Journal/ Conference	Pub Date	Title	Author(s)	Author Affiliation	Copyright Assertion	DOI	Author categories	Textual Evidence	Work of Gov't Disclaimer	Other Disclaimers	Preparers Comments
Phys. Rev. Lett. 104, 091302	Mar-10	Fermi Large Area Telescope Search for Photon Lines from 30 to 200 GeV and Dark Matter Implications	A. A. Abdo,1,2 M. Ackermann,3 M. Ajello,3 W. B. Atwood,4 L. Baldini,5 J. Ballet,6 G. Barbiellini,7,8 D. Bastieri,9,10 K. Bechtol,3 R. Bellazzini,5 B. Berenji,3 E. D. Bloom,3,* E. Bonamente,11,12 A. W. Borgland,3 A. Bouvier,3 J. Bregeon,5 A. Brez,5 M. Brigida,13,14 P. Bruel,15 T. H. Burnett,16 S. Buson,10 G. A. Caliandro,17 R. A. Cameron,3 P. A. Caraveo,18 S. Carrigan,10 J. M. Casandjian,6 C. Cecchi,11,12 O¨ . C¸ elik,19,20,21 A. Chekhtman,1,22 J. Chiang,3 S. Ciprini,12 R. Claus,3 J. Cohen-Tanugi,23 J. Conrad,24,25,26,† C. D. Dermer,1 A. de Angelis,27 F. de Palma,13,14 S. W. Digel,3 E. do Couto e Silva,3 P. S. Drell,3 A. Drlica-Wagner,3 R. Dubois,3 D. Dumora,28,29 Y. Edmonds,3 R. Essig,3 C. Farnier,23 C. Favuzzi,13,14 S. J. Fegan,15 W. B. Focke,3 P. Fortin,15 M. Frailis,27 Y. Fukazawa,30 S. Funk,3 P. Fusco,13,14 F. Gargano,14 D. Gasparrini,31 N. Gehrels,19,32,33 S. Germani,11,12 N. Giglietto,13,14 F. Giordano,13,14 T. Glanzman,3 G. Godfrey,3 I. A. Grenier,6 J. E. Grove,1 L. Guillemot,34 S. Guiriec,35 M. Gustafsson,10,9 D. Hadasch,36 A. K. Harding,19 D. Horan,15 R. E. Hughes,37 M. S. Jackson,25,38 G. Jo´hannesson,3 A. S. Johnson,3 R. P. Johnson,4 W. N. Johnson,1 T. Kamae,3 H. Katagiri,30 J. Kataoka,39 N. Kawai,40,41 M. Kerr,16 J. Kno¨dlseder,42 M. Kuss,5 J. Lande,3 L. Latronico,5 M. Llena Garde,24,25 F. Longo,7,8 F. Loparco,13,14 B. Lott,28,29 M. N. Lovellette,1 P. Lubrano,11,12 A. Makeev,1,22 M. N. Mazziotta,14 J. E. McEnery,19,33 C. Meurer,24,25 P. F. Michelson,3 W. Mitthumsiri,3 T. Mizuno,30 A. A. Moiseev,20,33 C. Monte,13,14 M. E. Monzani,3 A. Morselli,43 I. V. Moskalenko,3 S. Murgia,3 P. L. Nolan,3 J. P. Norris,44 E. Nuss,23 T. Ohsugi,30 N. Omodei,5 E. Orlando,45 J. F. Ormes,44 M. Ozaki,46 D. Paneque,3 J. H. Panetta,3 D. Parent,28,29 V. Pelassa,23 M. Pepe,11,12 M. Pesce-Rollins,5 F. Piron,23 S. Raino`,13,14 R. Rando,9,10 M. Razzano,5 A. Reimer,47,3 O. Reimer,47,3 T. Reposeur,28,29 J. Ripken,24,25 S. Ritz,4 A. Y. Rodriguez,17 M. Roth,16 H. F.-W. Sadrozinski,4 A. Sander,37 P. M. Saz Parkinson,4 J. D. Scargle,48 T. L. Schalk,4 A. Sellerholm,24,25 C. Sgro`, 5 E. J. Siskind,49 D. A. Smith,28,29 P. D. Smith,37 G. Spandre,5 P. Spinelli,13,14 J.-L. Starck,6 M. S. Strickman,1 D. J. Suson,50 H. Tajima,3 H. Takahashi,30 T. Tanaka,3 J. B. Thayer,3 J. G. Thayer,3 L. Tibaldo,9,10,6 D. F. Torres,36,17 Y. Uchiyama,3 T. L. Usher,3 V. Vasileiou,20,21 N. Vilchez,42 V. Vitale,43,51 A. P. Waite,3 P. Wang,3 B. L. Winer,37 K. S. Wood,1 T. Ylinen,38,52,25 and M. Ziegler4	1 Space Science Division, Naval Research Laboratory, Washington, D.C. 20375, USA 2 National Research Council Research Associate, National Academy of Sciences, Washington, D.C. 20001, USA 3 