Sample records for nearby www pages

  1. Rob Rutten's web pages June 19, 2014 1 Rob Rutten's WWW Pages --June 19, 2014

    E-Print Network [OSTI]

    Rutten, Rob

    Rob Rutten's web pages ­ June 19, 2014 1 Rob Rutten's WWW Pages -- June 19, 2014 http://www.staff.science.uu.nl/~rutte

  2. Tuesday, February 18, 2003 http://www.pppl.gov/ncsx/pvr/pvr.HTML Page: 1 NCSX Home Page

    E-Print Network [OSTI]

    pvr Tuesday, February 18, 2003 http://www.pppl.gov/ncsx/pvr/pvr.HTML Page: 1 NCSX Home Page PVR Chapter 5 - Ideal MHD Stability Chapter 6 - Resistive Stability Chapter 7 - Plasma Heating Chapter 8 VMEC (Steve Hirshman) Power and Particle Control in NCSX (Peter Mioduszewski) NCSX Heating: Neutral

  3. DOT WEB PAGES (plain text) 1 DOT WWW Pages --Plain Text Copy June 15, 2014

    E-Print Network [OSTI]

    Rutten, Rob

    ://www.staff.science.uu.nl/ rutte101/dot Plain version: no images, photographs or figures Contents 1 DOT news 1 2 DOT at a glance 2. The DOT website is now at http://www.staff.science.uu.nl/~rutte101/dot. The DOT database is now at ftp

  4. Page 1 of 6 The Castle 2012 www.queensu.ca/bisc

    E-Print Network [OSTI]

    Ellis, Randy

    energy production to run the Castle · Innovative sustainability courses and natural science field studiesPage 1 of 6 The Castle 2012 www.queensu.ca/bisc Sustainability in Action Our 15th century castle and its 550-acre grounds provide a unique setting and opportunity for sustainability found nowhere else

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

    National Nuclear Security Administration (NNSA)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742EnergyOn AprilAElectronic Input Options Gary L. Hirsch SNLMaythemeansIHome *Pending greenhouse

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

    National Nuclear Security Administration (NNSA)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742EnergyOn AprilAElectronic Input Options Gary L. Hirsch SNLMaythemeansIHome *Pending greenhouseEM

  7. NIID, Trinity College Dublin www.tcd.ie/niid Ph: 01 896 3885 Page 1 of 14 Certificate in Contemporary Living (CCL)

    E-Print Network [OSTI]

    O'Mahony, Donal E.

    NIID, Trinity College Dublin www.tcd.ie/niid Ph: 01 896 3885 Page 1 of 14 Certificate for support if needed. #12;NIID, Trinity College Dublin www.tcd.ie/niid Ph: 01 896 3885 Page 2 of 14 1 Address: Phone: Mobile: Email Address: #12;NIID, Trinity College Dublin www.tcd.ie/niid Ph: 01 896 3885

  8. www.publiclandsday.org Public Lands Program

    E-Print Network [OSTI]

    US Army Corps of Engineers

    awareness of local public lands and issues #12;www.publiclandsday.org Facebook.com - Fan Page http://www.facebook.com/pages/create.php #12;www.publiclandsday.org Facebook Fan Page http://www.facebook.com/pages/create.php #12;www.publiclandsday.org Facebook Fan Page #12;www.publiclandsday.org Facebook Fan Page #12;www.publiclandsday.org Facebook Event

  9. 1/28/09 3:40 PMBloomberg Printer-Friendly Page Page 1 of 2http://www.bloomberg.com/apps/news?pid=20670001&refer=science&sid=atoTqDydLoWA

    E-Print Network [OSTI]

    1/28/09 3:40 PMBloomberg Printer-Friendly Page Page 1 of 2http://www.bloomberg.com/apps/news?pidhttp://www.bloomberg.com/apps/news?pid=20670001&refer=science&sid=atoTqDydLoWA list of genes that may

  10. 1/3/09 12:05 AMCode of Ethics --Association for Computing Machinery Page 1 of 7http://www.acm.org/about/code-of-ethics

    E-Print Network [OSTI]

    Wright, Dawn Jeannine

    1/3/09 12:05 AMCode of Ethics -- Association for Computing Machinery Page 1 of 7http://www.acm.org/about/code computing is not mentioned in the imperatives of Section 1, the Code is concerned with how these fundamental -- Association for Computing Machinery Page 2 of 7http://www.acm.org/about/code-of-ethics 5. Acknowledgments

  11. Page 1 of 2 http://www.chorumtech.com/site/ofcohe1.htm 7/5/2001

    E-Print Network [OSTI]

    Chiao, Jung-Chih

    Page 1 of 2 http://www.chorumtech.com/site/ofcohe1.htm 7/5/2001 Back to list of Press Releases FOR IMMEDIATE RELEASE CHORUM TECHNOLOGIES TO PRESENT DYNAMIC OPTICAL SIGNAL PROCESSING TECHNOLOGY AT 2001 Relations 214-665-1334 214-498-5285 (mobile) meiw@fleishman.com Trade Shows Copyright © 2001 Chorum

  12. Updated 11/17/2013 Page 1 of 7 http://www.karabasoglu.com/ Orkun Karabasoglu, PhD

    E-Print Network [OSTI]

    Karabasoglu, Orkun

    Updated 11/17/2013 Page 1 of 7 http://www.karabasoglu.com/ Orkun Karabasoglu, PhD Assistant__________________________________________________________ Assistant Professor in Electrical and Computer Engineering (2013-present) Director of the Laboratory (Mechanical Engineering) Committee Members: Prof. Chris Atkeson (Robotics Institute), Prof. Illah Nourbakhsh

  13. www.grad.ubc.ca/forms page 1 of 1 last updated: 2014-04-11 DOCTORAL DISSERTATION APPROVAL

    E-Print Network [OSTI]

    Pulfrey, David L.

    www.grad.ubc.ca/forms page 1 of 1 last updated: 2014-04-11 DOCTORAL DISSERTATION APPROVAL with other forms for final dissertation submission. Student: Student number: Given Name Family Name Name Date of Dissertation Defence: Date (yyyy/mm/dd) Dissertation Title: As research supervisor

  14. Data Sheet Fujitsu ESPRIMO P910 E90+ Desktop PC Page 1 / 8 www.fujitsu.com/fts/ESPRIMO

    E-Print Network [OSTI]

    Fiebig, Peter

    *with Intel® Turbo Boost Technology (clock speed and will vary depending on workload and other variables generation Intel® CoreTM processor family, a switched monitor outlet and a power supply with up to 92 silent operations #12;Data Sheet Fujitsu ESPRIMO P910 E90+ Desktop PC Page 2 / 8 www

  15. URL: http://www.elsevier.nl/locate/entcs/volume68.html 18 pages Timed CSP = Closed Timed Automata 1

    E-Print Network [OSTI]

    Ouaknine, Joël

    URL: http://www.elsevier.nl/locate/entcs/volume68.html 18 pages Timed CSP = Closed Timed Automata 1 70118, USA Abstract We study the expressive power of an augmented version of Timed CSP and show constraints. We also show that this new version of Timed CSP is expressive enough to capture the most widely

  16. 05/24/2006 09:14 AMU.S. Department of Energy Page 1 of 2http://www.energy.gov/print/3666.htm

    E-Print Network [OSTI]

    05/24/2006 09:14 AMU.S. Department of Energy Page 1 of 2http://www.energy.gov/print/3666.htm News of Energy's (DOE) Office of Science, joined counterparts from China, the European Union, India, Japan of 2http://www.energy.gov/print/3666.htm By initialing the ITER agreement, U.S. representatives

  17. 7/29/08 11:02 AMPrager to Lead PPPL Page 1 of 3http://www.pppl.gov/PRAGERnews08.html

    E-Print Network [OSTI]

    7/29/08 11:02 AMPrager to Lead PPPL Page 1 of 3http://www.pppl.gov/PRAGERnews08.html For Immediate ReleaseFor Immediate Release July 18, 2008July 18, 2008 Prager to Lead PPPL Plainsboro, New Jersey:02 AMPrager to Lead PPPL Page 2 of 3http://www.pppl.gov/PRAGERnews08.html of the laboratory, which is funded

  18. 11/21/2006 11:22 AMU.S. Department of Energy Page 1 of 2http://www.doe.gov/print/4486.htm

    E-Print Network [OSTI]

    11/21/2006 11:22 AMU.S. Department of Energy Page 1 of 2http://www.doe.gov/print/4486.htm News.S. Department of Energy (DOE), today joined counterparts from China, the European Union, India, Japan.S. Department of Energy Page 2 of 2http://www.doe.gov/print/4486.htm was one of the original participants

  19. Page 1 rRmhard son. S :TJ ' @mamma o WEEE@ P EBEE@ www ...

    E-Print Network [OSTI]

    rRmhard son. S :TJ. ' @mamma o WEEE@. P EBEE@ www@ R n ggg-35151@ s mmmnnunnnnnn s BREW e. MEN wwonoz3rsuxmmwoovv. “Dimi NUIT'.

  20. 3/14/09 10:47 AMIs that granite counter in your home emitting radon? Page 1 of 4http://www.startribune.com/41239912.html?page=4&c=y

    E-Print Network [OSTI]

    Llope, William J.

    3/14/09 10:47 AMIs that granite counter in your home emitting radon? Page 1 of 4http://www.startribune.com/41239912.html?page=4&c=y Advertisement Is that granite counter in your home emitting radon? Homeowners seeking just the right granite for their countertops have something new to ponder, besides which color

  1. Page 1Effects of Pervasive Computing on Sustainable Development 17/04/2008 09:17:43 PMhttp://www.patmedia.net/tbookman/techsoc/Koehler.htm

    E-Print Network [OSTI]

    Loke, Seng W. - Loke, Seng W.

    Page 1Effects of Pervasive Computing on Sustainable Development 17/04/2008 09:17:43 PMhttp://www.patmedia.net/tbookman/techsoc/Koehler.htm Effects of Pervasive Computing on Sustainable Development #12;Page 2Effects of Pervasive Computing on Sustainable Development 17/04/2008 09:17:43 PMhttp

  2. Page

    Energy Savers [EERE]

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directed offOCHCO2:Introduction toManagementOPAM5 Accretion-of-DutiesPROPERTY3-0127Paducah3 Theof Page 2 This

  3. 05/05/2014 11:01Nanotechnology's Revolutionary Next Phase Page 1 of 7http://www.forbes.com/sites/brucedorminey/2013/02/26/nanotechnologys-civilization-changing-revolutionary-next-phase/

    E-Print Network [OSTI]

    05/05/2014 11:01Nanotechnology's Revolutionary Next Phase Page 1 of 7http://www.forbes.com/sites/brucedorminey/2013/02/26/nanotechnologys-civilization-changing-revolutionary-next-phase/ TECH (/TECHNOLOGY) 5:01Nanotechnology's Revolutionary Next Phase Page 2 of 7http://www.forbes.com/sites/brucedorminey/2013

  4. Page 1 of 2 Visit us online: www.mcgill.ca/caps 2013-08

    E-Print Network [OSTI]

    Barthelat, Francois

    jobs: Public historian, federal jobs, historical consulting, teaching, grant writing, etc. Leaving. AHA Data on the Historical Profession http://www.historians.org/info/AHA_Data.cfm US-based. Reports Academic http://postacademic.org/ Job Search Websites Museums and Heritage­ Jobs Canadian Heritage

  5. Page

    Energy Savers [EERE]

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directed offOCHCO2:Introduction toManagementOPAM5 Accretion-of-DutiesPROPERTY3-0127Paducah3 The follo\\ing

  6. Page

    Energy Savers [EERE]

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directed offOCHCO2:Introduction toManagementOPAM5 Accretion-of-DutiesPROPERTY3-0127Paducah3 The follo\\ing2

  7. Page

    Energy Savers [EERE]

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directed offOCHCO2:Introduction toManagementOPAM5 Accretion-of-DutiesPROPERTY3-0127Paducah3 The

  8. Page

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742EnergyOn April 23, 2014, an OHA Administrative Judge issuedEnergy1of Page This final rule

  9. Page

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level:Energy: Grid Integration Redefining What's Possible for RenewableSpeedingBiomassPPPO Website DirectoryCommunityFuture Use PaducahPage of 1

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

    Office of Environmental Management (EM)

    north of Femme Osage Slough by naturally occurring chemical reduction process and absorption onto aquifer materials. Page 2 of 2 DOE EM Groundwater Record 992011 http:...

  11. pages)

    Office of Environmental Management (EM)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742 33 1112011 Strategic2UraniumEnergy City ofiManage Presentation iManageorigins.indd origins.indd

  12. pages)

    Office of Environmental Management (EM)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742 33 1112011 Strategic2UraniumEnergy City ofiManage Presentation iManageorigins.indd origins.indd

  13. HoustonChronicle.com Page 1 of 2 http://www.chron.com/cs/CDA/printstory.hts/prn/texas/880944 4/23/2001

    E-Print Network [OSTI]

    Chiao, Jung-Chih

    HoustonChronicle.com Page 1 of 2 http://www.chron.com/cs/CDA/printstory.hts/prn/texas/880944 4 in Richardson, Texas (c) 2001 Business Wire. News/Assignment Editors & High-Tech Writers REMINDER...for Tuesday (April 17) --(BUSINESS WIRE)-- WHAT: Chorum Technologies' presentation of findings on advanced, all

  14. 1/12/11 1:51 PMComputer-Aided Brains: Scientific American Page 1 of 3http://www.scientificamerican.com/article.cfm?id=computer-aided-brains

    E-Print Network [OSTI]

    Salvucci, Dario D.

    » Scientific American Mind » October 2005 Head Lines | Mind & Brain Computer-Aided Brains By Brad Stenger1/12/11 1:51 PMComputer-Aided Brains: Scientific American Page 1 of 3http://www.scientificamerican.com/article.cfm?id=computer-aided-brains Image: For years, innovators have tried to devise computerized gadgetry to aid the brain. Advances have

  15. Protected Area Planning Principles and Strategies Page 1 of 18 http://www.forestry.umt.edu/personnel/faculty/borrie/papers/ecotourism.htm 8/14/2001

    E-Print Network [OSTI]

    Brown, Gregory G.

    , and economic dimensions remind us that natural resource planning and management in general, and protected areaProtected Area Planning Principles and Strategies Page 1 of 18 http://www.forestry.umt.edu/personnel/faculty/borrie/papers/ecotourism.htm 8/14/2001 Protected Area Planning Principles and Strategies William T. Borrie, Stephen F. Mc

  16. Department of Earth Sciences www.rhul.ac.uk/earthsciences Page 1 of 1 Does black carbon and humic materials in snow and ice decay?

    E-Print Network [OSTI]

    Sheldon, Nathan D.

    the and optics properties of black carbon change. As little as 10 ng of Black carbon in 1 g of snow can cause 1 of two more effective than carbon dioxide in changing global air temperatures.2 The successful candidateDepartment of Earth Sciences www.rhul.ac.uk/earthsciences Page 1 of 1 Does black carbon and humic

  17. www.myresources.com.au OIL & GAS BULLETIN VOL. 15, NO. 11 PAGE 9 Safety first: Oil rigs off the north west shelf will be studied for

    E-Print Network [OSTI]

    www.myresources.com.au OIL & GAS BULLETIN VOL. 15, NO. 11 PAGE 9 NEWS Safety first: Oil rigs off that as times and trends change, tight gas and shale gas is being more and more considered as a potentially prices rise, and a shift from coal to gas energy sources is experienced, tight gas and shale gas is now

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

    Gasoline and Diesel Fuel Update (EIA)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742 33 111 1,613 122 40 Buildingto17 34 44Year199873.4 66.1 56.2 50.4415 6833 (Thousand ShortGlossary

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

    Office of Environmental Management (EM)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742 33 1112011 Strategic2UraniumEnergy City of

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

    Office of Environmental Management (EM)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742 33Frequently20,000 Russian Nuclearand Characterization of aShiprock Responsible DOE Office: Office

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

    Office of Environmental Management (EM)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742 33Frequently20,000 Russian Nuclearand Characterization of aShiprock Responsible DOE Office:

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

    Office of Environmental Management (EM)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742 33Frequently20,000 Russian Nuclearand Characterization of aShiprock Responsible DOE Office:Union

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

    Office of Environmental Management (EM)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742 33Frequently20,000 Russian Nuclearand Characterization of aShiprock Responsible DOE

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

    Office of Environmental Management (EM)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742 33Frequently20,000 Russian Nuclearand Characterization of aShiprock Responsible DOETuba City

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

    Office of Environmental Management (EM)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742 33Frequently20,000 Russian Nuclearand Characterization of aShiprock Responsible DOETuba CityEast

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

    Office of Environmental Management (EM)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742 33Frequently20,000 Russian Nuclearand Characterization of aShiprock Responsible DOETuba

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

    Office of Environmental Management (EM)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742 33Frequently20,000 Russian Nuclearand Characterization of aShiprock Responsible DOETubaVOC)

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

    Office of Environmental Management (EM)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742 33Frequently20,000 Russian Nuclearand Characterization of aShiprock Responsible DOETubaVOC)West

  9. Computer Science This page for your convenience. See http://www.und.nodak.edu/dept/registrar/

    E-Print Network [OSTI]

    Delene, David J.

    Computer Science This page for your convenience. See http, Mahalko, Marsh (Chair), O'Neil, Reza, Stokke and Wiggen The underlying goal of the Department of Computer approach to the study of computer science while providing students with experience on state

  10. 05/26/2006 12:25 PMVOA News -Seven Nation Group to Pursue Fusion Energy Research Page 1 of 2http://www.voanews.com/english/2006-05-24-voa63.cfm?renderforprint=1

    E-Print Network [OSTI]

    05/26/2006 12:25 PMVOA News - Seven Nation Group to Pursue Fusion Energy Research Page 1 of 2http after signing the ITER agreement Print Seven Nation Group to Pursue Fusion Energy Research By David Mc - Seven Nation Group to Pursue Fusion Energy Research Page 2 of 2http://www.voanews.com/english/2006

  11. CNN.com -Bush to fund fusion energy machine -Jan. 30, 2003 Thursday, January 30, 2003 http://www.cnn.com/2003/TECH/science/01/30/fusion.science/index.html Page: 1

    E-Print Network [OSTI]

    ://www.cnn.com/2003/TECH/science/01/30/fusion.science/index.html Page: 1 The Web CNN.com Home Page World U.S. Weather Reports SERVICES Video Newswatch E-Mail Services CNN To Go SEARCH Web CNN.com Bush to fund fusion energy

  12. Nuclear Activity in Nearby Galaxies

    E-Print Network [OSTI]

    Thaisa Storchi-Bergmann

    1999-03-03T23:59:59.000Z

    I discuss some recent observational results in the research of nearby active galactic nuclei (AGN). These results cover three main topics: (i) evidences for the current paradigm for AGN's, which include a nuclear supermassive blackhole (SMBH) fed via an accretion disk; (ii) evidence that this paradigm may also apply to LINER's, the lowest luminous AGN's and to normal galaxies; (iii) evidences of how the fueling of the SMBH occurs and its relation to recent and intermediate age (10^6 to 10^8 yrs old) episodes of star formation.

  13. 11/13/14, 6:38 PM"Crappy Gabor paper": Overly honest citation slips into peer-reviewed journal Ethology. Page 1 of 7http://www.slate.com/blogs/future_tense/2014/11/11/_crappy_gabor_paper_overly_honest_citation_slips_into_peer_reviewed_journal.html

    E-Print Network [OSTI]

    Tomforde, Mark

    Ethology. Page 1 of 7http://www.slate.com/blogs/future_tense/2014/11/11/_crappy_gabor_paper into peer-reviewed journal Ethology. Page 2 of 7http://www.slate.com/blogs/future_tense/2014/11/11/_crappy-author Lillian Fritz-Laylin explained in a Slate post last year, overly honest asides are more commonly found

  14. 4/30/08 12:19 PMWomen Exploring the Oceans Page 1 of 5http://www.womenoceanographers.org/Default.aspx?pid=E1E3254E-1C80-4e6d-ABBF-1EC5F5436C3E&id=DawnWright

    E-Print Network [OSTI]

    Wright, Dawn Jeannine

    4/30/08 12:19 PMWomen Exploring the Oceans Page 1 of 5http://www.womenoceanographers.org/Default.aspx?pid of her office. #12;4/30/08 12:19 PMWomen Exploring the Oceans Page 2 of 5http://www.womenoceanographers.org/Default.aspx?pid

  15. 3/11/13 9:17 AMResearcher says interest in zombies waxes, wanes to mirror societal dissatisfaction -The Washington Post Page 1 of 5http://www.washingtonpost.com/entertainment/tv/researcher-says-inte...faction/2013/03/11/8a5d0472-8a2e-11e2-a88e-461ffa2e34e

    E-Print Network [OSTI]

    Duchowski, Andrew T.

    - The Washington Post Page 1 of 5http://www.washingtonpost.com/entertainment/tv/researcher-says-inte...faction/2013 to mirror societal dissatisfaction - The Washington Post Page 2 of 5http://www.washingtonpost.com/entertainment/tv/researcher-says-inte...faction

  16. 12-04-21 8:40 AMJSTOR: Isis, Vol. 103, No. 1 (March 2012), pp. 83-87 Page 1 of 7http://www.jstor.org/stable/10.1086/664979

    E-Print Network [OSTI]

    Vicedo, Marga

    12-04-21 8:40 AMJSTOR: Isis, Vol. 103, No. 1 (March 2012), pp. 83-87 Page 1 of 7http://www.jstor.org/stable/10.1086/664979 Isis Subscribe or Renew Published by: on behalf ofThe University of Chicago Press Kuhn presented Figure 1 #12;12-04-21 8:40 AMJSTOR: Isis, Vol. 103, No. 1 (March 2012), pp. 83-87 Page 2

  17. Microwell Plate Luminometer -LB 96V MicrolumatPlus luminomet... http://www.berthold.com.au/bioanalytical_pages/LB96V.html 1 of 3 3/19/06 1:31 PM

    E-Print Network [OSTI]

    Raizada, Manish N.

    ://www.berthold.com.au/bioanalytical_pages/LB96V.html 1 of 3 3/19/06 1:31 PM | Home | Industrial Measurement | Radiation Protection | Life for all applications in luminescence measurement. For overload detection, the optical channel is shutterGlow software offers the possibility to control the instrument with a Windows based system. Robot access

  18. 28/05/2008 18:53Malaria parasites fine-tune offspring's gender: study | Health | Reuters Page 1 of 2http://www.reuters.com/article/healthNews/idUSL2887819620080528?sp=true

    E-Print Network [OSTI]

    Gardner, Andy

    28/05/2008 18:53Malaria parasites fine-tune offspring's gender: study | Health | Reuters Page 1 of 2http://www.reuters.com/article/healthNews/idUSL2887819620080528?sp=true ÂĄ $ - Learn. Practice 2007 Broker Center sponsored links You are here: Home > News > Health > Article Reuters Widgets Get

  19. 12/24/2006 02:23 PMLoading "Oil Addiction Weakens the U.S. -Issues 2007 -MSNBC.com" Page 1 of 2http://www.msnbc.msn.com/id/16299314/site/newsweek/print/1/displaymode/1098/

    E-Print Network [OSTI]

    Deutch, John

    12/24/2006 02:23 PMLoading "Oil Addiction Weakens the U.S. - Issues 2007 - MSNBC.com" Page 1 of 2http://www.msnbc.msn.com/id/16299314/site/newsweek/print/1/displaymode/1098/ MSNBC.com Oil Addiction decades, energy has become a central problem in foreign policy. The surge in oil prices--and in oil

  20. http://www.staradvertiser.com/newspremium/20130824_Small_school_stands_tall_as_science_powerhouse_.html?id=220927791&c=n Page 1 of 3 Aug 28, 2013 07:39:07PM MDT

    E-Print Network [OSTI]

    http://www.staradvertiser.com/newspremium/20130824_Small_school_stands_tall_as_science_powerhouse_.html?id=220927791&c=n Page 1 of 3 Aug 28, 2013 07:39:07PM MDT Small school stands tall as science powerhouse POSTED roughly 2,000 feet, then transmitted data to Earth as it aero-braked and fell at prescribed speeds before

  1. 28/05/2009 16:25Global links will breed more dangerous parasites -University of Oxford Page 1 of 2http://www.ox.ac.uk/media/news_stories/2009/090528_3.html

    E-Print Network [OSTI]

    West, Stuart

    28/05/2009 16:25Global links will breed more dangerous parasites - University of Oxford Page 1 of 2http://www.ox.ac.uk/media/news_stories/2009/090528_3.html Global links will breed more dangerous that as the world becomes more connected so natural selection will favour more dangerous parasites. The team, from

  2. 9/18/09 2:07 PMSPACE.com --'Big Wave' Theory Offers Alternative to Dark Energy Page 1 of 8http://www.space.com/scienceastronomy/090817-dark-energy-alternative.html

    E-Print Network [OSTI]

    Temple, Blake

    9/18/09 2:07 PMSPACE.com -- 'Big Wave' Theory Offers Alternative to Dark Energy Page 1 of 8http://www.space.com/scienceastronomy/090817-dark-energy-alternative.html What is Dark Energy? Universe Might Be Bigger and Older Than Expected In New? Register: Join Now! 'Big Wave' Theory Offers Alternative to Dark Energy By Clara Moskowitz Staff

  3. 8/24/09 11:48 AMSPACE.com --'Big Wave' Theory Offers Alternative to Dark Energy Page 1 of 10http://www.space.com/scienceastronomy/090817-dark-energy-alternative.html#comments

    E-Print Network [OSTI]

    Temple, Blake

    8/24/09 11:48 AMSPACE.com -- 'Big Wave' Theory Offers Alternative to Dark Energy Page 1 of 10http://www.space.com/scienceastronomy/090817-dark-energy-alternative.html#comments What is Dark Energy? Universe Might Be Bigger and Older Than In New? Register: Join Now! 'Big Wave' Theory Offers Alternative to Dark Energy By Clara Moskowitz Staff

  4. Haszeldine et al s.haszeldine@ed.ac.uk Regulation for CCS beneath the UK offshore and onshore International Risk Governance Council www.irgc.org March, modified April 2007, Washington, USA Page 1

    E-Print Network [OSTI]

    Haszeldine, Stuart

    consumption". The Budget 2007 committed the UK to a competition to build the first UK electricity generation International Risk Governance Council www.irgc.org March, modified April 2007, Washington, USA Page 1 Regulation to the fore of the UK agenda since 2001. The Government has committed to aggressive CO2 targets well in excess

  5. 15/01/08 12:01The impact of gated Communities on property values: evidence of changes in real estate markets -Los ... -Cybergeo Page 1 of 23http://www.cybergeo.eu/index6225.html

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    (construction and maintenance costs of infrastructure within the gates). Such a structuring of residential space estate markets -Los ... - Cybergeo Page 1 of 23http://www.cybergeo.eu/index6225.html Cybergeo Systemic governments and land developers. Both agree to charge the homebuyer with the cost of urban sprawl

  6. 10/05/2013 10:34Cherwell.org -Oxford / News / Academic / The Hole Truth Page 1 of 2http://www.cherwell.org/news/academic/2013/05/09/the-hole-truth

    E-Print Network [OSTI]

    Gardner, Andy

    Walsh has published 6 articles Photograph: WikiImages The Hole Truth New research by Oxford academics10/05/2013 10:34Cherwell.org - Oxford / News / Academic / The Hole Truth Page 1 of 2http://www.cherwell.org/news/academic Colleges Academic Town Worcester Provost battles with Exeter building plan Teddy Hall Earth Sciences dinner

  7. 10/8/08 1:57 PMThe Maneater -Scientists, public talk about biofuels Page 1 of 2http://www.themaneater.com/stories/2008/4/4/scientists-public-talk-about-biofuels/

    E-Print Network [OSTI]

    Glaser, Rainer

    10/8/08 1:57 PMThe Maneater - Scientists, public talk about biofuels Page 1 of 2http://www.themaneater.com/stories/2008/4/4/scientists-public-talk-about-biofuels/ SearchNews: STRIPES age-requirement initiative waits on signatures Scientists, public talk about biofuels By Justin Myers April 4, 2008 The causes of rising gas

  8. To print this page, select File then Print from your browser URL: http://www.hgtvpro.com/hpro/nws_ind_nws_trends/article/0,2624,HPRO_26519_5943476,00.html

    E-Print Network [OSTI]

    on utility bills by decreasing energy and water consumption and to obtain national green certification and energy leaks to produce an estimated 49 percent decrease in energy consumption from the preTo print this page, select File then Print from your browser URL: http://www.hgtvpro.com/hpro/nws_ind_nws_trends

  9. 23/04/2012 15:45Cambridge University Engineering Department: News item Page 1 of 1http://www.eng.cam.ac.uk/news/stories/2008/alumni_event/

    E-Print Network [OSTI]

    Cipolla, Roberto

    23/04/2012 15:45Cambridge University Engineering Department: News item Page 1 of 1http://www.eng.cam.ac.uk/news/stories/2008/alumni_event/ © Department of Engineering at the University of Cambridge Information provided by web-editor Jane Hunter event organiser (left) Department of Engineering University of Cambridge

  10. 11/10/2010 17:32Cambridge University Engineering Department: News item Page 1 of 2http://www.eng.cam.ac.uk/news/stories/2010/RAE_fellowship/

    E-Print Network [OSTI]

    Cipolla, Roberto

    11/10/2010 17:32Cambridge University Engineering Department: News item Page 1 of 2http://www.eng.cam.ac.uk/news/stories/2010/RAE_fellowship/ Department of Engineering University of Cambridge > Engineering Department > News & Features Royal Academy of Engineering elected Professor Roberto Cipolla and Dr Ivor Day to a Fellowship 20

  11. Illinois Jobs Index release 11/28/2011 www.real.illinois.edu page 1 For August Illinois Job Index, the state and the Nation had positive job growth, the RMW had negative job growth.

