decision Units, NR-1, which is the source unit, and NR-2, the groundwater unit. There are 234 facilities, of which 76% have

  6. Page Not Found | U.S. DOE Office of Science (SC)

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

    Page Not Found Page Not Found Contact Information Office of Science U.S. Department of Energy 1000 Independence Ave., SW Washington, DC 20585 P: (202) 586-5430 The page that you have requested was not found. All News DOE Phonebook DOE Site Search GO Return Home

  7. 1. CONTRACT ID CODE PAGE of: PAGES AMENDM ENT OF SOLICITATION/MODIFICATION OF CONTRACT I -1 5

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

    of: PAGES AMENDM ENT OF SOLICITATION/MODIFICATION OF CONTRACT I -1 5 2. AMENDMENT/MODIFICATION NO. 3. EFFECTIVE DATE (0/1T 4. REQUISITION/PURCHASE REQ. NO. 5. PROJECT NO. (If applicable) 286 See Block 16C 12EM0014771 6. ISSUED BY CODE 7. AD)MINISTERED BY (If otherrtianItm 6) CODE U.S. Department of Energy Office of River Protection P. 0. Box 450, MIS 116-60 Richland, WA 99352 8. NAME AND ADDRESS OF CONTRACTOR (No., street. county.. State and ZIP code) 9A. AMENDMENT OF SOLICITATION NO. Bechtel

  8. High Statistics Study of Nearby Type 1a Supernovae. QUEST Camera Short Term

    Office of Scientific and Technical Information (OSTI)

    Maintenance: Final Technical Report (Technical Report) | SciTech Connect High Statistics Study of Nearby Type 1a Supernovae. QUEST Camera Short Term Maintenance: Final Technical Report Citation Details In-Document Search Title: High Statistics Study of Nearby Type 1a Supernovae. QUEST Camera Short Term Maintenance: Final Technical Report The Quest Camera was installed at the Palomar Obervatory in California. The camera was used to carry out a survey of low redshift Type 1a supernovae.The

  9. PAGE OF PAGES

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

    Map details Alaska Arizona Full Region Hawaii Marine Movements Northern California and Northern Nevada Pacific Northwest Southern California and Southern Nevada PADD 5 Transportation Fuels Markets Release date: September 30, 2015 Introduction This study examines supply, demand, and distribution of transportation fuels in Petroleum Administration for Defense District (PADD) 5, a region that includes the western states of California, Arizona, Nevada, Oregon, Washington, Alaska, and Hawaii. For

  10. Seeing and Reading Red: Hue and Color-word Correlation in Images and Attendant Text on the WWW

    SciTech Connect (OSTI)

    Newsam, S

    2004-07-12

    This work represents an initial investigation into determining whether correlations actually exist between metadata and content descriptors in multimedia datasets. We provide a quantitative method for evaluating whether the hue of images on the WWW is correlated with the occurrence of color-words in metadata such as URLs, image names, and attendant text. It turns out that such a correlation does exist: the likelihood that a particular color appears in an image whose URL, name, and/or attendant text contains the corresponding color-word is generally at least twice the likelihood that the color appears in a randomly chosen image on the WWW. While this finding might not be significant in and of itself, it represents an initial step towards quantitatively establishing that other, perhaps more useful correlations exist. These correlations form the basis for exciting novel approaches that leverage semi-supervised datasets, such as the WWW, to overcome the semantic gap that has hampered progress in multimedia information retrieval for some time now.

  11. High Statistics Study of Nearby Type 1a Supernovae. QUEST Camera...

    Office of Scientific and Technical Information (OSTI)

    Close Cite: Bibtex Format Close 0 pages in this document matching the terms "" Search For Terms: Enter terms in the toolbar above to search the full text of this document for ...

  12. KineticsFinal Report Cover Page Bakajin, O 59 BASIC BIOLOGICAL...

    Office of Scientific and Technical Information (OSTI)

    KineticsFinal Report Cover Page Bakajin, O 59 BASIC BIOLOGICAL SCIENCES; 42 ENGINEERING; CONSUMPTION RATES; DEAD TIME; DETECTION; DIFFUSION; DNA; ENERGY TRANSFER; FABRICATION;...

  13. WTP Contract No. DE-AC27-01RV14136 Page 1

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

    Num ber PEMP General Information A Introduction 1 B Roles and Responsibilities 2 C Process ... Page Perf. Objectives, Elem ents, & Measures PEMP General Information A. Introduction ...

  14. DOE Pages XML Data Services Manual | OSTI, US Dept of Energy...

    Office of Scientific and Technical Information (OSTI)

    Pages XML Data Services Manual Document Files and References Available Downloads for this Document: applicationpdf icon DOEPagesBetaXMLDataServicesManual.pdf Last updated on ...

  15. Ghana-Partnership for Action on Green Economy (PAGE) | Open Energy...

    Open Energy Info (EERE)

    Want, which recognizes the green economy as a vehicle for sustainable development and poverty eradication. PAGE will support 30 countries over the next seven years in building...

  16. Water Sampling At Twenty-Nine Palms Area (Page, Et Al., 2010...

    Open Energy Info (EERE)

    Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Exploration Activity: Water Sampling At Twenty-Nine Palms Area (Page, Et Al., 2010) Exploration Activity Details...

  17. Pages_OpenAccess_lock | OSTI, US Dept of Energy Office of Scientific and

    Office of Scientific and Technical Information (OSTI)

    Technical Information Pages_OpenAccess_lock Image: Image Gallery: EA Gallery 10 Last updated on Friday 09 September 2016

  18. WFIP NOAA Final Report - Page i DE-EE0003080 TABLE OF CONTENTS

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

    WFIP NOAA Final Report - Page i DE-EE0003080 TABLE OF CONTENTS TABLE OF CONTENTS ................................................................................................................................. i Executive Summary .................................................................................................................................. 1 1. Project Overview

  19. Chu Highlights Scientific Solutions to the Energy Crisis on New Facebook Page

    Broader source: Energy.gov [DOE]

    Facebook page will offer an inside look at efforts to transform the way we use and produce energy, as well as tips for reducing your home energy bill

  20. www.usiter.com

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

    com The ITER Project represents the frontier in fusion energy generation, and will deliver an international scientific laboratory that demonstrates the feasibility of hydrogen fusion as a source of clean power in the 21 st century. As of June 2016, over $830M has been awarded to US industry and universities, and obligated to DOE national laboratories in 43 states plus the District of Columbia. Hydrogen Fusion Progress on This map does not include contracts awarded to US Industry by the EU

  1. http://www

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

    Proposed Energy Transport Corridors

  2. www.srs.gov

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

    PBS 11C Nuclear Materials 260 255 PBS 12 Used Nuclear Fuel 24 41 PBS 13 Solid Waste 48 52 PBS 30 Soil & Groundwater Remediation 66 66 SRS Risk Management Operations 398 414 PBS 11C NM Stabilization & Disposition 1 (NEW) 284 296 311 15 Nuclear Material Management (NEW) 311 15 PBS 41 S&M, Risk Reduction & Deactivation 2 (NEW) 0 0 28 28 PBS 13 Solid Waste 48 52 51 (1) PBS 30 Soil & Groundwater Remediation 66 66 74 8 Environmental Cleanup (NEW) 153 35 PBS 14C Radioactive Liquid

  3. http://www

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

    Instruments and the Probes to which they are attached CHAPS 07 G-1 Instruments rev. 07-2-20 Instrument CVI non-CVI Gases Other PI TSI-3563 Neph 1 Ogren/Andrews TSI-3010 CPC 1 Ogren/Andrews PSAP Radiance 0 Laulainen PSAP NOAA 1 Ogren/Andrews AMS 1 Lee/Alexander FIMS 1 Wang LAPA-1 1 Dubey TRAC 1 Laskin TDL H2O 1 Ogren/Andrews CVI control 1 Ogren/Andrews CVI flow meters ? Ogren/Andrews CVI pumps 2 Ogren/Andrews CVI heat 0 Ogren/Andrews CVI zero air bottle 1 Ogren/Andrews CVI data system 1

  4. www.chemistryworld.org

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

    chemistryworld.org 46 | Chemistry World | April 2010 Catalysts for green energy A catalytic collaboration In a new collaborative effort to develop better catalysts for energy ...

  5. EA-1811: NewPage Corporation Wood Biomass to Liquid Fuel, Wisconsin Rapids, Wisconsin

    Broader source: Energy.gov [DOE]

    This EA will evaluate the environmental impacts of a proposal to provide federal funding to NewPage for final design, construction and operation of a demonstration scale biorefinery. The NewPage biorefinery facility would be integrated with the existing paper mill and produce up to 555 barrels per day (bpd) of clean hydrocarbon biofuel. This EA is has been cancelled.

  6. How to make x-ray simulation software working on WWW : a simple recipe based on seven years of experience.

    SciTech Connect (OSTI)

    Stepanov, S.; Biosciences Division

    2004-01-01

    Attaching WWW interfaces to scientific software opens new opportunities to researchers by making their results available to wide scientific community in a way complimentary to publication. We have shown that this task may be much easier than many used to think: the amount of additional code is small, the Common Gateway Interface (CGI) can be written in any language, not necessarily PERL, and the software can be interfaced on any operating system it was originally written and does not have to be ported to UNIX. This paper provides some useful recipes resulted from seven years of author's experience in developing and maintaining highly successful X-ray Web server project. All these solutions are based on free public domain software (Apache, GnuPlot, and InfoZip) and applicable for multiple computer platforms. Some practical examples are provided.

  7. UCAC4 nearby star survey: A search for our stellar neighbors

    SciTech Connect (OSTI)

    Finch, Charlie T.; Zacharias, Norbert; Subasavage, John P.; Henry, Todd J.; Riedel, Adric R.

    2014-12-01

    We use data from the U.S. Naval Observatory fourth CCD Astrograph Catalog (UCAC4) in combination with photometry from the AAVSO Photometric All-Sky Survey and Two Micron All-Sky Survey to identify stars within 25 pc of the Sun. A sample of nearby stars with accurate trigonometric parallaxes from the Research Consortium On Nearby Stars is used to generate a set of 16 new photometric color–M{sub K{sub s}} relations that provide distance estimates with uncertainties of 15%. This work expands the available suites of well-calibrated photometric distance relations that can be used to identify nearby stellar systems. The distance relations are used with quality cuts to extract an initial sample of stars from the UCAC4 estimated to be within 25 pc. Color, proper motion, and existing literature sources are then used to obtain a clean sample of red dwarfs, while limiting the amount of contamination from background giants, resulting in a sample of 1761 candidate nearby stars within 25 pc. Of these, 339 are new discoveries with no previously known published parallax or distance estimate, primarily with proper motions less than 0.2 arcsec yr{sup −1}. Five stars are estimated to be within 10 pc, with the nearest, TYC 3980 1081 1, with V=10.50 estimated to be at 5.9 pc. That several hundred new stars have been revealed so close to the Sun illustrates once again that there is considerable work yet to be done to map the solar neighborhood and that additional nearby stars are likely still to be discovered.

  8. Constraints on decaying dark matter from Fermi observations of nearby galaxies and clusters

    SciTech Connect (OSTI)

    Dugger, Leanna; Profumo, Stefano; Jeltema, Tesla E. E-mail: tesla@ucolick.org

    2010-12-01

    We analyze the impact of Fermi gamma-ray observations (primarily non-detections) of selected nearby galaxies, including dwarf spheroidals, and of clusters of galaxies on decaying dark matter models. We show that the fact that galaxy clusters do not shine in gamma rays puts the most stringent limits available to-date on the lifetime of dark matter particles for a wide range of particle masses and decay final states. In particular, our results put strong constraints on the possibility of ascribing to decaying dark matter both the increasing positron fraction reported by PAMELA and the high-energy feature in the electron-positron spectrum measured by Fermi. Observations of nearby dwarf galaxies and of the Andromeda Galaxy (M31) do not provide as strong limits as those from galaxy clusters, while still improving on previous constraints in some cases.

  9. Final-Publication-inttech_v6_n34_2013_paged.pdf

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    International Journal on Advances in Internet Technology, vol 6 no 3 & 4, year 2013, http://www.iariajournals.org/internet_technology/ 2013, © Copyright by authors, Published under agreement with IARIA - www.iaria.org On How to Provision Virtual Circuits for Network-Redirected Large-Sized, High-Rate Flows Zhenzhen Yan, Malathi Veeraraghavan Dept. of Electrical and Computer Engineering University of Virginia Charlottesville, VA, USA Email: {zy4d,mvee}@virginia.edu Chris Tracy, Chin Guok

  10. Request for Proposal No. DE-SOL-0008418 Section J, Appendix G, Page i

    National Nuclear Security Administration (NNSA)

    G, Page i SECTION J APPENDIX G PERSONNEL APPENDIX TABLE OF CONTENTS 1.0 Introduction .......................................................................................................................... 1 2.0 Definitions............................................................................................................................ 2 3.0 Compensation ...................................................................................................................... 2 3.1

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    21, Annual Fuel Oil and Kerosene Sales Report Page 1 U.S. DEPARTMENT OF ENERGY U.S. ENERGY ... No.: 2015.01 FORM EIA-821 ANNUAL FUEL OIL AND KEROSENE SALES REPORT INSTRUCTIONS 1. ...

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  15. U.S. Rare Earth Magnet Patents Table © 3-1-2016 page 1

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    Rare Earth Magnet Patents Table 3-1-2016 page 1 Disclaimer: This U.S. Rare Earth Magnet Patents Table contains a sample of the rare earth-magnet patents issued by the U.S. ...

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    Meeting-Dave Hepner Page 1 SRSRA TOWN HALL MEETING New Ellenton Community Center JUNE 27, 2014 After reviewing the notes and discussing the Town Hall Meeting held on June 27, 2014,...

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    Prominently positioned at the top of the new home page is a search box for DOE R&D results that provides one-step access to OSTI's flagship DOE STI product, SciTech Connect. The ...

  18. Request for Proposal No. DE-SOL-XXXXXX Section J, Appendix A, Page i

    National Nuclear Security Administration (NNSA)

    XXXXXX Section J, Appendix A, Page i SECTION J, APPENDIX A: STATEMENT OF WORK TABLE OF CONTENTS CHAPTER I. OBJECTIVES, SCOPE, AND REQUIREMENTS ......................................................................... 1 1.0 OBJECTIVE .................................................................................................................................................. 1 2.0 BACKGROUND

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    Directed Research & Development Page National Energy Research Scientific Computing Center T3E Individual Node Optimization Michael Stewart, SGI/Cray, 4/9/98 * Introduction * T3E Processor * T3E Local Memory * Cache Structure * Optimizing Codes for Cache Usage * Loop Unrolling * Other Useful Optimization Options * References 1 Laboratory Directed Research & Development Page National Energy Research Scientific Computing Center Introduction * Primary topic will be single processor

  20. Microfluidic device having an immobilized pH gradient and page gels for

    Office of Scientific and Technical Information (OSTI)

    protein separation and analysis (Patent) | SciTech Connect device having an immobilized pH gradient and page gels for protein separation and analysis Citation Details In-Document Search Title: Microfluidic device having an immobilized pH gradient and page gels for protein separation and analysis Disclosed is a novel microfluidic device enabling on-chip implementation of a two-dimensional separation methodology. Previously disclosed microscale immobilized pH gradients (IPG) are combined with

  1. Heat loads to divertor nearby components from secondary radiation evolved during plasma instabilities

    SciTech Connect (OSTI)

    Sizyuk, V. Hassanein, A.

    2015-01-15

    A fundamental issue in tokamak operation related to power exhaust during plasma instabilities is the understanding of heat and particle transport from the core plasma into the scrape-off layer and to plasma-facing materials. During abnormal and disruptive operation in tokamaks, radiation transport processes play a critical role in divertor/edge-generated plasma dynamics and are very important in determining overall lifetimes of the divertor and nearby components. This is equivalent to or greater than the effect of the direct impact of escaped core plasma on the divertor plate. We have developed and implemented comprehensive enhanced physical and numerical models in the upgraded HEIGHTS package for simulating detailed photon and particle transport in the evolved edge plasma during various instabilities. The paper describes details of a newly developed 3D Monte Carlo radiation transport model, including optimization methods of generated plasma opacities in the full range of expected photon spectra. Response of the ITER divertor's nearby surfaces due to radiation from the divertor-developed plasma was simulated by using actual full 3D reactor design and magnetic configurations. We analyzed in detail the radiation emission spectra and compared the emission of both carbon and tungsten as divertor plate materials. The integrated 3D simulation predicted unexpectedly high damage risk to the open stainless steel legs of the dome structure in the current ITER design from the intense radiation during a disruption on the tungsten divertor plate.

  2. The mass of the central black hole in the nearby Seyfert galaxy NGC 5273

    SciTech Connect (OSTI)

    Bentz, Misty C.; Horenstein, Daniel; Bazhaw, Craig; Manne-Nicholas, Emily R.; Ou-Yang, Benjamin J.; Anderson, Matthew; Jones, Jeremy; Norris, Ryan P.; Parks, J. Robert; Saylor, Dicy; Teems, Katherine G.; Turner, Clay

    2014-11-20

    We present the results of a reverberation-mapping program targeting NGC 5273, a nearby early-type galaxy with a broad-lined active galactic nucleus (AGN). Over the course of the monitoring program, NGC 5273 showed strong variability that allowed us to measure time delays in the responses of the broad optical recombination lines to changes in the continuum flux. A weighted average of these measurements results in a black hole mass determination of M {sub BH} = (4.7 ± 1.6) × 10{sup 6} M {sub ☉}. An estimate of the size of the black hole sphere of influence in NGC 5273 puts it just at the limit of the resolution achievable with current ground-based large aperture telescopes. NGC 5273 is therefore an important future target for a black hole mass determination from stellar dynamical modeling, especially because it is the only nearby early-type galaxy hosting an AGN with a reverberation-based mass, allowing the best comparison for the masses determined from these two techniques.

  3. IDENTIFYING NEARBY, YOUNG, LATE-TYPE STARS BY MEANS OF THEIR CIRCUMSTELLAR DISKS

    SciTech Connect (OSTI)

    Schneider, Adam; Song, Inseok; Melis, Carl; Zuckerman, B.; Bessell, Mike E-mail: song@physast.uga.edu E-mail: ben@astro.ucla.edu

    2012-10-01

    It has recently been shown that a significant fraction of late-type members of nearby, very young associations (age {approx}<10 Myr) display excess emission at mid-IR wavelengths indicative of dusty circumstellar disks. We demonstrate that the detection of mid-IR excess emission can be utilized to identify new nearby, young, late-type stars including two definite new members ('TWA 33' and 'TWA 34') of the TW Hydrae Association (TWA). Both new TWA members display mid-IR excess emission in the Wide-field Infrared Survey Explorer catalog and they show proper motion and youthful spectroscopic characteristics-namely, H{alpha} emission, strong lithium absorption, and low surface gravity features consistent with known TWA members. We also detect mid-IR excess-the first unambiguous evidence of a dusty circumstellar disk-around a previously identified UV-bright, young, accreting star (2M1337) that is a likely member of the Lower-Centaurus Crux region of the Scorpius-Centaurus Complex.

  4. Paging memory from random access memory to backing storage in a parallel computer

    DOE Patents [OSTI]

    Archer, Charles J; Blocksome, Michael A; Inglett, Todd A; Ratterman, Joseph D; Smith, Brian E

    2013-05-21

    Paging memory from random access memory (`RAM`) to backing storage in a parallel computer that includes a plurality of compute nodes, including: executing a data processing application on a virtual machine operating system in a virtual machine on a first compute node; providing, by a second compute node, backing storage for the contents of RAM on the first compute node; and swapping, by the virtual machine operating system in the virtual machine on the first compute node, a page of memory from RAM on the first compute node to the backing storage on the second compute node.