W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, California 94305, USA 4 Santa Cruz Institute for Particle Physics, Department of Physics and Department of Astronomy and Astrophysics, University of California at Santa Cruz, Santa Cruz, California 95064, USA 5 Istituto Nazionale di Fisica Nucleare, Sezione di Pisa, I-56127 Pisa, Italy 6 Laboratoire AIM, CEA-IRFU/CNRS/Université Paris Diderot, Service d’Astrophysique, CEA Saclay, 91191 Gif sur Yvette, France 7 Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, I-34127 Trieste, Italy 8 Dipartimento di Fisica, Università di Trieste, I-34127 Trieste, Italy 9 Istituto Nazionale di Fisica Nucleare, Sezione di Padova, I-35131 Padova, Italy 10 Dipartimento di Fisica “G. Galilei”, Università di Padova, I-35131 Padova, Italy 11 Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, I-06123 Perugia, Italy 12 Dipartimento di Fisica, Università degli Studi di Perugia, I-06123 Perugia, Italy 13 Dipartimento di Fisica, “M. Merlin” dell’Università e del Politecnico di Bari, I-70126 Bari, Italy 14 Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70126 Bari, Italy 15 Laboratoire Leprince-Ringuet, École polytechnique, CNRS/IN2P3, Palaiseau, France, USA 16 Department of Physics, University of Washington, Seattle, Washington 98195-1560, USA 17 Institut de Ciencies de l’Espai (IEEC-CSIC), Campus UAB, 08193 Barcelona, Spain 18I NAF-Istituto di Astrofisica Spaziale e Fisica Cosmica, I-20133 Milano, Italy 19 NASA Goddard Space Flight Center, Greenbelt, Maryland 20771, USA 20 Center for Research and Exploration in Space Science and Technology (CRESST) and NASA Goddard Space Flight Center, Greenbelt, Maryland 20771, USA 21 Department of Physics and Center for Space Sciences and Technology, University of Maryland Baltimore County, Baltimore, Maryland 21250, USA 22 George Mason University, Fairfax, Virginia 22030, USA 23 Laboratoire de Physique Théorique et Astroparticules, Université Montpellier 2, CNRS/IN2P3, Montpellier, France 24 Department of Physics, Stockholm University, AlbaNova, SE-106 91 Stockholm, Sweden 25 The Oskar Klein Centre for Cosmoparticle Physics, AlbaNova, SE-106 91 Stockholm, Sweden 26 Royal Swedish Academy of Sciences Research Fellow, funded by a grant from the K. A. Wallenberg Foundation 27 Dipartimento di Fisica, Università di Udine and Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, Gruppo Collegato di Udine, I-33100 Udine, Italy 28 Université de Bordeaux, Centre d’Études Nucléaires Bordeaux Gradignan, UMR 5797, Gradignan, 33175, France 29 CNRS/IN2P3, Centre d’Études Nucléaires Bordeaux Gradignan, UMR 5797, Gradignan, 33175, France 30 Department of Physical Sciences, Hiroshima University, Higashi-Hiroshima, Hiroshima 739-8526, Japan 31 Agenzia Spaziale Italiana (ASI) Science Data Center, I-00044 Frascati (Roma), Italy 32 Department of Astronomy and Astrophysics, Pennsylvania State University, University Park, Pennsylvania 16802, USA 33 Department of Physics and Department of Astronomy, University of Maryland, College