    E-Print Network [OSTI]

    Frank, Thomas D.

    Illinois Jobs Index release 11/28/2011 www.real.illinois.edu page 1 For August Illinois Job Index, the state and the Nation had positive job growth, the RMW had negative job growth. The Illinois Job Index Positive Sep 2011­ Oct 2011 Last 12 months Oct 2011 Total non-farm employment Growth Rate % Number of Jobs

  12. Illinois Jobs Index release 07/25/2011 www.real.illinois.edu page 1 For July Illinois Job Index, the state had negative job growth while the Nation and the RMW both had positive job growth.

    E-Print Network [OSTI]

    Shim, Moonsub

    Illinois Jobs Index release 07/25/2011 www.real.illinois.edu page 1 For July Illinois Job Index, the state had negative job growth while the Nation and the RMW both had positive job growth. The monthly Illinois Job Index and MSA Report are issued monthly as tools for elected officials, policy leaders

  13. Illinois Jobs Index release 3/14/2011 www.real.illinois.edu page 1 For January Illinois Job Index, the Nation, RMW and the state all had positive job growth.

    E-Print Network [OSTI]

    Anastasio, Thomas J.

    Illinois Jobs Index release 3/14/2011 www.real.illinois.edu page 1 For January Illinois Job Index, the Nation, RMW and the state all had positive job growth. The monthly Illinois Job Index and MSA Report months Jan 2011 Total non-farm employment Growth Rate % Number of Jobs Growth Rate% Number of Jobs Shadow

  14. Illinois Jobs Index release 4/25/2011 www.real.illinois.edu page 1 For March Illinois Job Index, the Nation, RMW and the state all had positive job growth.

    E-Print Network [OSTI]

    Anastasio, Thomas J.

    Illinois Jobs Index release 4/25/2011 www.real.illinois.edu page 1 For March Illinois Job Index, the Nation, RMW and the state all had positive job growth. The monthly Illinois Job Index and MSA Report months Mar 2011 Total non-farm employment Growth Rate % Number of Jobs Growth Rate% Number of Jobs Shadow

  15. Illinois Jobs Index release 06/27/2011 www.real.illinois.edu page 1 For June Illinois Job Index, the RMW had negative job growth while the Nation and the state both had positive job growth.

    E-Print Network [OSTI]

    Shim, Moonsub

    Illinois Jobs Index release 06/27/2011 www.real.illinois.edu page 1 For June Illinois Job Index, the RMW had negative job growth while the Nation and the state both had positive job growth. The monthly Illinois Job Index and MSA Report are issued monthly as tools for elected officials, policy leaders

  16. Illinois Jobs Index release 10/31/2011 www.real.illinois.edu page 1 For August Illinois Job Index, the state and the Nation had positive job growth, the RMW had negative job growth.

    E-Print Network [OSTI]

    Frank, Thomas D.

    Illinois Jobs Index release 10/31/2011 www.real.illinois.edu page 1 For August Illinois Job Index, the state and the Nation had positive job growth, the RMW had negative job growth. The Illinois Job Index Positive Aug 2011­ Sep 2011 Last 12 months Sep 2011 Total non-farm employment Growth Rate % Number of Jobs

  17. Illinois Jobs Index release 01/31/2011 www.real.illinois.edu page 1 For November Illinois Job Index, the state and the Nation had positive job growth, the RMW had negative job growth.

    E-Print Network [OSTI]

    Frank, Thomas D.

    Illinois Jobs Index release 01/31/2011 www.real.illinois.edu page 1 For November Illinois Job Index, the state and the Nation had positive job growth, the RMW had negative job growth. The Illinois Job Index Negative Nov 2011­ Dec 2011 Last 12 months Dec 2011 Total non-farm employment Growth Rate % Number of Jobs

  18. Notes on the PMC Journal List CSV file This CSV file, available from the Journal List page on the PMC site, http://www.ncbi.nlm.nih.gov/pmc/

    E-Print Network [OSTI]

    Levin, Judith G.

    Notes on the PMC Journal List CSV file This CSV file, available from the Journal List page on the PMC site, http://www.ncbi.nlm.nih.gov/pmc/ journals/, is a list of journals that currently deposit in PMC. It includes journals that are no longer in publication or no longer deposit material in PMC

  19. 9/18/09 2:59 PMDark Energy May Not Exist At All -Windows 7 Forums Page 1 of 5http://www.sevenforums.com/chillout-room/21411-dark-energy-may-not-exist-all.html

    E-Print Network [OSTI]

    Temple, Blake

    XP SP3 18 posts Nis, Serbia Dark Energy May Not Exist At All Quote: Experts in advanced mathematics9/18/09 2:59 PMDark Energy May Not Exist At All - Windows 7 Forums Page 1 of 5http://www.sevenforums.com/chillout-room/21411-dark-energy-may-not-exist-all.html User Name Remember Me? Password Register | Today's Posts

  20. 5/28/08 6:03 PMPrinceton University -PPPL to phase out compact stellarator experiment, upgrade spherical torus program Page 1 of 2http://www.princeton.edu/main/news/archive/S21/15/04A97/index.xml?section=topstories

    E-Print Network [OSTI]

    in an underestimation of its cost and a more prolonged construction process. An 18-month series of project reviews spherical torus program Page 1 of 2http://www.princeton.edu/main/news/archive/S21/15/04A97/index://www.pppl.gov/> (PPPL) will phase out construction of the National Compact Stellarator Experiment (NCSX) and instead

  1. 5/14/10 6:44 AMHow to Clean Up the Oil |Triple Pundit Page 1 of 3http://www.triplepundit.com/2010/05/how-to-clean-up-the-oil/

    E-Print Network [OSTI]

    Hazen, Terry

    , dumping 220,000 tons of heavy crude oil into the Atlantic. The spill was so large that the entire Brittany5/14/10 6:44 AMHow to Clean Up the Oil |Triple Pundit Page 1 of 3http://www.triplepundit.com/2010/05/how-to-clean-up-the-oil/ By RP Siegel | May 14th, 2010 View Comments How to Clean Up the Oil Like

  2. 12-04-21 8:41 AMJSTOR: Isis, Vol. 103, No. 1 (March 2012), pp. 111-125 Page 1 of 20http://www.jstor.org/stable/10.1086/664982

    E-Print Network [OSTI]

    Vicedo, Marga

    12-04-21 8:41 AMJSTOR: Isis, Vol. 103, No. 1 (March 2012), pp. 111-125 Page 1 of 20http://www.jstor.org/stable/10.1086/664982 Isis Subscribe or Renew Published by: on behalf ofThe University of Chicago Press in introducing students to the normal #12;12-04-21 8:41 AMJSTOR: Isis, Vol. 103, No. 1 (March 2012), pp. 111

  3. Imaging planets around nearby white dwarfs

    E-Print Network [OSTI]

    M. R. Burleigh; F. J. Clarke; S. T. Hodgkin

    2002-02-09T23:59:59.000Z

    We suggest that Jovian planets will survive the late stages of stellar evolution, and that white dwarfs will retain planetary systems in wide orbits (>5AU). Utilising evolutionary models for Jovian planets, we show that infra-red imaging with 8m class telescopes of suitable nearby white dwarfs should allow us to resolve and detect companions >3Mjup. Detection of massive planetary companions to nearby white dwarfs would prove that such objects can survive the final stages of stellar evolution, place constraints on the frequency of main sequence stars with planetary systems dynamically similar to our own and allow direct spectroscopic investigation of their composition and structure.

  4. Application page 1 Majors/Programs of StudyYou can apply using the common application or online: www.uml.edu/apply

    E-Print Network [OSTI]

    Massachusetts at Lowell, University of

    Applied/Computational Mathematics Bioinformatics Business Applications Computer Science Probability/Statistics: www.uml.edu/apply FRANCIS COLLEGE OF ENGINEERING Chemical Engineering* General Biological Engineering Nanomaterials Engineering Nuclear Engineering Paper Engineering Civil Engineering* Computer Engineering

  5. Page 1 of 5for more information, visit www.sustain.ubc.ca At UBC, sustainability isn't just a word to define--it's a word

    E-Print Network [OSTI]

    Laval, Bernard

    Website Reference Link Download Reference Link Email Contact Link did you know? Sustainability information visit: Sustainability Coordinators your sc This document was designed to be used as an interactive and search for reusable department items like furniture. www.reuseitubc.ca . Bookmark UBC Recyclopedia

  6. 10/1/10 8:07 PMDesert Varnish : Encyclopedia of Geography Page 1 of 4http://www.sage-ereference.com/geography/Article_n276.html

    E-Print Network [OSTI]

    Dorn, Ron

    categories of rock coatings Source: Author. Liu and other researchers in different settings://www.sage-ereference.com/geography/Article_n276.html Desert Varnish Desert varnish is but one of more than a dozen rock coatings (Table 1) that drastically alter the appearance of rock surfaces. The better term is rock varnish because this coating occurs

  7. THE ACS NEARBY GALAXY SURVEY TREASURY

    SciTech Connect (OSTI)

    Dalcanton, Julianne J.; Williams, Benjamin F.; Rosema, Keith; Gogarten, Stephanie M.; Christensen, Charlotte; Gilbert, Karoline; Hodge, Paul [Department of Astronomy, Box 351580, University of Washington, Seattle, WA 98195 (United States); Seth, Anil C. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Dolphin, Andrew [Raytheon, 1151 E. Hermans Road, Tucson, AZ 85756 (United States); Holtzman, Jon [Department of Astronomy, New Mexico State University, Box 30001, 1320 Frenger St., Las Cruces, NM 88003 (United States); Skillman, Evan D.; Weisz, Daniel [Department of Astronomy, University of Minnesota, 116 Church St. SE, Minneapolis, MN 55455 (United States); Cole, Andrew [School of Mathematics and Physics, University of Tasmania, Hobart, Tasmania (Australia); Girardi, Leo [Osservatorio Astronomico di Padova - INAF, Vicolo dell'Osservatorio 5, I-35122 Padova (Italy); Karachentsev, Igor D. [Special Astrophysical Observatory, Russian Academy of Sciences, Nizhnji Arkhyz, Karachai-Circessia Republic 369167 (Russian Federation); Olsen, Knut [NOAO, National Optical Astronomy Observatory 950 N. Cherry Ave., Tucson, AZ 85719 (United States); Freeman, Ken [Mount Stromlo Observatory, Research School of Astronomy and Astrophysics, The Australian National Univ., ACT 0200 (Australia); Gallart, Carme [Inst. de AstrofIsica de Canarias, VIa Lactea, s/n, 38200 La Laguna, Tenerife (Spain); Harris, Jason [Steward Observatory, Univ. of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721 (United States); De Jong, Roelof S. [Space Telescope Science Inst., 3700 San Martin Dr., Baltimore, MD 21218 (United States)], E-mail: jd@astro.washington.edu, E-mail: ben@astro.washington.edu, E-mail: krosema@astro.washington.edu, E-mail: stephanie@astro.washington.edu, E-mail: christensen@astro.washington.edu, E-mail: fabio@astro.washington.edu, E-mail: trq@astro.washington.edu, E-mail: aseth@cfa.harvard.edu (and others)

    2009-07-15T23:59:59.000Z

    The ACS Nearby Galaxy Survey Treasury (ANGST) is a systematic survey to establish a legacy of uniform multi-color photometry of resolved stars for a volume-limited sample of nearby galaxies (D < 4 Mpc). The survey volume encompasses 69 galaxies in diverse environments, including close pairs, small and large groups, filaments, and truly isolated regions. The galaxies include a nearly complete range of morphological types spanning a factor of {approx}10{sup 4} in luminosity and star formation rate. The survey data consist of images taken with the Advanced Camera for Surveys (ACS) on the Hubble Space Telescope (HST), supplemented with archival data and new Wide Field Planetary Camera 2 (WFPC2) imaging taken after the failure of ACS. Survey images include wide field tilings covering the full radial extent of each galaxy, and single deep pointings in uncrowded regions of the most massive galaxies in the volume. The new wide field imaging in ANGST reaches median 50% completenesses of m {sub F475W} = 28.0 mag, m {sub F606W} = 27.3 mag, and m {sub F814W} = 27.3 mag, several magnitudes below the tip of the red giant branch (TRGB). The deep fields reach magnitudes sufficient to fully resolve the structure in the red clump. The resulting photometric catalogs are publicly accessible and contain over 34 million photometric measurements of >14 million stars. In this paper we present the details of the sample selection, imaging, data reduction, and the resulting photometric catalogs, along with an analysis of the photometric uncertainties (systematic and random), for both ACS and WFPC2 imaging. We also present uniformly derived relative distances measured from the apparent magnitude of the TRGB.

  8. 9/19/13 11:37 AMLanguage skills key to export success says The British Chambers of Commerce Page 1 of 2http://www.growthbusiness.co.uk/news-and-market-deals/business-news/2098113/language-skills-key-to-export-success-says-bcc.thtml

    E-Print Network [OSTI]

    Su, Xiao

    9/19/13 11:37 AMLanguage skills key to export success says The British Chambers of Commerce Page 1 of 2http://www.growthbusiness.co.uk/news-and-market-deals/business-news/2098113/language-skills-key-to-export Language skills key to export success says BCC The British Chambers of Commerce (BCC) is calling on UK

  9. 7/9/10 2:34 PMWHO | Human African trypanosomiasis: number of new cases drops to historically low level in 50 years Page 1 of 2http://www.who.int/neglected_diseases/integrated_media/integrated_media_hat_june_2010/en/index.html

    E-Print Network [OSTI]

    Cross, George

    7/9/10 2:34 PMWHO | Human African trypanosomiasis: number of new cases drops to historically low level in 50 years Page 1 of 2http://www.who.int/neglected_diseases/integrated_media/integrated_media tropical diseases > Integrated media related to NTD printable version Human African trypanosomiasis: number

  10. 11/26/12 4:27 PMCoal mine fossils: Paleontology shows us past climate change. -Slate Magazine Page 1 of 4http://www.slate.com/articles/health_and_science/coal/2012/11/coal_mine_fossils_paleontology_shows_us_past_climate_change.single.html

    E-Print Network [OSTI]

    Montańez, Isabel Patricia

    11/26/12 4:27 PMCoal mine fossils: Paleontology shows us past climate change. - Slate Magazine Page 1 of 4http://www.slate.com/articles/health_and_science/coal/2012/11/coal_mine The Economist FollowFollow @slate@slate 467K followers LOG IN/REGISTER | NEWS & POLITICS TECH BUSINESS ARTS LIFE

  11. 9/18/09 2:42 PM'Big Wave' Theory Offers Alternative to Dark Energy -Tech Support Forum Page 1 of 4http://www.techsupportforum.com/relaxation-room/offline/406161-big-wave-theory-offers-alternative-dark-energy.html

    E-Print Network [OSTI]

    Temple, Blake

    9/18/09 2:42 PM'Big Wave' Theory Offers Alternative to Dark Energy - Tech Support Forum Page 1 of 4http://www.techsupportforum.com/relaxation-room/offline/406161-big-wave-theory-offers-alternative-dark-energy' Theory Offers Alternative to Dark Energy User Name Remember Me? Password Log in Site Map Register Donate

  12. 4/11/12 1:50 PMNobel Prizes: Year In Review 2010 --Britannica Online Encyclopedia Page 1 of 1http://www.britannica.com/EBchecked/topic/1719562/Nobel-Prizes-Year...-Review-2010/296811/Prize-for-Chemistry?sections=296811&view=print

    E-Print Network [OSTI]

    Berry, R. Stephen

    4/11/12 1:50 PMNobel Prizes: Year In Review 2010 -- Britannica Online Encyclopedia Page 1 of 1http://www.britannica.com/EBchecked/topic/1719562/Nobel-Prizes-Year...-Review-2010/296811/Prize-for-Chemistry?sections=296811&view=print Prize

  13. 24/05/2010 07:18Zoologger: Attack of the self-sacrificing child clones -life -12 May 2010 -New Scientist Page 1 of 3http://www.newscientist.com/article/dn18894-zoologger-attack-of-the-selfsacrificing-child-clones.html

    E-Print Network [OSTI]

    Gardner, Andy

    24/05/2010 07:18Zoologger: Attack of the self-sacrificing child clones - life - 12 May 2010 - New Scientist Page 1 of 3http://www.newscientist.com/article/dn18894-zoologger-attack Zoologger: Attack of the self-sacrificing child clones 16:49 12 May 2010 by Michael Marshall For similar

  14. 11/21/2006 01:20 PMThe Office of Science -Remarks on behalf of the United States Government Page 1 of 2http://www.sc.doe.gov/News_Information/News_Room/2006/ITER/RLO_Remarksfor_ITER_Signing_Ceremony.html

    E-Print Network [OSTI]

    /RLO_Remarksfor_ITER_Signing_Ceremony.html About the Office of Science News and Information Accomplishments/Awards Program Offices Research11/21/2006 01:20 PMThe Office of Science - Remarks on behalf of the United States Government Page 1 of 2http://www.sc.doe.gov/News_Information/News_Room/2006/ITER

  15. 03/05/2010 09:26Photos: 3D replicas to help sell your home? That's computer vision | Software | silicon.com Page 1 of 11http://www.silicon.com/technology/software/2010/03/30/photos-3d-...cas-to-help-sell-your-home-thats-computer-vision-39745647/print/

    E-Print Network [OSTI]

    Cipolla, Roberto

    model of Antony Gormley's head, printed via 3D printer Photo credits: Natasha Lomas03/05/2010 09:26Photos: 3D replicas to help sell your home? That's computer vision | Software | silicon.com Page 1 of 11http://www.silicon.com/technology/software/2010/03/30/photos-3d

  16. 5/10/10 7:22 AMTerry Hazen, Berkeley Lab: Deepwater Horizon Spill Detergents Could Make Bad Situation Worse Page 1 of 3http://www.outlookseries.com/N7/Science/3910_Terry_Hazen_Berkeley_La...water_Horizon_Spill_Detergents_Could_Situation_Worse_Terry_Hazen.

    E-Print Network [OSTI]

    Hazen, Terry

    5/10/10 7:22 AMTerry Hazen, Berkeley Lab: Deepwater Horizon Spill Detergents Could Make Bad Situation Worse Page 1 of 3http://www.outlookseries.com/N7/Science/3910_Terry_Hazen_Berkeley_La...water_Horizon_Spill Terry Hazen, Berkeley Lab: Deepwater Horizon Spill Detergents Could Make Bad Situation Worse May 6, 2010

  17. 5/10/10 7:04 AMCaution urged in oil spill cleanup -UPI.com Page 1 of 1http://www.upi.com/Science_News/2010/05/05/Caution-urged-in-oil-spill-cleanup/UPI-48201273087918/print/

    E-Print Network [OSTI]

    Hazen, Terry

    Horizon oil spill. Terry Hazen, a microbial ecologist at the Lawrence Berkeley National Laboratory, said5/10/10 7:04 AMCaution urged in oil spill cleanup - UPI.com Page 1 of 1http://www.upi.com/Science_News/2010/05/05/Caution-urged-in-oil-spill-cleanup/UPI-48201273087918/print/ Caution urged in oil spill

  18. FACHBEREICH GERMANY WWW

    E-Print Network [OSTI]

    Kerber, Manfred

    UNIVERSIT ¨ AT DES SAARLANDES FACHBEREICH INFORMATIK D­66041 SAARBR ¨ UCKEN GERMANY WWW: http on Auto­ mated Deduction, pages 371--385, Nancy, France, 1994. Springer Verlag, Berlin, Germany, LNAI 814 Fachbereich Informatik, Universit¨at des Saarlandes 66041 Saarbr¨ucken, Germany +49­681­302­f4628j4627g

  19. FACHBEREICH GERMANY WWW

    E-Print Network [OSTI]

    Kerber, Manfred

    UNIVERSIT ¨ AT DES SAARLANDES FACHBEREICH INFORMATIK D­66041 SAARBR ¨ UCKEN GERMANY WWW: http Deduction, pages 807--810, Nancy, France, 1994. Springer­ Verlag, Berlin, Germany. LNAI 814. #12; KEIM¨orn Richts J¨org Siekmann Fachbereich Informatik, Universit¨at des Saarlandes 66041 Saarbr¨ucken, Germany

  20. Boys and Girls, Be Ambitious! http://www.math.sci.hokudai.ac.jp/message/message-graduates/

    E-Print Network [OSTI]

    Nakamura, Iku

    ://www.math.sci.hokudai.ac.jp/ #12;AIKAWA, Hiroaki WebPage http://www.math.sci.hokudai.ac.jp/ aik/index-j.html Fatou Martin Harnack AKITA, Toshiyuki WebPage http://www.math.sci.hokudai.ac.jp/ akita/ Eilenberg-MacLane Coxeter #12;ASAKURA, Masanori ARAI, Asao ABE, Noriyuki WebPage http://www.math.sci.hokudai.ac.jp/ abenori/ #12;ISHIKAWA, Goo Web

  1. The Photometric Properties of Nearby Type Ia Supernovae

    E-Print Network [OSTI]

    Ganeshalingam, Mohan

    2012-01-01T23:59:59.000Z

    The Rise-Time Distribution of Nearby Type Ia Supernovae 3.1Highlight: The Physics of Supernovae, ed. W. Hillebrandt &1.1 Supernovae . . . . . . . . . . . . . . 1.1.1

  2. Science and Public Policy, 34(2), March 2007, pages 109116 DOI: 10.3152/030234207X190964; http://www.ingentaconnect.com/content/beech/spp

    E-Print Network [OSTI]

    Neff, Jason

    Science and Public Policy, 34(2), March 2007, pages 109­116 DOI: 10.3152/030234207X190964; http and policy circles. This paper reviews the literature on climate forecasting information and explores three, flooding in Peru and Ecuador and drought- related famine in southern Africa and India, revealed

  3. 10/19/11 9:03 AMMeatingplace.com -Technical Articles Page 1 of 4http://www.meatingplace.com/MembersOnly/technology/details.aspx?item=19896

    E-Print Network [OSTI]

    Bennett, Gisele

    Insight and best practices for beef, pork and poultry processors printer-friendly page more stories email Grade A or high-quality products. Grading is conducted through the USDA AMS (Agricultural Marketing bones, skin tears, exposed flesh and ensures good coverage of fat under the skin and meatiness

  4. 8/20/09 9:46 AMThe Hindu News Update Service Page 1 of 2http://www.thehindu.com/holnus/008200901031612.htm

    E-Print Network [OSTI]

    Su, Tin Tin

    Metro Plus Business Education Plus Open Page Book Review SciTech NXg Entertainment Cinema Plus Young and Nancy Guild, who authored a paper in the January 2 issue of the journal Science showing how peer they think know the right answer," said Michelle Smith, a science teaching fellow with CU's Science Education

  5. PAGE OF PAGES

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level:Energy: Grid Integration Redefining What's Possible for RenewableSpeedingBiomass and BiofuelsOversightand Simulated TemperatureEnergybONTRACT

  6. WWW-2005 Tutorial Web Content Mining

    E-Print Network [OSTI]

    Hu, Wen-Chen

    of surface Web and deep Web. Surface Web: pages that can be browsed using a browser. Deep Web: databasesWWW-2005 Tutorial Web Content Mining Bing Liu Department of Computer Science University of Illinois at Chicago (UIC) liub@cs.uic.edu http://www.cs.uic.edu/~liub The 14th International World Wide Web Conference

  7. 199/07/Tuesday 17h37Oasis, The Online Abstract Submission System Page 1 sur 2https://www.abstractsonline.com/submit/SubmitPrinterFriendly...%7D&MKey=%7B66F0352A%2D30DC%2D4B9F%2DB0CC%2DE851495B78DC%7D

    E-Print Network [OSTI]

    Demoulin, Pascal

    199/07/Tuesday 17h37Oasis, The Online Abstract Submission System Page 1 sur 2https):  Oral Preferred Additional Information (Complete): Status: Complete #12;199/07/Tuesday 17h37Oasis://www.abstractsonline.com/submit/SubmitPrinterFriendly...%7D&MKey=%7B66F0352A%2D30DC%2D4B9F%2DB0CC%2DE851495B78DC%7D Washington, DC 20009 Powered by OASIS

  8. 11-06-03 3:43 AMPolice officer seeks truth in South Africa -Winnipeg Free Press Page 1 of 3http://www.printthis.clickability.com/pt/cpt?expire=&title=Police+offic...com%2Flocal%2Fpolice-officer-seeks-truth-in-south-africa-123086533.html

    E-Print Network [OSTI]

    Martin, Jeff

    11-06-03 3:43 AMPolice officer seeks truth in South Africa - Winnipeg Free Press Page 1 of 3http://www.printthis.clickability.com/pt/cpt?expire=&title=Police+offic...com%2Flocal%2Fpolice-officer-seeks-truth-in-south-africa truth in South Africa By: Nick Martin Posted: 06/3/2011 1:00 AM | Comments: 0 #12;11-06-03 3:43 AMPolice

  9. 15/07/12 5:47 AMA World Without Coral Reefs -NYTimes.com Page 1 of 3http://www.nytimes.com/2012/07/14/opinion/a-world-without-coral-reefs.html?_r=2&hpw&pagewanted=print

    E-Print Network [OSTI]

    Botea, Adi

    15/07/12 5:47 AMA World Without Coral Reefs - NYTimes.com Page 1 of 3http://www.nytimes.com/2012/07/14/opinion/a-world-without-coral-reefs.html?_r=2&hpw&pagewanted=print July 13, 2012 A World Without Coral of the world's coral reefs, the nurseries of tropical coastal fish stocks. They have become zombie ecosystems

  10. Kinematic segregation of nearby disk stars from the Hipparcos database

    E-Print Network [OSTI]

    R. E. de Souza; R. Teixeira

    2007-04-25T23:59:59.000Z

    To better understand our Galaxy, we investigate the pertinency of describing the sys tem of nearby disk stars in terms of a two-components Schwarzschild velocity distributio n.Using the proper motion and parallax information of Hipparcos database, we determine t he parameters characterizing the local stellar velocity field of a sample of 22000 disk stars. The sample we use is essentially the same as the one described by the criteria ad opted to study the LSR and the stream motion of the nearby stellar population

  11. Motions of galaxies in the nearby universe with 2MASS

    E-Print Network [OSTI]

    Crook, Aidan Christopher

    2009-01-01T23:59:59.000Z

    I present the first model of a flow-field in the nearby Universe (cz < 12, 000 km s-') constructed from groups of galaxies identified in an all-sky flux-limited survey. The Two Micron All-Sky Redshift Survey (2MRS), upon ...

  12. http://www.slate.com/articles/life/do_the_math/2012/03/how_creativity_works_what_broadway_musicals_really_teach_us_about_collaboration_.html Page 1 of 2 26/04/2012 15:28 PM

    E-Print Network [OSTI]

    Kuzmanovic, Aleksandar

    http://www.slate.com/articles/life/do_the_math/2012/03/how_creativity_works, 2012, at 9:00 AM ET Slate.com Six Degrees of Innovation What Broadway musicals tell us about creativity a low Q. #12;http://www.slate.com/articles/life/do_the_math/2012/03/how_creativity_works

  13. http://www.slate.com/articles/technology/future_tense/2012/06/robocup_2012_how_robot_soccer_has_led_to_robotics_breakthroughs_.html Page 1 of 2 27/06/2012 06:31 AM

    E-Print Network [OSTI]

    Stryk, Oskar von

    http://www.slate.com/articles/technology/future_tense/2012/06/robocup_2012_how, June 14, 2012, at 6:24 PM ET Slate.com Why You Should Care About RoboCup Robot soccer's World Cup has stay to work on other robotic projects afterward," says Dorian Scholz, the team captain of #12;http://www.slate

  14. 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...

  15. NREL: Continuum Magazine Home Page

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Saleshttp://www.fnal.gov/directorate/nalcal/nalcal02_07_05_files/nalcal.gifNREL NRELChemicalIndustry PhotoPartnering:Winter

  16. NREL: Continuum Magazine Home Page

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Saleshttp://www.fnal.gov/directorate/nalcal/nalcal02_07_05_files/nalcal.gifNREL NRELChemicalIndustry

  17. NREL: Continuum Magazine Home Page

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Saleshttp://www.fnal.gov/directorate/nalcal/nalcal02_07_05_files/nalcal.gifNREL NRELChemicalIndustryIssue 3 Continuum. Clean

  18. NREL: Continuum Magazine Home Page

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Saleshttp://www.fnal.gov/directorate/nalcal/nalcal02_07_05_files/nalcal.gifNREL NRELChemicalIndustryIssue 3 Continuum.