  5. Attachment 1 - PIC Transcribed Flip Chart Notes Final Meeting Summary Page 12

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    - PIC Transcribed Flip Chart Notes Final Meeting Summary Page 12 Public Involvement Committee September 4, 2013 Strategic Planning: Quarters by month * Q1: Oct. - Dec. * Q2: Jan - March * Q3: April - June * Q4: July - Sept. Page 1 Strategic Planning: 2014 Topics (Interactive activity) * = priority topic for discussion at meeting; �= priority for future discussion | Quarter prioritized for discussion (Q1, Q2, Q3, Q4) * 100-F Proposed Plan | *** Q2 * 100 D-H Proposed Plan * Draft Land

  6. Contract Number DE-AC27-08RV14800 Continuation Page, Modification 360

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    Number DE-AC27-08RV14800 Continuation Page, Modification 360 Page 2 of 4 The following changes are hereby incorporated into the contract under the authority of Federal Acquisition Regulation (FAR) 52.243-2 Changes-Cost Reimbursement, at no additional cost to the Government. 1. Update Contract Section H-15(f), Key Personnel for this Contract, to update the list as follows: FROM: Name Position Mr. Lyden David Olson TOC Project Manager Mr. Robert E. Wilkinson Manager, ESH&Q Mr. Doug Greenwell

  7. Request for Proposal No. DE-SOL-0008470 Section J, Appendix A, Page i

    National Nuclear Security Administration (NNSA)

    J, Appendix A, Page i SECTION J, APPENDIX A: STATEMENT OF WORK TABLE OF CONTENTS CHAPTER I. BACKGROUND, OBJECTIVES, AND REQUIREMENTS .......................... 1 1.0 THE NATIONAL NUCLEAR SECURITY ADMINISTRATION (NNSA) MISSION .................................................. 1 2.0 MANAGEMENT & OPERATIONS .................................................................................................................... 1 3.0 REQUIREMENTS

  8. DOE PAGES

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    February 2016 DOE Organization Chart - February 2016 The DOE Organization Chart is a diagram of the U.S. Department of Energy's structure along with the relationships and relative ranks of its parts and positions/jobs. DOECHART-NONAMES-2016-February-22.pdf (81.63 KB) More Documents & Publications DOE Organization Chart - January

    January 2016 DOE Organization Chart - January 2016 The DOE Organization Chart is a diagram of the U.S. Department of Energy's structure along with the

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    Author Select Author Select

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    request for FY 2016 has allowed OREM to accelerate progress on spending ... will host the semi-annual meeting of the EM ... flow model status report at the February ...

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    Local Government Meynard ?1hU1a Pam Laen RoDer Larson Jerry Peltier Jim Curdy Bob Parks ... HBl1ford Pr.j.t Office " .713 Jidwin. uile4 Ff COrulcTtsUS ArlVloo 168 Ro:hland, W ...

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    Board-a federally appointed citizens panel providing independent recommendations and advice to DOE's Environmental Management Program The U.S. Department of Energy's (DOE) Oak Ridge Office of Environmental Management (OREM) continues to make headway in its mission to clean up deteriorating facilities and legacy waste from operations that began in the 1940s at the onset of the Manhattan Project- era. With DOE's cleanup program making steady progress at the East Tennessee Technology Park (ETTP),

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    heating operation in cold climates. GHP systems harvest the free and renewable energy (solar, geothermal, and heat removed from the built environment) stored in various ground...

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    Ecology DVD 2007 Annual Ecology Report for the Rocky Flats Site Click on the links below to access different portions of the electronic annual report. 2007 Annual Report Sections Vegetation Monitoring Report Revegetation Monitoring Report Present and Original Landfill Revegetation Monitoring Report Frog Vocalization Monitoring Report Rocky Flats Flora List (2007) (NOTE: If reports will not open as .pdf files when clicking on hyperlink below, go to Windows Explorer and open the directory on the

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    Ecology DVD 2008 Annual Ecology Report for the Rocky Flats Site Click on the links below to access different portions of the electronic annual report. 2008 Annual Report Sections Vegetation Surveys Report Revegetation Monitoring Report Wildlife Surveys Report Rocky Flats Flora List (2008) (NOTE: If reports will not open as .pdf files when clicking on hyperlinks go to Windows Explorer and open the directory on the DVD called: \2008 Annual Report\2008 Annual Report PDF Files. Then double-click on

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    ... November to try to allay fears by Nevada officials and citizens about shipping and disposing canisters containing uranium-233 from Oak Ridge at the Nevada National Security Site. ...

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    Environmental Reporting Requirements (To filter the table, type a word or phrase in the boxes below that corresponds with the column you would like to filter. Example, in the box above Report type "monitoring", then select the Go button or use the Enter key on your keyboard) (To reset your filter delete the contents from the boxes and select the Go button or the Enter key) Reporting Mechanism Scheduled or Unscheduled Reporting Notification or Other Frequency Due Date Origin of

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    Ecology Report for the Rocky Flats Site Ecology DVD Click on the links below to access different portions of the electronic annual report. 2009 Annual Report Sections Vegetation...

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    Ecology Report for the Rocky Flats Site Ecology DVD Click on the links below to access different portions of the electronic annual report. 2010 Annual Report Sections Vegetation...

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    Ecology DVD 2007 Annual Ecology Report for the Rocky Flats Site Click on the links below to access different portions of the electronic annual report. 2007 Annual Report Sections...

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    and what activities occurred there. Zone 1 was used for light industry and some waste management and is less contaminated than Zone 2. A remedial investigation feasibility...

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    ... in the subcontract general terms and conditions, and ... without sound records search and retrieval capability ... that it intends to enter into with the Portsmouth ...

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    Gulf of Mexico Proved Reserves and Production by Water Depth, 2009 1 Gulf of Mexico Proved Reserves and Production by Water Depth The Gulf of Mexico Federal Offshore region (GOM Fed) has long been one of the Nation's principal sources of proved reserves. At the end of 2009, the GOM Fed accounted for close to one-fifth of oil proved reserves (second only to Texas) and just over four percent of natural gas proved reserves (the country's seventh largest reporting region). 1 Natural gas proved

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    script writes out the header html. We are sorry to report that an error has occurred. Internal identifier for doc type not found. Return to RevCom | Return to Web Portal Need help? Email Technical Support. This site managed by the Office of Management / US Department of Energy Directives | Regulations | Technical Standards | Reference Library | DOE Forms | About Us | Privacy & Security Notice This script breaks up the email address to avoid spam

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    Improvement Catalyst (HI-Cat) Home Improvement Catalyst (HI-Cat) The Home Improvement Catalyst (HI-Cat) is a new DOE initiative focused on high impact opportunities to achieve energy savings in home improvements already planned or being undertaken by homeowners. The home improvement market represents $150 billion in annual investment, with over 14 million projects that involve replacement or upgrades of heating and cooling systems, windows, siding and roofs, insulation and other measures.

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    should help in transitioning from Bechtel Jacobs to UCOR. Issue 43 * July 2011 I N T H I S I S S U E Retiring Members Honored ...... 2 Student Representatives ... 3...

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    name of the report you want to view.) 2011 Photopoint Monitoring 2011 General Revegetation Monitoring Photos New Revegetation Locations in 2007-2009 (Insert DVD 2 to see this link)...

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    Files. Then double-click on the name of the report you want to view.) 2011 Photopoint Monitoring 2011 General Revegetation Monitoring Photos New Revegetation Locations in 2007-2009...

  13. Correlation of the highest energy cosmic rays with nearby extragalactic objects

    SciTech Connect (OSTI)

    Abraham, J.; Abreu, P.; Aglietta, M.; Aguirre, C.; Allard, D.; Allekotte, I.; Allen, J.; Allison, P.; Alvarez, C.; Alvarez-Muniz, J.; Ambrosio, M.; /Balseiro Inst., San Carlos de Bariloche /Buenos Aires, CONICET /CNEA, Buenos Aires /Pierre Auger Observ. /La Plata U. /Natl. Tech. U., San Rafael /Adelaide U. /Catholic U. of Bolivia, La Paz /Bolivia U. /Rio de Janeiro, CBPF /Sao Paulo U.

    2007-11-01

    Using data collected at the Pierre Auger Observatory during the past 3.7 years, we demonstrate that there is a correlation between the arrival directions of cosmic rays with energy above {approx} 6 x 10{sup 19} eV and the positions of active galactic nuclei (AGN) lying within {approx} 75 Mpc. We reject the hypothesis of an isotropic distribution of these cosmic rays at over 99% confidence level from a prescribed a priori test. The correlation we observe is compatible with the hypothesis that the highest energy particles originate from nearby extragalactic sources whose flux has not been significantly reduced by interaction with the cosmic background radiation. AGN or objects having a similar spatial distribution are possible sources.

  14. Astrophysical tests of modified gravity: Constraints from distance indicators in the nearby universe

    SciTech Connect (OSTI)

    Jain, Bhuvnesh; Vikram, Vinu; Sakstein, Jeremy

    2013-12-10

    We use distance measurements in the nearby universe to carry out new tests of gravity, surpassing other astrophysical tests by over two orders of magnitude for chameleon theories. The three nearby distance indicatorscepheids, tip of the red giant branch (TRGB) stars, and water masersoperate in gravitational fields of widely different strengths. This enables tests of scalar-tensor gravity theories because they are screened from enhanced forces to different extents. Inferred distances from cepheids and TRGB stars are altered (in opposite directions) over a range of chameleon gravity theory parameters well below the sensitivity of cosmological probes. Using published data, we have compared cepheid and TRGB distances in a sample of unscreened dwarf galaxies within 10 Mpc. We use a comparable set of screened galaxies as a control sample. We find no evidence for the order unity force enhancements expected in these theories. Using a two-parameter description of the models (the coupling strength and background field value), we obtain constraints on both the chameleon and symmetron screening scenarios. In particular we show that f(R) models with background field values f {sub R0} above 5 10{sup 7} are ruled out at the 95% confidence level. We also compare TRGB and maser distances to the galaxy NGC 4258 as a second test for larger field values. While there are several approximations and caveats in our study, our analysis demonstrates the power of gravity tests in the local universe. We discuss the prospects for additional improved tests with future observations.

  15. AN INFRARED CENSUS OF DUST IN NEARBY GALAXIES WITH SPITZER (DUSTINGS). I. OVERVIEW

    SciTech Connect (OSTI)

    Boyer, Martha L.; Sonneborn, George [Observational Cosmology Laboratory, Code 665, NASA Goddard Space Flight Center, Greenbelt, MD 20771 (United States); McQuinn, Kristen B. W.; Gehrz, Robert D.; Skillman, Evan [Minnesota Institute for Astrophysics, School of Physics and Astronomy, 116 Church Street SE, University of Minnesota, Minneapolis, MN 55455 (United States); Barmby, Pauline [Department of Physics and Astronomy, University of Western Ontario, London, ON, N6A 3K7 (Canada); Bonanos, Alceste Z. [IAASARS, National Observatory of Athens, GR-15236 Penteli (Greece); Gordon, Karl D.; Meixner, Margaret [STScI, 3700 San Martin Drive, Baltimore, MD 21218 (United States); Groenewegen, M. A. T. [Royal Observatory of Belgium, Ringlaan 3, B-1180 Brussels (Belgium); Lagadec, Eric [Laboratoire Lagrange, UMR7293, Univ. Nice Sophia-Antipolis, CNRS, Observatoire de la Cte d'Azur, F-06300 Nice (France); Lennon, Daniel [ESAEuropean Space Astronomy Centre, Apdo. de Correo 78, E-28691 Villanueva de la Caada, Madrid (Spain); Marengo, Massimo [Department of Physics and Astronomy, Iowa State University, Ames, IA 50011 (United States); Sloan, G. C. [Astronomy Department, Cornell University, Ithaca, NY 14853-6801 (United States); Van Loon, Jacco Th. [Astrophysics Group, Lennard-Jones Laboratories, Keele University, Staffordshire ST5 5BG (United Kingdom); Zijlstra, Albert, E-mail: martha.boyer@nasa.gov [Jodrell Bank Centre for Astrophysics, Alan Turing Building, University of Manchester, Manchester M13 9PL (United Kingdom)

    2015-01-01

    Nearby resolved dwarf galaxies provide excellent opportunities for studying the dust-producing late stages of stellar evolution over a wide range of metallicity (2.7 ? [Fe/H] ? 1.0). Here, we describe DUSTiNGS (DUST in Nearby Galaxies with Spitzer): a 3.6 and 4.5?m post-cryogen Spitzer Space Telescope imaging survey of 50 dwarf galaxies within 1.5 Mpc that is designed to identify dust-producing asymptotic giant branch (AGB) stars and massive stars. The survey includes 37 dwarf spheroidal, 8 dwarf irregular, and 5 transition-type galaxies. This near-complete sample allows for the building of statistics on these rare phases of stellar evolution over the full metallicity range. The photometry is >75% complete at the tip of the red giant branch for all targeted galaxies, with the exception of the crowded inner regions of IC10, NGC185, and NGC147. This photometric depth ensures that the majority of the dust-producing stars, including the thermally pulsing AGB stars, are detected in each galaxy. The images map each galaxy to at least twice the half-light radius to ensure that the entire evolved star population is included and to facilitate the statistical subtraction of background and foreground contamination, which is severe at these wavelengths. In this overview, we describe the survey, the data products, and preliminary results. We show evidence for the presence of dust-producing AGB stars in eight of the targeted galaxies, with metallicities as low as [Fe/H] = 1.9, suggesting that dust production occurs even at low metallicity.

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    Updated Buildings Sector Appliance and Equipment Costs and Efficiencies April 2015 Independent Statistics & Analysis www.eia.gov U.S. Department of Energy Washington, DC 20585 U.S. Energy Information Administration | Updated Buildings Sector Appliance and Equipment Costs and Efficiencies i This report was prepared by the U.S. Energy Information Administration (EIA), the statistical and analytical agency within the U.S. Department of Energy. By law, EIA's data, analyses, and forecasts are

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    Energy Savers [EERE]

    The Preface on pages xvii-xix has been altered to correct a typesetting error in the printed book. All of the text is unchanged, but sections of the text have been rearranged to place paragraphs in the proper order. Rickover and the Nuclear Navy Rickover and the Nuclear Navy THE DISCIPLINE OF TECHNOLOGY by Francis Duncan Naval Institute Press Annapolis, Maryland Published 1989 by the United States Naval Institute Annapolis, Maryland Copyright © 1989 on the foreword All rights reserved. Prepared

  18. Request for Proposal NO. DE-SOL-0008418 Section J, Appendix K, Page 1

    National Nuclear Security Administration (NNSA)

    NO. DE-SOL-0008418 Section J, Appendix K, Page 1 SECTION J APPENDIX K PROGRAM MANAGEMENT AND COST REPORTS The Contractor shall submit periodic cost, schedule, and technical performance plans and reports in such form and substance as required by the Contracting Officer. Reference Section J, Appendix A, Statement of Work, Chapter I, paragraph 3.3. Cost reports will include at a minimum: 1. Monthly general management reports to summarize schedule, labor and cost plans and status, and provide

  19. Getting on the same page-Safety Culture | Y-12 National Security Complex

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    Getting on the same ... Getting on the same page-Safety Culture Posted: July 21, 2015 - 5:27pm Safety culture encompasses our core values, attitudes and behaviors that emphasize safety - the protection of people and the environment - as the overriding priority of our work. The National Nuclear Security Administration Production Office and Consolidated Nuclear Security are committed to having a strong safety culture. The combined core values of NPO and CNS - trust, excellence, teamwork,

  20. Getting on the same page-transformation | Y-12 National Security Complex

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    Getting on the same ... Getting on the same page-transformation Posted: August 17, 2015 - 9:53am Transformation is an effort to unify the Pantex Plant and the Y-12 National Security Complex as one team, working better together, to serve the National Nuclear Security Administration's mission and deliver critical products and services. In the dynamic international nuclear environment, we must prove that our strong traditions and reputation of excellence are still relevant, while adapting our

  1. OSTIblog Articles in the DOE PAGES(Beta) Topic | OSTI, US Dept of Energy

    Office of Scientific and Technical Information (OSTI)

    Office of Scientific and Technical Information DOE PAGES(Beta) Topic How to Accelerate Public Access by Dr. Jeffrey Salmon 20 Apr, 2015 in For science agencies, access to federally funded research is a key part of our mission. And the very first requirement for federal agency public access plans directed by the White House Office of Science and Technology Policy (OSTP) was that the plans must encompass "a strategy for leveraging existing archives, where appropriate, and fostering

  2. 06.27.14 SRS Retirees Town Hall Meeting Q/A Period Summary Page 1

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

    Meeting Q/A Period Summary Page 1 NOTICE: SRSRA TOWN HALL MEETING QUESTION/ANSWER PERIOD SUMMARY New Ellenton Community Center JUNE 27, 2014 *105 in Attendance *Meeting Agenda & Handout available  Dave Moody, DOE-SR Manager  John Veldman, SRS Retirees Association (SRSRA) Board  Dave Hepner, DOE-SR Acquisitions Operations Division Director  Carol Barry, SRNS Benefits Q: Why are their 2 columns on the chart (referencing handout)? A: Left column is ERISA minimum, which is the

  3. Discretization error estimation and exact solution generation using the method of nearby problems.

    SciTech Connect (OSTI)

    Sinclair, Andrew J.; Raju, Anil; Kurzen, Matthew J.; Roy, Christopher John; Phillips, Tyrone S.

    2011-10-01

    The Method of Nearby Problems (MNP), a form of defect correction, is examined as a method for generating exact solutions to partial differential equations and as a discretization error estimator. For generating exact solutions, four-dimensional spline fitting procedures were developed and implemented into a MATLAB code for generating spline fits on structured domains with arbitrary levels of continuity between spline zones. For discretization error estimation, MNP/defect correction only requires a single additional numerical solution on the same grid (as compared to Richardson extrapolation which requires additional numerical solutions on systematically-refined grids). When used for error estimation, it was found that continuity between spline zones was not required. A number of cases were examined including 1D and 2D Burgers equation, the 2D compressible Euler equations, and the 2D incompressible Navier-Stokes equations. The discretization error estimation results compared favorably to Richardson extrapolation and had the advantage of only requiring a single grid to be generated.

  4. HERSCHEL AND SPITZER OBSERVATIONS OF SLOWLY ROTATING, NEARBY ISOLATED NEUTRON STARS

    SciTech Connect (OSTI)

    Posselt, B.; Pavlov, G. G.; Popov, S.; Wachter, S.

    2014-11-01

    Supernova fallback disks around neutron stars have been suspected to influence the evolution of the diverse neutron star populations. Slowly rotating neutron stars are the most promising places to find such disks. Searching for the cold and warm debris of old fallback disks, we carried out Herschel PACS (70 μm, 160 mu m) and Spitzer IRAC (3.6 μm, 4.5 μm) observations of eight slowly rotating (P ≈ 3-11 s) nearby (<1 kpc) isolated neutron stars. Herschel detected 160 μm emission (>5σ) at locations consistent with the positions of the neutron stars RX J0806.4-4123 and RX J2143.0+0654. No other significant infrared emission was detected from the eight neutron stars. We estimate probabilities of 63%, 33%, and 3% that, respectively, none, one, or both Herschel PACS 160 μm detections are unrelated excess sources due to background source confusion or an interstellar cirrus. If the 160 μm emission is indeed related to cold (10-22 K) dust around the neutron stars, this dust is absorbing and re-emitting ∼10% to ∼20% of the neutron stars' X-rays. Such high efficiencies would be at least three orders of magnitude larger than the efficiencies of debris disks around nondegenerate stars. While thin dusty disks around the neutron stars can be excluded as counterparts of the 160 μm emission, dusty asteroid belts constitute a viable option.

  5. Stellar and gaseous nuclear disks observed in nearby (U)LIRGs

    SciTech Connect (OSTI)

    Medling, Anne M.; U, Vivian; Guedes, Javiera; Max, Claire E.; Holden, Bradford; Mayer, Lucio; Roškar, Rok; Armus, Lee; Sanders, David E-mail: max@ucolick.org

    2014-03-20

    We present near-infrared integral field spectroscopy of the central kiloparsec of 17 nearby luminous and ultra-luminous infrared galaxies undergoing major mergers. These observations were taken with OSIRIS assisted by the Keck I and II Adaptive Optics systems, providing spatial resolutions of a few tens of parsecs. The resulting kinematic maps reveal gas disks in at least 16 out of 19 nuclei and stellar disks in 11 out of 11 nuclei observed in these galaxy merger systems. In our late-stages mergers, these disks are young (stellar ages <30 Myr) and likely formed as gas disks that became unstable to star formation during the merger. On average, these disks have effective radii of a few hundred parsecs, masses between 10{sup 8} and 10{sup 10} M {sub ☉}, and v/σ between 1 and 5. These disks are similar to those created in high-resolution hydrodynamical simulations of gas-rich galaxy mergers, and favor short coalescence times for binary black holes. The few galaxies in our sample in earlier stages of mergers have disks that are larger (r {sub eff} ∼ 200-1800 pc) and are likely remnants of the galactic disks that have not yet been completely disrupted by the merger.

