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State Name

Text Exerpt

California

SimilarPDF Deciphering Seismic Data 20-percent increase in renewable energy production by 2010 with an accelerated target of 33 percent .. and gravitational wave detection. Worlds Most Sensitive Detector For further information contact Darin Kinion 925-422-8798 https://str.llnl.gov/Mar09/pdfs/03.09.pdfPDF BAT Slew Survey BATSS and Gravitational Wave telescopes. Soft Gamma-ray Repeaters SGRs: 300-700 GRBs/yr 6X Swift/BAT rate and 30000 AGN: IRT redshifts for most! detector/telescope prototype for balloon-borne ProtoEXIST1 ProtoEXIST1 balloon flight in 2009 ProtoEXIST2 in 2010 to establish readiness

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exist.gsfc.nasa.gov/papers/aas  SimilarPDF Deciphering Seismic Data 20-percent

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California

Of the Signatures and Environments of .. OF SCIENCES ASTRONOMY AND ASTROPHYSICS SURVEY 2010 The subject matter of ERA 0043155780000-800120-617-621 BOY GRADUATE STUDIES BLDG 0-0 USAUS 43. . BROWNSVILLE CENTER FOR GRAVITATIONAL WAVE ASTRONOMY This proposal seeks www.usaspending.gov/ /NASA_ASSISTANCE_2009.10.19_ACCEPTED_TRANSACTIONS.txt Cassini Status. Titan Flyby 1073 km 667 mi Jan 12-2010 SCET Guy Webster/JPL 818-354-6278. Barely perceptible fluctuations in the speed of a Earth could provide sciences first direct detection of gravitational waves Cassini enabling the gravitational-wave experiment to use higher-frequency radio saturn.jpl.nasa.gov News Features News Releases Cassini Status. Titan Flyby 1073 km 667 mi Jan 12-2010 SCET Cassinis Gravitational Wave Experiment GWE completed on Jan 5. The Radio Science team was very pleased Latchup detection algorithm and thresholds for the Cosmic Dust Analyzer and 91109. Telephone 818-354-5011. Five Most Read Stories saturn.jpl.nasa.gov News Features Significant Events connected economic development experts at 337-593-1400 or go to the Lafayette Economic Ares I will replace the current space shuttles beginning in 2010 . in Livingston is dedicated to the detection of cosmic gravitational is a vital member in a developing global network of gravitational wave www.lafayettela.gov/pdf/presidents/lra_brochure.pdfRefereed Publications Resulting from Computations at NERSC 252:395-415-2008 Computational studies of the O2-evolving complex of Oceanic Ambient Noise as Background to Acoustic Neutrino Detection N. in the National Interest Plasma 2010 Committee Plasma Science Committee and H.-T. Janka The Gravitational Wave Burst Signal from Core Collapse of

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www.nersc.gov/projects/reports/ERCAPpubs08.php  AND SPACE ADMINISTRATION WI Detection

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California

V10.5.qxp Launch Date: January 2010. Design Life: 2 years. Measurements: Magnetic and .. Altitude: 400-700 km. Inclination: 13. Launch Date: January 1-2007. Design Life: 3 years . EFD Electric Field Detector. EPIC Energetic Particles and Ion Composition GWE Gravitational Wave Experiment. GLG/SWICS www.coastal.ssc.nasa.gov/ /Space20Observation20Systems20Booklet20v10.5.pdfCassini Equinox Mission: Significant Event Report for Week Ending Cassini Status. Titan Flyby 1073 km 667 mi Jan 12-2010 SCET data show preliminary detection of the synchrotron emission of high-energy electrons in the Jovian radiation belts. is an enabling system for the Gravitational Wave Experiment to be 91109. Telephone 818-354-5011. Five Most Read Stories

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cassini-2.jpl.nasa.gov/news/significantevents/sigevent20010202/  SimilarPDF Space Observation Systems Booklet

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District of Colombia - Washington DC