  19. NREL: Continuum Magazine Home Page

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Saleshttp://www.fnal.gov/directorate/nalcal/nalcal02_07_05_files/nalcal.gifNREL NRELChemicalIndustryIssue 3 Continuum.Spring

  20. NREL: Energy Sciences Home Page

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Saleshttp://www.fnal.gov/directorate/nalcal/nalcal02_07_05_files/nalcal.gifNRELPowerNewsletterAcademy AlumniNews

  1. Lyapunov indices with two nearby trajectories in a curved spacetime

    E-Print Network [OSTI]

    Xin Wu; Tian-Yi Huang; Hong Zhang

    2010-06-28T23:59:59.000Z

    We compare three methods for computing invariant Lyapunov exponents (LEs) in general relativity. They involve the geodesic deviation vector technique (M1), the two-nearby-orbits method with projection operations and with coordinate time as an independent variable (M2), and the two-nearby-orbits method without projection operations and with proper time as an independent variable (M3). An analysis indicates that M1 and M3 do not need any projection operation. In general, the values of LEs from the three methods are almost the same. As an advantage, M3 is simpler to use than M2. In addition, we propose to construct the invariant fast Lyapunov indictor (FLI) with two-nearby-trajectories and give its algorithm in order to quickly distinguish chaos from order. Taking a static axisymmetric spacetime as a physical model, we apply the invariant FLIs to explore the global dynamics of phase space of the system where regions of chaos and order are clearlyidentified.

  2. Lyapunov indices with two nearby trajectories in a curved spacetime

    SciTech Connect (OSTI)

    Wu, X. [Department of Physics, Nanchang University, Nanchang 330047 (China); Department of Astronomy, Nanjing University, Nanjing 210093 (China); Huang, T.-Y.; Zhang, H. [Department of Astronomy, Nanjing University, Nanjing 210093 (China)

    2006-10-15T23:59:59.000Z

    We compare three methods for computing invariant Lyapunov exponents (LEs) in general relativity. These methods involve the geodesic deviation vector technique (M1), the two-nearby-orbits method with projection operations and with coordinate time as the independant variable (M2), and the two-nearby-orbits method without projection operations and with proper time as the independent variable (M3). An analysis indicates that M1 and M3 do not need any projection operation. In general, the values of LEs from the three methods are almost the same. However, M2 fails for some specific cases. As a result, M3 is the most preferable to calculate LEs in most cases. In addition, we propose to construct the invariant fast Lyapunov indictor (FLI) with two-nearby-trajectories and give its algorithm in order to quickly distinguish chaos from order. Taking a static axisymmetric spacetime as a physical model, we apply different algorithms of the FLI to explore the global dynamics of phase space of the system where regions of chaos and order are clearly identified.

  3. 16/05/12 3:58 PMFloating robots use GPS-enabled smartphones to track water flow Page 1 of 5http://www.spacedaily.com/reports/Floating_robots_use_GPS_enabled_smartphones_to_track_water_flow_999.html

    E-Print Network [OSTI]

    monitoring technology, promising to transform the way government agencies monitor one of the state's most.com Water Conservation Award Siemens is proud to be sponsoring the 79th US Confererance of Mayors. www.siemens

  4. 02/09/2009 16:58Warming Of Arctic Current Over 30 Years Triggers Release Of Methane Gas Page 1 of 2http://www.sciencedaily.com/releases/2009/08/090814103231.htm

    E-Print Network [OSTI]

    Rohling, Eelco

    ) Standard Bank Growing emerging markets with players in the energy value chain www.standardbank.com Solar Installation Course Solar energy heating installation & renewable energ Climate Environmental Issues Renewable Energy Oceanography Water Reference Geologic temperature record

  5. 5/28/10 3:40 PMNSF Funds Ultra-Low Energy Circuits | The Fu Foundation School of Engineering & Applied Science -Columbia University Page 1 of 1http://www.engineering.columbia.edu/nsf-funds-microelectronic-systems-research

    E-Print Network [OSTI]

    Yang, Junfeng

    5/28/10 3:40 PMNSF Funds Ultra-Low Energy Circuits | The Fu Foundation School of Engineering://www.engineering.columbia.edu/nsf-funds-microelectronic-systems-research Columbia University Home Directory | Help NSF Funds Ultra-Low Energy Circuits (http://www.compeng.columbia.edu/) . The grant will fund their proposal to perform research in ultra low-power microelectronic systems, which

  6. Damage to nearby divertor components of ITER-like devices during giant ELMs and disruptions

    E-Print Network [OSTI]

    Harilal, S. S.

    Damage to nearby divertor components of ITER-like devices during giant ELMs and disruptions. Fusion 50 (2010) 115004 (7pp) doi:10.1088/0029-5515/50/11/115004 Damage to nearby divertor components. The simulation results of the integrated modelling indicate a significant potential damage of the divertor nearby

  7. 4/18/11 10:39 AMB.C. aspires to lead the country in research and development Page 1 of 6http://www.canada.com/story_print.html?id=713de69a-38b7-48a8-9d50-d96d0aa1142b&sponsor=

    E-Print Network [OSTI]

    4/18/11 10:39 AMB.C. aspires to lead the country in research and development Page 1 of 6http://www.canada.com/story_print.html?id=713de69a-38b7-48a8-9d50-d96d0aa1142b&sponsor= B.C. aspires to lead the country in research for economy, innovation and education" by 2010. #12;4/18/11 10:39 AMB.C. aspires to lead the country

  8. 5/7/10 7:36 AMEureka!: UMass researchers study messengers from the stars Page 1 of 3http://www.gazettenet.com/print/268409?CSAuthResp=%3Asession%...ss%3AMMkuMGHWo1eZ4aGIQGMuaQ%3D%3D&CSUserId=49689&CSGroupId=5

    E-Print Network [OSTI]

    Lovley, Derek

    /268409?CSAuthResp=%3Asession%...ss%3AMMkuMGHWo1eZ4aGIQGMuaQ%3D%3D&CSUserId=49689&CSGroupId=5 Published?CSAuthResp=%3Asession%...ss%3AMMkuMGHWo1eZ4aGIQGMuaQ%3D%3D&CSUserId=49689&CSGroupId=5 radioactive decay5/7/10 7:36 AMEureka!: UMass researchers study messengers from the stars Page 1 of 3http://www.gazettenet.com/print

  9. Cleaning Web Pages for Effective Web Content Mining

    E-Print Network [OSTI]

    Ezeife, Christie

    Cleaning Web Pages for Effective Web Content Mining Jing Li and C.I. Ezeife School of Computer://www.cs.uwindsor.ca/cezeife Abstract. Classifying and mining noise-free web pages will improve on accuracy of search results as well as search speed, and may benefit web- page organization applications (e.g., keyword-based search engines

  10. BioMed Central Page 1 of 14

    E-Print Network [OSTI]

    BioMed Central Page 1 of 14 (page number not for citation purposes) BMC Medical Genomics Open December 2008 BMC Medical Genomics 2008, 1:63 doi:10.1186/1755-8794-1-63 Received: 29 September 2008 is properly cited. #12;BMC Medical Genomics 2008, 1:63 http://www.biomedcentral.com/1755-8794/1/63 Page 2

  11. 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 5252011 http:...

  12. www.cicomglobal.comwww.cicomglobal.com www.cicomglobal.com

    E-Print Network [OSTI]

    Shamir, Ron

    , , ". " ,,,,­ , ". , #12;II. www.cicomglobal.comwww.cicomglobal.com , #12;TouchGraph SEO­ http://www.touchgraph.com/seo www.cicomglobal.com , #12;TouchGraph SEO­ http://www.touchgraph.com/seo www

  13. Infrared colour properties of nearby radio-luminous galaxies

    E-Print Network [OSTI]

    Yang, Xiao-hong; Huang, Yan

    2015-01-01T23:59:59.000Z

    By combining the data of the Two Micron All Sky Survey (2MASS), the Wide Field Infrared Survey Explorer (WISE) and the Akari satellite, we study the infrared colour properties of a sample of 2712 nearby radio-luminous galaxies (RLGs). These RLGs are divided into radio-loud (RL) active galactic nuclei (AGNs), mainly occurring at redshifts of $0.05$ 3.0. We also analyse the MIR colours of RL AGNs divided into low- and high-excitation radio galaxies (LERGs and HERGs, respectively). The ([3.4]-[4.6])$-$([4.6]-[12]) diagram clearly shows separate distributions of LERGs and HERGs and a region of overlap, which suggests that LERGs and HERGs have different MIR properties. LERGs are responsible for the double-core distribution of RL AGNs on the ([3.4]-[4.6])$-$([4.6]-[12]) diagram. In addition, we also suggest 90$-$140$\\mu$m band spectral index $\\alpha(90,140)<-1.4$ as a criterion of selecting nearby active galaxies with non-thermal emissions at FIR wavelengths.

  14. HI emission and absorption in nearby, gas-rich galaxies

    E-Print Network [OSTI]

    Reeves, S N; Allison, J R; Koribalski, B S; Curran, S J; Pracy, M B

    2015-01-01T23:59:59.000Z

    We present the results of a targeted search for intervening HI absorption in six nearby, gas-rich galaxies using the Australia Telescope Compact Array (ATCA). The sightlines searched have impact parameters of 10-20 kpc. By targeting nearby galaxies we are also able to map their HI emission, allowing us to directly relate the absorption-line detection rate to the extended HI distribution. The continuum sightlines intersect the HI disk in four of the six galaxies, but no intervening absorption was detected. Of these four galaxies, we find that three of the non-detections are the result of the background source being too faint. In the fourth case we find that the ratio of the spin temperature to the covering factor ($T_{\\mathrm{S}}/f$) must be much higher than expected ($\\gtrsim$5700 K) in order to explain the non-detection. We discuss how the structure of the background continuum sources may have affected the detection rate of HI absorption in our sample, and the possible implications for future surveys. Future...

  15. January 2011 Update www.Engage360.com

    E-Print Network [OSTI]

    January 2011 Update www.Engage360.com #12;TABLE OF CONTENTS section page 1. INTRODUCTION................................................................................. 1 2. RESIDENTIAL SECTOR INCLUDING LOW INCOME................................. 9 3. COMMERCIAL SECTOR...................................................................... 28 4. INDUSTRIAL SECTOR........................................................................ 38 5

  16. http://www.ornl.gov/smallbusiness December 7, 2009

    E-Print Network [OSTI]

    at www.ornl.gov/smallbusiness. 4. Register your business in the Supplier Information Database included on the website. 5. Send me your one-page, electronic capabilities statement/statement of qualifications to better

  17. Materials Research Lab -CCIMR Project Pages 2002 http://www.mrl.ucsb.edu/mrl/outreach/educational/CCIMR/interns02.html[6/1/12 10:21:44 AM

    E-Print Network [OSTI]

    Bigelow, Stephen

    Materials Research Lab - CCIMR Project Pages 2002 http For Teachers Education Contacts News CCIMR Project Pages 2002 City College Interns in Materials Research (CCIMR City College Mentor: Tobias Schaedler Faculty Sponsor: Dr. Carlos Levi Department: Materials Project

  18. 9/18/09 2:29 PM'Big Wave' Theory Offers Alternative to Dark Energy Page 1 of 6http://www.mastersconnection.com/index.php/articles/452-wave

    E-Print Network [OSTI]

    Temple, Blake

    9/18/09 2:29 PM'Big Wave' Theory Offers Alternative to Dark Energy Page 1 of 6http;9/18/09 2:29 PM'Big Wave' Theory Offers Alternative to Dark Energy Page 2 of 6http:29 PM'Big Wave' Theory Offers Alternative to Dark Energy Page 4 of 6http

  19. 23/01/2008 20:56Null Hypothesis | Straight Talking Page 1 of 2http://www.null-hypothesis.co.uk/science/straight-talking/item/selfish_bacteria_threaten_slime_cities

    E-Print Network [OSTI]

    West, Stuart

    and even cheat on each other," Diggle said. Sound like anyone you know? As Diggle hints, such human Experiment: Speed of Light Candiru: The Willy Fish For The Love Of PCR Video Games & Sick Leave 10 Rules.com Liquid Zeolite 100% Pure Zeolite 30ml bottles Lab- Certified 100% Bacteria-Free. www.liquid

  20. 9/2/08 9:41 AMWhat's Lurking in Your Countertop? -NYTimes.com Page 1 of 3http://www.nytimes.com/2008/07/24/garden/24granite.html

    E-Print Network [OSTI]

    Llope, William J.

    ://www.nytimes.com/2008/07/24/garden/24granite.html Tony Cenicola/The New York Times TESTING Reports of granite emitting Liebert measures the radiation and radon emanating from granite like that in Lynn Sugarman's kitchen tracks in the kitchen, which had richly grained cream, brown and burgundy granite countertops. His Geiger

  1. 09/11/2007 04:05 PMLife's ingredients may have `sprinkled' on Earth -Space.com -MSNBC.com Page 1 of 4http://www.msnbc.msn.com/id/20724322

    E-Print Network [OSTI]

    Glaser, Rainer

    .com BRIC Investor Report Free special report on Brazil, Russia, India & China Stocks www Games Innovation Video U.S. News Politics World News Business Sports Entertainment Health Tech / Science, eventually assemble into rings. Although adenine's first ring needs a tiny energy boost from starlight

  2. To print this page, select File then Print from your browser URL: http://www.hgtvpro.com/hpro/nws_ind_nws_trends/article/0,2624,HPRO_26519_5944661,00.html

    E-Print Network [OSTI]

    energy bills for homeowners and businesses alike. Although there is significant debate among members://www.hgtvpro.com/hpro/nws_ind_nws_trends/article/0,2624,HPRO_26519_5944661,00.html AIA Praises American Clean Energy and Security Act Passed by House (AIA) issued the following statement regarding the recent passage of the American Clean Energy

  3. 08/17/2006 12:09 PMOak Ridge National Laboratory -U.S. ITER Project Completes Management Team Page 1 of 2http://www.ornl.gov/ornlhome/print/press_release_print.cfm?ReleaseNumber=mr20060817-00

    E-Print Network [OSTI]

    1 of 2http://www.ornl.gov/ornlhome/print/press_release_print.cfm?ReleaseNumber=mr20060817 that began October 1, 2005, the 12-member contractor team will manage the U.S. contribution to ITER. ITER-USA. · Mr. Carl Strawbridge, Deputy Project Manager, of ORNL, who served as Deputy Project Manager

  4. To print this page, select then from your browserFile Print URL: http://www.knoxnews.com/kns/local_news/article/0,1406,KNS_347_3035209,00.html

    E-Print Network [OSTI]

    , which releases energy by splitting atoms, fusion occurs when light atoms fuse together to form helium, proponents say it would provide an almost unlimited supply of energy, without the amount of waste associated://www.knoxnews.com/kns/local_news/article/0,1406,KNS_347_3035209,00.html ORNL snares prime fusion energy project Teams with Princeton

  5. PageRank model of opinion formation on Ulam networks

    E-Print Network [OSTI]

    L. Chakhmakhchyan; D. Shepelyansky

    2013-11-03T23:59:59.000Z

    We consider a PageRank model of opinion formation on Ulam networks, generated by the intermittency map and the typical Chirikov map. The Ulam networks generated by these maps have certain similarities with such scale-free networks as the World Wide Web (WWW), showing an algebraic decay of the PageRank probability. We find that the opinion formation process on Ulam networks have certain similarities but also distinct features comparing to the WWW. We attribute these distinctions to internal differences in network structure of the Ulam and WWW networks. We also analyze the process of opinion formation in the frame of generalized Sznajd model which protects opinion of small communities.

  6. Page comments

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level:Energy: Grid Integration Redefining What's Possible for RenewableSpeedingBiomassPPPO Website DirectoryCommunityFuture Use

  7. ENVIROISSUES PAGE

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

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  8. Home Page

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  9. Catalog of Nearby Galaxies and the Local Cosmic Web

    E-Print Network [OSTI]

    Igor D. Karachentsev; Valentina E. Karachentseva; Walter K. Huchtmeier; Dmitry I. Makarov

    2004-10-04T23:59:59.000Z

    We compiled an all-sky catalog of 451 nearby galaxies, each having an individual distance estimate $D \\la 10$ Mpc or the radial velocity $V_{LG} -17.0$, which contribute about 4% to the local luminosity density, and $\\sim(10-16)$% to the local HI mass density. We found that the mean local barion density $\\Omega_b(<8$ Mpc) = 2.3% consists of only a half of the global barion density, $\\Omega_b=(4.7\\pm0.6)$% (Spergel et al. 2003). The mean-square pairwise difference of radial velocities is about 100 km s$^{-1}$ for spatial separations within 1 Mpc, increasing to $\\sim 300$ km s$^{-1}$ on a scale of $\\sim 3$ Mpc.

  10. Collection: Supernova Discoveries from the Nearby Supernova Factory

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  11. DATE: PAGE:

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  13. DOE PAGES

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  14. TITLE PAGE

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  16. Untitled Page

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  17. Error Page

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  18. JSP Page

    Office of Scientific and Technical Information (OSTI)

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  20. Page 1

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  1. Page 1

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  3. Home Page

    Office of Legacy Management (LM)

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  5. Home Page

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  7. Home Page

    Office of Legacy Management (LM)

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  8. Home Page

    Office of Legacy Management (LM)

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  9. Subject Pages

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office of ScienceandMesa del SolStrengthening a solid ... StrengtheningLab (NewportStudying

  10. 10/14/09 2:29 PM'Big Wave' Theory Offers Alternative to Dark Energy Page 1 of 3http://www.thirdeyeconcept.com/news/index.php?topic=10126.0

    E-Print Network [OSTI]

    Temple, Blake

    10/14/09 2:29 PM'Big Wave' Theory Offers Alternative to Dark Energy Page 1 of 3http > Forum > Duality > The Eye > 'Big Wave' Theory Offers Alternative to Dark Energy Pages: [1] Go Down SEND THIS TOPIC | PRINT Author Topic: 'Big Wave' Theory Offers Alternative to Dark Energy (Read 59 times) 'Big

  11. 9/18/09 2:17 PM'Big Wave' Theory Offers Alternative to Dark Energy Page 1 of 20http://www.freerepublic.com/focus/f-chat/2319699/posts

    E-Print Network [OSTI]

    Temple, Blake

    9/18/09 2:17 PM'Big Wave' Theory Offers Alternative to Dark Energy Page 1 of 20http' Theory Offers Alternative to Dark Energy Space.com ^ | 8/18/09 | Clara Moskowitz Posted on August 19'Big Wave' Theory Offers Alternative to Dark Energy Page 2 of 20http

  12. INFRARED SPECTRAL ENERGY DISTRIBUTIONS OF NEARBY GALAXIES D. A. Dale,1

    E-Print Network [OSTI]

    Joseph, Robert D.

    INFRARED SPECTRAL ENERGY DISTRIBUTIONS OF NEARBY GALAXIES D. A. Dale,1 G. J. Bendo,2 C. W ABSTRACT The Spitzer Infrared Nearby Galaxies Survey (SINGS) is carrying out a comprehensive) are presented using broad- band imaging data from Spitzer, 2MASS, ISO, IRAS, and SCUBA. The infrared colors

  13. MID-INFRARED SPECTRAL DIAGNOSTICS OF NUCLEAR AND EXTRANUCLEAR REGIONS IN NEARBY GALAXIES

    E-Print Network [OSTI]

    Draine, Bruce T.

    MID-INFRARED SPECTRAL DIAGNOSTICS OF NUCLEAR AND EXTRANUCLEAR REGIONS IN NEARBY GALAXIES D. A. Dale,13 and F. Walter5 Received 2006 February 24; accepted 2006 March 31 ABSTRACT Mid-infrared diagnostics are presented for a large portion of the Spitzer Infrared Nearby Galaxies Survey (SINGS) sample plus archival

  14. Erosion Damage of Nearby Plasma-Facing Components during a Disruption on the Divertor Plate*

    E-Print Network [OSTI]

    Harilal, S. S.

    Erosion Damage of Nearby Plasma-Facing Components during a Disruption on the Divertor Plate* A those of the United States Governmentor any agency thereof. #12;Erosion Damage of Nearby Plasma radiation emitted by heating of the vapor cloud. This radiation energy can cause serious erosion damage

  15. BioMed Central Page 1 of 5

    E-Print Network [OSTI]

    Alvarez, Nadir

    assembly pipeline groups nucleotide sequences into clusters before independently assembling each cluster://www.biomedcentral.com/1471-2164/10/5 Page 2 of 5 (page number not for citation purposes) Construction and content Formidable (summarized in Table 1). Computation and Database Design Fourmidable analyses ar

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

    E-Print Network [OSTI]

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

    2015-01-01T23:59:59.000Z

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

  17. The Nuclear Near-Infrared Spectral Properties of Nearby Galaxies

    E-Print Network [OSTI]

    Mason, R E; Martins, L; Riffel, R; Martin, O Gonzalez; Almeida, C Ramos; Dutra, D Ruschel; Ho, L C; Thanjavur, K; Flohic, H; Alonso-Herrero, A; Lira, P; McDermid, R; Riffel, R A; Schiavon, R P; Winge, C; Hoenig, M D; Perlman, E

    2015-01-01T23:59:59.000Z

    We present spectra of the nuclear regions of 50 nearby (D = 1 - 92 Mpc, median = 20 Mpc) galaxies of morphological types E to Sm. The spectra, obtained with the Gemini Near-IR Spectrograph on the Gemini North telescope, cover a wavelength range of approximately 0.85-2.5 microns at R~1300--1800. There is evidence that most of the galaxies host an active galactic nucleus (AGN), but the range of AGN luminosities (log (L2-10 keV [erg/s]) = 37.0-43.2) in the sample means that the spectra display a wide variety of features. Some nuclei, especially the Seyferts, exhibit a rich emission-line spectrum. Other objects, in particular the type 2 Low Ionisation Nuclear Emission Region galaxies, show just a few, weak emission lines, allowing a detailed view of the underlying stellar population. These spectra display numerous absorption features sensitive to the stellar initial mass function, as well as molecular bands arising in cool stars, and many other atomic absorption lines. We compare the spectra of subsets of galaxie...

  18. NREL: Awards and Honors - PAGE_TITLE

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  19. NREL: Distributed Grid Integration Home Page

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  20. Black holes at the centers of nearby dwarf galaxies

    SciTech Connect (OSTI)

    Moran, Edward C.; Shahinyan, Karlen; Sugarman, Hannah R.; Vélez, Darik O. [Astronomy Department, Wesleyan University, Middletown, CT 06459 (United States); Eracleous, Michael [Department of Astronomy and Astrophysics, and Institute for Gravitation and the Cosmos, The Pennsylvania State University, 525 Davey Lab, University Park, PA 16802 (United States)

    2014-12-01T23:59:59.000Z

    Using a distance-limited portion of the Sloan Digital Sky Survey (SDSS) Data Release 7, we have identified 28 active galactic nuclei (AGNs) in nearby (d?80 Mpc) low-mass, low-luminosity dwarf galaxies. The accreting objects at the galaxy centers are expected to be intermediate-mass black holes (IMBHs) with M{sub BH}?10{sup 6} M{sub ?}. The AGNs were selected using several optical emission-line diagnostics after careful modeling of the continuum present in the spectra. We have limited our survey to objects with spectral characteristics similar to those of Seyfert nuclei, excluding emission-line galaxies with ambiguous spectra that could be powered by stellar processes. Thus, as a set, the host galaxies in our sample are the least massive objects in the very local universe certain to contain central black holes. Our sample is dominated by narrow-line (type 2) AGNs, and it appears to have a much lower fraction of broad-line objects than that observed for luminous, optically selected Seyfert galaxies. Given our focus on the nearest objects included in the SDSS, our survey is more sensitive to low-luminosity emission than previous optical searches for AGNs in low-mass galaxies. The [O iii] ?5007 luminosities of the Seyfert nuclei in our sample have a median value of L{sub 5007}=2×10{sup 5} L{sub ?} and extend down to ?10{sup 4} L{sub ?}. Using published data for broad-line IMBH candidates, we have derived an [O iii] bolometric correction of log(L{sub bol}/L{sub 5007})=3.0±0.3, which is significantly lower than values obtained for high-luminosity AGNs. Applying this correction to our sample, we obtain minimum black hole mass estimates that fall mainly in the 10{sup 3} M{sub ?}–10{sup 4} M{sub ?} range, which is roughly where the predicted mass functions for different black hole seed formation scenarios overlap the most. In the stellar mass range that includes the bulk of the AGN host galaxies in our sample, we derive a lower limit on the AGN fraction of a few percent, indicating that active nuclei in dwarf galaxies are not as rare as previously thought.

  1. The Masses of Nearby Dwarfs can be Determined with Gravitational Microlensing

    E-Print Network [OSTI]

    B. Paczynski

    1995-04-27T23:59:59.000Z

    Microlensing of distant stars in the Milky Way by the nearby high proper motion stars offers a direct way to precisely measure the masses of single lower main sequence stars and brown dwarfs.

  2. Victoria Kostina Curriculum Vitae -August 12, 2014 Page 1 of 7 Victoria Kostina

    E-Print Network [OSTI]

    Low, Steven H.

    Victoria Kostina Curriculum Vitae - August 12, 2014 Page 1 of 7 Victoria Kostina Department at the Kalashnikov MIPT competition of student projects July 2004 #12;Victoria Kostina Curriculum Vitae Page 2 of 7 reading group http://www.princeton.edu/~wcomm/ #12;Victoria Kostina Curriculum Vitae Page 3 of 7 Grants

  3. 5/14/10 4:32 PMTechnology Review: Blogs: arXiv blog: First Mathematical Model of Cow Behavior Page 1 of 4http://www.technologyreview.com/blog/arxiv/25171/

    E-Print Network [OSTI]

    Bollt, Erik

    5/14/10 4:32 PMTechnology Review: Blogs: arXiv blog: First Mathematical Model of Cow Behavior Page | auf Deutsch | in Italiano | | in India Home Videos Blogs Briefings Community Magazine Newsletters Events Resources Subscribe Computing Web Communications Energy Materials Biomedicine Business arXiv blog

  4. 2/14/14 10:42 AMThe Age of Sustainable Development by Jeffrey D. Sachs -Project Syndicate Page 1 of 4http://www.project-syndicate.org/print/jeffrey-d--sachs-proposes-a-new-curriculum-for-a-new-era

    E-Print Network [OSTI]

    2/14/14 10:42 AMThe Age of Sustainable Development by Jeffrey D. Sachs - Project Syndicate Page 1--sachs-proposes-a-new-curriculum-for-a-new-era EDUCATION JEFFREY D. SACHS Jeffrey D. Sachs, Professor of Sustainable Development, Professor of Health The End of Poverty and Common Wealth. DEC 23, 2013 The Age of Sustainable Development NEW YORK ­ A half

  5. 2/14/14 10:42 AMThe Age of Sustainable Development by Jeffrey D. Sachs -Project Syndicate Page 1 of 4http://www.project-syndicate.org/print/jeffrey-d--sachs-proposes-a-new-curriculum-for-a-new-era

    E-Print Network [OSTI]

    2/14/14 10:42 AMThe Age of Sustainable Development by Jeffrey D. Sachs - Project Syndicate Page 1--sachs-proposes-a-new-curriculum-for-a-new-era EDUCATION JEFFREY D. SACHS Jeffrey D. Sachs, Professor of Sustainable Development, Professor of Health The End of Poverty and Common Wealth. DEC 23, 2013 The Age of Sustainable Development NEW YORK ­ A half

  6. FACHBEREICH GERMANY WWW

    E-Print Network [OSTI]

    Sorge, Volker

    UNIVERSIT ¨ AT DES SAARLANDES FACHBEREICH INFORMATIK D­66041 SAARBR ¨ UCKEN GERMANY WWW: http Saarlandes 66041 Saarbr¨ucken, Germany fchrisjsorgeg@ags.uni­sb.de http://www.ags.uni­sb.de/ 2 School

  7. TransForumNews from Argonne's Transportation Research Program www.transportation.anl.gov

    E-Print Network [OSTI]

    Kemner, Ken

    TransForumNews from Argonne's Transportation Research Program www.transportation.anl.gov Volume 14 Issue 2 2014 Contents #12;TransForumNews from Argonne's Transportation Research Program www.transportation.anl.gov VERIFI Shrinks Combustion Engine Development Cycles to Save Money and Time page 4 Argonne researchers

  8. TransForumNews from Argonne's Transportation Research Program www.transportation.anl.gov

    E-Print Network [OSTI]

    Kemner, Ken

    TransForumNews from Argonne's Transportation Research Program www.transportation.anl.gov Volume 14 Issue 2 2014 #12;TransForumNews from Argonne's Transportation Research Program www.transportation.anl.gov VERIFI Shrinks Combustion Engine Development Cycles to Save Money and Time page 4 Argonne researchers

  9. J.M. Butler, Proceedings of the International Symposium on Human Identification (2014) http://www.promega.com/products/pm/genetic-identity/ishi-conference-proceedings/proceedings-index-home/

    E-Print Network [OSTI]

    2014-01-01T23:59:59.000Z

    .promega.com/products/pm/genetic-identity/ishi-conference-proceedings/proceedings-index-home/ Page 1 of 18://www.promega.com/products/pm/genetic-identity/ishi-conference-proceedings/proceedings-index-home/ PageJ.M. Butler, Proceedings of the International Symposium on Human Identification (2014) http://www

  10. Set home page Bookmark site Add search Show/Hide Menu |Print this page Email to friend >Text Size A A A

    E-Print Network [OSTI]

    West, Stuart

    · ·Set home page Bookmark site Add search Show/Hide Menu |Print this page Email to friend >Text > Matter & Energy > Computers & Math > Fossils & Ruins Science Topics > Agriculture > Astronomy > Biology of ecology and evolutionary biology and animal behavior. For more information, please see our website: www

  11. Information as published on the Norris Medical Library web page

    E-Print Network [OSTI]

    Zhang, Li I.