  6. Characterizing mid-ultraviolet to optical light curves of nearby type IIn supernovae

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

    de la Rosa, Janie; Roming, Pete; Pritchard, Tyler; Fryer, Chris

    2016-03-21

    Here, we present early mid-ultraviolet and optical observations of Type IIn supernovae (SNe IIn) observed from 2007 to 2013. Our results focus on the properties of UV light curves: peak absolute magnitudes, temporal decay, and color evolution. During early times, this sample demonstrates that UV light decays faster than optical, and each event transitions from a predominantly UV-bright phase to an optically bright phase. In order to understand early UV behavior, we generate and analyze the sample's blackbody luminosity, temperature, and radius as the SN ejecta expand and cool. Since most of our observations were detected post maximum luminosity, wemore » introduce a method for estimating the date of peak magnitude. When our observations are compared based on filter, we find that even though these SNe IIn vary in peak magnitudes, there are similarities in UV decay rates. We use a simple semi-analytical SN model in order to understand the effects of the explosion environment on our UV observations. Understanding the UV characteristics of nearby SNe IIn during an early phase can provide valuable information about the environment surrounding these explosions, leading us to evaluating the diversity of observational properties in this subclass.« less

  7. The abundance properties of nearby late-type galaxies. I. The data

    SciTech Connect (OSTI)

    Pilyugin, L. S.; Grebel, E. K.; Kniazev, A. Y. E-mail: grebel@ari.uni-heidelberg.de

    2014-06-01

    We investigate the oxygen and nitrogen abundance distributions across the optical disks of 130 nearby late-type galaxies using around 3740 published spectra of H II regions. We use these data in order to provide homogeneous abundance determinations for all objects in the sample, including H II regions in which not all of the usual diagnostic lines were measured. Examining the relation between N and O abundances in these galaxies we find that the abundances in their centers and at their isophotal R {sub 25} disk radii follow the same relation. The variation in N/H at a given O/H is around 0.3 dex. We suggest that the observed spread in N/H may be partly caused by the time delay between N and O enrichment and the different star formation histories in galaxies of different morphological types and dimensions. We study the correlations between the abundance properties (central O and N abundances, radial O and N gradients) of a galaxy and its morphological type and dimension.

  8. Alma observations of nearby luminous infrared galaxies with various agn energetic contributions using dense gas tracers

    SciTech Connect (OSTI)

    Imanishi, Masatoshi; Nakanishi, Kouichiro

    2014-07-01

    We present the results of our ALMA Cycle 0 observations, using HCN/HCO{sup +}/HNC J = 4-3 lines, of six nearby luminous infrared galaxies with various energetic contributions from active galactic nuclei (AGNs) estimated from previous infrared spectroscopy. These lines are very effective for probing the physical properties of high-density molecular gas around the hidden energy sources in the nuclear regions of these galaxies. We find that HCN to HCO{sup +} J = 4-3 flux ratios tend to be higher in AGN-important galaxies than in starburst-dominated regions, as was seen at the J = 1-0 transition, while there is no clear difference in the HCN-to-HNC J = 4-3 flux ratios among observed sources. A galaxy with a starburst-type infrared spectral shape and very large molecular line widths shows a high HCN-to-HCO{sup +} J = 4-3 flux ratio, which could be due to turbulence-induced heating. We propose that enhanced HCN J = 4-3 emission relative to HCO{sup +} J = 4-3 could be used to detect more energetic activity than normal starbursts, including deeply buried AGNs, in dusty galaxy populations.

  9. Antideuteron production in {upsilon}(nS) decays and the nearby continuum

    SciTech Connect (OSTI)

    Asner, D. M.; Edwards, K. W.; Briere, R. A.; Chen, J.; Ferguson, T.; Tatishvili, G.; Vogel, H.; Watkins, M. E.; Rosner, J. L.; Adam, N. E.; Alexander, J. P.; Berkelman, K.; Cassel, D. G.; Duboscq, J. E.; Ecklund, K. M.; Ehrlich, R.; Fields, L.; Galik, R. S.; Gibbons, L.; Gray, R.

    2007-01-01

    Using CLEO data, we study the production of the antideuteron, d, in {upsilon}(nS) resonance decays and the nearby continuum. The branching ratios obtained are B{sup dir}({upsilon}(1S){yields}dX)=(3.36{+-}0.23{+-}0.25)x10{sup -5}, B({upsilon}(1S){yields}dX)=(2.86{+-}0.19{+-}0.21)x10{sup -5}, and B({upsilon}(2S){yields}dX)=(3.37{+-}0.50{+-}0.25)x10{sup -5}, where the 'dir' superscript indicates that decays produced via reannihilation of the bb pair to a {gamma}* are removed from both the signal and the normalizing number of {upsilon}(1S) decays in order to isolate direct decays of the {upsilon}(1S) to ggg, gg{gamma}. Upper limits at 90% C.L. are given for B({upsilon}(4S){yields}dX)<1.3x10{sup -5}, and continuum production {sigma}(e{sup +}e{sup -}{yields}dX)<0.031 pb. The {upsilon}(2S) data is also used to extract a limit on {chi}{sub bJ}{yields}dX. The results indicate enhanced deuteron production in ggg, gg{gamma} hadronization compared to {gamma}*{yields}qq. Baryon number compensation is also investigated with the large {upsilon}(1S){yields}dX sample.

  10. Update on the correlation of the highest energy cosmic rays with nearby extragalactic matter

    SciTech Connect (OSTI)

    Abreu, P.; Aglietta, M.; Ahn, E.J.; Allard, D.; Allekotte, I.; Allen, J.; Alvarez Castillo, J.; Alvarez-Muniz, J.; Ambrosio, M.; Aminaei, A.; Anchordoqui, L.; /Wisconsin U., Milwaukee /Lisbon, IST

    2010-06-01

    Data collected by the Pierre Auger Observatory through 31 August 2007 showed evidence for anisotropy in the arrival directions of cosmic rays above the Greisen-Zatsepin-Kuzmin energy threshold, 6 x 10{sup 19} eV. The anisotropy was measured by the fraction of arrival directions that are less than 3.1{sup o} from the position of an active galactic nucleus within 75 Mpc (using the Veron-Cetty and Veron 12th catalog). An updated measurement of this fraction is reported here using the arrival directions of cosmic rays recorded above the same energy threshold through 31 December 2009. The number of arrival directions has increased from 27 to 69, allowing a more precise measurement. The correlating fraction is (38{sub -6}{sup +7})%, compared with 21% expected for isotropic cosmic rays. This is down from the early estimate of (69{sub -13}{sup +11})%. The enlarged set of arrival directions is examined also in relation to other populations of nearby extragalactic objects: galaxies in the 2 Microns All Sky Survey and active galactic nuclei detected in hard X-rays by the Swift Burst Alert Telescope. A celestial region around the position of the radiogalaxy Cen A has the largest excess of arrival directions relative to isotropic expectations. The 2-point autocorrelation function is shown for the enlarged set of arrival directions and compared to the isotropic expectation.

  11. RUPRECHT 147: THE OLDEST NEARBY OPEN CLUSTER AS A NEW BENCHMARK FOR STELLAR ASTROPHYSICS

    SciTech Connect (OSTI)

    Curtis, Jason L.; Wright, Jason T.; Wolfgang, Angie; Brewer, John M.; Johnson, John Asher

    2013-05-15

    Ruprecht 147 is a hitherto unappreciated open cluster that holds great promise as a standard in fundamental stellar astrophysics. We have conducted a radial velocity survey of astrometric candidates with Lick, Palomar, and MMT observatories and have identified over 100 members, including 5 blue stragglers, 11 red giants, and 5 double-lined spectroscopic binaries (SB2s). We estimate the cluster metallicity from spectroscopic analysis, using Spectroscopy Made Easy (SME), and find it to be [M/H] = +0.07 {+-} 0.03. We have obtained deep CFHT/MegaCam g'r'i'z' photometry and fit Padova isochrones to the (g' - i') and Two Micron All Sky Survey (J - K{sub S} ) color-magnitude diagrams, using the {tau}{sup 2} maximum-likelihood procedure of Naylor, and an alternative method using two-dimensional cross-correlations developed in this work. We find best fits for Padova isochrones at age t = 2.5 {+-} 0.25 Gyr, m - M = 7.35 {+-} 0.1, and A{sub V} = 0.25 {+-} 0.05, with additional uncertainty from the unresolved binary population and possibility of differential extinction across this large cluster. The inferred age is heavily dependent on our choice of stellar evolution model: fitting Dartmouth and PARSEC models yield age parameters of 3 Gyr and 3.25 Gyr, respectively. At {approx}300 pc and {approx}3 Gyr, Ruprecht 147 is by far the oldest nearby star cluster.

  12. Imaging survey of subsystems in secondary components to nearby southern dwarfs

    SciTech Connect (OSTI)

    Tokovinin, Andrei

    2014-10-01

    To improve the statistics of hierarchical multiplicity, secondary components of wide nearby binaries with solar-type primaries were surveyed at the SOAR telescope for evaluating the frequency of subsystems. Images of 17 faint secondaries were obtained with the SOAR Adaptive Module that improved the seeing; one new 0.''2 binary was detected. For all targets, photometry in the g', i', z' bands is given. Another 46 secondaries were observed by speckle interferometry, resolving 7 close subsystems. Adding literature data, the binarity of 95 secondary components is evaluated. We found that the detection-corrected frequency of secondary subsystems with periods in the well-surveyed range from 10{sup 3} to 10{sup 5} days is 0.21 ± 0.06—same as the normal frequency of such binaries among solar-type stars, 0.18. This indicates that wide binaries are unlikely to be produced by dynamical evolution of N-body systems, but are rather formed by fragmentation.

  13. FINDING {eta} CAR ANALOGS IN NEARBY GALAXIES USING SPITZER. I. CANDIDATE SELECTION

    SciTech Connect (OSTI)

    Khan, Rubab; Stanek, K. Z.; Kochanek, C. S. E-mail: kstanek@astronomy.ohio-state.edu

    2013-04-10

    The late-stage evolution of the most massive stars such as {eta} Carinae is controlled by the effects of mass loss, which may be dominated by poorly understood eruptive mass ejections. Understanding this population is challenging because no true analogs of {eta} Car have been clearly identified in the Milky Way or other galaxies. We utilize Spitzer IRAC images of seven nearby ({approx}< 4 Mpc) galaxies to search for such analogs. We find 34 candidates with a flat or rising mid-IR spectral energy distributions toward longer mid-infrared wavelengths that emit >10{sup 5} L{sub Sun} in the IRAC bands (3.6 to 8.0 {mu}m) and are not known to be background sources. Based on our estimates for the expected number of background sources, we expect that follow-up observations will show that most of these candidates are not dust enshrouded massive stars, with an expectation of only 6 {+-} 6 surviving candidates. Since we would detect true analogs of {eta} Car for roughly 200 years post-eruption, this implies that the rate of eruptions like {eta} Car is less than the core-collapse supernova rate. It is possible, however, that every M > 40 M{sub Sun} star undergoes such eruptions given our initial results. In Paper II we will characterize the candidates through further analysis and follow-up observations, and there is no barrier to increasing the galaxy sample by an order of magnitude. The primary limitation of the present search is that Spitzer's resolution limits us to the shorter wavelength IRAC bands. With the James Webb Space Telescope, such surveys can be carried out at the far more optimal wavelengths of 10-30 {mu}m, allowing identification of {eta} Car analogs for millennia rather than centuries post-eruption.

  14. A CORRELATION BETWEEN SURFACE DENSITIES OF YOUNG STELLAR OBJECTS AND GAS IN EIGHT NEARBY MOLECULAR CLOUDS

    SciTech Connect (OSTI)

    Gutermuth, R. A.; Pipher, J. L.; Megeath, S. T.; Allen, T. S.; Myers, P. C.; Allen, L. E.

    2011-10-01

    We report the discovery and characterization of a power-law correlation between the local surface densities of Spitzer-identified, dusty young stellar objects (YSOs) and the column density of gas (as traced by near-IR extinction) in eight molecular clouds within 1 kpc and with 100 or more known YSOs. This correlation, which appears in data smoothed over size scales of {approx}1 pc, varies in quality from cloud to cloud; those clouds with tight correlations, MonR2 and Ophiuchus, are fit with power laws of slope 2.67 and 1.87, respectively. The spread in the correlation is attributed primarily to local gas disruption by stars that formed there or to the presence of very young subregions at the onset of star formation. We explore the ratio of the number of Class II to Class I sources, a proxy for the star formation age of a region, as a function of gas column density; this analysis reveals a declining Class II to Class I ratio with increasing column density. We show that the observed star-gas correlation is consistent with a star formation law where the star formation rate per area varies with the gas column density squared. We also propose a simple picture of thermal fragmentation of dense gas in an isothermal, self-gravitating layer as an explanation for the power law. Finally, we briefly compare the star-gas correlation and its implied star formation law with other recent proposed of star formation laws at similar and larger size scales from nearby star-forming regions.

  15. BAYESIAN ANALYSIS TO IDENTIFY NEW STAR CANDIDATES IN NEARBY YOUNG STELLAR KINEMATIC GROUPS

    SciTech Connect (OSTI)

    Malo, Lison; Doyon, Rene; Lafreniere, David; Artigau, Etienne; Gagne, Jonathan; Baron, Frederique; Riedel, Adric E-mail: doyon@astro.umontreal.ca E-mail: artigau@astro.umontreal.ca E-mail: baron@astro.umontreal.ca

    2013-01-10

    We present a new method based on a Bayesian analysis to identify new members of nearby young kinematic groups. The analysis minimally takes into account the position, proper motion, magnitude, and color of a star, but other observables can be readily added (e.g., radial velocity, distance). We use this method to find new young low-mass stars in the {beta} Pictoris and AB Doradus moving groups and in the TW Hydrae, Tucana-Horologium, Columba, Carina, and Argus associations. Starting from a sample of 758 mid-K to mid-M (K5V-M5V) stars showing youth indicators such as H{alpha} and X-ray emission, our analysis yields 214 new highly probable low-mass members of the kinematic groups analyzed. One is in TW Hydrae, 37 in {beta} Pictoris, 17 in Tucana-Horologium, 20 in Columba, 6 in Carina, 50 in Argus, 32 in AB Doradus, and the remaining 51 candidates are likely young but have an ambiguous membership to more than one association. The false alarm rate for new candidates is estimated to be 5% for {beta} Pictoris and TW Hydrae, 10% for Tucana-Horologium, Columba, Carina, and Argus, and 14% for AB Doradus. Our analysis confirms the membership of 58 stars proposed in the literature. Firm membership confirmation of our new candidates will require measurement of their radial velocity (predicted by our analysis), parallax, and lithium 6708 A equivalent width. We have initiated these follow-up observations for a number of candidates, and we have identified two stars (2MASSJ01112542+1526214, 2MASSJ05241914-1601153) as very strong candidate members of the {beta} Pictoris moving group and one strong candidate member (2MASSJ05332558-5117131) of the Tucana-Horologium association; these three stars have radial velocity measurements confirming their membership and lithium detections consistent with young age.

  16. Wide cool and ultracool companions to nearby stars from Pan-STARRS 1

    SciTech Connect (OSTI)

    Deacon, Niall R.; Liu, Michael C.; Magnier, Eugene A.; Aller, Kimberly M.; Best, William M. J.; Bowler, Brendan P.; Burgett, William S.; Chambers, Kenneth C.; Flewelling, H.; Kaiser, Nick; Kudritzki, Rolf-Peter; Morgan, Jeff S.; Tonry, John L.; Dupuy, Trent; Mann, Andrew W.; Redstone, Joshua A.; Draper, Peter W.; Metcalfe, Nigel; Hodapp, Klaus W.; Price, Paul A.; and others

    2014-09-10

    We present the discovery of 57 wide (>5'') separation, low-mass (stellar and substellar) companions to stars in the solar neighborhood identified from Pan-STARRS 1 (PS1) data and the spectral classification of 31 previously known companions. Our companions represent a selective subsample of promising candidates and span a range in spectral type of K7-L9 with the addition of one DA white dwarf. These were identified primarily from a dedicated common proper motion search around nearby stars, along with a few as serendipitous discoveries from our Pan-STARRS 1 brown dwarf search. Our discoveries include 23 new L dwarf companions and one known L dwarf not previously identified as a companion. The primary stars around which we searched for companions come from a list of bright stars with well-measured parallaxes and large proper motions from the Hipparcos catalog (8583 stars, mostly A-K dwarfs) and fainter stars from other proper motion catalogs (79170 stars, mostly M dwarfs). We examine the likelihood that our companions are chance alignments between unrelated stars and conclude that this is unlikely for the majority of the objects that we have followed-up spectroscopically. We also examine the entire population of ultracool (>M7) dwarf companions and conclude that while some are loosely bound, most are unlikely to be disrupted over the course of ?10 Gyr. Our search increases the number of ultracool M dwarf companions wider than 300 AU by 88% and increases the number of L dwarf companions in the same separation range by 82%. Finally, we resolve our new L dwarf companion to HIP 6407 into a tight (0.''13, 7.4 AU) L1+T3 binary, making the system a hierarchical triple. Our search for these key benchmarks against which brown dwarf and exoplanet atmosphere models are tested has yielded the largest number of discoveries to date.

  17. NGC1277: A MASSIVE COMPACT RELIC GALAXY IN THE NEARBY UNIVERSE

    SciTech Connect (OSTI)

    Trujillo, Ignacio; Vazdekis, Alexandre; Balcells, Marc; Snchez-Blzquez, Patricia

    2014-01-10

    As early as 10Gyr ago, galaxies with more than 10{sup 11} M {sub ?} of stars already existed. While most of these massive galaxies must have subsequently transformed through on-going star formation and mergers with other galaxies, a small fraction (?0.1%) may have survived untouched until today. Searches for such relic galaxies, useful windows to explore the early universe, have been inconclusive to date: galaxies with masses and sizes like those observed at high redshift (M {sub *} ? 10{sup 11} M {sub ?}; R{sub e} ? 1.5kpc) have been found in the local universe, but their stars are far too young for the galaxy to be a relic galaxy. This paper explores the first case of a nearby galaxy, NGC1277 (at a distance of 73 Mpc in the Perseus galaxy cluster), which fulfills many criteria to be considered a relic galaxy. Using deep optical spectroscopy, we derive the star formation history along the structure of the galaxy: the stellar populations are uniformly old (>10Gyr) with no evidence for more recent star formation episodes. The metallicity of their stars is super-solar ([Fe/H] = 0.20 0.04 with a smooth decline toward the outer regions) and ?-enriched ([?/Fe] = 0.4 0.1). This suggests a very short formation time scale for the bulk of the stars in this galaxy. This object also rotates very fast (V {sub rot} ? 300kms{sup 1}) and has a large central velocity dispersion (? > 300kms{sup 1}). NGC1277 allows the exploration in full detail of properties such as the structure, internal dynamics, metallicity, and initial mass function as they were at ?10-12Gyr ago when the first massive galaxies were built.

  18. Notice of Intent to Develop a Page Change to DOE O 413.3B, Program and Project Management for the Acquisition of Capital Assets

    Broader source: Directives, Delegations, and Requirements [Office of Management (MA)]

    2015-10-01

    The Page Change is a limited update to incorporate recent Secretarial policies and issues raised by external stakeholders

  19. Notice of Intent to Develop a Page Change to DOE O 413.3B, Program and Project Management for the Acquisition of Capital Assets

    Broader source: Directives, Delegations, and Requirements [Office of Management (MA)]

    The Page Change is a limited update to incorporate recent Secretarial policies and issues raised by external stakeholders

  20. Notice of Intent to Submit Page Changes to Revise DOE O 552.1A, Travel Policy and Procedures

    Broader source: Directives, Delegations, and Requirements [Office of Management (MA)]

    2016-01-07

    A page-change is being undertaken to reflect changes in responsibilities brought about by the August 2013 reorganization which transferred travel related functions and systems between the Office of Chief Financial Officer (OCFO) and the Office of Management (MA).

  1. Notice of Intent to Submit Page Changes to Revise DOE O 552.1A, Travel Policy and Procedures

    Broader source: Directives, Delegations, and Requirements [Office of Management (MA)]

    2016-01-07

    A page change is being undertaken to reflect changes in responsibilities brought about by the August 2013 reorganization which transferred travel related functions and systems between the Office of Chief Financial Officer (OCFO) and the Office of Management (MA).

  2. http://www.census.gov/

    National Nuclear Security Administration (NNSA)

    People & Households American Community Survey * Estimates * Projections Income | State Median Income * Poverty * Health Insurance International * Genealogy * Census 2000 * More ...