Similar separations would indicate the passage of a gravitational wave. .. station-serviced x-ray observatory would make possible the detection of very of the late 1990s to full capability to support the Bridge between Worlds before 2010. 0-365-738. Washington D.C.: U.S. Government Printing Office 1969. www.nasa.gov/ /383341main_6020-2020090814.5.The20Report20of20the20National20Commission20on SimilarPDF FISCAL YEAR will be the first space-based gravitational wave observatory. .. n Phone : 202-327-6000. V . ww.ey .com. Report of Independent Auditors managing the transition through the 5-year gap period 20102015 .. In FY 2007 our audit of the incident detection and response process and the results of the www.nasa.gov/ /202959main_NASA20FY07_Financial_Report_Addendum.pdf Similar 9-2008 Huston Ian Gravitational Wave Constraints on Multi-Brane 1076-2007 Chernin A.D. Detection of dark energy near the Local Group 2010-2006 Kainulainen Kimmo The WIMP of a Minimal Technicolor Theory .. X-Ray spectral variability of the radio-loud NLS1 galaxy PKS 0558-504 wmap.gsfc.nasa.gov/references.html SimilarPDF Aeronautics and Space Report of the President by 2010. Atlantis delivered the critical P3/P4 truss to the ISS to the design of reliable smoke detection for long-duration space missions and . Boeing 737 and 767-400 a Bombardier Global 5000 business jet an Airborne of 98 bolometers to probe directly for the gravitational wave signature of history.nasa.gov/presrep2006.pdf SimilarPDF NASA Scientific and Technical Aerospace Reports helpsti.nasa.gov or telephone the STI Help Desk at 443-757-5802. By 2010 the Marine Corps will also field an organic Tier II capability resident required for spaceborne gravitational wave detection: it will put two test www.sti.nasa.gov/Pubs/star/star0923.pdfPDF NASA Scientific and Technical Aerospace Reports by STI NASA Related articles All 33 versions helpsti.nasa.gov or telephone the STI Help Desk at 443-757-5802. sufficient for gravitational wave detection. SOP-I1 in 2010. Modeling and satellite data utilization studies will continue throughout the entire period to

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www.sti.nasa.gov/Pubs/star/star0824.pdf  Similar separations would indicate the

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Florida

At NERSC 100-786-800-2006 Characterization of Synthetic Oxomanganese Complexes and the . Yoon et al. The Robinson Gravitational Wave Background Telescope BICEP: a Ambient Noise as Background to Deep Ocean Transient Signal Detection Plasma 2010 Committee Plasma Science Committee National Research

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www.nersc.gov/projects/reports/ERCAPpubs07.php  SimilarRefereed Publications Resulting from Computations

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Illinois

Similar makes for direct and indirect dark matter detection and about the detailed properties of dark-matter 2010. Beyond this the network capacity will have to increase Approaches to the Delta I1/2 rule. Nuclear Physics B 514:313-335. . Listening to the Universe with Gravitational-Wave Astronomy. www.er.doe.gov/ascr/ProgramDocuments/Docs/HEPReport.pdfPDF Report to the Nuclear Science Advisory Committee gravitational wave emission in rapidly rotating neutron stars. strained then precision X-ray observations and possible future detection of gravitational wave This facility could be operational around 2010 and if Fax: 630-252-3903. Email: geesamananl.gov. Charles Glashausser www.er.doe.gov/np/nsac/docs/nsac-report-final1_Tribble.pdf REMOTE SENSING AT THE ULTIMATE LIMIT by DON AJ11 Related articles All 2 versions baseline of comparison was a standard two-mode coherent Light Detection at the laser interferometer gravitational wave observatory LIGO or on based on shared prior entanglement Physical Review Letters 85-9: 20102013 Aug 28-2000. . photons from a single-photon device Nature Vol 419: 594597

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www.dtic.mil/cgi-bin/GetTRDoc?LocationU2docGetTRDoc  Similar makes for direct and

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Text Exerpt

Louisiana

574-1001. On the Web: www.ornl.gov/reporter .. recorded gravitational wave event. The tubes of the detector are an L-shape because . these technologies marketable by 2010. www.ornl.gov/reporter/no39/july02.pdfLivingston Parish The Laser Interferometer Gravitational-Wave Observatory LIGO is a facility dedicated to the detection of cosmic gravitational waves and the harnessing of these waves for scientific Presidents Office 225-686-2266. Sheriffs Office 225-686-2241 Copyright 2010 Livingston Parish. All Rights Reserved. www.livingstonparishla.gov/default.aspx SimilarPDF Report from the SEUS Mar 25-2003 flown in the 2010-2020 time frame. The proposed mission has a 4 arc-minute . supersedes the Nuclear Systems Initiative and provides 250-500 kW ! . A gravitational wave detector LISA and exquisitely sensitive X-heseweb.nrl.navy.mil/gamma/dermer/commit/SEUS/SEUS_rpt_2-1.pdfPDF MAJOR RESEARCH EQUIPMENT FY 2004 Current FY 2006 FY 2007 FY 2008 FY 2009 FY 2010 going from about 160 ship operating days with the Alpha Helix up to 275-300 days with the ARRV. the most sensitive gravitational wave detector possible on Earth. www.kopio.bnl.gov/fy06_nsf.pdfPDF THE STATUS OF VIRGO by F Acernese 2007 Cited by 122 Related articles All 26 versions potential gravitational wave signal detection should be with the goal to start the engineering phase in 2010. REFERENCES 23-2005-557-565. 6 L.Barsotti et al. Proceedings of the 6th Amaldi. Conference ics-web4.sns.ornl.gov/icalepcs07/TOAB05/TOAB05.PDFPhysical Review D Phys. Rev. D 81-011501 Published Mon Jan 11-2010 section in pp collisions at sqrts 1.96 TeV using the CDF detector .. Discriminating strange star mergers from neutron star mergers by gravitational-wave measurements . M2GeV 291.4439.9 in contradiction with the established lower bound on M2. infolink.sandia.gov:8199/sfx_local? SimilarPDF Cavity QED Approaches Quantum Information Processing Quantum Computing by Q Computing Related articles All 6 versions Laser Interferometer Gravitational Wave Observatory . 5.2 Cavity QED itself provides an excellent single atom detector that could be employed . 2002-2003-2004-2005-2006-2007-2008-2009-2010-2011-2012 . of a one-atom laser in the regime of strong coupling Nature 425-268271-2003.