    Information as published on the Norris Medical Library web page http://www.usc.edu/hsc/nml/lib-services/cos.html COMMUNITY OF SCIENCE @ USC USC's membership in Community of Science (COS) provides you with access to web - Search the most comprehensive source of funding information available on the web, with up-to-date records

  12. Warner College of Natural Resources 2.10 Page 1

    E-Print Network [OSTI]

    , and scientific investigation of renewable and nonrenewable natural resources. Programs include the study of everyWarner College of Natural Resources _______________ 2.10 Page 1 Warner College of Natural Resources Office in Natural Resources Building, Room 101 (970) 491-6675 www.warnercnr.colostate.edu Professor Joyce

  13. Warner College of Natural Resources 2.10 Page 1

    E-Print Network [OSTI]

    Stephens, Graeme L.

    of renewable and nonrenewable natural resources. Programs include the study of every component of naturalWarner College of Natural Resources _______________ 2.10 Page 1 Warner College of Natural Resources Office in Natural Resources Building, Room 101 (970) 491-6675 www.warnercnr.colostate.edu Professor Joyce

  14. Academy Educational Enhancement Grants Page 1 of 11

    E-Print Network [OSTI]

    Academy Educational Enhancement Grants 2012-2013 Page 1 of 11 LSUHSC-NO Academy for the Advancement of Educational Scholarship February 2012 Educational Enhancement Grants LSUHSC-NO Academy for the Advancement are available in the OMERAD and an electronic version is also available on the Academy webpage:(http://www.learningcenter.lsuhsc.edu/academy

  15. Academy Educational Enhancement Grants Page 1 of 11

    E-Print Network [OSTI]

    Academy Educational Enhancement Grants 2012-2013 Page 1 of 11 LSUHSC-NO Academy for the Advancement-NO Academy for the Advancement of Educational Scholarship Office of Medical Education Research are available in the OMERAD and an electronic version is also available on the Academy webpage:(http://www.learningcenter.lsuhsc.edu/academy

  16. Page 1 of 7 University of Cambridge: Programme Specifications

    E-Print Network [OSTI]

    de Gispert, Adriŕ

    . The Programme was initially developed in collaboration with the Cambridge-MIT Institute (CMI). For more information on CMI, see http://www.cambridge-mit.org #12;Page 2 of 7 Programme Outcomes Successful students a specified period of time and to report it in writing and by seminar in an acceptable manner ­ this project

  17. FACHBEREICH GERMANY WWW

    E-Print Network [OSTI]

    Kerber, Manfred

    UNIVERSIT ¨ AT DES SAARLANDES FACHBEREICH INFORMATIK D­66041 SAARBR ¨ UCKEN GERMANY WWW: http, Universit¨ at des Saarlandes, Saar­ br¨ ucken, Germany #12; Planverfahren -- Skript zur Vorlesung

  18. FACHBEREICH GERMANY WWW

    E-Print Network [OSTI]

    Kerber, Manfred

    UNIVERSIT ¨ AT DES SAARLANDES FACHBEREICH INFORMATIK D­66041 SAARBR ¨ UCKEN GERMANY WWW: http Manfred Kerber Fachbereich Informatik, Universit¨at Kaiserslautern D­6750 Kaiserslautern, Germany kerber

  19. FACHBEREICH GERMANY WWW

    E-Print Network [OSTI]

    Sorge, Volker

    UNIVERSIT  AT DES SAARLANDES FACHBEREICH INFORMATIK D-66041 SAARBR  UCKEN GERMANY WWW: http, Universitat des Saarlandes, Germany fameierjpolletjsorgeg@ags.uni-sb.de http

  20. FACHBEREICH GERMANY WWW

    E-Print Network [OSTI]

    Kerber, Manfred

    UNIVERSIT ¨ AT DES SAARLANDES FACHBEREICH INFORMATIK D­66041 SAARBR ¨ UCKEN GERMANY WWW: http Informatik, Universit¨at des Saarlandes Postfach 1150, 66041 Saarbr¨ucken, Germany fhuang

  1. FACHBEREICH GERMANY WWW

    E-Print Network [OSTI]

    Kerber, Manfred

    UNIVERSIT ¨ AT DES SAARLANDES FACHBEREICH INFORMATIK D­66041 SAARBR ¨ UCKEN GERMANY WWW: http¨ucken Germany Abstract. The hallmark of traditional Artificial Intelligence (AI) research is the symbolic

  2. FACHBEREICH GERMANY WWW

    E-Print Network [OSTI]

    Kerber, Manfred

    UNIVERSIT ¨ AT DES SAARLANDES FACHBEREICH INFORMATIK D­66041 SAARBR ¨ UCKEN GERMANY WWW: http¨ucken Germany 1 Introduction The traditional paradigm of knowledge representation and processing in artificial

  3. FACHBEREICH GERMANY WWW

    E-Print Network [OSTI]

    Kerber, Manfred

    UNIVERSIT ¨ AT DES SAARLANDES FACHBEREICH INFORMATIK D­66041 SAARBR ¨ UCKEN GERMANY WWW: http, Fachbereich In­ formatik, Universit¨ at des Saarlandes, Saarbr¨ ucken, Germany #12; Sortenlogiken und ihre

  4. HIGH-VELOCITY CLOUDS IN THE NEARBY SPIRAL GALAXY M 83

    E-Print Network [OSTI]

    Miller, Eric D.

    We present deep H I 21 cm and optical observations of the face-on spiral galaxy M 83 obtained as part of a project to search for high-velocity clouds (HVCs) in nearby galaxies. Anomalous-velocity neutral gas is detected ...

  5. www.globalsubsidies.org THE GLOBAL SUBSIDIES INITIATIVE

    E-Print Network [OSTI]

    Toohey, Darin W.

    www.globalsubsidies.org THE GLOBAL SUBSIDIES INITIATIVE UNTOLD BILLIONS: FOSSIL-FUEL SUBSIDIES, THEIR IMPACTS AND THE PATH TO REFORM The Politics of Fossil-Fuel Subsidies #12;THE GLOBAL SUBSIDIES INITIATIVE | UNTOLD BILLIONS: FOSSIL-FUEL SUBSIDIES, THEIR IMPACTS AND THE PATH TO REFORM Page II The Politics

  6. www.facilities.ufl.edu BUSINESS AFFAIRS PLANNING DESIGN & CONSTRUCTION

    E-Print Network [OSTI]

    Slatton, Clint

    www.facilities.ufl.edu BUSINESS AFFAIRS PLANNING DESIGN & CONSTRUCTION PDC PROJECT MANAGEMENT GUIDE are available on the PDC website. The PM and CA shall use the PDC pay application checklist as a means to support the Cost of Work. PDC REVISED JANUARY 2014 PAGE 1 OF 3 #12;a)All trade contractors' pay

  7. Training Grant application, page 1 of 2 Application instructions for 2014-15 NIH Training Grant Traineeship

    E-Print Network [OSTI]

    Arnold, Jonathan

    Training Grant application, page 1 of 2 Application instructions for 2014-15 NIH Training Grant Traineeship Trainees are selected by the Training in a trainer's lab. Trainers: www.genetics.uga.edu/NIH_Training.html · Student must currently

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

    SciTech Connect (OSTI)

    Finch, Charlie T.; Zacharias, Norbert [U.S. Naval Observatory, Washington, DC 20392–5420 (United States); Subasavage, John P. [U.S. Naval Observatory, Flagstaff, AZ 86005–8521 (United States); Henry, Todd J. [RECONS Institute, Chambersburg, PA 17201 (United States); Riedel, Adric R., E-mail: finch@usno.navy.mil [Hunter College, New York, NY 10065 (United States)

    2014-12-01T23:59:59.000Z

    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.

  9. CAIRNS: The Cluster And Infall Region Nearby Survey II. Environmental Dependence of Infrared Mass-to-Light Ratios

    E-Print Network [OSTI]

    K. Rines; M. J. Geller; A. Diaferio; M. J. Kurtz; T. H. Jarrett

    2004-06-11T23:59:59.000Z

    CAIRNS (Cluster And Infall Region Nearby Survey) is a spectroscopic survey of the infall regions surrounding nine nearby rich clusters of galaxies. In Paper I, we used redshifts within $\\sim 10\\Mpc$ of the centers of the clusters to determine the mass profiles of the clusters based on the phase space distribution of the galaxies. Here, we use 2MASS photometry and an additional \

  10. NREL: Concentrating Solar Power Research - TroughNet Home Page

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Saleshttp://www.fnal.gov/directorate/nalcal/nalcal02_07_05_files/nalcal.gifNREL NRELChemical andWhatTechnology Basics

  11. FAB Support Page

    E-Print Network [OSTI]

    Functional Analysis Basics (FAB) Seminar Support Page Fall 2014: Meets TBA. Suggestions for FAB ... Hours: by appointment. Back to Carl Cowen's Home Page

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

    SciTech Connect (OSTI)

    Dugger, Leanna; Profumo, Stefano [Department of Astronomy and Department of Physics, University of California Berkeley, 601 Campbell Hall, Berkeley, CA (United States); Jeltema, Tesla E., E-mail: greentee01@gmail.com, E-mail: tesla@ucolick.org, E-mail: profumo@scipp.ucsc.edu [UCO/Lick Observatories, 1156 High St., Santa Cruz, CA 95064 (United States)

    2010-12-01T23:59:59.000Z

    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.

  13. Radio emission of nearby clusters of galaxies at 102. 5 MHz

    SciTech Connect (OSTI)

    Gubanov, A.G.; Dagkesamanskii, R.D.; Rudenko, V.A.

    1980-09-01T23:59:59.000Z

    Observations of 24 nearby Abell galaxy clusters with the Lebedev aperture-synthesis antenna array at 102.5 MHz indicate that the radio luminosity of a cluster increases with its richness class R. For clusters with R> or =1 the luminosity function conforms to a power law with exponent -0.85 in the range 3 x 10/sup 24/< or =L< or =3 x 10/sup 26/ W/Hz.

  14. Identification of four RXTE Slew Survey sources with nearby luminous active galactic nuclei

    E-Print Network [OSTI]

    M. Revnivtsev; S. Sazonov; E. Churazov; S. Trudolyubov

    2005-11-17T23:59:59.000Z

    Based on RXTE scans and observations with the SWIFT/XRT telescope and INTEGRAL observatory, we report the identification of four X-ray sources discovered during the RXTE Slew Survey of the |b|>10deg sky with nearby (z ~ 0.017-0.098) luminous (log L_2-10keV ~ 42.7-44 erg/s) active galactic nuclei. Two of the objects exhibit heavily intrinsically absorbed X-ray spectra (NHL~10^23 cm^-2).

  15. Oxygen Abundances in Nearby Stars. Clues to the formation and evolution of the Galactic disk

    E-Print Network [OSTI]

    I. Ramirez; C. Allende Prieto; D. L. Lambert

    2007-01-12T23:59:59.000Z

    The abundances of iron and oxygen are homogeneously determined in a sample of 523 nearby (d-0.3, we find no obvious indication of a sudden decrease (i.e., a 'knee') in the [O/Fe] vs. [Fe/H] pattern of thick-disk stars that would connect the thick and thin disk trends at a high metallicity. We conclude that Type Ia supernovae (SN Ia) did not contribute significantly to the chemical enrichment of the thick disk. [Abridged

  16. 4/20/12 9:52 PMPittsburgh Magazine | A Man and His Mission: Dr. Jim Withers Page 1 of 7http://www.pittsburghmagazine.com/core/pagetools.php?pageid=13286&...Jim-Withers%2Findex.php%3Fcparticle%3D3%26siarticle%3D2&mode=print

    E-Print Network [OSTI]

    Goldman, Steven A.

    ://www.pittsburghmagazine.com/core/pagetools.php?pageid=13286&...Jim-Withers%2Findex.php%3Fcparticle%3D3%26siarticle%3D2&mode=print Send to printer Close window://www.pittsburghmagazine.com/core/pagetools.php?pageid=13286&...Jim-Withers%2Findex.php%3Fcparticle%3D3%26siarticle%3D2&mode=print 54, who helped him build

  17. NEARBY PLANETARY SYSTEMS AS LENSES DURING PREDICTED CLOSE PASSAGES TO BACKGROUND STARS

    SciTech Connect (OSTI)

    Di Stefano, Rosanne; Matthews, James [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Lepine, Sebastien [Department of Astrophysics, Division of Physical Sciences, American Museum of Natural History, Central Park West at 79th Street, New York, NY 10024 (United States)

    2013-07-10T23:59:59.000Z

    The Einstein rings and proper motions of nearby stars tend to be large. Thus, every year some foreground stars within a few hundred parsecs of Earth induce gravitational lensing events in background stars. In some of these cases, the events may exhibit evidence of planets orbiting the nearby star. In fact, planets can even be discovered during relatively distant passages. Here, we study the lensing signatures associated with planets orbiting nearby high-proper-motion stars. We find the following. (1) Wide-orbit planets can be detected for all distances of closest approach between the foreground and background stars, potentially producing independent events long before and/or after the closest approach. (2) Close-orbit planets can be detected for intermediate distances of closest approach, producing quasiperiodic signatures that may occur days or weeks before and after the stellar-lens event. (3) Planets in the so-called zone for resonant lensing can significantly increase the magnification when the distance of closest approach is small, making the stellar-lens event easier to detect, while simultaneously providing evidence for planets. Because approaches close enough to allow planets to be detected can be predicted, we can plan observing strategies to take advantage of the theoretical framework built in this paper, which describes the sequence of expected effects in terms of a sequence of detection regimes.

  18. The Influence of Galactic Outflows on the Formation of Nearby Dwarf Galaxies

    E-Print Network [OSTI]

    Evan Scannapieco; Andrea Ferrara; Tom Broadhurst

    2000-04-20T23:59:59.000Z

    We show that the gas in growing density perturbations is vulnerable to the influence of winds outflowing from nearby collapsed galaxies that have already formed stars. This suggests that the formation of nearby galaxies with masses less than 10^9 solar masses is likely to be suppressed, irrespective of the details of galaxy formation. An impinging wind may shock heat the gas of a nearby perturbation to above the virial temperature, thereby mechanically evaporating the gas, or the baryons may be stripped from the perturbation entirely if they are accelerated to above the escape velocity. We show that baryonic stripping is the most effective of these two processes, because shock-heated clouds that are too large to be stripped are able to radiatively cool within a sound-crossing time, limiting evaporation. The intergalactic medium temperatures and star-formation rates required for outflows to have a significant influence on the formation of low-mass galaxies are consistent with current observations, but may soon be examined directly via associated distortions in the cosmic microwave background, and with near-infrared observations from the Next Generation Space Telescope, which may detect the supernovae from early-forming stars.

  19. The Oxygen Abundance of Nearby Galaxies from Sloan Digital Sky Survey Spectra

    E-Print Network [OSTI]

    L. S. Pilyugin; T. X. Thuan

    2007-07-19T23:59:59.000Z

    We have derived the oxygen abundance for a sample of nearby galaxies in the Data Release 5 of the Sloan Digital Sky Survey (SDSS) which possess at least two independent spectra of one or several HII regions with a detected [OIII]4363 auroral line. Since, for nearby galaxies, the [OII]3727 nebular line is out of the observed wavelength range, we propose a method to derive (O/H)_ff abundances using the classic Te method coupled with the ff relation. (O/H)_7325 abundances have also been determined, based on the [OII]7320,7330 line intensities, and using a small modification of the standard Te method. The (O/H)_ff and (O/H)_7325 abundances have been derived with both the one- and two-dimensional t_2 - t_3 relations. It was found that the (O/H)_ff abundances derived with the parametric two-dimensional t_2 - t_3 relation are most reliable. Oxygen abundances have been determined in 29 nearby galaxies, based on 84 individual abundance determinations in HII regions. Because of our selection methods, the metallicity of our galaxies lies in the narrow range 8.2 oxygen abundances in the disk of the spiral galaxy NGC 4490 is determined for the first time.

  20. FACHBEREICH GERMANY WWW

    E-Print Network [OSTI]

    Kerber, Manfred

    UNIVERSIT ¨ AT DES SAARLANDES FACHBEREICH INFORMATIK D­66041 SAARBR ¨ UCKEN GERMANY WWW: http, Universit¨at Kaiserslautern D­6750 Kaiserslautern, Germany Das wird n¨achstens schon besser gehen, Wenn Ihr

  1. FACHBEREICH GERMANY WWW

    E-Print Network [OSTI]

    Sorge, Volker

    UNIVERSIT ¨ AT DES SAARLANDES FACHBEREICH INFORMATIK D­66041 SAARBR ¨ UCKEN GERMANY WWW: http¨ucken, Germany fkohlhase---sorgeg@cs.uni­sb.de http://jswww.cs.uni­sb.de/f~kohlhase---~sorgeg Abstract Mechanised

  2. FACHBEREICH GERMANY WWW

    E-Print Network [OSTI]

    Kerber, Manfred

    UNIVERSIT ¨ AT DES SAARLANDES FACHBEREICH INFORMATIK D­66041 SAARBR ¨ UCKEN GERMANY WWW: http¨ucken Germany Abstract This report presents the main ideas underlying the\\Omega\\Gamma mkrp

  3. FACHBEREICH GERMANY WWW

    E-Print Network [OSTI]

    Kerber, Manfred

    UNIVERSIT ¨ AT DES SAARLANDES FACHBEREICH INFORMATIK D­66041 SAARBR ¨ UCKEN GERMANY WWW: http¨ucken, Germany, e­mail: kerber@cs.uni­sb.de. This work was supported by the Deutsche Forschungsgemeinschaft, SFB

  4. FACHBEREICH GERMANY WWW

    E-Print Network [OSTI]

    Kerber, Manfred

    UNIVERSIT ¨ AT DES SAARLANDES FACHBEREICH INFORMATIK D­66041 SAARBR ¨ UCKEN GERMANY WWW: http¨org H. Siekmann iii Universit¨at des Saarlandes Im Stadtwald D­66041 Saarbr¨ucken Germany Abstract

  5. FACHBEREICH GERMANY WWW

    E-Print Network [OSTI]

    Kerber, Manfred

    UNIVERSIT ¨ AT DES SAARLANDES FACHBEREICH INFORMATIK D­66041 SAARBR ¨ UCKEN GERMANY WWW: http Saarlandes Im Stadtwald, W­6600 Saarbr¨ucken 11, Germany fhuang---kerber---kohlhaseg@cs.uni­sb.de Abstract

  6. FACHBEREICH GERMANY WWW

    E-Print Network [OSTI]

    Kerber, Manfred

    UNIVERSIT ¨ AT DES SAARLANDES FACHBEREICH INFORMATIK D­66041 SAARBR ¨ UCKEN GERMANY WWW: http Saarlandes D­66041 Saarbr¨ucken, Germany e­mail: kerber@cs.uni­sb.de---melis@cs.uni­sb.de Begriffe ohne

  7. FACHBEREICH GERMANY WWW

    E-Print Network [OSTI]

    Kerber, Manfred

    UNIVERSIT ¨ AT DES SAARLANDES FACHBEREICH INFORMATIK D­66041 SAARBR ¨ UCKEN GERMANY WWW: http Informatik, Universit¨at des Saarlandes D­66041 Saarbr¨ucken, Germany Abstract This contribution presents

  8. FACHBEREICH GERMANY WWW

    E-Print Network [OSTI]

    Kerber, Manfred

    UNIVERSIT ¨ AT DES SAARLANDES FACHBEREICH INFORMATIK D­66041 SAARBR ¨ UCKEN GERMANY WWW: http@cs.uni­sb.de Fachbereich Informatik, Universit¨at des Saarlandes, 6600 Saarbr¨ucken, Germany Abstract: We transform a user

  9. FACHBEREICH GERMANY WWW

    E-Print Network [OSTI]

    Kerber, Manfred

    UNIVERSIT ¨ AT DES SAARLANDES FACHBEREICH INFORMATIK D­66041 SAARBR ¨ UCKEN GERMANY WWW: http¨at des Saarlandes D­66041 Saarbr¨ucken Germany fhuang---kerber---lassaadg@cs.uni­sb.de Abstract

  10. FACHBEREICH GERMANY WWW

    E-Print Network [OSTI]

    Kerber, Manfred

    UNIVERSIT ¨ AT DES SAARLANDES FACHBEREICH INFORMATIK D­66041 SAARBR ¨ UCKEN GERMANY WWW: http Universit¨at des Saarlandes D­66041 Saarbr¨ucken Germany fhuang---kerber---lassaadg@cs.uni­sb.de Abstract

  11. FACHBEREICH GERMANY WWW

    E-Print Network [OSTI]

    Kerber, Manfred

    UNIVERSIT ¨ AT DES SAARLANDES FACHBEREICH INFORMATIK D­66041 SAARBR ¨ UCKEN GERMANY WWW: http Fachbereich Informatik, Universit¨at des Saarlandes Im Stadtwald 15, 66041 Saarbr¨ucken, Germany e

  12. FACHBEREICH GERMANY WWW

    E-Print Network [OSTI]

    Kerber, Manfred

    UNIVERSIT ¨ AT DES SAARLANDES FACHBEREICH INFORMATIK D­66041 SAARBR ¨ UCKEN GERMANY WWW: http Fachbereich Informatik Universit¨at des Saarlandes Postfach 151150 D­66041 Saarbr¨ucken Germany fhuang

  13. FACHBEREICH GERMANY WWW

    E-Print Network [OSTI]

    Kerber, Manfred

    UNIVERSIT ¨ AT DES SAARLANDES FACHBEREICH INFORMATIK D­66041 SAARBR ¨ UCKEN GERMANY WWW: http Saarbr¨ucken, Germany fhuang,kerber,kohlhase,nesmith,richtsg@cs.uni­sb.de The discussion

  14. FACHBEREICH GERMANY WWW

    E-Print Network [OSTI]

    Kerber, Manfred

    UNIVERSIT ¨ AT DES SAARLANDES FACHBEREICH INFORMATIK D­66041 SAARBR ¨ UCKEN GERMANY WWW: http¨ucken, Germany +49­681­302­f4628j4627g fkerber---kohlhaseg@cs.uni­sb.de Abstract Even though it is not very often

  15. FACHBEREICH GERMANY WWW

    E-Print Network [OSTI]

    Kerber, Manfred

    UNIVERSIT ¨ AT DES SAARLANDES FACHBEREICH INFORMATIK D­66041 SAARBR ¨ UCKEN GERMANY WWW: http Im Stadtwald 15, D­66041 Saarbr¨ucken, Germany e­mail: kerber@cs.uni­sb.de Tel.: (+49) 681

  16. FACHBEREICH GERMANY WWW

    E-Print Network [OSTI]

    Kerber, Manfred

    UNIVERSIT ¨ AT DES SAARLANDES FACHBEREICH INFORMATIK D­66041 SAARBR ¨ UCKEN GERMANY WWW: http Manfred Kerber Fachbereich Informatik, Universit¨at des Saarlandes D­6600 Saarbr¨ucken, Germany kerber

  17. FACHBEREICH GERMANY WWW

    E-Print Network [OSTI]

    Kerber, Manfred

    UNIVERSIT ¨ AT DES SAARLANDES FACHBEREICH INFORMATIK D­66041 SAARBR ¨ UCKEN GERMANY WWW: http­66041 Saarbr¨ucken, Germany fhuang---kerber---richts---acsehng@cs.uni­sb.de #12; Abstract In this report

  18. FACHBEREICH GERMANY WWW

    E-Print Network [OSTI]

    Kerber, Manfred

    UNIVERSIT ¨ AT DES SAARLANDES FACHBEREICH INFORMATIK D­66041 SAARBR ¨ UCKEN GERMANY WWW: http Stadtwald 15, D­66041 Saarbr¨ucken, Germany e­mail: kerber@cs.uni­sb.de Tel.: (+49) 681­302­4628 March 17

  19. Nuclear Energy Page 570Page 570

    E-Print Network [OSTI]

    Nuclear Energy Page 570Page 570 #12;Energy Supply and Conservation/ Nuclear Energy FY 2007;Energy Supply and Conservation/Nuclear Energy/ Overview FY 2007 Congressional Budget Energy Supply and Conservation Office of Nuclear Energy, Science and Technology Overview Appropriation Summary by Program

  20. Nearby Outdoor Environmental Support of Older Adults' Yard Activities, Neighborhood Walking and Independent Living in the Community

    E-Print Network [OSTI]

    Wang, Zhe

    2011-02-22T23:59:59.000Z

    to remain healthy and gives them the ability to access daily-life services, and thus extend their independent years at home. Nearby outdoor environments on residential sites and in the neighborhoods may influence older adults' independent living through...

  1. Page | 1 www.hrs.colostate.edu Human Resource Services

    E-Print Network [OSTI]

    Introduce staff/coworkers Introduce primary constituents/clients/customers Tour workspace, departmentID and email PC setup Keys Specialized equipment issued Long distance telephone access setup Voicemail

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

    National Nuclear Security Administration (NNSA)

    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 Clark...

  3. www.leuphana.de www.leuphana.de/td-training

    E-Print Network [OSTI]

    Wagner, Stephan

    »www.leuphana.de »www.leuphana.de/td-training TD SUMMER SCHOOL 2014 Transdisciplinary Research Scharnhorststraße 1, C4.008, 21335 Lüneburg, Germany Fon +49.4131.677-2295 or -2028, td_training@leuphana.de Venue » www.leuphana.de/td-training OVERVIEW Transdisciplinary Research at the Science | Society Interface

  4. World Wide Web( WWW ) Greenberg Web

    E-Print Network [OSTI]

    Shirai, Kiyoaki

    WWW 1 World Wide Web( WWW ) WWW Web Web Greenberg Web 30% [1] Web WWW Web WWW [2] [3] WWW 2 2.1 WWW Web 1 1: · 1 · 1 #12;· Web Web 2: 2 2 Web 2.2 Web Web URL URL .html / Yahoo http://headlines.yahoo.co.jp/hl?a=2 0011205-00000101-yom-soci URL onmouseover on- mouseout JavaScript 2.1 2.3 URL URL 1. Web HTML 2. 1

  5. 1. CONTRACT ID CODE PAGE OF PAGES

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office of ScienceandMesa del(ANL-IN-03-032) -Less is more:culturingProtonAPRIL/MAY 2013

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

    SciTech Connect (OSTI)

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

    2010-05-03T23:59:59.000Z

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

  7. Timing the Nearby Isolated Neutron Star RX J1856.5-3754

    E-Print Network [OSTI]

    Van Kerkwijk, M H

    2007-01-01T23:59:59.000Z

    RX J1856.5-3754 is the X-ray brightest among the nearby isolated neutron stars. Its X-ray spectrum is thermal, and is reproduced remarkably well by a black-body, but its interpretation has remained puzzling. One reason is that the source did not exhibit pulsations, and hence a magnetic field strength--vital input to atmosphere models--could not be estimated. Recently, however, very weak pulsations were discovered. Here, we analyze these in detail, using all available data from the XMM-Newton and Chandra X-ray observatories. From frequency measurements, we set a 2-sigma upper limit to the frequency derivative of \\dot\

  8. Discovery of a large dust disk around the nearby star AU Microscopium

    E-Print Network [OSTI]

    Paul Kalas; Michael C. Liu; Brenda C. Matthews

    2004-03-05T23:59:59.000Z

    We present the discovery of a circumstellar dust disk surrounding AU Microscopium (AU Mic, GJ 803, HD 197481). This young M star at 10 parsec has the same age and origin as beta Pictoris, another nearby star surrounded by a dust disk. The AU Mic disk is detected between 50 AU and 210 AU radius, a region where dust lifetimes exceed the present stellar age. Thus, AU Mic is the nearest star where we directly observe the solid material required for planet formation. Since 85% of stars are M-type, the AU Mic disk provides new clues on how the majority of planetary systems might form and evolve.