  3. B WWW.PLAINSANDEASTERNCLEANLINE.COM

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

    The Plains & Eastern Clean Line will benefit Oklahoma by generating billions of dollars of investment in new wind energy projects, creating thousands of manufacturing and ...

  4. www.energy.gov/fe

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

    ... The program elements focus on gasification, oxy- combustion, advanced turbines, and other energy systems. While the primary focus is on coal-based power systems, improvements to ...

  5. YGG-15-0286r SAME PAGE ONETEAM Better Together What is Performance Excellence?

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

    YGG-15-0286r SAME PAGE ONETEAM Better Together What is Performance Excellence? Isn't this just another flavor-of-the-month campaign? Why should I care? How do we get there? Our mission is extremely important: We keep our country safe. The work we do every day ensures the U.S. remains the world's premier nuclear power, which keeps every other country on earth from attempting to use nuclear weapons. Our families, communities, and nation rely on us to do it right. That said, we share a common

  6. Project Schedules and Milestones Draft July 2014 Site Management Plan Page 1

    Office of Legacy Management (LM)

    Draft July 2014 Site Management Plan Page 1 5.0 Project Schedules and Milestones (FY 2015-FY 2017) 5.1 Establishing Project Schedules and Milestones As stated in Section 1.1.2, the Site Management Plan (SMP) establishes the overall plan for remedial actions at the Monticello Mill Tailings Site (MMTS) and milestones against which progress can be measured. The SMP also documents the overall plan for remedial actions at the Monticello Vicinity Properties site (MVP), which was deleted from the

  7. Project Schedules and Milestones Final August 2013 Site Management Plan Page 1

    Office of Legacy Management (LM)

    Final August 2013 Site Management Plan Page 1 5.0 Project Schedules and Milestones (FY 2014-FY 2016) 5.1 Establishing Project Schedules and Milestones As stated in Section 1.1.2, the Site Management Plan (SMP) establishes the overall plan for remedial actions at the Monticello Mill Tailings Site (MMTS) and milestones against which progress can be measured. The SMP also documents the overall plan for remedial actions at the Monticello Vicinity Properties site (MVP), which was deleted from the

  8. GUIDANCE ON APPLICATION OF FEDERAL VACANCIES REFORM ACT OF 1998 Page 1 of 13

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

    APPLICATION OF FEDERAL VACANCIES REFORM ACT OF 1998 Page 1 of 13 GUIDANCE ON APPLICATION OF FEDERAL VACANCIES REFORM ACT OF 1998 This memorandum provides guidance on the application of the Federal Vacancies Reform Act of1998 to vacancies in Senate-confirmed offices within the executive branch. March 22, 1999 MEMORANDUM FOR AGENCY GENERAL COUNSELS On October 21, 1998, the Federal Vacancies Reform Act of 1998 ("Vacancies Reform Act" or "Act") was signed into law. ( ) The

  9. Engstrom, Suyama, Vanni, Mattson, Serres, Cimon, Leckband Page 1 of 3

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

    RI/FS and Proposed Plan, 100-F, Draft A, v.1 Engstrom, Suyama, Vanni, Mattson, Serres, Cimon, Leckband Page 1 of 3 Draft Advice re: Remedial Investigation/Feasibility Study and Proposed Plan for Remediation of the 100-FR-1, 100-FR-2, 100-FR-3, 100-IU-2, and 100-IU-6 Operable Units, Draft A Background The Hanford Advisory Board (Board) appreciates the opportunity to provide comments and advice for the Remedial Investigation/Feasibility Study and Proposed Plan for Remediation of the 100-FR-1,

  10. 1. CNTRAT IDCODE PAGE OF PGES AMENDMENT OF SOLICITATION/MODIFICATION OF CONTRACT

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

    CNTRAT IDCODE PAGE OF PGES AMENDMENT OF SOLICITATION/MODIFICATION OF CONTRACT 1 OTATI OEPG FIP 5S 2, AMENDMENT/MODIFICATION NO. 3. EFFECTIVE DATE (M/IJ/Y) 4. REQUISITION/PURCHASE REQ. NO. 5. PROJECT NO. (If applicable) 313 See Block 16C1 6. ISSUED BY CODE 7. ADMINISTERED BY (If other than Item 6) CODE U.S. Department of Energy Office of River Protection P. 0. Box 450, MIS H6-60 Richland, WA 99352 8. NAME AND ADDRESS OF CONTRACTOR (No., stree, county, Slate and ZIP code) 9A. AMENDMENT OF

  11. U.S. Rare Earth Magnet Patents Table © 8-29-2016 page 1

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

    Rare Earth Magnet Patents Table © 8-29-2016 page 1 Disclaimer: This U.S. Rare Earth Magnet Patents Table contains a sample of the rare earth-magnet patents issued by the U.S. Patent and Trademark Office. It was created with key word searching. The Table is not all inclusive of U.S. magnet patents and does not include foreign patents. Some cells in the Table contain estimates, approximations or assessments. Please consult with a professional patent attorney or patent agent, possessing license to

  12. Central Plateau Cleanup Final Comments and Responses Document on Proposed Changes to Central Plateau Cleanup Page 1

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

    and Responses on Proposed TPA Changes to Central Plateau Cleanup Final Comments and Responses Document on Proposed Changes to Central Plateau Cleanup Page 1 Comments and Responses to the Tentative Agreement on Hanford Federal Facility Agreement and Consent Order Implementing Changes to Central Plateau Cleanup October 2010 Comments and Responses on Proposed TPA Changes to Central Plateau Cleanup Final Comments and Responses Document on Proposed Changes to Central Plateau Cleanup Page 2 Public

  13. THE STAR FORMATION HISTORY AND CHEMICAL EVOLUTION OF STAR-FORMING GALAXIES IN THE NEARBY UNIVERSE

    SciTech Connect (OSTI)

    Torres-Papaqui, J. P.; Coziol, R.; Ortega-Minakata, R. A.; Neri-Larios, D. M. E-mail: rcoziol@astro.ugto.mx E-mail: daniel@astro.ugto.mx

    2012-08-01

    We have determined the metallicity (O/H) and nitrogen abundance (N/O) of a sample of 122,751 star-forming galaxies (SFGs) from the Data Release 7 of the Sloan Digital Sky Survey. For all these galaxies we have also determined their morphology and obtained a comprehensive picture of their star formation history (SFH) using the spectral synthesis code STARLIGHT. The comparison of the chemical abundance with the SFH allows us to describe the chemical evolution of the SFGs in the nearby universe (z {<=} 0.25) in a manner consistent with the formation of their stellar populations and morphologies. A high fraction (45%) of the SFGs in our sample show an excess abundance of nitrogen relative to their metallicity. We also find this excess to be accompanied by a deficiency of oxygen, which suggests that this could be the result of effective starburst winds. However, we find no difference in the mode of star formation of the nitrogen-rich and nitrogen-poor SFGs. Our analysis suggests that they all form their stars through a succession of bursts of star formation extended over a period of few Gyr. What produces the chemical differences between these galaxies seems therefore to be the intensity of the bursts: the galaxies with an excess of nitrogen are those that are presently experiencing more intense bursts or have experienced more intense bursts in their past. We also find evidence relating the chemical evolution process to the formation of the galaxies: the galaxies with an excess of nitrogen are more massive, and have more massive bulges and earlier morphologies than those showing no excess. Contrary to expectation, we find no evidence that the starburst wind efficiency decreases with the mass of the galaxies. As a possible explanation we propose that the loss of metals consistent with starburst winds took place during the formation of the galaxies, when their potential wells were still building up, and consequently were weaker than today, making starburst winds more

  14. BROAD Ly{alpha} EMISSION FROM THREE NEARBY BL LACERTAE OBJECTS

    SciTech Connect (OSTI)

    Stocke, John T.; Danforth, Charles W. [CASA, Department of Astrophysical and Planetary Sciences, University of Colorado, 389-UCB, Boulder, CO 80309 (United States); Perlman, Eric S., E-mail: danforth@casa.colorado.edu, E-mail: stocke@casa.colorado.edu, E-mail: eperlman@fit.edu [Florida Institute of Technology, Physics and Space Sciences Department, 150 West University Boulevard, Melbourne, FL 32901 (United States)

    2011-05-10

    We present far-UV HST/COS spectra of four nearby BL Lac objects. BL Lac spectra are dominated by a smooth, power-law continuum which arises in a relativistic jet. However, the spectra are not necessarily featureless; weak, broad- and/or narrow-line emission is sometimes seen in high-quality optical spectra. We present detections of Ly{alpha} emission in HST/COS spectra of Mrk 421 (z = 0.030) and PKS 2005-489 (z = 0.071) as well as an archival HST/GHRS observation of Mrk 501 (z = 0.0337). Archival HST/STIS observations of PKS 2155-304 (z = 0.116) show no Ly{alpha} emission to a very low upper limit. Using the assumption that the broad-line region (BLR) clouds are symmetrically placed around the active galactic nucleus (AGN), we use these measured Ly{alpha} emission features to constrain either the relativistic {Gamma} values for the ionizing continuum produced by the jet (in the ionization-bounded case) or the mass of warm gas (in the density-bounded case). While realistic {Gamma} values can be obtained for all four cases, the values for Mrk 421 and PKS 2155-304 are high enough to suggest that covering factors of BLR clouds of {approx}1%-2% might be required to provide consistency with earlier values of Doppler boosting and viewing angles suggested for this class of BL Lacs. This discrepancy also exists in the case of M 87, where the amount of Doppler boosting in our direction is expected to be minimal, again suggestive of a small covering factor of BLR clouds. If, as these small covering factors might suggest, the assumptions of a density-bounded model could be more correct, then the observed Ly{alpha} luminosities require that BL Lac/FR 1 nuclei possess very little warm gas (10{sup -4} to 10{sup -5} M{sub sun}) as suggested by Guilbert et al. If these clouds are in pressure balance with a hotter ({approx}10{sup 6} K) gas, the BLR contains too little mass to power the AGN by accretion alone.

  15. Dark Matter Searches with Cherenkov Telescopes: Nearby Dwarf Galaxies or Local Galaxy Clusters?

    SciTech Connect (OSTI)

    Sanchez-Conde, Miguel A.; Cannoni, Mirco; Zandanel, Fabio; Gomez, Mario E.; Prada, Francisco; /IAA, Granada

    2012-06-06

    In this paper, we compare dwarf galaxies and galaxy clusters in order to elucidate which object class is the best target for gamma-ray DM searches with imaging atmospheric Cherenkov telescopes (IACTs). We have built a mixed dwarfs+clusters sample containing some of the most promising nearby dwarf galaxies (Draco, Ursa Minor, Wilman 1 and Segue 1) and local galaxy clusters (Perseus, Coma, Ophiuchus, Virgo, Fornax, NGC 5813 and NGC 5846), and then compute their DM annihilation flux profiles by making use of the latest modeling of their DM density profiles. We also include in our calculations the effect of DM substructure. Willman 1 appears as the best candidate in the sample. However, its mass modeling is still rather uncertain, so probably other candidates with less uncertainties and quite similar fluxes, namely Ursa Minor and Segue 1, might be better options. As for galaxy clusters, Virgo represents the one with the highest flux. However, its large spatial extension can be a serious handicap for IACT observations and posterior data analysis. Yet, other local galaxy cluster candidates with more moderate emission regions, such as Perseus, may represent good alternatives. After comparing dwarfs and clusters, we found that the former exhibit annihilation flux profiles that, at the center, are roughly one order of magnitude higher than those of clusters, although galaxy clusters can yield similar, or even higher, integrated fluxes for the whole object once substructure is taken into account. Even when any of these objects are strictly point-like according to the properties of their annihilation signals, we conclude that dwarf galaxies are best suited for observational strategies based on the search of point-like sources, while galaxy clusters represent best targets for analyses that can deal with rather extended emissions. Finally, we study the detection prospects for present and future IACTs in the framework of the constrained minimal supersymmetric standard model. We

  16. THE NEAR-INFRARED CORONAL LINE SPECTRUM OF 54 NEARBY ACTIVE GALACTIC NUCLEI

    SciTech Connect (OSTI)

    Rodriguez-Ardila, A.

    2011-12-20

    The relationship between the emission of coronal lines (CLs) and nuclear activity in 36 Type 1 and 18 Type 2 active galactic nuclei (AGNs) is analyzed, for the first time, based on near-infrared (0.8-2.4 {mu}m) spectra. The eight CLs studied, of Si, S, Fe, Al, and Ca elements and corresponding to ionization potentials (IPs) in the range 125-450 eV, are detected (3{sigma}) in 67% (36 AGNs) of the sample. Our analysis shows that the four most frequent CLs [Si VI] 1.963 {mu}m, [S VIII] 0.9913 {mu}m, [S IX] 1.252 {mu}m, and [Si X] 1.430 {mu}m display a narrow range in luminosity, with most lines located in the interval log L 39-40 erg s{sup -1}. We found that the non-detection is largely associated with either loss of spatial resolution or increasing object distance: CLs are essentially nuclear and easily lose contrast in the continuum stellar light for nearby sources or get diluted by the strong AGN continuum as the redshift increases. Yet, there are AGNs where the lack of coronal emission, i.e., lines with IP {>=} 100 eV, may be genuine. The absence of these lines reflects a non-standard AGN ionizing continuum, namely, a very hard spectrum lacking photons below a few Kev. The analysis of the line profiles points out a trend of increasing FWHM with increasing IPs up to energies around 300 eV, where a maximum in the FWHM is reached. For higher IP lines, the FWHM remains nearly constant or decreases with increasing IPs. We ascribe this effect to an increasing density environment as we approach the innermost regions of these AGNs, where densities above the critical density of the CLs with IPs larger than 300 eV are reached. This sets a strict range limit for the density in the boundary region between the narrow and the broad region of 10{sup 8}-10{sup 9} cm{sup -3}. A relationship between the luminosity of the CLs and that of the soft and hard X-ray emission and the soft X-ray photon index is observed: the coronal emission becomes stronger with both increasing X

  17. SUB-MILLIMETER TELESCOPE CO (2-1) OBSERVATIONS OF NEARBY STAR-FORMING GALAXIES

    SciTech Connect (OSTI)

    Jiang, Xue-Jian; Gu, Qiusheng; Wang, Zhong; Wang, Junzhi; Zhang, Zhi-Yu

    2015-01-20

    We present CO J = 2-1 observations toward 32 nearby gas-rich star-forming galaxies selected from the ALFALFA and Wide-field Infrared Survey Explorer (WISE) catalogs, using the Sub-millimeter Telescope (SMT). Our sample is selected to be dominated by intermediate-M {sub *} galaxies. The scaling relations between molecular gas, atomic gas, and galactic properties (stellar mass, NUV – r, and WISE color W3 – W2) are examined and discussed. Our results show the following. (1) In the galaxies with stellar mass M {sub *} ≤10{sup 10} M {sub ☉}, the H I fraction (f {sub H} {sub I} ≡ M {sub H} {sub I}/M {sub *}) is significantly higher than that of more massive galaxies, while the H{sub 2} gas fraction (f{sub H{sub 2}} ≡ M{sub H{sub 2}}/M {sub *}) remains nearly unchanged. (2) Compared to f{sub H{sub 2}}, f {sub H} {sub I} correlates better with both M {sub *} and NUV – r. (3) A new parameter, WISE color W3 – W2 (12-4.6 μm), is introduced, which is similar to NUV – r in tracing star formation activity, and we find that W3 – W2 has a tighter anti-correlation with log f{sub H{sub 2}} than the anti-correlation of (NUV – r)-f {sub H} {sub I}, (NUV – r)-f{sub H{sub 2}}, and (W3 – W2)-f {sub H} {sub I}. This indicates that W3 – W2 can trace the H{sub 2} fraction in galaxies. For the gas ratio M{sub H{sub 2}}/M {sub H} {sub I} , only in the intermediate-M {sub *} galaxies it appears to depend on M {sub *} and NUV – r. We find a tight correlation between the molecular gas mass M{sub H{sub 2}} and 12 μm (W3) luminosities (L {sub 12} {sub μm}), and the slope is close to unity (1.03 ± 0.06) for the SMT sample. This correlation may reflect that the cold gas and dust are well mixed on a global galactic scale. Using the all-sky 12 μm (W3) data available in WISE, this correlation can be used to estimate CO flux for molecular gas observations and can even predict H{sub 2} mass for star-forming galaxies.

  18. Add Java extensions to your wiki: Java applets can bring dynamic functionality to your wiki pages

    SciTech Connect (OSTI)

    Scarberry, Randall E.

    2008-08-12

    Virtually everyone familiar with today’s world wide web has encountered the free online encyclopedia Wikipedia many times. What you may not know is that Wikipedia is driven by an excellent open-source product called MediaWiki which is available to anyone for free. This has led to a proliferation of wiki sites devoted to just about any topic one can imagine. Users of a wiki can add content -- all that is required of them is that they type in their additions into their web browsers using the simple markup language called wikitext. Even better, the developers of wikitext made it extensible. With a little server-side development of your own, you can add your own custom syntax. Users aware of your extensions can then utilize them on their wiki pages with a few simple keystrokes. These extensions can be custom decorations, formatting, web applications, and even instances of the venerable old Java applet. One example of a Java applet extension is the Jmol extension (REF), used to embed a 3-D molecular viewer. This article will walk you through the deployment of a fairly elaborate applet via a MediaWiki extension. By no means exhaustive -- an entire book would be required for that -- it will demonstrate how to give the applet resize handles using using a little Javascript and CSS coding and some popular Javascript libraries. It even describes how a user may customize the extension somewhat using a wiki template. Finally, it explains a rudimentary persistence mechanism which allows applets to save data directly to the wiki pages on which they reside.

  19. A Temporal Locality-Aware Page-Mapped Flash Translation Layer

    SciTech Connect (OSTI)

    Kim, Youngjae; Gupta, Aayush; Urgaonkar, Bhuvan

    2013-01-01

    The poor performance of random writes has been a cause of major concern which needs to be addressed to better utilize the potential of flash in enterprise-scale environments. We examine one of the important causes of this poor performance: the design of the flash translation layer (FTL) which performs the virtual-to-physical address translations and hides the erase-before-write characteristics of flash. We propose a complete paradigm shift in the design of the core FTL engine from the existing techniques with our Demand-Based Flash Translation Layer (DFTL) which selectively caches page- level address mappings. Our experimental evaluation using FlashSim with realistic enterprise-scale workloads endorses the utility of DFTL in enterprise-scale storage systems by demonstrating: 1) improved performance, 2) reduced garbage collection overhead and 3) better overload behavior compared with hybrid FTL schemes which are the most popular implementation methods. For example, a predominantly random-write dominant I/O trace from an OLTP application running at a large financial institution shows a 78% improvement in average response time (due to a 3-fold reduction in operations of the garbage collector), compared with the hybrid FTL scheme. Even for the well-known read-dominant TPC-H benchmark, for which DFTL introduces additional overheads, we improve system response time by 56%. Moreover, interestingly, when write-back cache on DFTL-based SSD is enabled, DFTL even outperforms the page-based FTL scheme, improving their response time by 72% in Financial trace.

  20. OVERVIEW OF THE SDSS-IV MaNGA SURVEY: MAPPING NEARBY GALAXIES AT APACHE POINT OBSERVATORY

    SciTech Connect (OSTI)

    Bundy, Kevin; Bershady, Matthew A.; Wake, David A.; Tremonti, Christy; Diamond-Stanic, Aleksandar M.; Law, David R.; Cherinka, Brian; Yan, Renbin; Snchez-Gallego, Jos R.; Drory, Niv; MacDonald, Nicholas; Weijmans, Anne-Marie; Thomas, Daniel; Masters, Karen; Coccato, Lodovico; Aragn-Salamanca, Alfonso; Avila-Reese, Vladimir; Badenes, Carles; Falcn-Barroso, Jsus; Belfiore, Francesco; and others

    2015-01-01

    We present an overview of a new integral field spectroscopic survey called MaNGA (Mapping Nearby Galaxies at Apache Point Observatory), one of three core programs in the fourth-generation Sloan Digital Sky Survey (SDSS-IV) that began on 2014 July 1. MaNGA will investigate the internal kinematic structure and composition of gas and stars in an unprecedented sample of 10,000 nearby galaxies. We summarize essential characteristics of the instrument and survey design in the context of MaNGA's key science goals and present prototype observations to demonstrate MaNGA's scientific potential. MaNGA employs dithered observations with 17 fiber-bundle integral field units that vary in diameter from 12'' (19 fibers) to 32'' (127 fibers). Two dual-channel spectrographs provide simultaneous wavelength coverage over 3600-10300 at R ? 2000. With a typical integration time of 3 hr, MaNGA reaches a target r-band signal-to-noise ratio of 4-8 ({sup 1} per 2'' fiber) at 23 AB mag arcsec{sup 2}, which is typical for the outskirts of MaNGA galaxies. Targets are selected with M {sub *} ? 10{sup 9} M {sub ?} using SDSS-I redshifts and i-band luminosity to achieve uniform radial coverage in terms of the effective radius, an approximately flat distribution in stellar mass, and a sample spanning a wide range of environments. Analysis of our prototype observations demonstrates MaNGA's ability to probe gas ionization, shed light on recent star formation and quenching, enable dynamical modeling, decompose constituent components, and map the composition of stellar populations. MaNGA's spatially resolved spectra will enable an unprecedented study of the astrophysics of nearby galaxies in the coming 6yr.