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qist.lanl.gov/pdfs/cavity_qed.pdf  Phone 576-0470. E-mail barnesdsornl.gov fax:

State Name

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Maryland

A Non Sequitur Proverb: fashion alliterative imputable choice Region by CE Dorman 2001 All 4 versions and the ST Strategy to 2010 additional documents it would be good to have 301-227-5565 which should make it easy to follow up from ONR Hq. . lasers including a competitor for the LIGO gravitational wave detection program.

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www.dtic.mil/cgi-bin/GetTRDoc?ADADA442656LocationU2  PDF ST in the Asia-Pacific

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Maryland

LISA T.Stebbinsnasa.gov 1-301-286-3642 laser system expected by 2010. Laser Frequency. Noise Mitigation. Reduce laser frequency noise LISA Proposal for a Laser-Interferometric Gravitational Wave Detector in Space lisa.gsfc.nasa.gov/Documentation/Astro2010_RFI2_LISA.pdfPDF March 27-2009 Dear Astro2010 Committee: Thank-you for the Doug Burke Chandra X-ray Centre Astro 2010 Town Hall meeting .. Italy VIRGO will be detecting the gravitational wave chirps from neutron . temperatures with any set of line fluxes and any detector that same However the inversion is not an easy problem see Kashyap Drake 1998ApJ 503-450 Judge ixo.gsfc.nasa.gov/decadal /PDFs/astro2010TownHallMA_final.pdf SimilarPDF Conference Guide with Abstracts Fax: 865.329.0422. Mailing Address: P.O. Box 2543 Virgo is the largest gravitational wave detec-tor in Europe. detector. All actions initiated by the operator and horizon in 2010 the FIP market will be uncer-neutrons.ornl.gov/conf/icalepcs07/icalepcs07_guide.pdfPDF the way to Installation of core optics for the Laser Interferometer Gravitational Wave. Observatory. . Simulated response of linear collider detector to the production of two Z bosons. Each .. 250-500 GeV with an eventual goal of reaching the TeV region. .. double the federal research and development budget by 2010.

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www.fnal.gov/pub/forphysicists/hepapbook/  SimilarPDF Laser Interferometer Space Antenna

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New Mexico

Sufficient to provide policy makers and funding agencies with enough .. detectors. This study will allow a coherent and well-Neutrino oscillations in Venice 505-513-2006. .. In combination with electromagnetic and perhaps gravitational-wave observations a true

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lartpc-docdb.fnal.gov/0002/000256/003/LAGUNA-FP7_PartB.pdf  2010 a full conceptual design

State Name

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Ohio

2010. Dayton OH 45459-4248-937-433-2886 Antenna LISA gravitational wave detection experiment where extremely precise

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sbir.nasa.gov/SBIR/abstracts/08-1.html  240 W Elmwood Drive Suite

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Other

By LIS Antenna Related articles Tel: 49-511-762-2229. Fax: 49-511-762-2784 e-mail: kvdmpq.mpg.de . 20052010 would be ideal from the point of view of technological The earliest concept for a laser gravitational wave detector in space appears to have

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maxim.gsfc.nasa.gov/documents/Mission  by LIS Antenna Related articles

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Virginia

Similarnsf.gov News US National Science Foundation NSF National Science Board Releases Science and Engineering Indicators 2010. Released January 15-2010 Astronomers Get New Tools for Gravitational-wave Detection Tel: 703-292-5111 FIRS: 800-877-8339 TDD: 800-281-8749

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www.nsf.gov/news/  Similarnsf.gov News US National Science