  9. Courtesy of Sandro Ierovante Distributed by WWW.LENSINC.NET

    E-Print Network [OSTI]

    Kleinfeld, David

    Courtesy of Sandro Ierovante Distributed by WWW.LENSINC.NET #12;Distributed by WWW.LENSINC.NET #12;Distributed by WWW.LENSINC.NET #12;Distributed by WWW.LENSINC.NET #12;Distributed by WWW.LENSINC.NET #12;Distributed by WWW.LENSINC.NET #12;Distributed by WWW.LENSINC.NET #12;Distributed by WWW.LENSINC.NET #12

  10. PAGE Cover: Top Photo

    Energy Savers [EERE]

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directed offOCHCO2:Introduction toManagementOPAM PolicyOfEnergyOutreach toOverviewOverview P - . . -PAGE

  11. Page 1 of 1

    Energy Savers [EERE]

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directed offOCHCO2:Introduction toManagementOPAM5 Accretion-of-DutiesPROPERTY3-0127Paducah3 Theof Page 2 This

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    Energy Savers [EERE]

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directed offOCHCO2:Introduction toManagementOPAM5 Accretion-of-DutiesPROPERTY3-0127Paducah3 Theof Page 2

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    Energy Savers [EERE]

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directed offOCHCO2:Introduction toManagementOPAM5 Accretion-of-DutiesPROPERTY3-0127Paducah3 Theof Page 2This

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    Energy Savers [EERE]

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directed offOCHCO2:Introduction toManagementOPAM5 Accretion-of-DutiesPROPERTY3-0127Paducah3 Theof Page

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    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742EnergyOn April 23, 2014, an OHA Administrative Judge issuedEnergy1of Page This finalof Page 2

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742EnergyOn April 23, 2014, an OHA Administrative Judge issuedEnergy1of Page This finalof Page

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page onYouTube YouTube Note: Since the.pdfBreaking ofOilNEWResponse(Expired) |CERCLA Process & Public Involvement This is a

  18. Page | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov YouKizildere I Geothermal Pwer PlantMunhall,Missouri:EnergyOssian, New York:Ozark,Pacific GasPage" Showing 177

  19. Active Networks as a tool to integrate DGActive Networks as a tool to integrate DG www.econ.no

    E-Print Network [OSTI]

    Page 1 Active Networks as a tool to integrate DGActive Networks as a tool to integrate DG www.econ.no Active networks as a tool toActive networks as a tool to integrate large amounts ofintegrate large GaardestrupGaardestrup, C.,, C., TechwiseTechwise #12;Page 2 Active Networks as a tool to integrate DGActive

  20. HI observations of nearby galaxies I. The first list of the Karachentsev catalog

    E-Print Network [OSTI]

    W. K. Huchtmeier; I. D. Karachentsev; V. E. Karachentseva; M. Ehle

    1999-11-18T23:59:59.000Z

    We present HI observations of the galaxies in the first list of the Karachentsev catalog of previously unknown nearby dwarf galaxies (Karachentseva & Karachentsev 1998). This survey covers all known nearby galaxy groups within the Local Volume (i.e. within 10 Mpc) and their environment, that is about 25% of the total sky. A total of 257 galaxies have been observed with a detection rate of 60%. We searched a frequency band corresponding to heliocentric radial velocities from -470 km/s to about +4000 km/s. Non-detections are either due to limited coverage in radial velocity, confusion with Local HI (mainly in the velocity range -140 km/s to +20 km/s, or lack of sensitivity for very weak emission. 25% of the detected galaxies are located within the Local Volume. Those galaxies are dwarf galaxies judged by their optical linear diameter (1.4 +/- 0.2 kpc on the average), their mean total HI mass (4.6 E7 solar masses), and their observed linewidths (39 km/s).

  1. HERSCHEL FAR-INFRARED AND SUBMILLIMETER PHOTOMETRY FOR THE KINGFISH SAMPLE OF NEARBY GALAXIES

    SciTech Connect (OSTI)

    Dale, D. A. [Department of Physics and Astronomy, University of Wyoming, Laramie, WY 82071 (United States); Aniano, G.; Draine, B. T. [Department of Astrophysical Sciences, Princeton University, Princeton, NJ 08544 (United States); Engelbracht, C. W.; Hinz, J. L.; Montiel, E. J. [Steward Observatory, University of Arizona, Tucson, AZ 85721 (United States); Krause, O.; Groves, B. A. [Max-Planck-Institut fuer Astronomie, Koenigstuhl 17, D-69117 Heidelberg (Germany); Roussel, H. [Institut d'Astrophysique de Paris, UMR7095 CNRS, Universite Pierre and Marie Curie, 98 bis Boulevard Arago, 75014 Paris (France); Appleton, P. N. [NASA Herschel Science Center, IPAC, California Institute of Technology, Pasadena, CA 91125 (United States); Armus, L.; Beirao, P. [Spitzer Science Center, California Institute of Technology, MC 314-6, Pasadena, CA 91125 (United States); Bolatto, A. D. [Department of Astronomy, University of Maryland, College Park, MD 20742 (United States); Brandl, B. R. [Leiden Observatory, Leiden University, P.O. Box 9513, 2300 RA Leiden (Netherlands); Calzetti, D.; Crocker, A. F. [Department of Astronomy, University of Massachusetts, Amherst, MA 01003 (United States); Croxall, K. V. [Department of Physics and Astronomy, University of Toledo, Toledo, OH 43606 (United States); Galametz, M. [Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA (United Kingdom); Gordon, K. D. [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States); Hao, C.-N., E-mail: ddale@uwyo.edu [Tianjin Astrophysics Center, Tianjin Normal University, Tianjin 300387 (China); and others

    2012-01-20T23:59:59.000Z

    New far-infrared and submillimeter photometry from the Herschel Space Observatory is presented for 61 nearby galaxies from the Key Insights on Nearby Galaxies: A Far-Infrared Survey with Herschel (KINGFISH) sample. The spatially integrated fluxes are largely consistent with expectations based on Spitzer far-infrared photometry and extrapolations to longer wavelengths using popular dust emission models. Dwarf irregular galaxies are notable exceptions, as already noted by other authors, as their 500 {mu}m emission shows evidence for a submillimeter excess. In addition, the fraction of dust heating attributed to intense radiation fields associated with photodissociation regions is found to be (21 {+-} 4)% larger when Herschel data are included in the analysis. Dust masses obtained from the dust emission models of Draine and Li are found to be on average nearly a factor of two higher than those based on single-temperature modified blackbodies, as single blackbody curves do not capture the full range of dust temperatures inherent to any galaxy. The discrepancy is largest for galaxies exhibiting the coolest far-infrared colors.

  2. CAIRNS: The Cluster And Infall Region Nearby Survey I. Redshifts and Mass Profiles

    E-Print Network [OSTI]

    K. Rines; M. J. Geller; M. J. Kurtz; A. Diaferio

    2003-06-25T23:59:59.000Z

    The CAIRNS (Cluster And Infall Region Nearby Survey) project is a spectroscopic survey of the infall regions surrounding eight nearby, rich, X-ray luminous clusters of galaxies. We collect 15665 redshifts (3471 new or remeasured) within \\sim 5-10 Mpc of the centers of the clusters, making it the largest study of the infall regions of clusters. We determine cluster membership and the mass profiles of the clusters based on the phase space distribution of the galaxies. All of the clusters display decreasing velocity dispersion profiles. The mass profiles are fit well by functional forms based on numerical simulations but exclude an isothermal sphere. Specifically, NFW and Hernquist models provide good descriptions of cluster mass profiles to their turnaround radii. Our sample shows that the predicted infall pattern is ubiquitous in rich, X-ray luminous clusters over a large mass range. The caustic mass estimates are in excellent agreement with independent X-ray estimates at small radii and with virial estimates at intermediate radii. The mean ratio of the caustic mass to the X-ray mass is 1.03\\pm0.11 and the mean ratio of the caustic mass to the virial mass (when corrected for the surface pressure term) is 0.93\\pm0.07. We further demonstrate that the caustic technique provides reasonable mass estimates even in merging clusters.

  3. The resolved star-formation relation in nearby active galactic nuclei

    E-Print Network [OSTI]

    Casasola, Viviana; Combes, Francoise; Garcia-Burillo, Santiago

    2015-01-01T23:59:59.000Z

    We present an analysis of the relation between star formation rate (SFR) surface density (sigmasfr) and mass surface density of molecular gas (sigmahtwo), commonly referred to as the Kennicutt-Schmidt (K-S) relation, at its intrinsic spatial scale, i.e. the size of giant molecular clouds (10-150 pc), in the central, high-density regions of four nearby low-luminosity active galactic nuclei (AGN). We used interferometric IRAM CO(1-0) and CO(2-1), and SMA CO(3-2) emission line maps to derive sigmahtwo and HST-Halpha images to estimate sigmasfr. Each galaxy is characterized by a distinct molecular SF relation at spatial scales between 20 to 200 pc. The K-S relations can be sub-linear, but also super-linear, with slopes ranging from 0.5 to 1.3. Depletion times range from 1 and 2Gyr, compatible with results for nearby normal galaxies. These findings are valid independently of which transition, CO(1-0), CO(2-1), or CO(3-2), is used to derive sigmahtwo. Because of star-formation feedback, life-time of clouds, turbule...

  4. On The Linearity of The Black Hole - Bulge Mass Relation in Active and in Nearby Galaxies

    E-Print Network [OSTI]

    Ari Laor

    2001-01-23T23:59:59.000Z

    Analysis of PG quasar observations suggests a nonlinear relation between the black hole mass, M_BH, and the bulge mass, M_bulge, although a linear relation, as proposed for nearby galaxies, cannot be ruled out. New M_BH values for nearby galaxies from Gebhardt et al., and L_bulge measurements for Seyfert 1 galaxies from Virani et al., are used here to obtain a more accurate value for the slope of the M_BH-M_bulge relation. The combined sample of 40 active and non-active galaxies suggests a significantly nonlinear relation, M_BH\\propto M_bulge^{1.53\\pm 0.14}. Further support for a nonlinear relation is provided by the slope of the M_BH-stellar velocity dispersion relation found recently, and by the low M_BH found in late type spiral galaxies. The mean M_BH/M_bulge ratio is therefore not a universal constant, but rather drops from ~0.5% in bright (M_V ~ -22) ellipticals, to ~0.05% in low luminosity (M_V ~ -18) bulges. Hubble Space Telescope determinations of M_BH in late type spirals, and of the bulge magnitude in narrow line Seyfert 1 galaxies (both predicted to have low M_BH), can further test the validity of the nonlinear M_BH-M_bulge relation.

  5. 26/03/2009 12:58NO SUCH THING AS ARSEHOLE BEES, SAY EXPERTS -The Daily Mash Page 1 of 2http://www.thedailymash.co.uk/animals/animals-headlines/no-such-thing-as-arsehole-bees%2c-say-experts-200903241660/

    E-Print Network [OSTI]

    Gardner, Andy

    SATAN MAKES ROOM FOR PARENTS WHO COMPLAINED ABOUT DISABLED TV ADHOLE2 Your email address Enter search HEADLINES Via RSS: Via Twitter: ADHOLE1 MASH TV: MASH TV: SEARCH THE DAILY MASH Go TOP TEN THIS MONTH PUT term... Bees and Bee Keeping Bees, Bee Keeping and Bee Products Know More about It! www

  6. FACHBEREICH GERMANY WWW

    E-Print Network [OSTI]

    Kerber, Manfred

    UNIVERSIT ¨ AT DES SAARLANDES FACHBEREICH INFORMATIK D­66041 SAARBR ¨ UCKEN GERMANY WWW: http--242, Springer Verlag, Berlin, Germany, LNAI 397, 1989. #12; Some Aspects of Analogy in Mathematical Reasoning Manfred Kerber Fachbereich Informatik, Universit¨at Kaiserslautern D­6750 Kaiserslautern, West Germany

  7. FACHBEREICH GERMANY WWW

    E-Print Network [OSTI]

    Kerber, Manfred

    UNIVERSIT ¨ AT DES SAARLANDES FACHBEREICH INFORMATIK D­66041 SAARBR ¨ UCKEN GERMANY WWW: http by Tactics Manfred Kerber Fachbereich Informatik Universit¨at des Saarlandes D­66041 Saarbr¨ucken, Germany e­mail: kerber@cs.uni­sb.de Axel Pr¨acklein Neue Fahrstr. 13 D­75181 Pforzheim, Germany e­mail: prckln

  8. FACHBEREICH GERMANY WWW

    E-Print Network [OSTI]

    Kerber, Manfred

    UNIVERSIT ¨ AT DES SAARLANDES FACHBEREICH INFORMATIK D­66041 SAARBR ¨ UCKEN GERMANY WWW: http­Fachgruppe Deduktionssysteme'', Darm­ stadt, Germany, p.13, 1994. #12; Formalizing Mathematics with Dependent Sorts Manfred¨ucken, Germany +49­681­302­f4628j4627g fkerber---kohlhaseg@cs.uni­sb.de Abstract While axiomatic set theory

  9. FACHBEREICH GERMANY WWW

    E-Print Network [OSTI]

    Kerber, Manfred

    UNIVERSIT ¨ AT DES SAARLANDES FACHBEREICH INFORMATIK D­66041 SAARBR ¨ UCKEN GERMANY WWW: http: In J¨urgen Kunze, Herbert Stoyan, eds., Workshop­ Proceedings der KI­94, Saarb¨ucken, Germany, p.279¨orn Richts Fachbereich Informatik, Universit¨at des Saarlandes Postfach 151150, D­66041 Saarbr¨ucken, Germany

  10. FACHBEREICH GERMANY WWW

    E-Print Network [OSTI]

    Kerber, Manfred

    UNIVERSIT ¨ AT DES SAARLANDES FACHBEREICH INFORMATIK D­66041 SAARBR ¨ UCKEN GERMANY WWW: http as: In J¨urgen Kunze, Herbert Stoyan, eds., Workshop­ Proceedings der KI­94, Saarb¨ucken, Germany, p¨ucken, Germany fhuang---kerber---richts---acsehng@cs.uni­sb.de Methods are the basic units which make up proof

  11. FACHBEREICH GERMANY WWW

    E-Print Network [OSTI]

    Kerber, Manfred

    UNIVERSIT ¨ AT DES SAARLANDES FACHBEREICH INFORMATIK D­66041 SAARBR ¨ UCKEN GERMANY WWW: http--792, Nancy, France, 1994. Springer­Verlag, Berlin, Germany. LNAI 814. #12; \\Omega\\Gamma mkrp: A Proof¨org Siekmann Fachbereich Informatik, Universit¨at des Saarlandes Postfach 1150, 66041 Saarbr¨ucken, Germany

  12. FACHBEREICH GERMANY WWW

    E-Print Network [OSTI]

    Kerber, Manfred

    UNIVERSIT ¨ AT DES SAARLANDES FACHBEREICH INFORMATIK D­66041 SAARBR ¨ UCKEN GERMANY WWW: http­19, Fachbereich Informatik, Uni­ versit¨at Kaiserslautern, Kaiserslautern, Germany #12; How to Prove Higher Order Kaiserslautern, West Germany UUCP: kerber@informatik.uni­kl.de Abstract In this paper we are interested in using

  13. FACHBEREICH GERMANY WWW

    E-Print Network [OSTI]

    Kerber, Manfred

    UNIVERSIT ¨ AT DES SAARLANDES FACHBEREICH INFORMATIK D­66041 SAARBR ¨ UCKEN GERMANY WWW: http Fachbereich Informatik Universit¨at des Saarlandes 6600 Saarbr¨ucken, Germany fkerber---melisg@cs.uni­sb.de J¨org H. Siekmann DFKI German Research Center for AI 6600 Saarbr¨ucken, Germany siekmann

  14. FACHBEREICH GERMANY WWW

    E-Print Network [OSTI]

    Kerber, Manfred

    UNIVERSIT ¨ AT DES SAARLANDES FACHBEREICH INFORMATIK D­66041 SAARBR ¨ UCKEN GERMANY WWW: http 379--390, Saarbr¨ucken, Germany, 1994. Springer Verlag, Berlin, Germany, LNAI 861. #12; Adapting Fachbereich Informatik, Universit¨at des Saarlandes 66041 Saarbr¨ucken, Germany fhuang

  15. Page1.PDF

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    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level:Energy: Grid Integration Redefining What's Possible for RenewableSpeedingBiomassPPPO Website DirectoryCommunityFuture Use

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    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level:Energy: Grid Integration Redefining What's Possible for RenewableSpeedingBiomassPPPO Website DirectoryCommunityFuture Use

  17. Page1.PDF

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    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level:Energy: Grid Integration Redefining What's Possible for RenewableSpeedingBiomassPPPO Website DirectoryCommunityFuture Use

  18. 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...

  19. RMOTC - Articles - Page 2

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

    Geothermal Energy Holds Strong Presence at Renewable Energy World Conference Geothermal Energy Weekly, March 5, 2010 (Page 4) Oil Production Waste Stream: A Source of Electrical...

  20. Carl Cowen's Home Page

    E-Print Network [OSTI]

    Mar 9, 2015 ... How to Get an Academic Job (Basic Skills Workshop) · ICM Korea Satellite: ... Support Page for Functional Analysis Basics (FAB) Seminar ...

  1. PAGE Cover: Top Photo

    Energy Savers [EERE]

    includes a rooftop photovoltaic system, daylighting, natural ventilation, and a next-generation, energy efficient data center. 14 PAGE ORGANIZATIONAL RESPONSIBILITY AND...

  2. ARM - Front Page

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006Datastreamstwrcam40m DocumentationJanuary 9, 2009 [Events, Feature StoriesgovCampaignsSurfacegovFront Page

  3. Page 1 of2

    Energy Savers [EERE]

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directed offOCHCO2:Introduction toManagementOPAM5 Accretion-of-DutiesPROPERTY3-0127Paducah3 Theof Pageof2 The

  4. Page 1 of 2

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    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742EnergyOn April 23, 2014, an OHA Administrative Judge issuedEnergy1of Page This finalof

  5. Page 1 of 2

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    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742EnergyOn April 23, 2014, an OHA Administrative Judge issuedEnergy1of Page This finalofa new

  6. Page 1 of 2

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    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742EnergyOn April 23, 2014, an OHA Administrative Judge issuedEnergy1of Page This finalofa

  7. Page 1 of 2

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    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742EnergyOn April 23, 2014, an OHA Administrative Judge issuedEnergy1of Page This

  8. Page 1 of 2

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    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742EnergyOn April 23, 2014, an OHA Administrative Judge issuedEnergy1of Page ThisFor additional

  9. Page 1 of 2

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    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742EnergyOn April 23, 2014, an OHA Administrative Judge issuedEnergy1of Page ThisFor

  10. Page 1 of2

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742EnergyOn April 23, 2014, an OHA Administrative Judge issuedEnergy1of Page ThisForThis

  11. Page 1 of2

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    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742EnergyOn April 23, 2014, an OHA Administrative Judge issuedEnergy1of Page

  12. NewPage Corporation

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

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

  13. Page 1 of

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    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level:Energy: Grid Integration Redefining What's Possible for RenewableSpeedingBiomassPPPO Website DirectoryCommunityFuture Use PaducahPage of

  14. Page 11, Links

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    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level:Energy: Grid Integration Redefining What's Possible for RenewableSpeedingBiomassPPPO Website DirectoryCommunityFuture Use PaducahPage of111

  15. Page 8, Benefit Forms

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level:Energy: Grid Integration Redefining What's Possible for RenewableSpeedingBiomassPPPO Website DirectoryCommunityFuture Use PaducahPage5 of8 of

  16. WIPP Home Page Search

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742EnergyOnItemResearch >Internship Program TheSiteEureka AnalyticsLargeHome Page Search Enter

  17. WIPP Home Page header

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742EnergyOnItemResearch >Internship Program TheSiteEureka AnalyticsLargeHome Page Search Enter |

  18. WIPP Stakeholder Information Page

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742EnergyOnItemResearch >Internship Program TheSiteEureka AnalyticsLargeHome Page Directional

  19. Page 6Page 5Page 2 Events and Research News in Engineering and Science Today www.ces.clemson.edu

    E-Print Network [OSTI]

    Duchowski, Andrew T.

    to chart the oceans' basins and to study gravitational anomalies, sea currents, global warming, and tidal distinction of being the first person to receive a Ph.D. in electrical engineering from Clemson. Following chemical researchers in his generation ­ not only in terms of productivity, but also in the quality

  20. www.eia.gov U.S. Energy Information Administration Independent Statistics & Analysis

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov YouKizildere IRaghuraji Agro IndustriesTownDells,1Stocksa. Appliances by Climate6,1996 http://www.eia.doe.govEffects of

  1. A Comparison of Independent Star Formation Diagnostics for a UV-Selected Sample of Nearby Galaxies

    E-Print Network [OSTI]

    Sullivan, M; Chan, B; Cram, L; Ellis, R; Treyer, M A; Hopkins, A; Sullivan, Mark; Mobasher, Bahram; Chan, Ben; Cram, Lawrence; Ellis, Richard; Treyer, Marie; Hopkins, Andrew

    2001-01-01T23:59:59.000Z

    We present results from a decimetric radio survey undertaken with the Very Large Array as part of a longer term goal to inter-compare star formation and dust extinction diagnostics, on a galaxy by galaxy basis, for a representative sample of nearby galaxies. For our survey field, Selected Area 57, star formation rates derived from 1.4GHz luminosities are compared with earlier nebular emission line and ultraviolet (UV) continuum diagnostics. We find broad correlations, over several decades in luminosity, between H-alpha, the UV continuum and 1.4GHz diagnostics. However, the scatter in these relations is found to be larger than observational errors, with offsets between the observed relations and those expected assuming constant star-formation histories and luminosity-independent extinction models. We investigate the physical origin of the observed relations, and conclude the discrepancies between different star-formation diagnostics can only be partly explained by simple models of dust extinction in galaxies. ...

  2. Very-High Energy Gamma-Ray Flux Limits for Nearby Active Galactic Nuclei

    E-Print Network [OSTI]

    T. Herr; W. Hofmann; for the H. E. S. S. Collaboration

    2008-11-18T23:59:59.000Z

    Combining the results of targeted observations, H.E.S.S. has accumulated a large amount of extra-galactic exposure at TeV energies. Due to its large field of view a considerable part of the sky (0.6 sr) has been observed with high sensitivity outside the targeted observation positions. Since this exposure region contains little inherent bias, it is well suited for studies of extra-galactic source populations. Given the correlation between ultra-high energy cosmic rays and nearby extra-galactic objects recently claimed by the Auger collaboration, this unbiased sky sample by H.E.S.S. is of interest since it includes (besides the targeted sources) 63 AGN within 100 Mpc, for which very-high energy gamma-ray flux limits are derived.

  3. Young massive star clusters in nearby galaxies. I. Identification and general properties of cluster systems

    E-Print Network [OSTI]

    Soeren S. Larsen; Tom Richtler

    1999-02-19T23:59:59.000Z

    Using ground-based UBVRI+Halpha CCD photometry we have been carrying out a search for young massive star clusters (YMCs) in a sample consisting of 21 nearby spiral galaxies. We find a large variety concerning the richness of the cluster systems, with some galaxies containing no YMCs at all and others hosting very large numbers of YMCs. Examples of galaxies with poor cluster systems are NGC 300 and NGC 4395, while the richest cluster systems are found in the galaxies NGC 5236, NGC 2997 and NGC 1313. The age distributions of clusters in these galaxies show no obvious peaks, indicating that massive star clusters are formed as an ongoing process rather than in bursts. This is in contrast to what is observed in starbursts and merger galaxies. The radial distributions of clusters follow the Halpha surface brightness. For the galaxies in our sample there is no correlation between the morphological type and the presence of YMCs

  4. THE ACS NEARBY GALAXY SURVEY TREASURY. III. CEPHEIDS IN THE OUTER DISK OF M81

    SciTech Connect (OSTI)

    McCommas, Les P.; Williams, Benjamin F.; Dalcanton, Julianne J.; Davis, Matthew R. [Astronomy Department, University of Washington, Box 351580, Seattle, WA 98195 (United States); Yoachim, Peter [Department of Astronomy and McDonald Observatory, University of Texas, Austin, TX 78712 (United States); Dolphin, Andrew E. [Raytheon Corporation, 870 Winter Street Waltham, MA 02451 (United States)], E-mail: lmccomma@astro.washington.edu, E-mail: jd@astro.washington.edu, E-mail: ben@astro.washington.edu, E-mail: mrdavis@astro.washington.edu, E-mail: yoachim@astro.as.utexas.edu, E-mail: adolphin@ratheon.com

    2009-06-15T23:59:59.000Z

    The ACS Nearby Galaxy Survey Treasury (ANGST) has acquired deep ACS imaging of a field in the outer disk of the large spiral galaxy M81. These data were obtained over a total of 20 Hubble Space Telescope orbits, providing a baseline long enough to reliably identify Cepheid variable stars in the field. Fundamental mode and first overtone types have been distinguished through comparative fits with corresponding Cepheid light curve templates derived from principal component analysis of confirmed Cepheids in the Large Magellanic Cloud (LMC), Small Magellanic Cloud, and Milky Way. A distance modulus of 27.78 {+-} 0.05 {sub r} {+-} 0.14 {sub s} with a corresponding distance of 3.60 {+-} 0.23 Mpc has been calculated from a sample of 11 fundamental mode and two first overtone Cepheids (assuming an LMC distance modulus of {mu}{sub LMC} = 18.41 {+-} 0.10 {sub r} {+-} 0.13 {sub s})

  5. No nearby counterparts to the moving objects in the Hubble Deep Field

    E-Print Network [OSTI]

    Chris Flynn; J. Sommer-Larsen; B. Fuchs; David S. Graff; Samir Salim; .

    1999-12-14T23:59:59.000Z

    Ibata et al (1999) have recently discovered faint, moving objects in the Hubble Deep Field. The quantity, magnitudes and proper motions of these objects are consistent with old white dwarfs making up the Galactic dark halo. We review a number of ground-based proper motion surveys in which nearby dark halo white dwarfs might be present, if they have the colours and absolute magnitudes proposed. No such objects have been found, whereas we argue here that several times more would be expected than in the Hubble Deep Field. We conclude it is unlikely that hydrogen atmosphere white dwarfs make up a significant fraction of the halo dark matter. No limits can be placed yet on helium atmosphere dwarfs from optical searches.

  6. Structure, dynamical impact and origin of magnetic fields in nearby galaxies in the SKA era

    E-Print Network [OSTI]

    Beck, Rainer; Colafrancesco, Sergio; Dettmar, Ralf-Jürgen; Ferričre, Katia; Fletcher, Andrew; Heald, George; Heesen, Volker; Horellou, Cathy; Krause, Marita; Lou, Yu-Qing; Mao, Sui Ann; Paladino, Rosita; Schinnerer, Eva; Sokoloff, Dmitry; Stil, Jeroen; Tabatabaei, Fatemeh

    2015-01-01T23:59:59.000Z

    Magnetic fields are an important ingredient of the interstellar medium (ISM). Besides their importance for star formation, they govern the transport of cosmic rays, relevant to the launch and regulation of galactic outflows and winds, which in turn are pivotal in shaping the structure of halo magnetic fields. Mapping the small-scale structure of interstellar magnetic fields in many nearby galaxies is crucial to understand the interaction between gas and magnetic fields, in particular how gas flows are affected. Elucidation of the magnetic role in, e.g., triggering star formation, forming and stabilising spiral arms, driving outflows, gas heating by reconnection and magnetising the intergalactic medium has the potential to revolutionise our physical picture of the ISM and galaxy evolution in general. Radio polarisation observations in the very nearest galaxies at high frequencies (>= 3 GHz) and with high spatial resolution (<= 5") hold the key here. The galaxy survey with SKA1 that we propose will also be a...

  7. The 60-month all-sky BAT Survey of AGN and the Anisotropy of Nearby AGN

    SciTech Connect (OSTI)

    Ajello, M.; /KIPAC, Menlo Park; Alexander, D.M.; /Durham U.; Greiner, J.; /Garching, Max Planck Inst., MPE; Madejski, G.M.; /KIPAC, Menlo Park; Gehrels, N.; /NASA, Goddard; Burlon, D.; /Garching, Max Planck Inst., MPE

    2012-04-02T23:59:59.000Z

    Surveys above 10 keV represent one of the the best resources to provide an unbiased census of the population of Active Galactic Nuclei (AGN). We present the results of 60 months of observation of the hard X-ray sky with Swift/BAT. In this timeframe, BAT detected (in the 15-55 keV band) 720 sources in an all-sky survey of which 428 are associated with AGN, most of which are nearby. Our sample has negligible incompleteness and statistics a factor of {approx}2 larger over similarly complete sets of AGN. Our sample contains (at least) 15 bona-fide Compton-thick AGN and 3 likely candidates. Compton-thick AGN represent a {approx}5% of AGN samples detected above 15 keV. We use the BAT dataset to refine the determination of the LogN-LogS of AGN which is extremely important, now that NuSTAR prepares for launch, towards assessing the AGN contribution to the cosmic X-ray background. We show that the LogN-LogS of AGN selected above 10 keV is now established to a {approx}10% precision. We derive the luminosity function of Compton-thick AGN and measure a space density of 7.9{sub -2.9}{sup +4.1} x 10{sup -5} Mpc{sup -3} for objects with a de-absorbed luminosity larger than 2 x 10{sup 42} erg s{sup -1}. As the BAT AGN are all mostly local, they allow us to investigate the spatial distribution of AGN in the nearby Universe regardless of absorption. We find concentrations of AGN that coincide spatially with the largest congregations of matter in the local ({le} 85 Mpc) Universe. There is some evidence that the fraction of Seyfert 2 objects is larger than average in the direction of these dense regions.

  8. 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 Côte d'Azur, F-06300 Nice (France); Lennon, Daniel [ESA—European Space Astronomy Centre, Apdo. de Correo 78, E-28691 Villanueva de la Cańada, 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)

    2015-01-01T23:59:59.000Z

    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 IC 10, NGC 185, and NGC 147. 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.