  1. Nearby-fluids equilibria. II. Zonal flows in a high-{beta}, self-organized plasma experiment

    SciTech Connect (OSTI)

    Steinhauer, L.C.; Guo, H.Y.

    2006-05-15

    The field and flow structure observed in a high-{beta} field reversed configuration (FRC) produced in the translation, confinement, and sustainment (TCS) experiment are modeled using the newly developed nearby-fluids equilibrium model. These results are the first evidence that experimental FRCs have complex flows, that is nonrigid rotational flow and poloidal flow, both with maximum speeds nearly half the Alfven speed. The interpretive approach is an innovative 'backwards' method using the nearby-fluids platform for two-fluid equilibria. The most remarkable outcome is the prediction of a poloidal flow structure with significant zonal features. The poloidal flow has never been directly measured in FRCs; thus this discovery results from applying the flowing equilibrium model as an interpretive tool. The poloidal flows explain the unusual toroidal field structure observed in TCS. Zonal features in the rotational flow are also inferred from the unfolding of chord-integrated measurements. The results also indicated that a broad core of the FRC is very close to a minimum energy state.

  2. A CENSUS OF BROAD-LINE ACTIVE GALACTIC NUCLEI IN NEARBY GALAXIES: COEVAL STAR FORMATION AND RAPID BLACK HOLE GROWTH

    SciTech Connect (OSTI)

    Trump, Jonathan R.; Fang, Jerome J.; Faber, S. M.; Koo, David C.; Kocevski, Dale D.

    2013-02-15

    We present the first quantified, statistical map of broad-line active galactic nucleus (AGN) frequency with host galaxy color and stellar mass in nearby (0.01 < z < 0.11) galaxies. Aperture photometry and z-band concentration measurements from the Sloan Digital Sky Survey are used to disentangle AGN and galaxy emission, resulting in estimates of uncontaminated galaxy rest-frame color, luminosity, and stellar mass. Broad-line AGNs are distributed throughout the blue cloud and green valley at a given stellar mass, and are much rarer in quiescent (red sequence) galaxies. This is in contrast to the published host galaxy properties of weaker narrow-line AGNs, indicating that broad-line AGNs occur during a different phase in galaxy evolution. More luminous broad-line AGNs have bluer host galaxies, even at fixed mass, suggesting that the same processes that fuel nuclear activity also efficiently form stars. The data favor processes that simultaneously fuel both star formation activity and rapid supermassive black hole accretion. If AGNs cause feedback on their host galaxies in the nearby universe, the evidence of galaxy-wide quenching must be delayed until after the broad-line AGN phase.

  3. XMM-NEWTON OBSERVATIONS OF LUMINOUS SOURCES IN NEARBY GALAXIES NGC 4395, NGC 4736, AND NGC 4258

    SciTech Connect (OSTI)

    Akyuz, A.; Avdan, H.; Kayaci, S.; Ozel, M. E.; Sonbas, E.; Balman, S.

    2013-03-15

    We present the results of a study of non-nuclear discrete sources in a sample of three nearby spiral galaxies (NGC 4395, NGC 4736, and NGC 4258) based on XMM-Newton archival data supplemented with Chandra data for spectral and timing analyses. A total of 75 X-ray sources have been detected within the D{sub 25} regions of the target galaxies. The large collecting area of XMM-Newton makes the statistics sufficient to obtain spectral fitting for 16 (about 20%) of these sources. Compiling the extensive archival exposures available, we were able to obtain the detailed spectral shapes of diverse classes of point sources. We have also studied temporal properties of these luminous sources. Eleven of them are found to show short-term (less than 80 ks) variation while eight of them show long-term variation within factors of {approx}2-5 during a time interval of {approx}2-12 years. Timing analysis provides strong evidence that most of these sources are accreting X-ray binary systems. One source that has properties different from others was suspected to be a supernova remnant, and our follow-up optical observation confirmed this. Our results indicate that sources within the three nearby galaxies are showing a variety of source populations, including several ultraluminous X-ray sources, X-ray binaries, transients together with a super soft source, and a background active galactic nucleus candidate.

  4. Management of wildlife causing damage at Argonne National Laboratory-East, DuPage County, Illinois

    SciTech Connect (OSTI)

    1995-04-01

    The DOE, after an independent review, has adopted an Environmental Assessment (EA) prepared by the US Department of Agriculture (USDA) which evaluates use of an Integrated Wildlife Damage Management approach at Argonne National Laboratory-East (ANL-E) in DuPage County, Illinois (April 1995). In 1994, the USDA issued a programmatic Environmental Impact Statement (EIS) that covers nationwide animal damage control activities. The EA for Management of Wildlife Causing Damage at ANL-E tiers off this programmatic EIS. The USDA wrote the EA as a result of DOE`s request to USDA to prepare and implement a comprehensive Wildlife Management Damage Plan; the USDA has authority for animal damage control under the Animal Damage Control Act of 1931, as amended, and the Rural Development, Agriculture and Related Agencies Appropriations Act of 1988. DOE has determined, based on the analysis in the EA, that the proposed action does not constitute a major Federal action significantly affecting the quality of the human environment within the meaning of the National Environmental Policy Act of 1969 (NEPA). Therefore, the preparation of an EIS is not required. This report contains the Environmental Assessment, as well as the Finding of No Significant Impact (FONSI).

  5. BANYAN. II. Very low mass and substellar candidate members to nearby, young kinematic groups with previously known signs of youth

    SciTech Connect (OSTI)

    Gagn, Jonathan; Lafrenire, David; Doyon, Ren; Malo, Lison; Artigau, tienne

    2014-03-10

    We present Bayesian Analysis for Nearby Young AssociatioNs II (BANYAN II), a modified Bayesian analysis for assessing the membership of later-than-M5 objects to any of several Nearby Young Associations (NYAs). In addition to using kinematic information (from sky position and proper motion), this analysis exploits 2MASS-WISE color-magnitude diagrams in which old and young objects follow distinct sequences. As an improvement over our earlier work, the spatial and kinematic distributions for each association are now modeled as ellipsoids whose axes need not be aligned with the Galactic coordinate axes, and we use prior probabilities matching the expected populations of the NYAs considered versus field stars. We present an extensive contamination analysis to characterize the performance of our new method. We find that Bayesian probabilities are generally representative of contamination rates, except when a parallax measurement is considered. In this case contamination rates become significantly smaller and hence Bayesian probabilities for NYA memberships are pessimistic. We apply this new algorithm to a sample of 158 objects from the literature that are either known to display spectroscopic signs of youth or have unusually red near-infrared colors for their spectral type. Based on our analysis, we identify 25 objects as new highly probable candidates to NYAs, including a new M7.5 bona fide member to Tucana-Horologium, making it the latest-type member. In addition, we reveal that a known L2? dwarf is co-moving with a bright M5 dwarf, and we show for the first time that two of the currently known ultra red L dwarfs are strong candidates to the AB Doradus moving group. Several objects identified here as highly probable members to NYAs could be free-floating planetary-mass objects if their membership is confirmed.

  6. SUBARU AND GEMINI HIGH SPATIAL RESOLUTION INFRARED 18 {mu}m IMAGING OBSERVATIONS OF NEARBY LUMINOUS INFRARED GALAXIES

    SciTech Connect (OSTI)

    Imanishi, Masatoshi; Imase, Keisuke; Oi, Nagisa; Ichikawa, Kohei

    2011-05-15

    We present the results of a ground-based, high spatial resolution infrared 18 {mu}m imaging study of nearby luminous infrared galaxies (LIRGs), using the Subaru 8.2 m and Gemini-South 8.1 m telescopes. The diffraction-limited images routinely achieved with these telescopes in the Q band (17-23 {mu}m) allow us to investigate the detailed spatial distribution of infrared emission in these LIRGs. We then investigate whether the emission surface brightnesses are modest, as observed in starbursts, or are so high that luminous active galactic nuclei (AGNs; high emission surface brightness energy sources) are indicated. The sample consists of 18 luminous buried AGN candidates and starburst-classified LIRGs identified in earlier infrared spectroscopy. We find that the infrared 18 {mu}m emission from the buried AGN candidates is generally compact, and the estimated emission surface brightnesses are high, sometimes exceeding the maximum value observed in and theoretically predicted for a starburst phenomenon. The starburst-classified LIRGs usually display spatially extended 18 {mu}m emission and the estimated emission surface brightnesses are modest, within the range sustained by a starburst phenomenon. The general agreement between infrared spectroscopic and imaging energy diagnostic methods suggests that both are useful tools for understanding the hidden energy sources of the dusty LIRG population.

  7. No X-rays from the very nearby type Ia SN 2014J: Constraints on its environment

    SciTech Connect (OSTI)

    Margutti, R.; Parrent, J.; Kamble, A.; Soderberg, A. M.; Milisavljevic, D.; Drout, M. R.; Kirshner, R. [Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138 (United States); Foley, R. J. [Astronomy Department, University of Illinois at Urbana-Champaign, 1002 W. Green Street, Urbana, IL 61801 (United States)

    2014-07-20

    Deep X-ray observations of the post-explosion environment around the very nearby Type Ia SN 2014J (d{sub L} = 3.5 Mpc) reveal no X-ray emission down to a luminosity L{sub x} < 7 10{sup 36} erg s{sup 1} (0.3-10 keV) at ?t ? 20 days after the explosion. We interpret this limit in the context of inverse Compton emission from upscattered optical photons by the supernova shock and constrain the pre-explosion mass-loss rate of the stellar progenitor system to be M-dot <10{sup ?9} M{sub ?} yr{sup ?1} (for wind velocity v{sub w} = 100 km s{sup 1}). Alternatively, the SN shock might be expanding into a uniform medium with density n{sub CSM} < 3 cm{sup 3}. These results rule out single-degenerate (SD) systems with steady mass loss until the terminal explosion and constrain the fraction of transferred material lost at the outer Lagrangian point to be ?1%. The allowed progenitors are (1) white dwarf-white dwarf progenitors, (2) SD systems with unstable hydrogen burning experiencing recurrent nova eruptions with recurrence time t < 300 yr, and (3) stars where the mass loss ceases before the explosion.

  8. Power line fault current coupling to nearby natural gas pipelines: Volume 3, Analysis of pipeline coating impedance: Final report

    SciTech Connect (OSTI)

    Dabkowski, J.; Frazier, M. J.

    1988-08-01

    This report is a compilation of results obtained from two research programs. The response of a pipeline and coating at the higher voltage excitation levels encountered under power line fault conditions appears to be dominated by conduction at holiday sites in the coating. A simple analytical model was developed for predicting the resistance of a pipeline coating holiday as a function of the voltage produced across the pipeline coating by a nearby faulted power transmission line. The model was initially validated using coated pipeline samples stressed by a capacitive discharge voltage. Additional validation tests were then performed at the Pacific Gas and Electric Company's High Voltage Engineering Research Facility using high voltage ac waveforms for fault simulation. The principle program objective was to develop, both by laboratory and controlled field testing, an electrical resistance characterization for the pipeline coating as a function of the applied voltage level. The development of this model will allow a more accurate prediction of coupled voltage levels to a pipeline during fault current conditions. 54 figs, 3 tabs.

  9. THE JAMES CLERK MAXWELL TELESCOPE NEARBY GALAXIES LEGACY SURVEY. II. WARM MOLECULAR GAS AND STAR FORMATION IN THREE FIELD SPIRAL GALAXIES

    SciTech Connect (OSTI)

    Warren, B. E.; Wilson, C. D.; Sinukoff, E.; Israel, F. P.; Van der Werf, P. P.; Serjeant, S.; Bendo, G. J.; Clements, D. L.; Brinks, E.; Irwin, J. A.; Knapen, J. H.; Leech, J.; Tan, B. K.; Matthews, H. E.; Muehle, S.; Mortimer, A. M. J.; Petitpas, G.; Spekkens, K.; Tilanus, R. P. J.; Usero, A. E-mail: wilson@physics.mcmaster.c E-mail: israel@strw.leidenuniv.n

    2010-05-01

    We present the results of large-area {sup 12}CO J = 3-2 emission mapping of three nearby field galaxies, NGC 628, NGC 3521, and NGC 3627, completed at the James Clerk Maxwell Telescope as part of the Nearby Galaxies Legacy Survey. These galaxies all have moderate to strong {sup 12}CO J = 3-2 detections over large areas of the fields observed by the survey, showing resolved structure and dynamics in their warm/dense molecular gas disks. All three galaxies were part of the Spitzer Infrared Nearby Galaxies Survey sample, and as such have excellent published multiwavelength ancillary data. These data sets allow us to examine the star formation properties, gas content, and dynamics of these galaxies on sub-kiloparsec scales. We find that the global gas depletion time for dense/warm molecular gas in these galaxies is consistent with other results for nearby spiral galaxies, indicating this may be independent of galaxy properties such as structures, gas compositions, and environments. Similar to the results from The H I Nearby Galaxy Survey, we do not see a correlation of the star formation efficiency with the gas surface density consistent with the Schmidt-Kennicutt law. Finally, we find that the star formation efficiency of the dense molecular gas traced by {sup 12}CO J = 3-2 is potentially flat or slightly declining as a function of molecular gas density, the {sup 12}CO J = 3-2/J = 1-0 ratio (in contrast to the correlation found in a previous study into the starburst galaxy M83), and the fraction of total gas in molecular form.

  10. OSTI, US Dept of Energy, Office of Scientific and Technical Informatio...

    Office of Scientific and Technical Information (OSTI)

    (http:www.scienceaccelerator.gov) resource (on page 16), and the plan listed OSTI's newest product, the DOE Green Energy portal (http:www.osti.govgreenenergy) (page 17). ...

  11. United Illuminating Co | Open Energy Information

    Open Energy Info (EERE)

    Website: www.uinet.comwpsportaluinet Outage Hotline: 800-722-5584 Green Button Access: Implemented Green Button Landing Page: www.uinet.com Green Button Reference Page:...

  12. JEA | Open Energy Information

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    Jacksonville, Florida Service Territory: Florida Website: www.jea.com Green Button Access: Implemented Green Button Landing Page: www.jea.com Green Button Reference Page:...

  13. Jordan

    National Nuclear Security Administration (NNSA)

    href"http:www.ctbto.orgfileadminuseruploadpdfIFE-14FinalcorrectedSinglePagesWEB.pdf">http:www.ctbto.orgfileadminuseruploadpdfIFE-14FinalcorrectedSinglePages...

  14. Pacific Gas & Electric Co | Open Energy Information

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    Green Button Access: Implemented Green Button Landing Page: www.pge.commyhomemyacco Green Button Reference Page: www.pge.commyhomemyacco References: EIA Form EIA-861 Final...

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    Green Button Access: Implemented Green Button Landing Page: www.txu.comenresidentia Green Button Reference Page: www.txu.comenresidentia References: EIA Form EIA-861 Final...

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    Green Button Access: Implemented Green Button Landing Page: www.pepco.comhomebillin Green Button Reference Page: www.pepcoholdings.comabo References: EIA Form EIA-861 Final...

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  1. Next Update: November 2016

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  3. Word Pro - A

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    Web Page: http:www.eia.govtotalenergydatamonthlyappendices. Source: U.S. Department ... Table B3. Other Physical Conversion Factors Web Page: http :www.eia.govtotalenergy...

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  5. Issue a New Department of Energy Acquisition Guide Chapter 6.5 Competition Advocate Responsibilities and Revise Pages in Chapters 6.1 and 7.1.

    Office of Energy Efficiency and Renewable Energy (EERE)

    Attached is a new chapter of the DOE Acquisition Guide entitled Competition Advocate Responsibilities. It provides a comprehensive overview of the topic. The new chapter necessitates page changes to Chapters 6.1 and 7.1.

  6. Microfluidic device having an immobilized pH gradient and PAGE gels for protein separation and analysis

    DOE Patents [OSTI]

    Sommer, Gregory J.; Hatch, Anson V.; Singh, Anup K.; Wang, Ying-Chih

    2012-12-11

    Disclosed is a novel microfluidic device enabling on-chip implementation of a two-dimensional separation methodology. Previously disclosed microscale immobilized pH gradients (IPG) are combined with perpendicular polyacrylamide gel electrophoresis (PAGE) microchannels to achieve orthogonal separations of biological samples. Device modifications enable inclusion of sodium dodecyl sulfate (SDS) in the second dimension. The device can be fabricated to use either continuous IPG gels, or the microscale isoelectric fractionation membranes we have also previously disclosed, for the first dimension. The invention represents the first all-gel two-dimensional separation microdevice, with significantly higher resolution power over existing devices.

  7. Microfluidic device having an immobilized pH gradient and page gels for protein separation and analysis

    DOE Patents [OSTI]

    Sommer, Gregory J; Hatch, Anson V; Singh, Anup K; Wang, Ying-Chih

    2014-05-20

    Disclosed is a novel microfluidic device enabling on-chip implementation of a two-dimensional separation methodology. Previously disclosed microscale immobilized pH gradients (IPG) are combined with perpendicular polyacrylamide gel electrophoresis (PAGE) microchannels to achieve orthogonal separations of biological samples. Device modifications enable inclusion of sodium dodecyl sulfate (SDS) in the second dimension. The device can be fabricated to use either continuous IPG gels, or the microscale isoelectric fractionation membranes we have also previously disclosed, for the first dimension. The invention represents the first all-gel two-dimensional separation microdevice, with significantly higher resolution power over existing devices.

  8. Notice of Intent to Develop a Page Change to DOE O 443.1B, Protection of Human Research Subjects

    Broader source: Directives, Delegations, and Requirements [Office of Management (MA)]

    2015-07-16

    The purpose of the page change is to harmonize the definitions in this Order with those in the Federal regulations for the protection of human subjects (10 CFR Part 745). Specifically, splitting the definition "human subject research" into "research" and "human subject," and adopting, verbatim, the definitions of "research" and "human subject" from 10 CFR Part 745. We also propose adding to this section the definition of "generalizable," since the determination of whether a project is "research" in 10 CFR Part 745 hinges on whether the work being conducted is generalizable. Additionally, we propose making several small corrections and updates to the references, links, and organization titles.

  9. Nearby Supernova Factory Observations of SN 2005gj: Another TypeIa Supernova in a Massive Circumstellar Envelope

    SciTech Connect (OSTI)

    Aldering, G.; Antilogus, P.; Bailey, S.; Baltay, C.; Bauer, A.; Blanc, N.; Bongard, S.; Copin, Y.; Gangler, E.; Gilles, S.; Kessler, R.; Kocevski, D.; Lee, B.C.; Loken, S.; Nugent, P.; Pain, R.; Pecontal, E.; Pereira, R.; Perlmutter, S.; Rabinowitz, D.; Rigaudier, G.; Scalzo, R.; Smadja, G.; Thomas, R.C.; Wang, L.; Weaver, B.A.; Rabinowitz, D.; Bauer, A.