  9. THE NATURE OF STARBURSTS. I. THE STAR FORMATION HISTORIES OF EIGHTEEN NEARBY STARBURST DWARF GALAXIES

    SciTech Connect (OSTI)

    McQuinn, Kristen B. W.; Skillman, Evan D.; Stark, David; Weisz, Daniel [Department of Astronomy, School of Physics and Astronomy, 116 Church Street, S.E., University of Minnesota, Minneapolis, MN 55455 (United States); Cannon, John M. [Department of Physics and Astronomy, Macalester College, 1600 Grand Avenue, Saint Paul, MN 55105 (United States); Dalcanton, Julianne; Williams, Benjamin [Department of Astronomy, Box 351580, University of Washington, Seattle, WA 98195 (United States); Dolphin, Andrew [Raytheon Company, 1151 E. Hermans Road, Tucson, AZ 85706 (United States); Hidalgo-RodrIguez, Sebastian [Instituto de Astrofisica de Canarias, VIa Lactea s/n. E38200, La Laguna, Tenerife, Canary Islands (Spain); Holtzman, Jon, E-mail: kmcquinn@astro.umn.ed [Department of Astronomy, New Mexico State University, Box 30001-Department 4500, 1320 Frenger Street, Las Cruces, NM 88003 (United States)

    2010-09-20T23:59:59.000Z

    We use archival Hubble Space Telescope observations of resolved stellar populations to derive the star formation histories (SFHs) of 18 nearby starburst dwarf galaxies. In this first paper, we present the observations, color-magnitude diagrams (CMDs), and the SFHs of the 18 starburst galaxies, based on a homogeneous approach to the data reduction, differential extinction, and treatment of photometric completeness. We adopt a star formation rate (SFR) threshold normalized to the average SFR of the individual system as a metric for classifying starbursts in SFHs derived from resolved stellar populations. This choice facilitates finding not only the currently bursting galaxies but also 'fossil' bursts increasing the sample size of starburst galaxies in the nearby (D < 8 Mpc) universe. Thirteen of the eighteen galaxies are experiencing ongoing bursts and five galaxies show fossil bursts. From our reconstructed SFHs, it is evident that the elevated SFRs of a burst are sustained for hundreds of Myr with variations on small timescales. A long >100 Myr temporal baseline is thus fundamental to any starburst definition or identification method. The longer lived bursts rule out rapid 'self-quenching' of starbursts on global scales. The bursting galaxies' gas consumption timescales are shorter than the Hubble time for all but one galaxy confirming the short-lived nature of starbursts based on fuel limitations. Additionally, we find that the strength of the H{alpha} emission usually correlates with the CMD-based SFR during the last 4-10 Myr. However, in four cases, the H{alpha} emission is significantly less than what is expected for models of starbursts; the discrepancy is due to the SFR changing on timescales of a few Myr. The inherently short timescale of the H{alpha} emission limits identifying galaxies as starbursts based on the current characteristics which may or may not be representative of the recent SFH of a galaxy.

  10. Page 1 of 4 Postfach 10 10 62 -80084 Mnchen, Germany

    E-Print Network [OSTI]

    Page 1 of 4 Postfach 10 10 62 - 80084 München, Germany Telefon: +49 89 2108-0 Fax: +49 89 2108-1111 Internet: http://www.mpfp.mpg.de Jean-Paul-Straße 12 - 53173 Bonn, Germany Telefon: +49 228 833-0 Fax: +49 themselves in Germany or which should be developed further. The 2014 Max Planck Research Award

  11. Statistics Page 233Sonoma State University 2012-2013 Catalog DEPARTMENT OF MATHEMATICS AND STATISTICS

    E-Print Network [OSTI]

    Ravikumar, B.

    Statistics Page 233Sonoma State University 2012-2013 Catalog STATISTICS DEPARTMENT OF MATHEMATICS AND STATISTICS Darwin Hall 114 phone: (707) 664-2368 fax: (707) 664-3535 www.sonoma.edu/math DEPARTMENT CHAIR Sam Brannen STATISTICS PROGRAM ADVISORS Susan Herring Elaine McDonald-Newman Scott Nickleach ADMINISTRATIVE

  12. Statistics Page 239Sonoma State University 2014-2015 Catalog DEPARTMENT OF MATHEMATICS AND STATISTICS

    E-Print Network [OSTI]

    Ravikumar, B.

    Statistics Page 239Sonoma State University 2014-2015 Catalog STATISTICS DEPARTMENT OF MATHEMATICS AND STATISTICS Darwin Hall 114 phone: (707) 664-2368 fax: (707) 664-3535 www.sonoma.edu/math DEPARTMENT CHAIR Brigitte Lahme STATISTICS PROGRAM ADVISORS Susan Herring Elaine Newman ADMINISTRATIVE COORDINATOR Marybeth

  13. Page 28 Housing Services Sonoma State University 2011-2012 Catalog Zinfandel Hall

    E-Print Network [OSTI]

    Ravikumar, B.

    Page 28 Housing Services Sonoma State University 2011-2012 Catalog Zinfandel Hall (707) 664-2541 Fax: (707) 664-4158 e-mail: ssu.housing@sonoma.edu www.sonoma.edu/housing On-Campus Housing The Residential Community provides comfortable, convenient cam- pus housing for 3,000 single students

  14. Housing Services Page 27Sonoma State University 2014-2015 Catalog (707) 664-2541

    E-Print Network [OSTI]

    Ravikumar, B.

    Housing Services Page 27Sonoma State University 2014-2015 Catalog (707) 664-2541 email: ssu.housing@sonoma.edu www.sonoma.edu/housing Student Center 3rd Floor, Suite 3020 On-Campus Housing The Residential Community provides comfortable, convenient campus housing for 3,100 single students. The Community

  15. Page 28 Housing Services Sonoma State University 2012-2013 Catalog Zinfandel Hall

    E-Print Network [OSTI]

    Ravikumar, B.

    Page 28 Housing Services Sonoma State University 2012-2013 Catalog Zinfandel Hall (707) 664-2541 Fax: (707) 664-4158 e-mail: ssu.housing@sonoma.edu www.sonoma.edu/housing On-Campus Housing The Residential Community provides comfortable, convenient cam- pus housing for 3,000 single students

  16. Page 28 Housing Services Sonoma State University 2013-2014 Catalog (707) 664-2541

    E-Print Network [OSTI]

    Ravikumar, B.

    Page 28 Housing Services Sonoma State University 2013-2014 Catalog (707) 664-2541 Fax: (707) 664-4158 email: ssu.housing@sonoma.edu www.sonoma.edu/housing On-Campus Housing The Residential Community provides comfortable, convenient campus housing for 3,100 single students. The Community is a unique mix

  17. See Chair's Message, page 5 moved to the few halls with

    E-Print Network [OSTI]

    Gilchrist, James F.

    See Chair's Message, page 5 moved to the few halls with power (e.g. Brodhead), whereas many others Whitaker Laboratory 5 E. Packer Ave. Bethlehem, PA 18015 www.lehigh.edu/ ~inmatsci Chair's MessageChair's MessageChair's MessageChair's Message #12;P A G E 2 Mat Camp extends outside Valley The MSE department

  18. Education: ELSE Page 115Sonoma State University 2011-2012 Catalog Department Office

    E-Print Network [OSTI]

    Ravikumar, B.

    's Credential Office for updates on program details and policy statements and to visit the education websiteEducation: ELSE Page 115Sonoma State University 2011-2012 Catalog Department Office Stevenson Hall 1078 (707) 664-4203 fax: (707) 664-2483 www.sonoma.edu/education aDministrative cOOrDinatOr Leslie

  19. Page 148 Education: ELSE Sonoma State University 2006-2008 Catalog Department Office

    E-Print Network [OSTI]

    Ravikumar, B.

    to consult the School of Education's Credential Office for updates on program details and policy statementsPage 148 Education: ELSE Sonoma State University 2006-2008 Catalog Department Office Stevenson Hall 1078 (707) 664-4203 fax (707) 664-2483 www.sonoma.edu/education aDministrative cOOrDinatOr Leslie

  20. 2014 Internship Syllabus Page 1 of 4 MIS 353: Internship in Management Information Systems

    E-Print Network [OSTI]

    Ghosh, Joydeep

    2014 Internship Syllabus Page 1 of 4 MIS 353: Internship in Management Information Systems 2014 for reflection while you perform a professional internship that enhances your ability to achieve your career. Section 2. Contact Information Course website: http://www.mccombs.utexas.edu/BBA/Career-Services/Internship

  1. 2014 Internship Syllabus Page 1 of 4 OM 353: Internship in Operations

    E-Print Network [OSTI]

    Ghosh, Joydeep

    2014 Internship Syllabus Page 1 of 4 OM 353: Internship in Operations Spring 2014 Section 1 a professional internship that enhances your ability to achieve your career objectives. Intended outcomes include website: www.mccombs.utexas.edu/BBA/Career-Services/Internship-Requirement.aspx Internship Coordinator

  2. Geology Page 145Sonoma State University 2012-2013 Catalog DEPARTMENT OFFICE

    E-Print Network [OSTI]

    Ravikumar, B.

    Geology Page 145Sonoma State University 2012-2013 Catalog GEOLOGY DEPARTMENT OFFICE Darwin Hall 116 (707) 664-2334 www.sonoma.edu/geology DEPARTMENT CHAIR Matthew J. James ADMINISTRATIVE COORDINATOR Cory Programs Offered Bachelor of Science in Geology Bachelor of Arts in Earth Sciences Minor in Geology Minor

  3. Page 148 Geology Sonoma State University 2014-2015 Catalog DEPARTMENT OFFICE

    E-Print Network [OSTI]

    Ravikumar, B.

    Page 148 Geology Sonoma State University 2014-2015 Catalog GEOLOGY DEPARTMENT OFFICE Darwin Hall 116 (707) 664-2334 www.sonoma.edu/geology DEPARTMENT CHAIR Matthew J. James ADMINISTRATIVE COORDINATOR. Smith Programs Offered Bachelor of Science in Geology Bachelor of Arts in Earth Science Minor in Geology

  4. Page 148 Geology Sonoma State University 2011-2012 Catalog Department Office

    E-Print Network [OSTI]

    Ravikumar, B.

    Page 148 Geology Sonoma State University 2011-2012 Catalog Department Office Darwin Hall 116 (707) 664-2334 www.sonoma.edu/geology Department chair Matthew J. James aDministrative cOOrDinatOr Jen E. Smith Programs Offered Bachelor of Science in Geology Bachelor of Arts in Earth Sciences Minor

  5. Page144 Geology Sonoma State University 2013-2014 Catalog Department Office

    E-Print Network [OSTI]

    Ravikumar, B.

    Page144 Geology Sonoma State University 2013-2014 Catalog geology Department Office DarwinHall116 (707)664-2334 www.sonoma.edu/geology Department chair MatthewJ.James aDministrative cE.Smith Programs Offered Bachelor of Science in Geology Bachelor of Arts in Earth Science Minor in Geology Minor

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

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOEThe Bonneville PowerCherries 82981-1cnHigh School football High School football Fancy footwork at

  7. Company City State Website ABB International www.abb.com

    E-Print Network [OSTI]

    McGaughey, Alan

    :www.qinetiq-na.com Quantapoint Pittsburgh PA www.quantapoint.com Quintax CNC Routers Stow OH www.quintax.com Redzone

  8. WASEDAUNIVERSITY http://www.sci.waseda.ac.jp/research/

    E-Print Network [OSTI]

    Kasahara, Hironori

    ://www.ase.sci.waseda.ac.jp/ http://www.waseda.jp/ips/ http://www.waseda.jp/weee/ INDEX 2015 5 2 31http

  9. GroupWeb: A WWW Browser as Real Time Groupware Saul Greenberg and Mark Roseman

    E-Print Network [OSTI]

    Greenberg, Saul

    and conferencing. Keywords Word wide web, groupware, shared visual workspaces. INTRODUCTION The World Wide Web and navigate World Wide Web pages in real time. Its groupware features include document and view slavingGroupWeb: A WWW Browser as Real Time Groupware Saul Greenberg and Mark Roseman Department

  10. www.physicstoday.org November 2012 Physics Today 59 Nuclear energy can provide great

    E-Print Network [OSTI]

    www.physicstoday.org November 2012 Physics Today 59 Nuclear energy can provide great The Nuclear on keeping costs and book length in check. For example, most of the graphics use gray- scale, with only a few pages in the cen- ter providing color plates. In addition, in many places additional graphics could have

  11. 2011/2012 University of Delaware Library www.udel.edu/library WELCOME TO THE LIBRARY

    E-Print Network [OSTI]

    Gao, Guang R.

    2011/2012 University of Delaware Library www.udel.edu/library WELCOME TO THE LIBRARY New Library Home Page University of Delaware Library OFFICE OF THE VICE PROVOST & MAY MORRIS DIRECTOR OF LIBRARIES-831-2231 Fax: 302-831-1046 Greetings, Welcome to the University of Delaware Library which includes the Morris

  12. The Neutron Scattering Society of America http:///www.neutronscattering.org

    E-Print Network [OSTI]

    The Neutron Scattering Society of America http:///www.neutronscattering.org Page 8 of 9 Dr. Claire of the Neutron Scattering Society of America (NSSA) with the citation "For pioneering a new methodology and computational chemistry" The Neutron Scattering Society of America (NSSA) established the Prize for Outstanding

  13. www.risoe.dk www.risoe.dk

    E-Print Network [OSTI]

    www.risoe.dk www.risoe.dk LOAD ALLEVIATION ON WIND TURBINE BLADES USING VARIABLE AIRFOIL GEOMETRY work · 2D computations · Tools · Main Results · 3D computations · Tools · Main Results · Wind tunnel expansion of the airfoil deflections · Unsteady terms associated with wake modelled by the computationally

  14. www.risoe.dk www.risoe.dk

    E-Print Network [OSTI]

    www.risoe.dk www.risoe.dk LOAD ALLEVIATION ON WIND TURBINE BLADES USING VARIABLE AIRFOIL GEOMETRY Results · Wind tunnel testing · The model · Preliminary results · Conclusions · Future work #12;Motivation at the trailing edge? · Potential thin-airfoil theory: #12;But why at the trailing edge? · Potential thin

  15. MID-INFRARED IRS SPECTROSCOPY OF NGC 7331: A FIRST LOOK AT THE SPITZER INFRARED NEARBY GALAXIES SURVEY (SINGS) LEGACY

    E-Print Network [OSTI]

    Draine, Bruce T.

    MID-INFRARED IRS SPECTROSCOPY OF NGC 7331: A FIRST LOOK AT THE SPITZER INFRARED NEARBY GALAXIES to 38 m using all modules of Spitzer's Infrared Spectrograph (IRS). A strong new dust emission feature with standard photodissociation region (PDR) models. Either additional PDR heating or shocks are required

  16. The Evolving ISM in the Milky Way & Nearby Galaxies ISM Theory: Gas Phases, Turbulence, and Star Formation

    E-Print Network [OSTI]

    and fills much of the volume near the Galactic midplan, and cold atomic gas, which is organized into denseThe Evolving ISM in the Milky Way & Nearby Galaxies ISM Theory: Gas Phases, Turbulence, and Star modeling efforts have begun to take into account the effects of multiscale, time- dependent processes

  17. Temperature profile for glacial ice at the South Pole: Implications for life in a nearby subglacial lake

    E-Print Network [OSTI]

    Price, P. Buford

    by P. Buford Price, April 22, 2002 Airborne radar has detected 100 lakes under the Antarctic ice cap-induced melting temperature of freshwater ice. To produce the strong radar signal, the frozen lake must consistTemperature profile for glacial ice at the South Pole: Implications for life in a nearby subglacial

  18. New Page 1

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  19. DOE PAGES Beta

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    National Nuclear Security Administration (NNSA)

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  2. About / FAQ | DOE PAGES

    Office of Scientific and Technical Information (OSTI)

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  3. 21 briefing pages total

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  7. LCLS AMO web page

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  8. Stellarator News Home Page

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  12. WIPP Stakeholder Information Page

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  13. WIPP Stakeholder Information Page

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  14. WIPP Stakeholder Information Page

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  15. WIPP Stakeholder Information Page

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  16. WIPP Stakeholder Information Page

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  17. WIPP Stakeholder Information Page

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  18. WIPP Stakeholder Information Page

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  19. Cover and Title Page

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  20. DA326576 (2 pages)

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  1. PDSF Group Pages

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  2. Palm Physics Page

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  3. Transforming Biomass - main page

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  4. David Gates home page

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  5. 2page.indd

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    National Nuclear Security Administration (NNSA)

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  7. Aprun MAN Page

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  8. Webinar Summary Page 1

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  10. CAMD Cleanroom Login Page

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  11. Yennello Group Home Page

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  16. Feedback | DOE PAGES

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  17. www.ornl.gov OAKRIDGENATIONALLABORATORY

    E-Print Network [OSTI]

    www.ornl.gov OAKRIDGENATIONALLABORATORY MANAGED BY UT-BATTELLE FOR THE DEPARTMENT OF ENERGY continue to delay construction of more towers. These problems are highlighted in the Report of the President's National Energy Policy Development Study (http://www.whitehouse.gov/energy/) and the National

  18. Vertical broad-line region structure in nearby active galactic nuclei

    E-Print Network [OSTI]

    Kollatschny, W

    2013-01-01T23:59:59.000Z

    Broad emission lines are emitted in the surroundings of supermassive black holes in the centers of active galactic nuclei (AGN). This region is spatially not resolved. We intend to get information on the structure and geometry of this broad emitting line region (BLR) based on line profile observations. We model the rotational and turbulent velocities in the line-emitting regions based on observed full-width at half maximum line values (FWHM) and {\\sigma}_{line} of the variable broad emission lines in four nearby AGN: NGC 3783, NGC 7469, NGC 5548, and 3C 390.3. On the basis of these velocities, we estimate the height of the line-emitting regions above the midplane in context with their distances from the center. The H{\\beta} lines are emitted in a more flattened configuration above the midplane in comparison to the highly ionized lines. The H{\\beta} lines originate at heights of 0.7 to 1.6 light-days and at distances of 1.4 to 24 light-days with height/distance (H/R) ratios of only 0.07 to 0.5. The highly ioni...

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

    SciTech Connect (OSTI)

    Abreu, P.; /Lisbon, IST; Aglietta, M.; /Turin U. /INFN, Turin; Ahn, E.J.; /Fermilab; Allard, D.; /APC, Paris; Allekotte, I.; /Centro Atomico Bariloche; Allen, J.; /New York U.; Alvarez Castillo, J.; /Mexico U., ICN; Alvarez-Muniz, J.; /Santiago de Compostela U.; Ambrosio, M.; /INFN, Naples /Naples U.; Aminaei, A.; /Nijmegen U., IMAPP; Anchordoqui, L.; /Wisconsin U., Milwaukee /Lisbon, IST

    2010-06-01T23:59:59.000Z

    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.

  20. An astrometric companion to the nearby metal-poor, low-mass star LHS 1589

    E-Print Network [OSTI]

    Sebastien Lepine; R. Michael Rich; Michael M. Shara; Kelle L. Cruz; Andrew Skemer

    2007-07-20T23:59:59.000Z

    We report the discovery of a companion to the high proper motion star LHS 1589, a nearby high-velocity, low-mass subdwarf. The companion (LHS 1589B) is located 0.224+/-0.004" to the southwest of the primary (LHS 1589A), and is 0.5 magnitude fainter than the primary in the K_s band. The pair was resolved with the IRCAL infrared camera at Lick Observatory, operating with the Laser Guide Star Adaptive Optics system. A low-resolution spectrum of the unresolved pair obtained at the MDM observatory shows the source to be consistent with a cool subdwarf of spectral subtype sdK7.5. A photometric distance estimate places the metal-poor system at a distance d=81+/-18 parsecs from the Sun. We also measure a radial velocity V_rad=67+/-8 km/s which, together with the proper motion and estimated distance, suggests that the pair is roaming the inner Galactic halo on a highly eccentric orbit. With a projected orbital separation s=18.1+/-4.8 AU, and a crude estimate of the system's total mass, we estimate the orbital period of the system to be in the range 75 yr metal-poor, low-mass stars.

  1. Effervescent heating: constraints from nearby cooling flow clusters observed with XMM-Newton

    E-Print Network [OSTI]

    Rocco Piffaretti; Jelle Kaastra

    2006-05-15T23:59:59.000Z

    We have used deprojected radial density and temperature profiles of a sample of 16 nearby CF clusters observed with XMM-Newton to test whether the effervescent heating model can satisfactorily explain the dynamics of CF clusters. For each cluster we derived the required extra heating as a function of cluster-centric distance for various values of the unknown parameters $\\dot M$ (mass deposition rate) and $f_c$ (conduction efficiency). We fitted the extra heating curve using the AGN effervescent heating function and derived the AGN parameters $L$ (the time-averaged luminosity) and $r_0$ (the scale radius where the bubbles start rising in the ICM). While we do not find any solution with the effervescent heating model for only one object, we do show that AGN and conduction heating are not cooperating effectively for half of the objects in our sample. For most of the clusters we find that, when a comparison is possible, the derived AGN scale radius $r_0$ and the observed AGN jet extension have the same order of magnitude. The AGN luminosities required to balance radiative losses are substantially lowered if the fact that the AGN deposits energy within a finite volume is taken into account. For the Virgo cluster, we find that the AGN power derived from the effervescent heating model is in good agreement with the observed jet power.

  2. Starburst Anatomy: Stellar and Nebular Properties of Nearby Giant HII Regions

    E-Print Network [OSTI]

    William H. Waller

    1996-12-27T23:59:59.000Z

    Resolution of nearby giant HII regions into their stellar and nebular constituents provides fundamental insights for interpreting more distant and powerful starburst activity. The following summarizes recent advances in our understanding of the stellar populations and nebular energetics associated with giant HII regions. Photometry and spectroscopy of ionizing clusters in the Galaxy, LMC, and SMC reveal no significant relation between metallicity and the slope of the power-law initial mass function (IMF). HST/WFPC2 photometry of 3 giant HII regions in M33 also does not show any consistent trend involving metal abundance and IMF slope -- contrary to predictions based on emission-line ratios. The upper stellar mass limit appears to be constrained more by cluster age than by anything else. The ionizing luminosities from some of the resolved stellar populations are insufficient to account for the ionization rates inferred from measurements of the composite (integrated) H-alpha emission. Absorption of stellar EUV emission by nebular dust grains would only amplify these photoionizing shortfalls. Leakage of ionizing photons from the HII regions would further exacerbate the situation. What then is providing the additional ionization? Prospects for higher stellar EUV luminosities and/or alternative sources of nebular ionization (e.g. shocks) are evaluated with this question in mind.

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

    SciTech Connect (OSTI)

    Sinclair, Andrew J. (Auburn University Auburn, AL); Raju, Anil (Auburn University Auburn, AL); Kurzen, Matthew J. (Virginia Tech Blacksburg, VA); Roy, Christopher John (Virginia Tech Blacksburg, VA); Phillips, Tyrone S. (Virginia Tech Blacksburg, VA)

    2011-10-01T23:59:59.000Z

    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. Fundamental Parameters of Nearby Stars from the Comparison with Evolutionary Calculations: Masses, Radii and Effective temperatures

    E-Print Network [OSTI]

    Carlos Allende Prieto; David L. Lambert

    1999-11-02T23:59:59.000Z

    The Hipparcos mission has made it possible to constrain the positions of nearby field stars in the colour-magnitude diagram with very high accuracy. These positions can be compared with the predictions of stellar evolutionary calculations to provide information on the basic parameters of the stars: masses, radii, effective temperatures, ages, and chemical composition. The degeneracy between mass, age, and metallicity is not so large as to prevent a reliable estimate of masses, radii and effective temperatures, at least for stars of solar metallicity. The evolutionary models of Bertelli et al. (1994) predict those parameters finely, and furthermore, the applied transformation from the theoretical (log g-Teff) to the observational (Mv-B-V) plane is precise enough to derive radii with an uncertainty of ~ 6%, masses within ~ 8%, and Teffs within ~ 2% for a certain range of the stellar parameters. This is demonstrated by means of comparison with the measurements in eclipsing binaries and the InfraRed Flux Method. The application of the interpolation procedure in the theoretical isochrones to the stars within 100 pc from the Sun observed with Hipparcos provides estimates for 17,219 stars

  5. A Chandra study of particle acceleration in the multiple hotspots of nearby radio galaxies

    E-Print Network [OSTI]

    M. J. Hardcastle; J. H. Croston; R. P. Kraft

    2007-07-19T23:59:59.000Z

    We present Chandra observations of a small sample of nearby classical double radio galaxies which have more than one radio hotspot in at least one of their lobes. The X-ray emission from the hotspots of these comparatively low-power objects is expected to be synchrotron in origin, and therefore to provide information about the locations of high-energy particle acceleration. In some models of the relationship between the jet and hotspot the hotspots that are not the current jet termination point should be detached from the energy supply from the active nucleus and therefore not capable of accelerating particles to high energies. We find that in fact some secondary hotspots are X-ray sources, and thus probably locations for high-energy particle acceleration after the initial jet termination shock. In detail, though, we show that the spatial structures seen in X-ray are not consistent with naive expectations from a simple shock model: the current locations of the acceleration of the highest-energy observable particles in powerful radio galaxies need not be coincident with the peaks of radio or even optical emission.

  6. A Search for "Dwarf" Seyfert Nuclei. VI. Properties of Emission-Line Nuclei in Nearby Galaxies

    E-Print Network [OSTI]

    Luis C. Ho; Alexei V. Filippenko; Wallace L. W. Sargent

    2002-10-02T23:59:59.000Z

    We use the database from Paper III to quantify the global and nuclear properties of emission-line nuclei in the Palomar spectroscopic survey of nearby galaxies. We show that the host galaxies of Seyferts, LINERs, and transition objects share remarkably similar large-scale properties and local environments. The distinguishing traits emerge on nuclear scales. Compared with LINERs, Seyfert nuclei are an order of magnitude more luminous and exhibit higher electron densities and internal extinction. We suggest that Seyfert galaxies possess characteristically more gas-rich circumnuclear regions, and hence a more abundant fuel reservoir and plausibly higher accretion rates. The differences between the ionization state of the narrow emission-line regions of Seyferts and LINERs can be partly explained by the differences in their nebular properties. Transition-type objects are consistent with being composite (LINER/\\hii) systems. With very few exceptions, the stellar population within the central few hundred parsecs of the host galaxies is uniformly old, a finding that presents a serious challenge to starburst or post-starburst models for these objects. Seyferts and LINERs have virtually indistinguishable velocity fields as inferred from their line widths and line asymmetries. All three classes of objects obey a strong correlation between line width and line luminosity. We argue that the angular momentum content of circumnuclear gas may be an important factor in determining whether a nucleus becomes active. Finally, we discuss some possible complications for the unification model of Seyfert galaxies posed by our observations. (Abridged)

  7. Temperature profiles of a representative sample of nearby X-ray galaxy clusters

    E-Print Network [OSTI]

    G. W. Pratt; H. Boehringer; J. H. Croston; M. Arnaud; S. Borgani; A. Finoguenov; R. F. Temple

    2006-09-18T23:59:59.000Z

    A study of the structural and scaling properties of the temperature distribution of the hot, X-ray emitting intra-cluster medium of galaxy clusters, and its dependence on dynamical state, can give insights into the physical processes governing the formation and evolution of structure. We analyse the X-ray temperature profiles from XMM-Newton observations of 15 nearby (z temperature range from 2.5 keV to 8.5 keV, and present a variety of X-ray morphologies. We derive accurate projected temperature profiles to ~ 0.5 R_200, and compare structural properties (outer slope, presence of cooling core) with a quantitative measure of the X-ray morphology as expressed by power ratios. We also compare the results to recent cosmological numerical simulations. Once the temperature profiles are scaled by an average cluster temperature (excluding the central region) and the estimated virial radius, the profiles generally decline in the region 0.1 R_200 temperature decrement appear to be slightly more regular. The present results lend further evidence to indicate that clusters are a regular population, at least outside the core region.

  8. SMT CO (2-1) Observations of Nearby Star-Forming Galaxies

    E-Print Network [OSTI]

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

    2014-01-01T23:59:59.000Z

    We present CO $J$=2-1 observations towards 32 nearby gas-rich star-forming galaxies selected from the ALFALFA and WISE catalogs, using the Sub-millimeter Telescope. Our sample is selected to be dominated by intermediate-$M_{\\rm *}$ 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 that (1). In the galaxies with stellar mass $M_{\\rm *}$ $\\leqslant 10^{10}$ $M_{\\odot}$, HI fraction ($f_{\\rm HI}$ $\\equiv$ $M_{\\rm HI}$/$M_{\\rm *}$) is significantly higher than that of more massive galaxies, while H$_2$ gas fraction ($f_{\\rm H_2}$ $\\equiv$ $M_{\\rm H_2}$/$M_{\\rm *}$) remain nearly unchanged. (2). Comparing with $f_{\\rm H_2}$, $f_{\\rm HI}$ correlates better with both $M_{\\rm *}$ and NUV$- r$. (3). A new parameter, WISE color W3$-$W2 (12\\,$\\mu$m$-$4.6\\,$\\mu$m) is introduced, which is similar to NUV$- r$ in tracing star formation activity, and we find that W3$-$W2 has a tighter anti-corr...