    2006-06-01

    We report the independent discovery and follow-up observations of supernova 2005gj by the Nearby Supernova Factory. This is the second confirmed case of a ''hybrid'' Type Ia/IIn supernova, which like the prototype SN 2002ic, we interpret as the explosion of a white dwarf interacting with a circumstellar medium. Our early-phase photometry of SN 2005gj shows that the strength of the interaction between the supernova ejecta and circumstellar material is much stronger than for SN 2002ic. Our .rst spectrum shows a hot continuum with broad and narrow H{alpha} emission. Later spectra, spanning over 4 months from outburst, show clear Type Ia features combined with broad and narrow H{gamma}, H{beta},H{alpha} and He I {lambda}{lambda}5876,7065 in emission. At higher resolution, P Cygni profiles are apparent. Surprisingly, we also observe an inverted P Cygni profile for [O III] {lambda}5007. We find that the lightcurve and measured velocity of the unshocked circumstellar material imply mass loss as recently as 8 years ago. This is in contrast to SN 2002ic, for which an inner cavity in the circumstellar material was inferred. Within the context of the thin-shell approximation, the early lightcurve is well-described by a flat radial density profile for the circumstellar material. However, our decomposition of the spectra into Type Ia and shock emission components allows for little obscuration of the supernova, suggesting an aspherical or clumpy distribution for the circumstellar material. We suggest that the emission line velocity profiles arise from electron scattering rather than the kinematics of the shock. This is supported by the inferred high densities, and the lack of evidence for evolution in the line widths. Ground- and space-based photometry, and Keck spectroscopy, of the host galaxy are used to ascertain that the host galaxy has low metallicity (Z/Z{sub {circle_dot}} < 0.3; 95% confidence) and that this galaxy is undergoing a significant star formation event that

  10. A WIDELY SEPARATED, HIGHLY OCCLUDED COMPANION TO THE NEARBY LOW-MASS T TAURI STAR TWA 30

    SciTech Connect (OSTI)

    Looper, Dagny L.; Pitts, Mark A.; Bochanski, John J.; Burgasser, Adam J.; Mohanty, Subhanjoy; Mamajek, Eric E.; Faherty, Jacqueline K.; West, Andrew A.

    2010-11-15

    We report the discovery of TWA 30B, a wide ({approx}3400 AU), co-moving M dwarf companion to the nearby ({approx}42 pc) young star TWA 30. Companionship is confirmed from their statistically consistent proper motions and radial velocities (RVs), as well as a chance alignment probability of only 0.08%. Like TWA 30A, the spectrum of TWA 30B shows signatures of an actively accreting disk (H I and alkali line emission) and forbidden emission lines tracing outflowing material ([O I], [O II], [O III], [S II], and [N II]). We have also detected [C I] emission in the optical data, marking the first such detection of this line in a pre-main-sequence star. Negligible RV shifts in the emission lines relative to the stellar frame of rest ({Delta}V {approx}< 30 km s{sup -1}) indicate that the outflows are viewed in the plane of the sky and that the corresponding circumstellar disk is viewed edge-on. Indeed, TWA 30B appears to be heavily obscured by its disk, given that it is 5 mag fainter than TWA 30A at K band despite having a slightly earlier spectral type (M4 versus M5). The near-infrared spectrum of TWA 30B also evinces an excess that varies on day timescales, with colors that follow classical T Tauri tracks as opposed to variable reddening (as is the case for TWA 30A). Multi-epoch data show this excess to be well modeled by a black body component with temperatures ranging from 630 to 880 K and emitting areas that scale inversely with the temperature. The variable excess may arise from disk structure such as a rim or a warp at the inner disk edge located at a radial distance of {approx}3-5 R{sub sun}. As the second and third closest actively accreting and outflowing stars to the Sun (after TWA 3), TWA 30AB presents an ideal system for a detailed study of star and planetary formation processes at the low-mass end of the hydrogen-burning spectrum.

  11. A SURVEY OF THE HIGH ORDER MULTIPLICITY OF NEARBY SOLAR-TYPE BINARY STARS WITH Robo-AO

    SciTech Connect (OSTI)

    Riddle, Reed L.; Bui, Khanh; Dekany, Richard G.; Kulkarni, Shrinivas; Tendulkar, Shriharsh P.; Tokovinin, Andrei; Mason, Brian D.; Hartkopf, William I.; Roberts, Lewis C. Jr.; Baranec, Christoph; Law, Nicholas M.; Burse, Mahesh P.; Das, H. K.; Punnadi, Sujit; Ramaprakash, A. N.

    2015-01-20

    We conducted a survey of nearby binary systems composed of main sequence stars of spectral types F and G in order to improve our understanding of the hierarchical nature of multiple star systems. Using Robo-AO, the first robotic adaptive optics instrument, we collected high angular resolution images with deep and well-defined detection limits in the Sloan Digital Sky Survey i' band. A total of 695 components belonging to 595 systems were observed. We prioritized observations of faint secondary components with separations over 10'' to quantify the still poorly constrained frequency of their subsystems. Of the 214 secondaries observed, 39 contain such subsystems; 19 of those were discovered with Robo-AO. The selection-corrected frequency of secondary subsystems with periods from 10{sup 3.5} to 10{sup 5}days is 0.12 0.03, the same as the frequency of such companions to the primary. Half of the secondary pairs belong to quadruple systems where the primary is also a close pair, showing that the presence of subsystems in both components of the outer binary is correlated. The relatively large abundance of 2+2 quadruple systems is a new finding, and will require more exploration of the formation mechanism of multiple star systems. We also targeted close binaries with periods less than 100 yr, searching for their distant tertiary components, and discovered 17 certain and 2 potential new triples. In a subsample of 241 close binaries, 71 have additional outer companions. The overall frequency of tertiary components is not enhanced, compared to all (non-binary) targets, but in the range of outer periods from 10{sup 6} to 10{sup 7.5}days (separations on the order of 500 AU), the frequency of tertiary components is 0.16 0.03, exceeding the frequency of similar systems among all targets (0.09) by almost a factor of two. Measurements of binary stars with Robo-AO allowed us to compute first orbits for 9 pairs and to improve orbits of another 11 pairs.

  12. TORUS AND ACTIVE GALACTIC NUCLEUS PROPERTIES OF NEARBY SEYFERT GALAXIES: RESULTS FROM FITTING INFRARED SPECTRAL ENERGY DISTRIBUTIONS AND SPECTROSCOPY

    SciTech Connect (OSTI)

    Alonso-Herrero, Almudena; Ramos Almeida, Cristina; Mason, Rachel; Asensio Ramos, Andres; Rodriguez Espinosa, Jose Miguel; Perez-Garcia, Ana M.; Roche, Patrick F.; Levenson, Nancy A.; Elitzur, Moshe; Packham, Christopher; Young, Stuart; Diaz-Santos, Tanio

    2011-08-01

    We used the CLUMPY torus models and a Bayesian approach to fit the infrared spectral energy distributions and ground-based high angular resolution mid-infrared spectroscopy of 13 nearby Seyfert galaxies. This allowed us to put tight constraints on torus model parameters such as the viewing angle i, the radial thickness of the torus Y, the angular size of the cloud distribution {sigma}{sub torus}, and the average number of clouds along radial equatorial rays N{sub 0}. We found that the viewing angle i is not the only parameter controlling the classification of a galaxy into type 1 or type 2. In principle, type 2s could be viewed at any viewing angle i as long as there is one cloud along the line of sight. A more relevant quantity for clumpy media is the probability for an active galactic nucleus (AGN) photon to escape unabsorbed. In our sample, type 1s have relatively high escape probabilities, P{sub esc} {approx} 12%-44%, while type 2s, as expected, tend to have very low escape probabilities. Our fits also confirmed that the tori of Seyfert galaxies are compact with torus model radii in the range 1-6 pc. The scaling of the models to the data also provided the AGN bolometric luminosities L{sub bol}(AGN), which were found to be in good agreement with estimates from the literature. When we combined our sample of Seyfert galaxies with a sample of PG quasars from the literature to span a range of L{sub bol}(AGN) {approx} 10{sup 43}-10{sup 47} erg s{sup -1}, we found plausible evidence of the receding torus. That is, there is a tendency for the torus geometrical covering factor to be lower (f{sub 2} {approx} 0.1-0.3) at high AGN luminosities than at low AGN luminosities (f{sub 2} {approx} 0.9-1 at {approx}10{sup 43}-10{sup 44} erg s{sup -1}). This is because at low AGN luminosities the tori appear to have wider angular sizes (larger {sigma}{sub torus}) and more clouds along radial equatorial rays. We cannot, however, rule out the possibility that this is due to

  13. Microsoft Word - EM Roadmap Rev 0 Dec 17 2010.docx

    Office of Environmental Management (EM)

    ... http:www.ig.energy.gov Other Relevant Sites The Whitehouse http:www.whitehouse.gov USA.gov http:www.usa.govindex.shtml Back cover Page ...

  14. Southwestern Electric Power Co | Open Energy Information

    Open Energy Info (EERE)

    Website: www.swepco.com Twitter: @SWEPCoNews Outage Map: www.swepco.comoutagesoutageM Green Button Access: Planned Green Button Reference Page: www.aep.comnewsroomnews...

  15. Notice of Intent to Develop a Page Change for DOE O 420.1C, Facility Safety

    Broader source: Directives, Delegations, and Requirements [Office of Management (MA)]

    2013-06-21

    The Page Change will be strictly limited in scope to changes necessary to accomplish the following objectives: (1) to invoke revised DOE-STD- 1104-20xx, Review and Approval of Nuclear Facility Safety Basis and Safety Design Basis Document, as a required method; (2) to invoke revised DOE-STD-3009-20xx, Preparation of Nonreactor Nuclear Facility Documented Safety Analysis, as a required method for new nuclear facilities as discussed below; and (3) to make miscellaneous administrative corrections and clarifications based on the one-year implementation review required by DOE O 251.1C, Departmental Directives Program. This JM is an update to one approved June 21, 2013.

  16. http://www.ornl.gov/Procurement.PDF

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    8/93 1. All Grade 5 and Grade 8 fasteners of foreign origin which do not bear any manufacturer's headmarks: Grade 5 Grade 8 2. Grade 5 fasteners with the following manufacturers' headmarks: J Jinn Her (TW) KS Kosaka Kogyo (JP) J KS 3. Grade 8 fasteners with the following manufacturers' headmarks: A Asahi Mfg (JP) KS Kosaka Kogyo (JP) A KS NF RT NF Nippon Fasteners (JP) RT Takai Ltd (JP) H Hinomoto Metal (JP) FM Fastener Co (of JP) H FM J M MS KY M Minamida Sieybo (JP) KY Kyoei (JP) MS Minato

  17. www.energy.gov/management/department

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    management/department -energy-asset-management-plan asset management principles asset management policy asset management principles * Support DOE's missions and strategic goals. * Provide for safe, secure, and healthy workplaces. * Use public and commercial benchmarks and best practices. * Employ lifecycle cost-benefit analysis in decision making. * Promote full and appropriate utilization. * Dispose or repurpose unneeded assets. * Provide appropriate levels of investment. * Record inventory and

  18. www.sandia.gov/research/robotics

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    sandia.gov/research/robotics Sandia National Laboratories has designed a self-guided .50 caliber projectile that utilizes a laser designated target and is configured to be fired from a small caliber, smooth bore gun barrel. Self-guided projectiles increase the probability of hit on targets at long range. System Design The self-guided projectile utilizes a laser designator and is fired from a small caliber smooth bore gun barrel. The nose of the bullet is equipped with an optical sensor along

  19. http://www.bea.gov/regional/rims/

    National Nuclear Security Administration (NNSA)

    to estimate the economic impacts of a wide range of projects, such as building a new sports facility or expanding an airport; of natural disasters, such as Hurricane Katrina; or...

  20. Recent Articles on www.anl.gov

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    even" property"content:encoded">

    Microwave heat improves nanostructured molybdenum disulfide catalyst's ability to produce hydrogen.

    Mon, 26 Oct 2015...

  1. http://www.cemp.dri.edu/cemp/

    National Nuclear Security Administration (NNSA)

    It is the intent of the CEMP to provide to the public accurate, near real-time monitoring data through this web site. However, it should be noted that these data are provisional ...

  2. http://www.springvalleyhospital.com/Home

    National Nuclear Security Administration (NNSA)

    Note: The information on this Web site is provided as general health guidelines and may ... for the content or any errors or omissions in the information provided by this Web site. ...

  3. https://www.centennialhillshospital.com/Home

    National Nuclear Security Administration (NNSA)

    ...Home Note: The information on this Web site is provided as general health ... for the content or any errors or omissions in the information provided by this Web site. ...

  4. Search for associated Higgs boson production WH ---> WWW* ---> l+- nu l-prime+- nu-prime + X in p anti-p collisions at s**(1/2) = 1.96-TeV

    SciTech Connect (OSTI)

    Abazov, V.M.; Abbott, B.; Abolins, M.; Acharya, B.S.; Adams, M.; Adams, T.; Agelou, M.; Agram, J.-L.; Ahn, S.H.; Ahsan, M.; Alexeev, G.D.; /Buenos Aires U. /Rio de Janeiro, CBPF /Rio de Janeiro State U. /Sao Paulo, IFT /Alberta U. /Simon Fraser U. /York U., Canada /McGill U. /Beijing, Inst. High Energy Phys. /Hefei, CUST /Andes U., Bogota

    2006-07-01

    The authors present a search for associated Higgs boson production in the process p{bar p} {yields} WH {yields} WWW* {yields} {ell}{sup {+-}}{nu} {ell}{prime}{sup {+-}} {nu}{prime} + X in final states containing two like-sign isolated electrons or muons (e{sup {+-}}e{sup {+-}}, e{sup {+-}} {mu}{sup {+-}}, or {mu}{sup {+-}} {mu}{sup {+-}}). The search is based on D0 Run II data samples corresponding to integrated luminosities of 360-380 pb{sup -1}. No excess is observed over the predicted standard model background. They set 95% C.L. upper limits on {sigma}(p{bar p} {yields} WH) x Br(H {yields} WW*) between 3.2 and 2.8 pb for Higgs masses from 115 to 175 GeV.

  5. CARMA SURVEY TOWARD INFRARED-BRIGHT NEARBY GALAXIES (STING). III. THE DEPENDENCE OF ATOMIC AND MOLECULAR GAS SURFACE DENSITIES ON GALAXY PROPERTIES

    SciTech Connect (OSTI)

    Wong, Tony; Xue, Rui; Bolatto, Alberto D.; Fisher, David B.; Vogel, Stuart N.; Leroy, Adam K.; Blitz, Leo; Rosolowsky, Erik; Bigiel, Frank; Ott, Jrgen; Rahman, Nurur; Walter, Fabian

    2013-11-01

    We investigate the correlation between CO and H I emission in 18 nearby galaxies from the CARMA Survey Toward IR-Bright Nearby Galaxies (STING) at sub-kpc and kpc scales. Our sample, spanning a wide range in stellar mass and metallicity, reveals evidence for a metallicity dependence of the H I column density measured in regions exhibiting CO emission. Such a dependence is predicted by the equilibrium model of McKee and Krumholz, which balances H{sub 2} formation and dissociation. The observed H I column density is often smaller than predicted by the model, an effect we attribute to unresolved clumping, although values close to the model prediction are also seen. We do not observe H I column densities much larger than predicted, as might be expected were there a diffuse H I component that did not contribute to H{sub 2} shielding. We also find that the H{sub 2} column density inferred from CO correlates strongly with the stellar surface density, suggesting that the local supply of molecular gas is tightly regulated by the stellar disk.

  6. Request to Make a Page Change to DOE O 329.2, Excepted Service Authority for Exceptionally Well Qualified (EWQ) EQ Pay Plan Employees

    Broader source: Directives, Delegations, and Requirements [Office of Management (MA)]

    2015-05-21

    The purpose of the page change is to allow more efficient and effective management of the EWQ authority. The revisions will delegate authorities for certain personnel actions that previously required approval from the Executive Resources Board (ERB) and/or Senior Management Review Board (SMRB) directly to the Head of the Departmental Element.

  7. Non-Destructive Evaluation of Slot-Die-Coated Lithium Secondary Battery Electrodes by In-Line Laser Caliper and IR Thermography Methods-Journal Cover Page

    SciTech Connect (OSTI)

    Mohanty, Debasish; Li, Jianlin; Born, Rachael; Maxey, L Curt; Dinwiddie, Ralph Barton; Daniel, Claus; Wood III, David L

    2014-01-01

    Note: This is a cover page for the 'Analytical Methods' journal, which was requested by the journal editor for consideration. The article has already been published and the PTS publication ID is 44000. The acknowledgements are same as mentioned in the PTS publication ID 44000.

  8. New Page 1

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    the Idaho National LaboratoryCentral Characterization Project Remote-Handled Waste Visual Examination Process, Audit A-10-03, dated November 24, 2009 Transmittal of the...

  10. Blue Title Page

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    commercial viability is the test Natural Gas Q - What is your view on the short and long term average price of natural gas? 4 Q - Regarding price volatility and possible supply ...

  11. Full page fax print

    National Nuclear Security Administration (NNSA)

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  13. Subsurface Knowledge Reference Page

    Broader source: Energy.gov [DOE]

    The below listing provides additional references related to Subsurface & Groundwater Remediation.  The references are categorized by documents types (e.g., Strategic Plans, Groundwater Plume...

  14. Yennello Group Home Page

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    Cyclotron Chemistry Dept. Physics Dept. College of Science Texas A&M University The Group Activities Publications Articles Talks and Posters Detectors Links Pictures Women in Nuclear Science Internal Documents Contacts run photos people photos equipment photos Copyright © 2009 Texas A&M University Cyclotron Institute MS #3366 College Station TX 77843-3366 Phone: 979-845-1411 Fax: 979-845-1899

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    This is a Request for Information (RFI) only. DOE will not pay for information provided under this RFI and no project will be supported as a result of this RFI. This RFI is not accepting applications for financial assistance or financial incentives. DOE may or may not issue a Funding Opportunity Announcement (FOA) based on consideration of the input received from this RFI. REQUEST FOR INFORMATION DE-FOA-0001346 Office of Technology Transitions U.S. Department of Energy ISSUE DATE: May 6, 2015

  17. Technical Workshop Intro Page

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    President Obama issued a Presidential Memorandum on January 9 directing the administration to conduct a Quadrennial Energy Review (QER), which is an interagency task force co-chaired by the...

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    ... nid00029. (core affinity 3) This example runs all PEs on NUMA node 1: % aprun -n 8 -sl 1 .xthi | sort Application 225119 resources: utime 0s, stime 0s Hello from rank 0, ...

  1. David Gates home page

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    Friedman About Us David Friedman - Assistant Secretary for Energy Efficiency and Renewable Energy (Acting) Photo of David Friedman. As Acting Assistant Secretary for the Office of Energy Efficiency and Renewable Energy (EERE), David Friedman leads the organization to transition the nation to a clean energy economy. He oversees six major technology and strategic areas, including Energy Efficiency, Renewable Power, Sustainable Transportation, Strategic Programs, Financial Management, and Business

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    6 WIPP Stakeholder Information Documents Closure of Underground Hazardous Waste Disposal Unit Submittal of Final Audit Reports Audit Report A-07-16 for INL/CCP RH Waste Characterization Activities dated November 22, 2006 Transmittal of the Certification Audit Report for SRS A-07-01 dated November 21, 2006 Annual Proposed Acceptable Knowledge Sufficiency Determination List Annual Report Submittals Submittal of Acceptable Knowledge Sufficiency Determination Notice of Submittal of a Dispute

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    2007 WIPP Stakeholder Information Documents Closure of Underground Hazardous Waste Disposal Unit Submittal of Final Audit Reports Transmittal of the Certification Audit Report A-07-14 of the AMWTP dated September 27, 2007 Transmittal of the Certification Audit Report A-07-03 of the ANL-CCP dated September 18, 2007 Final Audit Report A-07-24 of the SRS-CCP Battelle Columbus RH Waste dated September 6, 2007 Transmittal of the Certification Audit Report for the Hanford Site, Audit A-07-10 dated

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    8 WIPP Stakeholder Information Documents Closure of Underground Hazardous Waste Disposal Unit Submittal of Final Audit Reports Transmittal of the Certification Audit Report for the Advanced Mixed Waste Treatment Program, A-08-19 dated November 25, 2008 Transmittal of the Certification Audit Report for the Hanford TRU Program dated October 15, 2008 Transmittal of the Certification Audit Report for the Argonne National Laboratory-Central Characterization Project, Audit A-08-24 dated September 17,

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    10 WIPP Stakeholder Information Documents Closure of Underground Hazardous Waste Disposal Unit Submittal of Final Audit Reports Transmittal of the Recertification Audit Report for the Advanced Mixed Waste Treatment Project, Audit A-10-24, dated December 14, 2010 Transmittal of Carlsbad Field Office Final Audit Report A-10-23, Argonne National Laboratory Central Characterization Project for Remote Handled Waste Characterization dated October 14, 2010 Transmittal of Recertification Audit Report

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    2 WIPP Stakeholder Information Documents Closure of Underground Hazardous Waste Disposal Unit Submittal of Final Audit Reports Final Audit Report for the Argonne National Laboratory Central Characterization Project Recertification Audit A-12-16 dated December 19, 2012 Transmittal of the Final Audit Report for Recertification Audit A-12-14, INL Analytical Laboratories Utilizing the Central Characterization Project dated December 12, 2012 Transmittal of the Final Audit Report for Los Alamos

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    3 WIPP Stakeholder Information Documents Closure of Underground Hazardous Waste Disposal Unit Notification of Panel 6 Closure and Final Waste Emplacement dated November 5, 2013 Submittal of Final Audit Reports Transmittal of the Final Audit Report for Recertification Audit A-14-01 of the Advanced Mixed Waste Treatment Project dated December 9, 2013 Final Audit Report for the Argonne National Laboratory Central Characterization Program Recertification Audit A-13-24 dated November 22, 2013

  10. WIPP Stakeholder Information Page

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    List Annual Report Submittals Transmittal of Waste Isolation Pilot Plant Annual Geotechnical Analysis Report dated October 30, 2015 Submittal of Acceptable Knowledge...

  11. Full page photo

    Office of Environmental Management (EM)

    Full Text Glossary Full Text Glossary The full-text glossary includes terms used throughout the website and in Biomass Program publications. Terms are listed alphabetically for easy reference. The term index lists all of the terms defined in the glossary. A | B | C | D | E | F | G | H | I | J | K | L | M | N | O | P | Q | R | S | T | U | V | W | X | Y | Z A acid: A solution that has an excess of hydrogen ions (H+), with a pH of less than 7. acetic acid: An acid with the structure of C2H4O2.

  12. PAGE Cover: Top Photo

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

    ... negative performance trends, and share lessons learned. ... petroleumincreasing alternative fuel use. * Code of Federal ... of public access vehicle bridges; and 49 CFR Part ...

  13. Trident Web page

    SciTech Connect (OSTI)

    Johnson, Randall P.; Fernandez, Juan C.

    2012-06-25

    An Extensive Diagnostic Suite Enables Cutting-edge Research at Trident The Trident Laser Facility at Los Alamos National Laboratory is an extremely versatile Nd:glass laser system dedicated to high energy density physics research and fundamental laser-matter interactions. Trident's Unique Laser Capabilities Provide an Ideal Platform for Many Experiments. The laser system consists of three high energy beams which can be delivered into two independent target experimental areas. The target areas are equipped with an extensive suite of diagnostics for research in ultra-intense laser matter interactions, dynamic material properties, and laser-plasma instabilities. Several important discoveries and first observations have been made at Trident including laser-accelerated MeV mono-energetic ions, nonlinear kinetic plasma waves, transition between kinetic and fluid nonlinear behavior, as well as other fundamental laser-matter interaction processes. Trident's unique long-pulse capabilities have enabled state-of-the-art innovations in laser-launched flyer-plates, and other unique loading techniques for material dynamics research.

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    ... 11 ) Maintain adequate emergency tank space per the Tank ... to handle unanticipated problems that could require additional tank space. 6,0 plannIng Bases 6.1 Reference Date ...

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    ... 11 ) Maintain adequate emergency tank space per the Tank ... to handle unanticipated problems that could require additional tank space. 6,0 planning Bases 6,1 Reference Date ...

  16. FTA Main Page

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

    Argonne Researchers to Study Chicago Emergency Evacuation System PACE bus $2.9 million grant will lead to better emergency transportation planning and response for cities in U.S. ARGONNE, Ill - A group of Argonne researchers will be studying methods and creating tools for building more resilient mass transit systems to evacuate major cities under a $2.9 million grant announced today by the U.S. Department of Transportation's Federal Transit Administration. The project will bring together

  17. Native Intern Profile Page

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

    The intern will work with the executive management teams to solve other problems as they arise. Morgan Gray Tribal A liation: Chickasaw Nation University: Oklahoma State University ...

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

    The FAL provides Contracting Officers (COs) and grants personnel guidance regarding the use of A-I33 audits and the Federal Audit Clearinghouse (F AC). The purpose of the F AL is...

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    WIPP Stakeholder Information Index 2016 WIPP Stakeholder Information Documents 2015 WIPP Stakeholder Information Documents 2014 WIPP Stakeholder Information Documents 2013 WIPP Stakeholder Information Documents 2012 WIPP Stakeholder Information Documents 2011 WIPP Stakeholder Information Documents 2010 WIPP Stakeholder Information Documents 2009 WIPP Stakeholder Information Documents 2008 WIPP Stakeholder Information Documents 2007 WIPP Stakeholder Information Documents 2006 WIPP Stakeholder

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    any warranty, express or implied, including the warranties of merchantability and fitness for a particular purpose. Nor do they assume any legal liability or responsibility...

  1. PDSF Group Pages

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    Help Staff Blogs Request Repository Mailing List Need Help? Out-of-hours Status and Password help Call operations: 1-800-66-NERSC, option 1 or 510-486-6821 Account Support ...

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    Policies User Surveys NERSC Users Group Help Staff Blogs Request Repository Mailing List Need Help? Out-of-hours Status and Password help Call operations: 1-800-66-NERSC, option 1 ...

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    Form - 853 Kb - Allows an employee to enroll or waive health insurance coverage. SF-2817 - Life Insurance Election Form (Federal Employee Group Life Insurance) - 120 Kb - ...

  4. NewPage Corporation

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

    gas-to-liquids plant at Wisconsin Rapids Mill to replace natural gas use and produce ... Technology and Feedstocks: * 497 bone dry tons per day of woody biomass comprised of mill ...

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    PSAs Help You Save Energy and Money New PSAs Help You Save Energy and Money June 10, 2013 - 2:47pm Addthis Rebecca Matulka Rebecca Matulka Former Digital Communications Specialist, Office of Public Affairs Looking for energy-saving tips? Check out Energy Saver for great advice on saving energy and money at home. Watch the other Energy Saver PSAs from the Energy Department and Ad Council. Editor's Note (September 2014): The PSAs have been removed from this blog post because this campaign with Ad

  6. Page | Open Energy Information

    Open Energy Info (EERE)

    CU Document Property:NEPA CategoricalExclusion Property:NEPA Consultant Property:NEPA DNA Worksheet Property:NEPA Decision Property:NEPA Document Property:NEPA EA EIS Report...

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    STANDARD FORM 120-A. APRIL 1957 GEN. SERV. ADMIN, FPMR (41 CFR) 101-43.311 CONTINUATION ... ITEM NO. (a) DESCRIPTION (b) PER UNIT (f) TOTAL (g) STANDARD FORM 120A APRIL 1957 EDITION

  8. 21 briefing pages total

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    not necessarily mean entitlement to a payment p. 9 Key Definitions Reservist-a member ... reservist differential Law bars payment of differential for civilian paid hours ...

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    safety Management (ISM). Metrics and targets to assess performance, including benchmarking of key functional areas with other DOE contractors, industry and research...

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    XRAYOPS -- APS Experiment Hall X-ray Operations Problem List About XRAYOPS English (USA) This is a moderated list to facilitate communications about APS x-ray operations to...

  12. 2page.indd

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

    Figure 1. Uranium concentrate production in the United States, 1996 - 2nd quarter 2016 pounds U 3 O 8 0 500,000 1,000,000 1,500,000 2,000,000 2,500,000 3,000,000 3,500,000 4,000,000 4,500,000 5,000,000 5,500,000 6,000,000 6,500,000 1996 1997 1998 1999 2000 2001 2002 2003 2004 2005 2006 2007 2008 2009 2010 2011 2012 2013 2014 2015 P2016 1st quarter 2nd quarter 3rd quarter 4th quarter P = Preliminary data. Source: U.S. Energy Information Administration: Form EIA-851A and Form EIA-851Q,

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    4 Department of Energy Carlsbad Field Office Environmental Assessment for the Actinide Chemistry and Repository Science Laboratory U.S. Department of Energy Final June 2002 Final Environmental Assessment for Actinide Chemistry and Repository Science Laboratory TABLE OF CONTENTS CHAPTER 1: INTRODUCTION AND STATEMENT OF PURPOSE AND NEED ......................1-1 1.1 PURPOSE AND NEED FOR AGENCY ACTION ........................................................1-1 1.2 BACKGROUND

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    )lIJfjlHfllmj)mmllillruJt ((I(m(ti.JmlmmmlllWI ll .. . I*mw lffi )( HI I) SOVELEV RECELEV 40 40 Immlll1 illllmJil11)Immm lfm lli m l.lmillm(mj...

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    users prepare successful proposals. The information will be made available on the LCLS-AMO web site after the meeting. Please see the workshop announcement for more information. ...

  18. THE LICK-CARNEGIE EXOPLANET SURVEY: A 3.1 M{sub +} PLANET IN THE HABITABLE ZONE OF THE NEARBY M3V STAR GLIESE 581

    SciTech Connect (OSTI)

    Vogt, Steven S.; Rivera, E. J.; Haghighipour, N.; Henry, Gregory W.; Williamson, Michael H.

    2010-11-01

    We present 11 years of HIRES precision radial velocities (RVs) of the nearby M3V star Gliese 581, combining our data set of 122 precision RVs with an existing published 4.3-year set of 119 HARPS precision RVs. The velocity set now indicates six companions in Keplerian motion around this star. Differential photometry indicates a likely stellar rotation period of {approx}94 days and reveals no significant periodic variability at any of the Keplerian periods, supporting planetary orbital motion as the cause of all the RV variations. The combined data set strongly confirms the 5.37-day, 12.9-day, 3.15-day, and 67-day planets previously announced by Bonfils et al., Udry et al., and Mayor et al.. The observations also indicate a fifth planet in the system, GJ 581f, a minimum-mass 7.0 M{sub +} planet orbiting in a 0.758 AU orbit of period 433 days, and a sixth planet, GJ 581g, a minimum-mass 3.1 M{sub +} planet orbiting at 0.146 AU with a period of 36.6 days. The estimated equilibrium temperature of GJ 581g is 228 K, placing it squarely in the middle of the habitable zone of the star and offering a very compelling case for a potentially habitable planet around a very nearby star. That a system harboring a potentially habitable planet has been found this nearby, and this soon in the relatively early history of precision RV surveys, indicates that {eta}{sub +}, the fraction of stars with potentially habitable planets, is likely to be substantial. This detection, coupled with statistics of the incompleteness of present-day precision RV surveys for volume-limited samples of stars in the immediate solar neighborhood, suggests that {eta}{sub +} could well be on the order of a few tens of percent. If the local stellar neighborhood is a representative sample of the galaxy as a whole, our Milky Way could be teeming with potentially habitable planets.

  19. BANYAN. V. A SYSTEMATIC ALL-SKY SURVEY FOR NEW VERY LATE-TYPE LOW-MASS STARS AND BROWN DWARFS IN NEARBY YOUNG MOVING GROUPS

    SciTech Connect (OSTI)

    Gagn, Jonathan; Lafrenire, David; Doyon, Ren; Malo, Lison; Artigau, tienne

    2015-01-10

    We present the BANYAN All-Sky Survey (BASS) catalog, consisting of 228 new late-type (M4-L6) candidate members of nearby young moving groups (YMGs) with an expected false-positive rate of ?13%. This sample includes 79 new candidate young brown dwarfs and 22 planetary-mass objects. These candidates were identified through the first systematic all-sky survey for late-type low-mass stars and brown dwarfs in YMGs. We cross-matched the Two Micron All Sky Survey and AllWISE catalogs outside of the galactic plane to build a sample of 98,970 potential ?M5 dwarfs in the solar neighborhood and calculated their proper motions with typical precisions of 5-15 mas yr{sup 1}. We selected highly probable candidate members of several YMGs from this sample using the Bayesian Analysis for Nearby Young AssociatioNsII tool (BANYANII). We used the most probable statistical distances inferred from BANYANII to estimate the spectral type and mass of these candidate YMG members. We used this unique sample to show tentative signs of mass segregation in the AB Doradus moving group and the Tucana-Horologium and Columba associations. The BASS sample has already been successful in identifying several new young brown dwarfs in earlier publications, and will be of great interest in studying the initial mass function of YMGs and for the search of exoplanets by direct imaging; the input sample of potential close-by ?M5 dwarfs will be useful to study the kinematics of low-mass stars and brown dwarfs and search for new proper motion pairs.

  20. AN INFRARED CENSUS OF DUST IN NEARBY GALAXIES WITH SPITZER (DUSTiNGS). II. DISCOVERY OF METAL-POOR DUSTY AGB STARS

    SciTech Connect (OSTI)

    Boyer, Martha L.; Sonneborn, George; McQuinn, Kristen B. W.; Gehrz, Robert D.; Skillman, Evan; Barmby, Pauline; Bonanos, Alceste Z.; Gordon, Karl D.; Meixner, Margaret; Groenewegen, M. A. T.; Lagadec, Eric; Lennon, Daniel; Marengo, Massimo; McDonald, Iain; Zijlstra, Albert; Sloan, G. C.; Van Loon, Jacco Th.

    2015-02-10

    The DUSTiNGS survey (DUST in Nearby Galaxies with Spitzer) is a 3.6 and 4.5 μm imaging survey of 50 nearby dwarf galaxies designed to identify dust-producing asymptotic giant branch (AGB) stars and massive stars. Using two epochs, spaced approximately six months apart, we identify a total of 526 dusty variable AGB stars (sometimes called ''extreme'' or x-AGB stars; [3.6]-[4.5] > 0.1 mag). Of these, 111 are in galaxies with [Fe/H] < –1.5 and 12 are in galaxies with [Fe/H] < –2.0, making them the most metal-poor dust-producing AGB stars known. We compare these identifications to those in the literature and find that most are newly discovered large-amplitude variables, with the exception of ≈30 stars in NGC 185 and NGC 147, 1 star in IC 1613, and 1 star in Phoenix. The chemical abundances of the x-AGB variables are unknown, but the low metallicities suggest that they are more likely to be carbon-rich than oxygen-rich and comparisons with existing optical and near-IR photometry confirm that 70 of the x-AGB variables are confirmed or likely carbon stars. We see an increase in the pulsation amplitude with increased dust production, supporting previous studies suggesting that dust production and pulsation are linked. We find no strong evidence linking dust production with metallicity, indicating that dust can form in very metal-poor environments.

  1. Computers and small satellites: How FORTE is utilizing the WWW as a {open_quotes}paperless{close_quotes} information resource and the development of a unique resource management planning tool

    SciTech Connect (OSTI)

    Roussel-Dupre, D.; Carter, M.; Franz, R.

    1997-10-01

    The Fast-On-orbit Recording of Transient Events (FORTE) satellite is the second satellite to be developed and flown by Los Alamos National Laboratory and is scheduled to be launched August, 1997 by a Pegasus XL rocket. FORTE follows in the footsteps of the ALEXIS satellite in utilizing a very small operations crew for mission operations. Partially based upon the ALEXIS automation and World Wide Web (WWW) usage for data dissemination, FORTE began at an early stage of ground processing to use the web as a repository of information about all aspects of the satellite. Detailed descriptions of the various satellite and experiment components, cable diagrams, integration photographs as well as extensive test data have all been compiled into a single site as a means of archiving the data at a single location. In this manner, it is readily available during times of ground testing, ground station operation training as well as anomaly resolution. Small satellites usually require extensive effort to optimize operation under minimal resources. For the FORTE satellite, a unique planning tool has been developed over the past 2 years which balances the various resources of the satellite (power, memory, downlink, on board command buffer, etc.) to provide the maximum data acquisition. This paper will concentrate on a description of both the extensive web interface and the planning tool. 6 refs.

  2. Nuclear Regulatory Commission issuances: Opinions and decisions of the Nuclear Regulatory Commission with selected orders, July 1--December 31, 1996. Volume 44, Pages 1--432

    SciTech Connect (OSTI)

    1997-10-01

    The hardbound edition of the Nuclear Regulatory Commission Issuances is a final compilation of the monthly issuances. It includes all of the legal precedents for the agency within a six-month period. Any opinions, decisions, denials, memoranda and orders of the Commission inadvertently omitted from the monthly softbounds and any corrections submitted by the NRC legal staff to the printed softbound issuances are contained in the hardbound edition. Cross references in the text and indexes are to the NRCI page numbers which are the same as the page numbers in this publication. Issuances are referred to as follows: Commission--CLI, Atomic Safety and Licensing Boards--LBP, Administrative Law Judges--ALJ, Directors` Decisions--DD, and Decisions on Petitions for Rulemaking--DPRM.

  3. RAP Committee: Draft Advice re: Hanford LTS Program, v.1 Suyama, Engstrom, Vanni, Mattson, Serres, Cimon, Leckband Page 1 of 2

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

    Hanford LTS Program, v.1 Suyama, Engstrom, Vanni, Mattson, Serres, Cimon, Leckband Page 1 of 2 Draft Advice re: Hanford Long-Term Stewardship Program Background The purpose of this advice is to present Hanford Advisory Board (Board) recommendations to the U.S. Department of Energy - Richland Operations Office (DOE-RL) for consideration concerning the current 100-F Area and other planned site transitions to the Long-term Stewardship (LTS) Program. The Board's perception of the LTS Program's

  4. VERY LONG BASELINE ARRAY IMAGING OF PARSEC-SCALE RADIO EMISSIONS IN NEARBY RADIO-QUIET NARROW-LINE SEYFERT 1 GALAXIES

    SciTech Connect (OSTI)

    Doi, Akihiro; Asada, Keiichi; Inoue, Makoto; Fujisawa, Kenta; Nagai, Hiroshi; Hagiwara, Yoshiaki; Wajima, Kiyoaki

    2013-03-01

    We conducted Very Long Baseline Array (VLBA) observations of seven nearby narrow-line Seyfert 1 (NLS1) galaxies at 1.7 GHz ({lambda}18 cm) with milliarcsecond resolution. This is the first systematic very long baseline interferometry study focusing on the central parsec-scale regions of radio-quiet NLS1s. Five of the seven were detected at a brightness temperature of {approx}> 5 Multiplication-Sign 10{sup 6} K and contain radio cores with high brightness temperatures of >6 Multiplication-Sign 10{sup 7} K, indicating a nonthermal process driven by jet-producing central engines as in radio-loud NLS1s and other active galactic nucleus classes. VLBA images of MRK 1239, MRK 705, and MRK 766 exhibit parsec-scale jets with clear linear structures. A large portion of the radio power comes from diffuse emission components that are distributed within the nuclear regions ({approx}< 300 pc), which is a common characteristic throughout the observed NLS1s. Jet kinetic powers limited by the Eddington limit may be insufficient to allow the jets to escape to kiloparsec scales for these radio-quiet NLS1s with low-mass black holes of {approx}< 10{sup 7} M {sub Sun }.

  5. Star formation properties in barred galaxies. III. Statistical study of bar-driven secular evolution using a sample of nearby barred spirals

    SciTech Connect (OSTI)

    Zhou, Zhi-Min; Wu, Hong; Cao, Chen E-mail: hwu@bao.ac.cn

    2015-01-01

    Stellar bars are important internal drivers of secular evolution in disk galaxies. Using a sample of nearby spiral galaxies with weak and strong bars, we explore the relationships between the star formation feature and stellar bars in galaxies. We find that galaxies with weak bars tend coincide with low concentrical star formation activity, while those with strong bars show a large scatter in the distribution of star formation activity. We find enhanced star formation activity in bulges toward stronger bars, although not predominantly, consistent with previous studies. Our results suggest that different stages of the secular process and many other factors may contribute to the complexity of the secular evolution. In addition, barred galaxies with intense star formation in bars tend to have active star formation in their bulges and disks, and bulges have higher star formation densities than bars and disks, indicating the evolutionary effects of bars. We then derived a possible criterion to quantify the different stages of the bar-driven physical process, while future work is needed because of the uncertainties.

  6. Addendum for the Phase II Groundwater Flow Model of Corrective Action Unit 98: Frenchman Flat, NevadaTest Site, Nye County, Nevada, Revision 0 (page changes)

    SciTech Connect (OSTI)

    John McCord

    2007-05-01

    This document, which makes changes to Phase II Groundwater Flow Model of Corrective Action Unit 98: Frenchman Flat, Nevada Test Site, Nye County, Nevada, S-N/99205--074, Revision 0 (May 2006) was prepared to address review comments on this final document provided by the Nevada Division of Environmental Protection (NDEP) in a letter dated June 20, 2006. The document includes revised pages that address NDEP review comments and comments from other document users. Change bars are included on these pages to identify where the text was revised. In addition to the revised pages, the following clarifications are made: Section 6.0 Conceptual Model Uncertainty Analyses. Please note that in this section figures showing the observed versus simulated well head (Figures 6-1, 6-5, 6-7, 6-16, 6-28, 6-30, 6-32, 6-34, 6-37, 6-42, 6-47, 6-52, 6-57, 6-62, 6-71, and 6-86) have a vertical break in scale on the y axis. Section 7.0 Parameter Sensitivity Analysis. In Section 7.2, the parameter perturbation analysis defines two components of the objective function PHI. These two components include the WELL component that represents the head portion of the objective function as measured in wells and the FLUX component that represents the lateral boundary flux portion of the objective function. In the text and figures in Section 7.2, the phrases well portion of the objective function and head portion of the objective function are used interchangeably in discussions of the WELL component of the objective function.