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

    SciTech Connect (OSTI)

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

    2013-06-20T23:59:59.000Z

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

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

    SciTech Connect (OSTI)

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

    2013-06-20T23:59:59.000Z

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

  11. Central Mass Profiles of the Nearby Cool-core Galaxy Clusters Hydra A and A478

    E-Print Network [OSTI]

    Okabe, N; Tamura, T; Fujita, Y; Takizawa, M; Matsushita, K; Fukazawa, Y; Futamase, T; Kawaharada, M; Miyazaki, S; Mochizuki, Y; Nakazawa, K; Ohashi, T; Ota, N; Sasaki, T; Sato, K; Tam, S I

    2015-01-01T23:59:59.000Z

    We perform a weak-lensing study of the nearby cool-core galaxy clusters, Hydra A ($z=0.0538$) and A478 ($z=0.0881$), of which brightest cluster galaxies (BCGs) host powerful activities of active galactic nuclei (AGNs). For each cluster, the observed tangential shear profile is well described either by a single Navarro--Frenk--White model or a two-component model including the BCG as an unresolved point mass. For A478, we determine the BCG and its host-halo masses from a joint fit to weak-lensing and stellar photometry measurements. We find that the choice of initial mass functions (IMFs) can introduce a factor of two uncertainty in the BCG mass, whereas the BCG host halo mass is well constrained by data. We perform a joint analysis of weak-lensing and stellar kinematics data available for the Hydra A cluster, which allows us to constrain the central mass profile without assuming specific IMFs.We find that the central mass profile ($r<300$ kpc) determined from the joint analysis is in excellent agreement wi...

  12. WASEDAUNIVERSITY http://www.sci.waseda.ac.jp

    E-Print Network [OSTI]

    Kasahara, Hironori

    ://www.cse.sci.waseda.ac.jp/ http://www.ase.sci.waseda.ac.jp/ http://www.waseda.jp/ips/ http://www.waseda.jp/weee/ INDEX 2014 5

  13. 07/10/2010 14:54Tug of War Pits Genes of Parents in the Fetus -NYTimes.com Page 1 of 4http://www.nytimes.com/2010/09/14/health/14gene.html?_r=1&pagewanted=print

    E-Print Network [OSTI]

    Gardner, Andy

    07/10/2010 14:54Tug of War Pits Genes of Parents in the Fetus - NYTimes.com Page 1 of 4http.nytreprints.com for samples and additional information. Order a reprint of this article now. September 13, 2010 Tug of War;07/10/2010 14:54Tug of War Pits Genes of Parents in the Fetus - NYTimes.com Page 2 of 4http

  14. Department of Mathematics: Course Page

    E-Print Network [OSTI]

    ... offered in Spring 2015. Past course pages are available here: ... ADA policies: please see our ADA Information page for more details. In the event of a missed ...

  15. http://www

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level:Energy: Grid Integration Redefining What'sis Taking Over OurThe Iron4 Self-Scrubbing:,, , .,Shreve; University of0a.2/049/03Instruments and

  16. http://www

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level:Energy: Grid Integration Redefining What'sis Taking Over OurThe Iron4 Self-Scrubbing:,, , .,Shreve; University of0a.2/049/03Instruments

  17. www.chemistryworld.org

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office of ScienceandMesa del SolStrengtheningWildfires mayYuan T.ExternalscriptEnv LANL

  18. www.usiter.com

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office of ScienceandMesa del SolStrengtheningWildfires mayYuan T.ExternalscriptEnv LANLFebruary 12, 2015 |ForAs

  19. www.bpa.gov

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level:Energy: Grid Integration Redefining What'sis Taking Over OurThe Iron4 Self-Scrubbing:,, ,Development1U CO1) 1 Winter FuelsYOUR BENEFITPart IE

  20. www.usiter.com

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742EnergyOnItemResearch >Internship ProgramBiomass and Biofuels

  1. http://www

    Office of Environmental Management (EM)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742 33Frequently20,000 Russian Nuclearand Characterization of a LargerMilrowOU

  2. EMIS Quick User Guide Search page (details on page 2)

    E-Print Network [OSTI]

    Barthelat, Francois

    search terms in foreign languages You can enter search terms in foreign languages by: - Using your: Please note that we have a Cyrillic and Arabic keyboards available through the Search page. EnteringEMIS Quick User Guide Search page (details on page 2) The News page: Access the latest news

  3. WISEP J180026.60+013453.1: A NEARBY LATE-L DWARF NEAR THE GALACTIC PLANE

    SciTech Connect (OSTI)

    Gizis, John E.; Castro, Philip J. [Department of Physics and Astronomy, University of Delaware, Newark, DE 19716 (United States); Burgasser, Adam J. [Center for Astrophysics and Space Science, University of California San Diego, La Jolla, CA 92093 (United States); Faherty, Jacqueline K.; Shara, Michael M. [Department of Astrophysics, American Museum of Natural History, New York, NY 10034 (United States)

    2011-11-15T23:59:59.000Z

    We report a nearby L7.5 dwarf discovered using the Preliminary Data Release of the Wide-field Infrared Survey Explorer (WISE) and the Two Micron All Sky Survey. WISEP J180026.60+013453.1 has a motion of 0.42 arcsec yr{sup -1} and an estimated distance of 8.8 {+-} 1.0 pc. With this distance, it currently ranks as the sixth closest known L dwarf, although a trigonometric parallax is needed to confirm this distance. It was previously overlooked because it lies near the Galactic plane (b = 12 Degree-Sign ). As a relatively bright and nearby late L dwarf with normal near-infrared colors, W1800+0134 will serve as a benchmark for studies of cloud-related phenomena in cool substellar atmospheres.

  4. 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: khan@astronomy.ohio-state.edu, E-mail: kstanek@astronomy.ohio-state.edu, E-mail: ckochanek@astronomy.ohio-state.edu [Department of Astronomy, The Ohio State University, 140 W. 18th Ave., Columbus, OH 43210 (United States)

    2013-04-10T23:59:59.000Z

    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.

  5. In situ measurements of rock salt permeability changes due to nearby excavation

    SciTech Connect (OSTI)

    Stormont, J.C. (Sandia National Labs., Albuquerque, NM (United States)); Howard, C.L. (RE/SPEC, Inc., Carlsbad, NM (United States)); Daemen, J.J.K. (Nevada Univ., Reno, NV (United States). Mackay School of Mines)

    1991-07-01T23:59:59.000Z

    The Small-Scale Mine-By was an in situ experiment to measure changes in brine and gas permeability of rock salt as a result of nearby excavation. A series of small-volume pressurized brine- and gas-filled test intervals were established 8 m beneath the floor of Room L1 in the WIPP underground. The test intervals were isolated in the bottom of the 4.8-cm diameter monitoring boreholes with inflatable rubber packers, and are initially pressurized to about 2 MPa. Both brine- and gas-filled test intervals were located 1.25, 1.5, 2, 3, and 4 r from the center of a planned large-diameter hole, where r is the radius of the large-diameter hole. Prior to the drilling of the large-diameter borehole, the responses of both the brine- and gas-filled test intervals were consistent with the formation modeled as a very low permeability, low porosity porous medium with a significant pore (brine) pressure and no measurable gas permeability. The drilling of the mine-by borehole created a zone of dilated, partially saturated rock out to about 1.5 r. The formation pressure increases from near zero at 1.5 r to the pre-excavation value at 4 r. Injection tests reveal a gradient of brine permeabilities from 5 {times} 10{sup {minus}18} m{sup 2} at 1.25 r to about the pre-excavation value (10{sup {minus}21} m{sup 2}) by 3 r. Gas-injection tests reveal measurable gas permeability is limited to within 1.5 r. 17 refs., 24 figs., 6 tabs.

  6. LONG-TERM OPTICAL CONTINUUM COLOR VARIABILITY OF NEARBY ACTIVE GALACTIC NUCLEI

    SciTech Connect (OSTI)

    Sakata, Yu; Minezaki, Takeo; Yoshii, Yuzuru; Uchimoto, Yuka Katsuno; Sugawara, Shota [Institute of Astronomy, School of Science, University of Tokyo, 2-21-1 Osawa, Mitaka, Tokyo 181-0015 (Japan); Kobayashi, Yukiyasu [National Astronomical Observatory, 2-21-1 Osawa, Mitaka, Tokyo 181-8588 (Japan); Koshida, Shintaro [Department of Astronomy, School of Science, University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0013 (Japan); Aoki, Tsutomu; Tomita, Hiroyuki [Kiso Observatory, Institute of Astronomy, School of Science, University of Tokyo, 10762-30 Mitake, Kiso, Nagano 397-0101 (Japan); Enya, Keigo; Suganuma, Masahiro, E-mail: yusakata@ioa.s.u-tokyo.ac.j [Institute of Space and Astronomical Science, Japan Aerospace Exploration Agency, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8510 (Japan)

    2010-03-01T23:59:59.000Z

    We examine whether the spectral energy distribution of optical continuum emission of active galactic nuclei (AGNs) changes during flux variation, based on accurate and frequent monitoring observations of 11 nearby Seyfert galaxies and QSOs carried out in the B, V, and I bands for seven years by the MAGNUM telescope. The multi-epoch flux data in any two different bands obtained on the same night show a very tight linear flux-to-flux relationship for all target AGNs. The flux of the host galaxy within the photometric aperture is carefully estimated by surface brightness fitting to available high-resolution Hubble Space Telescope images and MAGNUM images. The flux of narrow emission lines in the photometric bands is also estimated from available spectroscopic data. We find that the non-variable component of the host galaxy plus narrow emission lines for all target AGNs is located on the fainter extension of the linear regression line of multi-epoch flux data in the flux-to-flux diagram. This result strongly indicates that the spectral shape of AGN continuum emission in the optical region ({approx}4400-7900 A) does not systematically change during flux variation. The trend of spectral hardening that optical continuum emission becomes bluer as it becomes brighter, which has been reported by many studies, is therefore interpreted as the domination of the variable component of the nearly constant spectral shape of an AGN as it brightens over the non-variable component of the host galaxy plus narrow lines, which is usually redder than AGN continuum emission.

  7. 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 [Departement de physique and Observatoire du Mont-Megantic, Universite de Montreal, Montreal, QC H3C 3J7 (Canada)] [Departement de physique and Observatoire du Mont-Megantic, Universite de Montreal, Montreal, QC H3C 3J7 (Canada); Riedel, Adric, E-mail: malo@astro.umontreal.ca, E-mail: doyon@astro.umontreal.ca, E-mail: david@astro.umontreal.ca, E-mail: artigau@astro.umontreal.ca, E-mail: gagne@astro.umontreal.ca, E-mail: baron@astro.umontreal.ca, E-mail: riedel@phy-astr.gsu.edu [Department of Astrophysics, American Museum of Natural History, Central Park West at 79th Street, New York, NY 10024 (United States)] [Department of Astrophysics, American Museum of Natural History, Central Park West at 79th Street, New York, NY 10024 (United States)

    2013-01-10T23:59:59.000Z

    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.

  8. XMM-Newton Studies of the Source Population and the Hot Interstellar Medium in Nearby Galaxies

    E-Print Network [OSTI]

    W. Pietsch

    2002-12-20T23:59:59.000Z

    First results of X-ray source population studies in nearby galaxies show the potential of XMM-Newton observations. I will report on first XMM-Newton M31 results and on three of our XMM-Newton projects, an X-ray source population study in the Magellanic Clouds (MCs), a deep raster survey of M33, and an investigation of the hot interstellar medium (ISM) in the halo of edge-on galaxies. XMM-Newton results on several other galaxies and sources within are presented by other authors in these proceedings. Our MC study is build up of deep pointings probing MC sources down to 10^33 erg s^-1 and shallower pointings to confirm candidates from our ROSAT derived lists of X-ray binaries, super-soft sources, and supernova remnants. First XMM-Newton detections of a 455 s pulsar in the Small Magellanic Cloud and the results of the Large Magellanic Cloud deep field confirm the validity of our strategy. Our M33 raster pointing aims for luminosities as low as 10^35 erg s^-1, a factor of 10 below the sensitivity limit of the ROSAT observations. The survey will allow us to characterize the sources using extent, spectra, hardness ratios and time variability to build up an unprecedented census of the X-ray source content of M33. Of specific interest are the active source in the nuclear area and the diffuse emission in the inner disk. XMM-Newton observations of the active galaxy NGC 3079 and of the starburst galaxy NGC 253 are used to characterize the point-like sources and the hot ISM in the disk and from the halo of these galaxies.

  9. The ESO Nearby Abell Cluster Survey VIII. Morphological and spectral classification of galaxies

    E-Print Network [OSTI]

    T. Thomas; P. Katgert

    2005-10-10T23:59:59.000Z

    We have determined the morphological types of 2295 galaxies from the ESO Nearby Abell Cluster Survey (ENACS) from CCD images made with the Dutch telescope on La Silla. The reliability of our classification appears to be quite comparable to that of other classifiers. Recalibration of the ENACS spectral classification shows that early- and late- type galaxies can be distinguished from their spectra with 83% reliability. Ellipticals and S0 galaxies cannot be distinguished spectrally, while spectral classification of late spirals has a reliability of 70%. We derive average pseudo-colors and linestrengths from the ENACS spectra for the galaxies of different morphological types, considering bright (M -20) subsets of the galaxies without emission lines (non-ELG) separately. We find a strong and significant correlation between the average color and the average strength of the metal absorption lines. The average metallicity decreases and the average color gets bluer towards later Hubble type. In each morphological class the faint galaxies are bluer and less metal-rich than the bright ones. This extends the well-established color-magnitude relation of early-type galaxies to (late) spirals. Bright early spirals may, on average, have somewhat stronger H-delta absorption than the other galaxies, which could be due to recent starformation. The galaxies with emission lines (ELG) have a bluer spectral continuum than the non-ELG, and the amount of blueing hardly depends on morphological type. The fraction of ELG depends strongly on morphological type but it varies very little with projected distance from the cluster center.

  10. Starbursts and the triggering of the activity in nearby powerful radio galaxies

    E-Print Network [OSTI]

    C. Tadhunter; T. G. Robinson; R. M. Gonzalez Delgado; K. Wills; R. Morganti

    2004-10-05T23:59:59.000Z

    We present high quality long-slit spectra for three nearby powerful radio galaxies 3C293, 3C305, PKS1345+12. These were taken with the aim of characterising the young stellar populations (YSP), and thereby investigating the evolution of the host galaxies, as well as the events that triggered the activity. Isochrone spectral synthesis modelling of the wide wavelength coverage spectra of nuclear and off-nuclear continuum-emitting regions have been used to estimate the ages, masses and luminosities of the YSP component, taking full account of reddening effects and potential contamination by activity-related components. We find that the YSP make a substantial contribution to the continuum flux in the off-nuclear regions on a radial scale of 1 - 20kpc in all three objects. Moreover, in two objects we find evidence for reddened post-starburst stellar populations in the near-nuclear regions of the host galaxies. The YSP are relatively old (0.1- 2Gyr), massive and make up a large proportion (~1 - 50%) of the total stellar mass in the regions of galaxies sampled by the observations. Overall, these results are consistent with the idea that AGN activity in some radio galaxies is triggered by major gas-rich mergers. Therefore, these radio galaxies form part of the subset of early-type galaxies that is evolving most rapidly in the local universe. Intriguingly, the results also suggest that the radio jets are triggered relatively late in the merger sequence, and that there is an evolutionary link between radio galaxies and luminous/ultra-luminous infrared galaxies.

  11. THE ACS NEARBY GALAXY SURVEY TREASURY. XI. THE REMARKABLY UNDISTURBED NGC 2403 DISK

    SciTech Connect (OSTI)

    Williams, Benjamin F.; Dalcanton, Julianne J.; Stilp, Adrienne; Radburn-Smith, David [Department of Astronomy, Box 351580, University of Washington, Seattle, WA 98195 (United States); Dolphin, Andrew [Raytheon, 1151 E. Hermans Road, Tucson, AZ 85706 (United States); Skillman, Evan D., E-mail: ben@astro.washington.edu, E-mail: jd@astro.washington.edu, E-mail: adrienne@astro.washington.edu, E-mail: dolphin@raytheon.com, E-mail: skillman@astro.umn.edu [Department of Astronomy, University of Minnesota, 116 Church St. SE, Minneapolis, MN 55455 (United States)

    2013-03-10T23:59:59.000Z

    We present detailed analysis of color-magnitude diagrams of NGC 2403, obtained from a deep (m {approx}< 28) Hubble Space Telescope (HST) Wide Field Planetary Camera 2 observation of the outer disk of NGC 2403, supplemented by several shallow (m {approx}< 26) HST Advanced Camera for Surveys fields. We derive the spatially resolved star formation history of NGC 2403 out to 11 disk scale lengths. In the inner portions of the galaxy, we compare the recent star formation rates (SFRs) we derive from the resolved stars with those measured using GALEX FUV + Spitzer 24{mu} fluxes, finding excellent agreement between the methods. Our measurements also show that the radial gradient in recent SFR mirrors the disk exponential profile to 11 scale lengths with no break, extending to SFR densities a factor of {approx}100 lower than those that can be measured with GALEX and Spitzer ({approx}2 Multiplication-Sign 10{sup -6} M{sub Sun} yr{sup -1} kpc{sup -2}). Furthermore, we find that the cumulative stellar mass of the disk was formed at similar times at all radii. We compare these characteristics of NGC 2403 to those of its ''morphological twins'', NGC 300 and M 33, showing that the structure and age distributions of the NGC 2403 disk are more similar to those of the relatively isolated system NGC 300 than to those of the Local Group analog M 33. We also discuss the environments and HI morphologies of these three nearby galaxies, comparing them to integrated light studies of larger samples of more distant galaxy disks. Taken together, the physical properties and evolutionary history of NGC 2403 suggest that the galaxy has had no close encounters with other M 81 group members and may be falling into the group for the first time.

  12. OBSERVATIONAL CONSTRAINTS ON THE MOLECULAR GAS CONTENT IN NEARBY STARBURST DWARF GALAXIES

    SciTech Connect (OSTI)

    McQuinn, Kristen B. W.; Skillman, Evan D. [Department of Astronomy, School of Physics and Astronomy, 116 Church Street, S.E., University of Minnesota, Minneapolis, MN 55455 (United States); Dalcanton, Julianne J.; Weisz, Daniel R.; Williams, Benjamin F. [Department of Astronomy, Box 351580, University of Washington, Seattle, WA 98195 (United States); Dolphin, Andrew E. [Raytheon Company, 1151 E. Hermans Road, Tucson, AZ 85756 (United States); Cannon, John M. [Department of Physics and Astronomy, Macalester College, 1600 Grand Avenue, Saint Paul, MN 55105 (United States); Holtzman, Jon, E-mail: kmcquinn@astro.umn.edu [Department of Astronomy, New Mexico State University, Box 30001, Department 4500, 1320 Frenger Street, Las Cruces, NM 88003 (United States)

    2012-06-01T23:59:59.000Z

    Using star formation histories derived from optically resolved stellar populations in 19 nearby starburst dwarf galaxies observed with the Hubble Space Telescope, we measure the stellar mass surface densities of stars newly formed in the bursts. By assuming a star formation efficiency (SFE), we then calculate the inferred gas surface densities present at the onset of the starbursts. Assuming an SFE of 1%, as is often assumed in normal star-forming galaxies, and assuming that the gas was purely atomic, translates to very high H I surface densities ({approx}10{sup 2}-10{sup 3} M{sub Sun} pc{sup -2}), which are much higher than have been observed in dwarf galaxies. This implies either higher values of SFE in these dwarf starburst galaxies or the presence of significant amounts of H{sub 2} in dwarfs (or both). Raising the assumed SFEs to 10% or greater (in line with observations of more massive starbursts associated with merging galaxies), still results in H I surface densities higher than observed in 10 galaxies. Thus, these observations appear to require that a significant fraction of the gas in these dwarf starbursts galaxies was in the molecular form at the onset of the bursts. Our results imply molecular gas column densities in the range 10{sup 19}-10{sup 21} cm{sup -2} for the sample. In the galaxies where CO observations have been made, these densities correspond to values of the CO-H{sub 2} conversion factor (X{sub CO}) in the range >(3-80) Multiplication-Sign 10{sup 20} cm{sup -2} (K km s{sup -1}){sup -1}, or up to 40 Multiplication-Sign greater than Galactic X{sub CO} values.

  13. CONSTRAINTS ON PLANET OCCURRENCE AROUND NEARBY MID-TO-LATE M DWARFS FROM THE MEARTH PROJECT

    SciTech Connect (OSTI)

    Berta, Zachory K.; Irwin, Jonathan; Charbonneau, David, E-mail: zberta@cfa.harvard.edu [Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138 (United States)

    2013-10-01T23:59:59.000Z

    The MEarth Project is a ground-based photometric survey intended to find planets transiting the closest and smallest main-sequence stars. In its first four years, MEarth discovered one transiting exoplanet, the 2.7 R{sub ?} planet GJ1214b. Here, we answer an outstanding question: in light of the bounty of small planets transiting small stars uncovered by the Kepler mission, should MEarth have found more than just one planet so far? We estimate MEarth's ensemble sensitivity to exoplanets by performing end-to-end simulations of 1.25 × 10{sup 6} observations of 988 nearby mid-to-late M dwarfs, gathered by MEarth between 2008 October and 2012 June. For 2-4 R{sub ?} planets, we compare this sensitivity to results from Kepler and find that MEarth should have found planets at a rate of 0.05-0.36 planets yr{sup –1} in its first four years. As part of this analysis, we provide new analytic fits to the Kepler early M dwarf planet occurrence distribution. When extrapolating between Kepler's early M dwarfs and MEarth's mid-to-late M dwarfs, we find that assuming the planet occurrence distribution stays fixed with respect to planetary equilibrium temperature provides a good match to our detection of a planet with GJ1214b's observed properties. For larger planets, we find that the warm (600-700 K), Neptune-sized (4 R{sub ?}) exoplanets that transit early M dwarfs like Gl436 and GJ3470 occur at a rate of <0.15 star{sup –1} (at 95% confidence) around MEarth's later M dwarf targets. We describe a strategy with which MEarth can increase its expected planet yield by 2.5 × without new telescopes by shifting its sensitivity toward the smaller and cooler exoplanets that Kepler has demonstrated to be abundant.

  14. Old School, . . . page 4

    E-Print Network [OSTI]

    of the mission is to measure x-ray polarization in pulsars, gamma-ray bursts, and solar flares. Mark Mc reinflated the balloon program. the Gamma-ray Polarimeter experiment or GraPe received $2 million from nasaH scientists and engineers created for the Compton Gamma-ray Observatory (CGrO). -- continued on page 3 In rock

  15. page 1 1 Introduction

    E-Print Network [OSTI]

    #12;#12;#12;#12;#12;#12;page 1 1 Introduction Techniques to recover object shapes from reflectance. The sunlight can be regarded as yellow point light source whose movement is restricted to the ecliptic1 reflection components from the object surface. Reflection from object surfaces may have multiple 1. The great

  16. Distributed Paging Yair Bartal

    E-Print Network [OSTI]

    Bartal, Yair

    . We survey distributed data management problems including distributed paging, file allocation fantastically on an annual basis. This survey deals with distributed data management problems. Such prob­ lems in distributed data management is the de­ sign of a dynamic allocation of file copies in a network in order

  17. CONTENTS PAGE INTRODUCTION

    E-Print Network [OSTI]

    Aslaksen, Helmer

    THE APPLICATIONS AND VALIDITY OF BODE'S LAW CAN WE EXPLAIN BODE'S LAW USING GRAVITY? 8 Law of Gravitation 8 Centre#12;#12;CONTENTS CONTENTS PAGE INTRODUCTION WHO, HOW AND WHEN IS THE BODE'S LAW DISCOVERED? 1 THE BODE'S LAW HOW THE BODE'S LAW SATISFIED URANUS 3 HOW THE BODE'S LAW LED TO THE DISCOVERY OF CERES

  18. www.softmatter.org COMMUNICATION

    E-Print Network [OSTI]

    Weibel, Douglas B.

    www.softmatter.org COMMUNICATION George M. Whitesides et al. Phase separation of 2D meso-scale Coulombic crystals from meso-scale polarizable `solvent' ISSN 1744-683X REVIEW Matthew F. Copeland

  19. Page 7 Page 8Page 8Page 4 Events and Research News in Engineering and Science Today www.ces.clemson.edu

    E-Print Network [OSTI]

    Duchowski, Andrew T.

    1993 to 2000. She was also the chief technology officer of nanoSEC, a startup company formed disciplines. I am a believer in the Clemson Top 20 plan. The potential for the college is tremendous for many technology officer of nanoSEC, a startup company formed to manufacture and market nanocomposites produced

  20. Page 246 Statistics Sonoma State University 2008-2010 Catalog Department Of mathematics anD statistics

    E-Print Network [OSTI]

    Ravikumar, B.

    Page 246 Statistics Sonoma State University 2008-2010 Catalog Department Of mathematics anD statistics Darwin Hall 114 phone: (707) 664-2368 fax: (707) 664-3535 www.sonoma.edu/math Department chair Ben Ford statistics prOGram aDvisOrs Susan Herring Elaine McDonald-Newman Cora Neal Scott Nickleach a

  1. The next generation of agricultural scientists 'show off'at the IOA Postgraduate Showcase. story page 8

    E-Print Network [OSTI]

    Tobar, Michael

    page 8 Dr Michael Chaney AO Chancellor,TheUniversityof Western Australia In this issue Challenges of Western Australia Newsletter Number 3 December 2007 www.ioa.uwa.edu.au #12;2 UWA Institute of Agriculture photo:BrendonCant Future economic growth in Australia will depend on the ability of Australia's major

  2. Page 118 Education: Educational Leadership and Special Education (ELSE) Sonoma State University 2008-2010 Catalog Department Office

    E-Print Network [OSTI]

    Ravikumar, B.

    are advised to consult the School of Education's Credential Office for updates on program details and policyPage 118 Education: Educational Leadership and Special Education (ELSE) Sonoma State University 2008-2010 Catalog Department Office Stevenson Hall 1078 (707) 664-4203 fax (707) 664-2483 www.sonoma.edu/education

  3. Symmetry, Integrability and Geometry: Methods and Applications SIGMA ? (200?), 00?, ?? pages Structure theory for second order 2D superintegrable

    E-Print Network [OSTI]

    Miller, Willard

    Symmetry, Integrability and Geometry: Methods and Applications SIGMA ? (200?), 00?, ?? pages online ???? Original article is available at http://www.emis.de/journals/SIGMA/200?/00?/ Abstract], for a precise definition, it has been shown that the algebra is finite dimensional and closes at order six

  4. Page 1 TXCRDC Notes on Computing in CRDCs Texas A&M University Census Research Data Center

    E-Print Network [OSTI]

    Bermúdez, José Luis

    ://www.stata.com/ #12;Page 2 ­ TXCRDC Notes on Computing in CRDCs R. R is a language and environment for statistical -------------------------- SAS, Stata, and R Special purpose statistical packages ----------------- HLM, SUDAAN Specialized code written for S runs unaltered under R. R provides a wide variety of statistical (linear

  5. Research Office/Wellcome Trust/13.04.11 Page 1 of 3 Wellcome Trust Investigator Awards

    E-Print Network [OSTI]

    Research Office/Wellcome Trust/13.04.11 Page 1 of 3 Wellcome Trust Investigator Awards Internal's Investigator Awards scheme are available at: http://www.wellcome.ac.uk/Funding/investigator-awards/index.htm 1) Funding available · award value will be in the range of Ł100k - Ł425k per year for up to 7 years · only

  6. 10/5/08 10:00 AMSeeing Red and Blue Can Divide a Species --of Fish -NYTimes.com Page 1 of 1http://www.nytimes.com/2008/10/07/science/07obfish.html?_r=1&ref=science&pagewanted=print&oref=slogin

    E-Print Network [OSTI]

    Carleton, Karen L.

    10/5/08 10:00 AMSeeing Red and Blue Can Divide a Species -- of Fish - NYTimes.com Page 1 of 1http Red and Blue Can Divide a Species -- of Fish By HENRY FOUNTAIN Geographic isolation is a driving force features. In the other, found in shallower waters, the males are blue. What's more, in some parts

  7. 9/25/10 12:27 PMLEED certification efforts remain strong -Dallas Business Journal Page 1 of 2http://www.bizjournals.com/dallas/stories/2010/08/02/story3.html?s=industry&b=1280721600%5E3731231&t=printable

    E-Print Network [OSTI]

    want LEED-certified buildings to save money on energy costs and to attract the nation's top talent9/25/10 12:27 PMLEED certification efforts remain strong - Dallas Business Journal Page 1 of 2http Larger Dallas Business Journal - August 2, 2010 /dallas/stories/2010/08/02/story3.html

  8. 024/01/Wednesday 17h44Geophysical Constraints on the Nature of Atlantis Massif, 30N MAR Page 1 sur 2http://www.agu.org/cgi-bin/SFgate/SFgate?language=English&verbo...%2034995275%20%2fdata2%2fepubs%2fwais%2fdata%2ffm05%2ffm05.txt

    E-Print Network [OSTI]

    Demouchy, Sylvie

    024/01/Wednesday 17h44Geophysical Constraints on the Nature of Atlantis Massif, 30°N MAR Page 1 sur AN: T33G-05 INVITED TI:Geophysical Constraints on the Nature of Atlantis Massif, 30° N MAR AU challenges prior interpretations that this OCC was mainly ultramafic, geophysical data having suggested much

  9. 08/04/2005 09:17 AMPentagon's New Goal: Put Science Into Scripts -New York Times Page 1 of 2http://www.nytimes.com/2005/08/04/movies/04flyb.html?ei=5070&en=ac6783c49c5cc94f&ex=1123819200&emc=eta1&pagewanted=print

    E-Print Network [OSTI]

    Valero-Cuevas, Francisco

    for help with accuracy. For now, though, the hopes of the Pentagon for a science-friendly cinema seem08/04/2005 09:17 AMPentagon's New Goal: Put Science Into Scripts - New York Times Page 1 of 2http=print August 4, 2005 Pentagon's New Goal: Put Science Into Scripts By DAVID M. HALBFINGER LOS ANGELES, Aug. 3

  10. Deformation of Compliant Fault Zones Induced by Nearby Earthquakes: Theoretical Investigations in Three Dimensions and Applications to The East California Shear Zone

    E-Print Network [OSTI]

    Kang, Jingqian

    2014-02-21T23:59:59.000Z

    Using dynamic modeling of earthquake rupture on a strike-slip fault and seismic wave propagation in a three dimensional inhomogeneous elastoplastic medium, I investigate the inelastic response of compliant fault zones to nearby earthquakes. I...