  7. ON THE CARBON-TO-OXYGEN RATIO MEASUREMENT IN NEARBY SUN-LIKE STARS: IMPLICATIONS FOR PLANET FORMATION AND THE DETERMINATION OF STELLAR ABUNDANCES

    SciTech Connect (OSTI)

    Fortney, Jonathan J.

    2012-03-10

    Recent high-resolution spectroscopic analysis of nearby FGK stars suggests that a high C/O ratio of greater than 0.8, or even 1.0, is relatively common. Two published catalogs find C/O > 0.8 in 25%-30% of systems, and C/O > 1.0 in {approx}6%-10%. It has been suggested that in protoplanetary disks with C/O > 0.8 that the condensation pathways to refractory solids will differ from what occurred in our solar system, where C/O = 0.55. The carbon-rich disks are calculated to make carbon-dominated rocky planets, rather than oxygen-dominated ones. Here we suggest that the derived stellar C/O ratios are overestimated. One constraint on the frequency of high C/O is the relative paucity of carbon dwarf stars (10{sup -3}-10{sup -5}) found in large samples of low-mass stars. We suggest reasons for this overestimation, including a high C/O ratio for the solar atmosphere model used for differential abundance analysis, the treatment of a Ni blend that affects the O abundance, and limitations of one-dimensional LTE stellar atmosphere models. Furthermore, from the estimated errors on the measured stellar C/O ratios, we find that the significance of the high C/O tail is weakened, with a true measured fraction of C/O > 0.8 in 10%-15% of stars, and C/O > 1.0 in 1%-5%, although these are still likely overestimates. We suggest that infrared T-dwarf spectra could show how common high C/O is in the stellar neighborhood, as the chemistry and spectra of such objects would differ compared to those with solar-like abundances. While possible at C/O > 0.8, we expect that carbon-dominated rocky planets are rarer than others have suggested.

  8. CHARACTERIZATION OF THE NEARBY L/T BINARY BROWN DWARF WISE J104915.57-531906.1 AT 2 pc FROM THE SUN

    SciTech Connect (OSTI)

    Kniazev, A. Y.; Vaisanen, P.; Potter, S. B.; Crawford, S.; Gulbis, A. A. S.; Muzic, K.; Mehner, A.; Boffin, H. M. J.; Melo, C.; Ivanov, V. D.; Girard, J.; Mawet, D.; Schmidtobreick, L.; Kurtev, R.; Borissova, J.; Huelamo, N.; Minniti, D.; Ishibashi, K.; Beletsky, Y.; Buckley, D. A. H.; and others

    2013-06-20

    WISE J104915.57-531906.1 is a L/T brown dwarf binary located 2 pc from the Sun. The pair contains the closest known brown dwarfs and is the third closest known system, stellar or sub-stellar. We report comprehensive follow-up observations of this newly uncovered system. We have determined the spectral types of both components (L8 {+-} 1, for the primary, agreeing with the discovery paper; T1.5 {+-} 2 for the secondary, which was lacking spectroscopic type determination in the discovery paper) and, for the first time, their radial velocities (V{sub rad} {approx} 23.1, 19.5 km s{sup -1}) using optical spectra obtained at the Southern African Large Telescope and other facilities located at the South African Astronomical Observatory (SAAO). The relative radial velocity of the two components is smaller than the range of orbital velocities for theoretically predicted masses, implying that they form a gravitationally bound system. We report resolved near-infrared JHK{sub S} photometry from the Infrared Survey Facility telescope at the SAAO which yields colors consistent with the spectroscopically derived spectral types. The available kinematic and photometric information excludes the possibility that the object belongs to any of the known nearby young moving groups or associations. Simultaneous optical polarimetry observations taken at the SAAO 1.9 m give a non-detection with an upper limit of 0.07%. For the given spectral types and absolute magnitudes, 1 Gyr theoretical models predict masses of 0.04-0.05 M{sub Sun} for the primary, and 0.03-0.05 M{sub Sun} for the secondary.

  9. INTEGRAL FIELD SPECTROSCOPY AND MULTI-WAVELENGTH IMAGING OF THE NEARBY SPIRAL GALAXY NGC 5668 : AN UNUSUAL FLATTENING IN METALLICITY GRADIENT

    SciTech Connect (OSTI)

    Marino, R. A.; Gil de Paz, A.; Castillo-Morales, A.; Perez-Gonzalez, P. G.; Gallego, J.; Zamorano, J.; Sanchez, S. F.

    2012-07-20

    We present an analysis of the full bidimensional optical spectral cube of the nearby spiral galaxy NGC 5668, observed with the Pmas fiber PAcK Integral Field Unit (IFU) at the Calar Alto observatory 3.5 m telescope. We make use of broadband imaging to provide further constraints on the evolutionary history of the galaxy. This data set will allow us to improve our understanding of the mechanisms that drive the evolution of disks. We investigated the properties of 62 H II regions and concentric rings in NGC 5668 and derived maps in ionized-gas attenuation and chemical (oxygen) abundances. We find that while inward of r {approx}36'' {approx} 4.4 kpc {approx} 0.36 (D{sub 25}/2) the derived O/H ratio follows the radial gradient typical of spiral galaxies, the abundance gradient beyond r {approx} 36'' flattens out. The analysis of the multi-wavelength surface brightness profiles of NGC 5668 is performed by fitting these profiles with those predicted by chemo-spectrophotometric evolutionary models of galaxy disks. From this, we infer a spin and circular velocity of {lambda} = 0.053 and v{sub c} = 167 km s{sup -1}, respectively. The metallicity gradient and rotation curve predicted by this best-fitting galaxy model nicely match the values derived from the IFU observations, especially within r {approx}36''. The same is true for the colors despite some small offsets and a reddening in the bluest colors beyond that radius. On the other hand, deviations of some of these properties in the outer disk indicate that a secondary mechanism, possibly gas transfer induced by the presence of a young bar, must have played a role in shaping the recent chemical and star formation histories of NGC 5668.

  10. A PLANETARY SYSTEM AROUND THE NEARBY M DWARF GJ 667C WITH AT LEAST ONE SUPER-EARTH IN ITS HABITABLE ZONE

    SciTech Connect (OSTI)

    Anglada-Escude, Guillem; Butler, R. Paul; Arriagada, Pamela; Minniti, Dante; Vogt, Steven S.; Rivera, Eugenio J.; Haghighipour, Nader; Carter, Brad D.; Tinney, C. G.; Wittenmyer, Robert A.; Bailey, Jeremy A.; O'Toole, Simon J.; Jones, Hugh R. A.; Jenkins, James S.

    2012-05-20

    We re-analyze 4 years of HARPS spectra of the nearby M1.5 dwarf GJ 667C available through the European Southern Observatory public archive. The new radial velocity (RV) measurements were obtained using a new data analysis technique that derives the Doppler measurement and other instrumental effects using a least-squares approach. Combining these new 143 measurements with 41 additional RVs from the Magellan/Planet Finder Spectrograph and Keck/High Resolution Echelle Spectrometer spectrometers reveals three additional signals beyond the previously reported 7.2 day candidate, with periods of 28 days, 75 days, and a secular trend consistent with the presence of a gas giant (period {approx}10 years). The 28 day signal implies a planet candidate with a minimum mass of 4.5 M{sub Circled-Plus} orbiting well within the canonical definition of the star's liquid water habitable zone (HZ), that is, the region around the star at which an Earth-like planet could sustain liquid water on its surface. Still, the ultimate water supporting capability of this candidate depends on properties that are unknown such as its albedo, atmospheric composition, and interior dynamics. The 75 day signal is less certain, being significantly affected by aliasing interactions among a potential 91 day signal, and the likely rotation period of the star at 105 days detected in two activity indices. GJ 667C is the common proper motion companion to the GJ 667AB binary, which is metal-poor compared to the Sun. The presence of a super-Earth in the HZ of a metal-poor M dwarf in a triple star system supports the evidence that such worlds should be ubiquitous in the Galaxy.

  11. Investigating nearby star-forming galaxies in the ultraviolet with HST/COS spectroscopy. I. Spectral analysis and interstellar abundance determinations

    SciTech Connect (OSTI)

    James, B. L.; Aloisi, A.; Sohn, S. T.; Wolfe, M. A.; Heckman, T.

    2014-11-10

    This is the first in a series of three papers describing a project with the Cosmic Origins Spectrograph on the Hubble Space Telescope to measure abundances of the neutral interstellar medium (ISM) in a sample of nine nearby star-forming galaxies. The goal is to assess the (in)homogeneities of the multiphase ISM in galaxies where the bulk of metals can be hidden in the neutral phase, yet the metallicity is inferred from the ionized gas in the H II regions. The sample, spanning a wide range in physical properties, is to date the best suited to investigate the metallicity behavior of the neutral gas at redshift z = 0. ISM absorption lines were detected against the far-ultraviolet spectra of the brightest star-forming region(s) within each galaxy. Here we report on the observations, data reduction, and analysis of these spectra. Column densities were measured by a multicomponent line-profile fitting technique, and neutral-gas abundances were obtained for a wide range of elements. Several caveats were considered, including line saturation, ionization corrections, and dust depletion. Ionization effects were quantified with ad hoc CLOUDY models reproducing the complex photoionization structure of the ionized and neutral gas surrounding the UV-bright sources. An 'average spectrum of a redshift z = 0 star-forming galaxy' was obtained from the average column densities of unsaturated profiles of neutral-gas species. This template can be used as a powerful tool for studies of the neutral ISM at both low and high redshift.

  12. Erosional remnants and adjacent unconformities along an eolian-marine boundary of the Page Sandstone and Carmel Formation, Middle Jurassic, south-central Utah

    SciTech Connect (OSTI)

    Jones, L.S.; Blakey, R.C. (Univ. of Northern Arizona, Flagstaff, AZ (United States). Dept. of Geology)

    1993-09-01

    Sandstone ridges along the marine-eolian boundary of the Middle Jurassic Page Sandstone (eolian) with the lower Carmel Formation (restricted marine) in south-central Utah have been identified as erosional remnants consisting of strata of siliciclastic sabkha and eolian origin. The ridges lie within two distinct units of the Thousand Pockets Tongue of the Page. Two equally plausible models explain the genesis of these ridges. One model involves (1) early cementation of eolian and sabkha strata, (2) wind erosion leading to development of yardangs and unconformities, (3) yardang tilting due to evaporite dissolution, and (4) renewed deposition and burial. The alternative model explains ridge development through (1) subsidence, with tilting, of eolian and sabkha strata into evaporites due to loading from linear dunes, (2) evaporite dissolution and unconformity development, and (3) renewed deposition and burial. These models provide important clues about the nature of a missing part of the rock record. Reconstruction of units that were deposited but later eroded improves paleogeographic interpretation and here indicates that the Carmel paleo-shoreline was considerably farther to the northwest than previously believed.

  13. San Diego Gas & Electric Co | Open Energy Information

    Open Energy Info (EERE)

    San Diego, California Service Territory: California Website: www.sdge.com Green Button Access: Implemented Green Button Landing Page: www.sdge.comcustomer-ser Green Button...

  14. NSTAR Electric Company | Open Energy Information

    Open Energy Info (EERE)

    Service Territory: Massachusetts Website: www.nstar.comresidential Green Button Access: Implemented Green Button Landing Page: www.nstar.comresidential Green Button...

  15. Energy Northwest | Open Energy Information

    Open Energy Info (EERE)

    Northwest Jump to: navigation, search Name: Energy Northwest Place: Washington Website: www.energy-northwest.comPages Twitter: @EnergyNorthwest Facebook: https:www.facebook.com...

  16. Reliant Energy Retail Services LLC | Open Energy Information

    Open Energy Info (EERE)

    Facebook: https:www.facebook.comreliantenergy Outage Hotline: 1-866-222-7100 Green Button Access: Implemented Green Button Landing Page: www.reliant.comWelcome.d...

  17. Reliant Energy Power Supply LLC | Open Energy Information

    Open Energy Info (EERE)

    Supply LLC Place: Texas Service Territory: Texas Website: www.reliant.comWelcome.do Green Button Access: Implemented Green Button Landing Page: www.reliant.comWelcome.d...

  18. NSTAR Electric Company | Open Energy Information

    Open Energy Info (EERE)

    Massachusetts Service Territory: Massachusetts Website: www.nstar.comresidential Green Button Access: Implemented Green Button Landing Page: www.nstar.comresidential...

  19. PacifiCorp (Oregon) | Open Energy Information

    Open Energy Info (EERE)

    https:www.facebook.compagesPacificorp121474841237049 Outage Hotline: 1-877-508-5088 Green Button Access: Implemented Green Button Reference Page: www.pacificpower.netabou...

  20. Austin Energy | Open Energy Information

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    Territory: Texas Website: www.austinenergy.com Outage Map: my.austinenergy.comoutages Green Button Access: Implemented Green Button Landing Page: www.austinenergy.com...

  1. Potomac Electric Power Co | Open Energy Information

    Open Energy Info (EERE)

    Columbia Service Territory: District of Columbia, Maryland Website: www.pepco.comhome Green Button Access: Implemented Green Button Landing Page: www.pepco.comhomebillin...

  2. Portland General Electric Co | Open Energy Information

    Open Energy Info (EERE)

    Landing Page: www.portlandgeneral.comd Green Button Reference Page: energy.govarticlesgreen References: EIA Form EIA-861 Final Data File for 2010 - File1a1 Energy...

  3. User:Nlangle/CategoryLists | Open Energy Information

    Open Energy Info (EERE)

    Organizations, Trade Groups |ReferencesOrganization's "Contact" Pagecite web|urlhttp:www.renewsindia.comcontact.php|titleRE News India: "Contact" Page...

  4. [pic] EERE Web Site Statistics - Solar Decathlon

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

    ... |1.|Department of Energy Solar Decathlon Home Page http: www. solardecathl on. org |43,756|61,116| |2.|EERE: Department of Energy Solar Decathlon Home Page http: ...

  5. OSTIblog Articles in the osti mission Topic | OSTI, US Dept of...

    Office of Scientific and Technical Information (OSTI)

    ...) resource (on page 16), and the plan listed OSTI's newest product, the DOE Green Energy portal (http:www.osti.govgreenenergy) (page 17). The DOE plan also accounted ...

  6. OSTIblog Articles in the r&d findings Topic | OSTI, US Dept of...

    Office of Scientific and Technical Information (OSTI)

    ...) resource (on page 16), and the plan listed OSTI's newest product, the DOE Green Energy portal (http:www.osti.govgreenenergy) (page 17). The DOE plan also accounted ...

  7. OSTIblog Articles in the Open government Topic | OSTI, US Dept...

    Office of Scientific and Technical Information (OSTI)

    ...) resource (on page 16), and the plan listed OSTI's newest product, the DOE Green Energy portal (http:www.osti.govgreenenergy) (page 17). The DOE plan also accounted ...

  8. Word Pro - S11

    Annual Energy Outlook [U.S. Energy Information Administration (EIA)]

    Web Page: http:www.eia.govtotalenergydatamonthlyinternational. Sources: Tables ... Note: OPEC is the Organization of the Petroleum Exporting C ountries. Web Page: http:...

  9. FINDING η CAR ANALOGS IN NEARBY GALAXIES USING Spitzer. II. IDENTIFICATION OF AN EMERGING CLASS OF EXTRAGALACTIC SELF-OBSCURED STARS

    SciTech Connect (OSTI)

    Khan, Rubab; Kochanek, C. S.; Stanek, K. Z.; Gerke, Jill

    2015-02-01

    Understanding the late-stage evolution of the most massive stars such as η Carinae is challenging because no true analogs of η Car have been clearly identified in the Milky Way or other galaxies. In Khan et al., we utilized Spitzer IRAC images of 7 nearby (≲ 4 Mpc) galaxies to search for such analogs, and found 34 candidates with flat or red mid-IR spectral energy distributions. Here, in Paper II, we present our characterization of these candidates using multi-wavelength data from the optical through the far-IR. Our search detected no true analogs of η Car, which implies an eruption rate that is a fraction 0.01 ≲ F ≲ 0.19 of the core-collapse supernova (ccSN) rate. This is roughly consistent with each M {sub ZAMS} ≳ 70 M {sub ☉} star undergoing one or two outbursts in its lifetime. However, we do identify a significant population of 18 lower luminosity (log (L/L {sub ☉}) ≅ 5.5-6.0) dusty stars. Stars enter this phase at a rate that is a fraction 0.09 ≲ F ≲ 0.55 of the ccSN rate, and this is consistent with all 25 < M {sub ZAMS} < 60 M {sub ☉} stars undergoing an obscured phase at most lasting a few thousand years once or twice. These phases constitute a negligible fraction of post-main-sequence lifetimes of massive stars, which implies that these events are likely to be associated with special periods in the evolution of the stars. The mass of the obscuring material is of order ∼M {sub ☉}, and we simply do not find enough heavily obscured stars for theses phases to represent more than a modest fraction (∼10% not ∼50%) of the total mass lost by these stars. In the long term, the sources that we identified will be prime candidates for detailed physical analysis with the James Webb Space Telescope.

  10. Public Service Co of NH | Open Energy Information

    Open Energy Info (EERE)

    800-662-7764 Outage Map: www.eversource.comContentgen Green Button Access: Implemented Green Button Landing Page: www.psnh.comSaveEnergyMo Green Button Reference Page:...

  11. ,"Maine Natural Gas Summary"

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

    ,"Excel File Name:","ngsumlsumdcusmem.xls" ,"Available from Web Page:","http:www.eia.govdnavngngsumlsumdcusmem.htm" ,"Source:","Energy Information ...

  12. Workbook Contents

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

    mbblpdm.xls" ,"Available from Web Page:","http:www.eia.govdnavpetpetcrdcrpdnadcmbblpdm.htm" ,"Source:","Energy Information Administration" ,"For Help, ...

  13. ,"Kentucky Natural Gas Consumption by End Use"

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

    ,"Excel File Name:","ngconssumdcuskym.xls" ,"Available from Web Page:","http:www.eia.govdnavngngconssumdcuskym.htm" ,"Source:","Energy Information ...

  14. Workbook Contents

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

    mbblm.xls" ,"Available from Web Page:","http:www.eia.govdnavpetpetconspsupdcnusmbblm.htm" ,"Source:","Energy Information Administration" ,"For Help,...

  15. Workbook Contents

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

    mbblpdm.xls" ,"Available from Web Page:","http:www.eia.govdnavpetpetconspsupdcnusmbblpdm.htm" ,"Source:","Energy Information Administration" ,"For Help,...

  16. Workbook Contents

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

    File Name:","petpnpinptdcnusmbblm.xls" ,"Available from Web Page:","http:www.eia.govdnavpetpetpnpinptdcnusmbblm.htm" ,"Source:","Energy Information ...

  17. Workbook Contents

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

    ,"Excel File Name:","petpripropaepllpaptadpgalm.xls" ,"Available from Web Page:","http:www.eia.govdnavpetpetpripropaepllpaptadpgalm.htm" ,"Source:","Energy ...

  18. Workbook Contents

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

    ,"Excel File Name:","petpriallmgdnusptadpgalm.xls" ,"Available from Web Page:","http:www.eia.govdnavpetpetpriallmgdnusptadpgalm.htm" ,"Source:","Energy ...

  19. ,"Pennsylvania Heat Content of Natural Gas Consumed"

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

    ,"Excel File Name:","ngconsheatdcuspam.xls" ,"Available from Web Page:","http:www.eia.govdnavngngconsheatdcuspam.htm" ,"Source:","Energy Information ...

  20. ,"Pennsylvania Underground Natural Gas Storage - All Operators...

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

    ,"Excel File Name:","ngstorsumdcuspam.xls" ,"Available from Web Page:","http:www.eia.govdnavngngstorsumdcuspam.htm" ,"Source:","Energy Information ...