  11. For more travel information, please visit-www.ox.ac.uk/visitors_friends/maps_and_directions/directions.html

    E-Print Network [OSTI]

    Henderson, Gideon

    will be Friday 18 January 2013. The Department offers a wide range of Graduate Studies Projects. A list of projects can be found on the Department web page: www.earth.ox.ac.uk/graduate_admissions/graduate_projects_2013-14. You may apply for an existing project, or propose your own. Applications are invited from

  12. Texas Tech University Student Financial Aid & Scholarships 806-742-3144 | scholarships@ttu.edu | www.scholarships.ttu.edu

    E-Print Network [OSTI]

    Gelfond, Michael

    @ttu.edu | www.scholarships.ttu.edu West Hall 205 | Lubbock, TX 79409 page 1 as of 9/13/13 TEXAS TECH SCHOLARSHIPCONTACT US Texas Tech University Student Financial Aid & Scholarships 806-742-3144 | scholarships:00pm Address Address for Overnight Mail Texas Tech University Texas Tech University Scholarship Office

  13. www.water-alternatives.org Volume 4 | Issue 3 Aubriot, O. and Prabhakar, P.I. 2011. Water institutions and

    E-Print Network [OSTI]

    www.water-alternatives.org Volume 4 | Issue 3 Aubriot, O. and Prabhakar, P.I. 2011. Water institutions and the 'revival' of tanks in South India: What is at stake locally? Water Alternatives 4(3): 325-346 Aubriot and Prabhakar: The 'revival' of tanks in South India Page | 325 Water Institutions

  14. energy.gov -Speeches (Print Version) Tuesday, February 4, 2003 http://www.energy.gov/HQDocs/speeches/2003/febss/

    E-Print Network [OSTI]

    threats, and we have reduced the risk of accidents in nuclear fuel cycle facilities worldwide. Thanksenergy.gov - Speeches (Print Version) Tuesday, February 4, 2003 http://www.energy.gov/HQDocs/speeches/2003/febss/ 04BudgetPressConferenceRemarks_v.html Page: 1 Press Conference Remarks Energy Secretary

  15. www.kostic.niu.edu Nanofluids

    E-Print Network [OSTI]

    Kostic, Milivoje M.

    1 www.kostic.niu.edu 1 Nanofluids: Advanced Flow and Heat Transfer Fluids Prof. M. Kostic.kostic.niu.edu 2 Wet-Nanotechnology: nanofluids at NIU in collaboration with ANL www.kostic.niu.edu 3 First NIU Nanofluids www.kostic.niu.edu 4 Dry- vs. Wet-nanotechnology · Fluids (gases & liquids) vs. Solids in Nature

  16. 8/12/08 9:34 AMTo Swim Underwater, Some Insects Carry a Bubble as a Lung -NYTimes.com Page 1 of 2http://www.nytimes.com/2008/08/12/science/12insect.html?_r=1&oref=slogin&ref=science&pagewanted=print

    E-Print Network [OSTI]

    Flynn, Morris R.

    . As insects breathe in and out through tiny holes in the abdomen, oxygen decreases in the bubble and carbon8/12/08 9:34 AMTo Swim Underwater, Some Insects Carry a Bubble as a Lung - NYTimes.com Page 1 of 2=slogin&ref=science&pagewanted=print August 12, 2008 Come Up for Air? Not These Insects, Which Carry a Bubble as a Lung By KENNETH CHANG

  17. 12/2/08 11:41 AMOpen Membership -Rise of College Club Teams Creates a Whole New Level of Success -NYTimes.com Page 1 of 5http://www.nytimes.com/2008/12/02/sports/02club.html?_r=1&th=&emc=th&pagewanted=print

    E-Print Network [OSTI]

    Bradley, Elizabeth

    12/2/08 11:41 AMOpen Membership - Rise of College Club Teams Creates a Whole New Level of Success Membership - Rise of College Club Teams Creates a Whole New Level of Success - NYTimes.com Page 2 of 5http=&emc=th&pagewanted=print Open Membership Playing for the Love of the Sport December 2, 2008 OPEN MEMBERSHIP Rise of College Club

  18. 11/10/09 12:30 PMIraq Swears by Bomb Detector U.S. Sees as Useless -NYTimes.com Page 1 of 4http://www.nytimes.com/2009/11/04/world/middleeast/04sensors.html?_r=1

    E-Print Network [OSTI]

    Llope, William J.

    11/10/09 12:30 PMIraq Swears by Bomb Detector U.S. Sees as Useless - NYTimes.com Page 1 of 4http.Y. / REGION BUSINESS TECHNOLOGY SCIENCE HEALTH SPORTS OPINION ARTS STYLE TRAVEL JOBS REAL ESTATE AUTOS AFRICA Detector U.S. Sees as Useless Johan Spanner for The New York Times A device used by Iraqi forces to detect

  19. Datacenter Sustainability Page 1 Sustainability

    E-Print Network [OSTI]

    Chaudhuri, Surajit

    Datacenter Sustainability Page 1 Datacenter Sustainability #12;Datacenter Sustainability Page 2 sustainability imperative and how advanced technologies, smart business practices, and strategic partnerships are helping us reduce our impact on the environment. Also learn how our investments in efficient, sustainable

  20. ISO/TC 211/WG 9/N 014 Number of Pages:17

    E-Print Network [OSTI]

    Imai, Hiroshi

    ISO/TC 211/WG 9/N 014 2004-08-16 Number of Pages:17 ISO/TC 211 Geographic Information Distribution: Members of Working Group 9 ISO/TC 211 Secretariat ISO/TC 211/WG9 Convenor Telephone: + 81 3 5841://www-imai.is.s.u-tokyo.ac.jp/wg9/ #12;© ISO 2004 ­ All rights reserved Document type: International Standard Document subtype

  1. ISO/TC 211/WG 9/N 006 Number of Pages: 41

    E-Print Network [OSTI]

    Imai, Hiroshi

    ISO/TC 211/WG 9/N 006 2003-01-22 Number of Pages: 41 ISO/TC 211 Geographic Information of Working Group 9 ISO/TC 211 Secretariat ISO/TC 211/WG9 Convenor Telephone: + 81 3 5841 4117 Telefax: + 81 3 113-0033, Japan E-mail: imai@is.s.u-tokyo.ac.jp URL: http://www-imai.is.s.u-tokyo.ac.jp/wg9/ #12;© ISO

  2. ISO/TC 211/WG 9/N 002 Number of Pages: 19

    E-Print Network [OSTI]

    Imai, Hiroshi

    ISO/TC 211/WG 9/N 002 2002-05-30 Number of Pages: 19 ISO/TC 211 Geographic Information till 2002-06-14 Reference: None Distribution: Members of Working Group 9 ISO/TC 211 Secretariat ISO@is.s.u-tokyo.ac.jp URL: http://www-imai.is.s.u-tokyo.ac.jp/wg9/ #12;© ISO 2002 ­ All rights reserved ISO TC 211 N

  3. ISO/TC 211/WG 9/N 003 Number of Pages: 30

    E-Print Network [OSTI]

    Imai, Hiroshi

    ISO/TC 211/WG 9/N 003 2002-06-04 Number of Pages: 30 ISO/TC 211 Geographic Information: Members of Working Group 9 ISO/TC 211 Secretariat ISO/TC 211/WG9 Convenor Telephone: + 81 3 5841 4117://www-imai.is.s.u-tokyo.ac.jp/wg9/ #12;© ISO/IEC 2002 -- All rights reserved ISO/IEC TC 211/SC N Date: 2002-03-6 ISO-IEC_ ISO/IEC TC

  4. ISO/TC 211/WG 9/N 013 Number of Pages:20

    E-Print Network [OSTI]

    Imai, Hiroshi

    ISO/TC 211/WG 9/N 013 2004-08-07 Number of Pages:20 ISO/TC 211 Geographic Information Distribution: Members of Working Group 9 ISO/TC 211 Secretariat ISO/TC 211/WG9 Convenor Telephone: + 81 3 5841://www-imai.is.s.u-tokyo.ac.jp/wg9/ #12;© ISO 2004 ­ All rights reserved Document type: International Standard Document subtype

  5. ISO/TC 211/WG 9/N 005 Number of Pages: 60

    E-Print Network [OSTI]

    Imai, Hiroshi

    ISO/TC 211/WG 9/N 005 2002-08-26 Number of Pages: 60 ISO/TC 211 Geographic Information: Reference: None Distribution: Members of Working Group 9 ISO/TC 211 Secretariat ISO/TC 211/WG9 Convenor://www-imai.is.s.u-tokyo.ac.jp/wg9/ #12;© ISO 2002 -- All rights reserved ISO TC 211/SC N Date: 2002-08-26 ISO/WD 19131 ISO TC 211

  6. ISO/TC 211/WG 9/N 004 Number of Pages: 21

    E-Print Network [OSTI]

    Imai, Hiroshi

    ISO/TC 211/WG 9/N 004 2002-07-20 Number of Pages: 21 ISO/TC 211 Geographic Information action: Reference: None Distribution: Members of Working Group 9 ISO/TC 211 Secretariat ISO/TC 211/WG9://www-imai.is.s.u-tokyo.ac.jp/wg9/ #12;© ISO 2002 -- All rights reserved ISO TC 211/SC N 1310 Date: 2002-07-20 ISO/PDTS 19127 ISO TC

  7. ISO/TC 211/WG 9/N 016 Number of Pages: 87

    E-Print Network [OSTI]

    Imai, Hiroshi

    ISO/TC 211/WG 9/N 016 2004-10-28 Number of Pages: 87 ISO/TC 211 Geographic Information ISO/TC 211 Secretariat ISO/TC 211/WG9 Convenor Telephone: + 81 3 5841 4117 Telefax: + 81 3 5800 6933-8656, Japan E-mail: imai@is.s.u-tokyo.ac.jp URL: http://www-imai.is.s.u-tokyo.ac.jp/wg9/ #12;ISO/PDTS © ISO

  8. ISO/TC 211/WG 9/N 012 Number of Pages: 58

    E-Print Network [OSTI]

    Imai, Hiroshi

    ISO/TC 211/WG 9/N 012 2004-07-12 Number of Pages: 58 ISO/TC 211 Geographic Information of Working Group 9 ISO/TC 211 Secretariat ISO/TC 211/WG9 Convenor Telephone: + 81 3 5841 4117 Telefax: + 81 3 113-8656, Japan E-mail: imai@is.s.u-tokyo.ac.jp URL: http://www-imai.is.s.u-tokyo.ac.jp/wg9/ #12;ISO

  9. WVU NEURO-INTERN www.hsc.wvu.edu/wvucn/

    E-Print Network [OSTI]

    Mohaghegh, Shahab

    NEURO-INTERN www.hsc.wvu.edu/wvucn/ Summer-Internships-(SURI) WVU NEURO-INTERN www.hsc.wvu.edu/wvucn/ Summer-Internships-(SURI) WVU NEURO-INTERN www.hsc.wvu.edu/wvucn/ Summer-Internships-(SURI) WVU NEURO-INTERN www.hsc.wvu.edu/wvucn/ Summer-Internships-(SURI) WVU NEURO-INTERN www

  10. Library and Information Center http://www.library.gatech.edu

    E-Print Network [OSTI]

    Nair, Sankar

    Economy: http://www.fueleconomy.gov/ Historical Energy Data: http://www.eia.doe.gov/overview_hd.html Environment Day: http://www.nasa.gov/topics/earth/earthday/ Air AirBase: http://air-climate.eionet.europa.eu/databases/airbase/ AirNow: http://www.airnow.gov/ C-MAP: http://www.epa.gov/airmarkt/maps/c-map.html Climate Climate

  11. NEAT, An Astrometric Telescope To Probe Planetary Systems Down To The Earth Mass Around Nearby Solar-Type Stars

    E-Print Network [OSTI]

    Malbet, F; Goullioud, R; Shao, M; Lagage, P -O; Cara, C; Durand, G; Feautrier, P; Jakobsson, B; Hinglais, E; Mercier, M

    2011-01-01T23:59:59.000Z

    The NEAT (Nearby Earth Astrometric Telescope) mission is a proposition submitted to ESA for its 2010 call for M-size mission. The main scientific goal is to detect and characterize planetary systems in an exhaustive way down to 1 Earth mass in the habitable zone and further away, around nearby stars for F, G, and K spectral types. This survey would provide the actual planetary masses, the full characterization of the orbits including their inclination, for all the components of the planetary system down to that mass limit. Extremely- high-precision astrometry, in space, can detect the dynamical effect due to even low mass orbiting planets on their central star, reaching those scientific goals. NEAT will continue the work performed by Hipparcos (1mas precision) and Gaia (7{\\mu}as aimed) by reaching a precision that is improved by two orders of magnitude (0.05{\\mu}as, 1{\\sigma} accuracy). The two modules of the payload, the telescope and the focal plane, must be placed 40m away leading to a formation flying opt...

  12. Page1A.PDF

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level:Energy: Grid Integration Redefining What's Possible for RenewableSpeedingBiomassPPPO Website DirectoryCommunityFuture UseProbabilistic

  13. Tank Waste Committee Page 1

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

  14. Tank Waste Committee Page 1

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level:Energy: Grid Integration Redefining What'sis Taking Over Our InstagramStructureProposedPAGESafety Tag:8, 2013 FINAL MEETING

  15. PAGES_24X30poster

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level:Energy: Grid Integration Redefining What's Possible for RenewableSpeedingBiomass and BiofuelsOversightand Simulated TemperatureEnergybONTRACT

  16. Power Systems Group Home Page

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

    General Information ASD Groups ESHQA Operations Argonne Home > Advanced Photon Source > Power Systems Group This page is currently under construction. Old PS Group Site (visible...

  17. Kevin L. Rotz's Web Page

    E-Print Network [OSTI]

    Kevin's Page. My name is Kevin L. Rotz, and I am currently a sixth year graduate student in the Purdue University Department of Mathematics. During the spring ...

  18. Department of Energy Home Page

    Office of Scientific and Technical Information (OSTI)

    US DEPARTMENT OF ENERGY Search Home Page Contents ABOUT DOE About The Department of Energy (Learn about the Department of Energy, its mission, plans, organizational structure,...

  19. Hanford Advisory Board Page 1

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office of Science (SC) EnvironmentalGyroSolé(tm) Harmonic EngineHIV andApril 8-9, Advisory BoardPage 1

  20. Hanford Advisory Board Page 1

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office of Science (SC) EnvironmentalGyroSolé(tm) Harmonic EngineHIV andApril 8-9, Advisory BoardPage

  1. Sample page | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directedAnnual Siteof Energy 2,AUDITCalifornia Sector: WindRiegotec Internacionalhas been rated 13[1][2]

  2. TTW - PageMaker 2

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level:Energy: Grid Integration Redefining What'sis Taking Over Our InstagramStructureProposedPAGE Creating a Geologic Play-13, 2004OUR5, 2004 By

  3. TTW - PageMaker 2

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level:Energy: Grid Integration Redefining What'sis Taking Over Our InstagramStructureProposedPAGE Creating a Geologic Play-13, 2004OUR5, 2004 By2,

  4. TTW - PageMaker 2

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level:Energy: Grid Integration Redefining What'sis Taking Over Our InstagramStructureProposedPAGE Creating a Geologic Play-13, 2004OUR5, 2004

  5. Create Page | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directedAnnual Siteof Energy 2,AUDIT REPORTEnergy Offshore Place:WindOilCowal Wind Energy Ltd JumpCreate

  6. Final Meeting Summary Page 1

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOEThe Bonneville Power AdministrationField8,Dist.New Mexico Feb.Information 91, 20159, 2012Page 1 Health,

  7. WWW.G8.ARMY.MIL WWW.G8.ARMY.MIL

    E-Print Network [OSTI]

    US Army Corps of Engineers

    2014 WWW.G8.ARMY.MIL 2014 WWW.G8.ARMY.MIL Army EquipmEnt modErnizAtion plAn #12;The estimated cost .......................................................................................... 75 #12;#12;7 www.g8.army.mil The Army Equipment Modernization Plan 2014 describes the Army Research

  8. Mountain Promise page 1 ountain PromisM e

    E-Print Network [OSTI]

    Baltisberger, Jay H.

    Community supported agriculture page 6 Organic vs. conventional page 9 Industrial hemp page 12 toolbox

  9. Page 1 of 100 Full Screen

    E-Print Network [OSTI]

    Römisch, Werner

    ()d. #12;Home Page Title Page Contents Page 7 of 100 Go Back Full Screen Close Quit The behavior of bothHome Page Title Page Contents Page 1 of 100 Go Back Full Screen Close Quit Scenario Generation Uncertainty Quantification in Industrial and Energy Applications: Experiences and Challenges, Minneapolis

  10. CAIRNS: The Cluster And Infall Region Nearby Survey III. Environmental Dependence of H-alpha Properties of Galaxies

    E-Print Network [OSTI]

    Kenneth Rines; Margaret J. Geller; Michael J. Kurtz; Antonaldo Diaferio

    2005-06-27T23:59:59.000Z

    We investigate the environmental dependence of star formation in cluster virial regions and infall regions as part of CAIRNS (Cluster And Infall Region Nearby Survey), a large spectroscopic survey of the infall regions surrounding nine nearby rich clusters of galaxies. Our long-slit spectroscopy yields estimates of star formation rates in environments from cluster cores to the general large-scale structure. The fraction of galaxies with current star formation in their inner disks as traced by H-alpha emission increases with distance from the cluster and converges to the ``field'' value only at 2-3 virial radii, in agreement with other investigations. However, among galaxies with significant current star formation (EW[Ha]geq2\\AA), there is no difference in the distribution of EW[Ha] inside and outside the virial radius. This surprising result, first seen by Carter et al., suggests that (1) star formation is truncated on either very short timescales or only at moderate and high redshifts or (2) that projection effects contaminate the measurement. The number density profiles of star-forming and non-star-forming galaxies indicate that, among galaxies projected inside the virial radius, at least half of the former and 20% of the latter are ``infall interlopers,'' galaxies in the infall region but outside the virial region. The kinematics of star-forming galaxies in the infall region closely match those of absorption-dominated galaxies. This result shows that the star forming galaxies in the infall regions are not interlopers from the field and excludes one model of the backsplash scenario of galaxy transformation. Finally, we quantify systematic uncertainties in estimating the global star formation in galaxies from their inner disks.

  11. HIGH IONIZATION SPECIES IN THE NEARBY INTERSTELLAR MEDIUM FROM AN EXHAUSTIVE ANALYSIS OF THE IUE INES DATABASE

    SciTech Connect (OSTI)

    Freire Ferrero, R.; Halbwachs, J.-L. [Observatoire Astronomique, Universite de Strasbourg, 11 rue de l'Universite, 67.000 Strasbourg (France); Morales Duran, C.; Cabo Cubeiro, A. M., E-mail: rubens.freire@astro.unistra.fr, E-mail: jean-louis.halbwachs@astro.unistra.fr, E-mail: morales@cab.inta-csic.es, E-mail: amcabo@cab.inta-csic.es [LAEX, Centro de Astrobiologia (CAB, CSIC-INTA), LAEFF, European Space Astronomy Centre, P.O. Box 78, 28691 Villanueva de la Canada, Madrid (Spain)

    2012-02-15T23:59:59.000Z

    Main-sequence (MS) and giant late-B and early-A type stars are the best targets for searching for nearby interstellar (IS) Si IV and C IV resonance lines because they are not able to produce them, either in atmospheric layers or in their circumstellar environment, and because many stars of these spectral types are nearby and located in the local interstellar medium (LISM). In addition, the use of certain stars hotter than B6 can lead to misinterpretations (e.g., alpha Arae). This work analyzes the reliable Short-Wavelength Prime high-resolution UV spectra of 558 B6-A9 type stars observed by the International Ultraviolet Explorer at distances lower than 400 pc from the Sun. For the first time, this work utilizes the entire INES database to extract stellar and IS information in a systematic way from homogeneous data. Stars were classified into seven groups: normal (MS and subgiant), giant, peculiar, emission line, Algols, pre-main sequence or Herbig Ae/Be, and shell stars. Only 10 normal stars, located beyond 90 pc, show weak Si IV and C IV absorptions and are clustered around the direction of Sco-Cen, while 85 located closer than 90 pc, as well as another 89 beyond 90 pc, do not show any absorptions at all. We conclude that these highly ionized species originate most probably in the LISM, at 90 pc from the Sun, corresponding to the warm interaction zone (IZ), where the expanding Loop I super-shell and the Local Bubble collide. We base our results on a robust statistical analysis of both spectral types and spatial distributions of the different stellar groups we defined. Our estimated column densities N of both ions are similar to those obtained by other authors for distant stars, suggesting that these absorptions concentrate fundamentally in the IZ. A logarithmic correlation between N and the distance D confirms these results.

  12. Circumnuclear Dust in Nearby Active and Inactive Galaxies. II. Bars, Nuclear Spirals, and the Fueling of Active Galactic Nuclei

    E-Print Network [OSTI]

    Paul Martini; Michael W. Regan; John S. Mulchaey; Richard W. Pogge

    2002-12-17T23:59:59.000Z

    (Abridged) We present a detailed study of the relation between circumnuclear dust morphology, host galaxy properties, and nuclear activity in nearby galaxies. We use our sample of 123 nearby galaxies with visible--near-infrared colormaps from the Hubble Space Telescope to create well-matched, "paired" samples of 28 active and 28 inactive galaxies, as well as 19 barred and 19 unbarred galaxies, that have the same host galaxy properties. Comparison of the barred and unbarred galaxies shows that grand design nuclear dust spirals are only found in galaxies with a large-scale bar. Tightly wound nuclear dust spirals, in contrast, show a strong tendency to avoid galaxies with large-scale bars. Comparison of the AGN and inactive samples shows that nuclear dust spirals, which may trace shocks and angular momentum dissipation in the ISM, occur with comparable frequency in both active and inactive galaxies. The only difference between the active and inactive galaxies is that several inactive galaxies appear to completely lack dust structure in their circumnuclear region, while none of the AGN lack this structure. The comparable frequency of nuclear spirals in active and inactive galaxies, combined with previous work that finds no significant differences in the frequency of bars or interactions between well-matched active and inactive galaxies, suggests that no universal fueling mechanism for low-luminosity AGN operates at spatial scales greater than ~100 pc radius from the galactic nuclei. The similarities instead suggest that the lifetime of nuclear activity is less than the characteristic inflow time from these spatial scales. An order-of-magnitude estimate of this inflow time is the dynamical timescale. This sets an upper limit of several million years to the lifetime of an individual episode of nuclear activity.

  13. www.yorku.ca/research Ergonomics Laboratory

    E-Print Network [OSTI]

    www.yorku.ca/research Ergonomics Laboratory -- Biomechanics At York School of Kinesiology Salas The Ergonomics Laboratory creates healthier workplaces by reducing individuals' risk of developing

  14. Club! page 16 Using magnets

    E-Print Network [OSTI]

    Weston, Ken

    at the Magnet Lab like? Often, it's about solving problems. That's what engineers Scott Bole and Lee Marks didRobotics Club! page 16 Using magnets to analyze oil page 28 #12;editor's note What's a typical day recently. Their story began when Lee noticed something odd going on during a magnet-building project: When

  15. Page 1 of 3 INSTRUCTIONS

    E-Print Network [OSTI]

    McQuade, D. Tyler

    /Dean Alts · Click . · Enter SHARE for SetID if not prepopulated. · Search for and select the OMNI Userid/29/2008 The terms "Chair" and "Dean" are used generically to represent unit hierarchy. A new page (Grants. #12;Page 2 of 3 · Do not change Eff Date or Status. · Search for and select the OMNI Userid

  16. Web Page Error 404.1 Page Cannot be Found

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office of ScienceandMesa del SolStrengthening aTurbulenceUtilizeRuralthe emergency response assets of DOE and

  17. www.uscnorriscancerhospital.org i Inside: Empowered by Information, page 6 || A Concert to Cure Cancer, page 14

    E-Print Network [OSTI]

    Rohs, Remo

    Carmen A. Puliafito, M.D., M.B.A. Dean, Keck School of Medicine of USC Jane Brust Associate Senior Vice. Corey, M.D. Marshall Ezralow Quinn Ezralow Larry J. Freeman Tom Fuelling Peter A. Jones, Ph.D., D

  18. Serving the Marshall Space Flight Center Community www.nasa.gov/centers/marshall/about/star/index.html June 5, 2013 Inside This Issue

    E-Print Network [OSTI]

    Serving the Marshall Space Flight Center Community www.nasa.gov/centers/marshall/about/star/index.html June 5, 2013 Inside This Issue: Turn It Off, Marshall Simple Power Conservation Could Save $1.5M: Ned Wright on Exploring the Universe with WISE page 6 Check us out online! Scan the QR code Marshall

  19. http://www.LearnerAssociates.net This Dissertation/Thesis Guide has been created to assist graduate students in the successful

    E-Print Network [OSTI]

    Sheridan, Jennifer

    http://www.LearnerAssociates.net 1 This Dissertation/Thesis Guide has been created to assist its sale. Page 1 Writing and Presenting Your Thesis or Dissertation1 S. Joseph Levine, Ph.D. Michigan a thesis or dissertation in areas related to the discipline of adult learning. It has been my purpose

  20. U.S. to Participate in Fusion Project Thursday, January 30, 2003 http://www.nytimes.com/aponline/national/AP-Fusion-Energy-Plan.html?pagewanted=

    E-Print Network [OSTI]

    States plan to build a $5 billion fusion reactor, called the International Thermonuclear ExperimentalU.S. to Participate in Fusion Project Thursday, January 30, 2003 http://www.nytimes.com/aponline/national/AP-Fusion-Energy-Plan.html?pagewanted= print&position=top Page: 1 January 30, 2003 U.S. to Participate in Fusion Project By THE ASSOCIATED

  1. Theorizing the carbon economy: introduction to the special issue The term `carbon economy'often has an adjective placed nearby: the `new'carbon economy,

    E-Print Network [OSTI]

    of carbon capture and storage and nuclear technologies. These dimensionsöand surface-level to deeperTheorizing the carbon economy: introduction to the special issue The term `carbon economy'often has an adjective placed nearby: the `new'carbon economy, the `low' carbon economy, the carbon `neutral' economy

  2. www.mmu.ac.uk/careers Careers & Employability Service

    E-Print Network [OSTI]

    .mmu.ac.uk/careers Identifying courses · www.prospects.ac.uk/search_courses.htm · www.jobs.ac.uk · www.Findamasters.com · www.mmu.ac.uk/careers PG Professional/Vocational courses: Courses to allow you to enter certain professions Courses involve lectures for the first two terms then a research project for the final term (often finishing after

  3. NREL: Biomass Research Home Page

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office of Science (SC)Integrated CodesTransparency Visit | National Nuclear13 DenverIntegratedPhoto of a

  4. NREL: Buildings Research Home Page

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office of Science (SC)Integrated CodesTransparency Visit | National Nuclear13 DenverIntegratedPhoto of

  5. NREL: Computational Science Home Page

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    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office of Science (SC)Integrated CodesTransparency Visit | National Nuclear13 DenverIntegratedPhoto

  6. NREL: Continuum Magazine Home Page

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    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office of Science (SC)Integrated CodesTransparency Visit | National Nuclear13Summer 2015 / Issue 8

  7. NREL: Continuum Magazine Home Page

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office of Science (SC)Integrated CodesTransparency Visit | National Nuclear13Summer 2015 / Issue 8Spring

  8. NREL: Continuum Magazine Home Page

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office of Science (SC)Integrated CodesTransparency Visit | National Nuclear13Summer 2015 / Issue 8Spring

  9. NREL: Education Center Home Page

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

  10. NREL: Geothermal Technologies Home Page

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

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

  11. NREL: International Activities Home Page

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

  12. NREL: Research Facilities Home Page

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

  13. NREL: Solar Research Home Page

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

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

  14. NREL: Sustainable NREL Home Page

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  15. NREL: Technology Deployment Home Page

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  16. NREL: Technology Transfer Home Page

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  17. NREL: Transportation Research Home Page

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  18. Hanford Advisory Board Page 1

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  19. Hanford Advisory Board Page 1

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    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office of Science (SC) EnvironmentalGyroSolé(tm) Harmonic EngineHIV andApril 8-9, 2015 FINAL MEETINGMarch

  20. Hanford Advisory Board Page 1

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office of Science (SC) EnvironmentalGyroSolé(tm) Harmonic EngineHIV andApril 8-9, 2015 FINAL