Park, Maryland 20742, USA 34 Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany 35 Center for Space Plasma and Aeronomic Research (CSPAR), University of Alabama in Huntsville, Huntsville, Alabama 35899, USA 36 Institució Catalana de Recerca i Estudis Avançats (ICREA), Barcelona, Spain 37 Department of Physics, Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, Ohio 43210, USA 38 Department of Physics, Royal Institute of Technology (KTH), AlbaNova, SE-106 91 Stockholm, Sweden 39 Waseda University, 1-104 Totsukamachi, Shinjuku-ku, Tokyo, 169-8050, Japan 40 Department of Physics, Tokyo Institute of Technology, Meguro City, Tokyo 152-8551, Japan 41 Cosmic Radiation Laboratory, Institute of Physical and Chemical Research (RIKEN), Wako, Saitama 351-0198, Japan 42 Centre d’Étude Spatiale des Rayonnements, CNRS/UPS, BP 44346, F-30128 Toulouse Cedex 4, France 43 Istituto Nazionale di Fisica Nucleare, Sezione di Roma “Tor Vergata”, I-00133 Roma, Italy 44 Department of Physics and Astronomy, University of Denver, Denver, Colorado 80208, USA 45 Max-Planck Institut für Extraterrestrische Physik, 85748 Garching, Germany 46 Institute of Space and Astronautical Science, JAXA, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8510, Japan 47 Institut für Astro- und Teilchenphysik and Institut für Theoretische Physik, Leopold-Franzens-Universität Innsbruck, A-6020 Innsbruck, Austria 48 Space Sciences Division, NASA Ames Research Center, Moffett Field, California 94035-1000, USA 49 NYCB Real-Time Computing Inc., Lattingtown, New York 11560-1025, USA 50 Department of Chemistry and Physics, Purdue University Calumet, Hammond, Indiana 46323-2094, USA 51 Dipartimento di Fisica, Università di Roma “Tor Vergata”, I-00133 Roma, Italy 52 School of Pure and Applied Natural Sciences, University of Kalmar, SE-391 82 Kalmar, Sweden	©2010 The American Physical Society	10.1103/PhysRevLett.104.091302	Employee	1 Space Science Division, Naval Research Laboratory, Washington, D.C. 20375, USA 19 NASA Goddard Space Flight Center, Greenbelt, Maryland 20771, USA 20 Center for Research and Exploration in Space Science and Technology (CRESST) and NASA Goddard Space Flight Center, Greenbelt, Maryland 20771, USA 48 Space Sciences Division, NASA Ames Research Center, Moffett Field, California 94035-1000, USA	No	N/A
Advances in Space Research Volume 14, Issue 2, February 1994, Pages 137-146	Feb-94	Overview of the NASA balloon R&D program	I.Steve Smith Jr	National Aeronautics and Space Administration, Goddard Space Flight Center, Wallops Flight Facility, Wallops Island, VA 23337, U.S.A.	Copyright © 1993 Published by Elsevier Ltd.	10.1016/0273-1177(94)90080-9	Employee	National Aeronautics and Space Administration, Goddard Space Flight Center, Wallops Flight Facility, Wallops Island, VA 23337, U.S.A.	No	N/A
AIP Conference Proceedings 1358, 130 (2011)	Aug-11	GRB 081029: Understanding Multiple Afterglow Components	S. T. Holland a,c, M. De Pasquale d, J. Mao e, T. Sakamoto a,c, P. Schady g,d, S. Covino e, P. D’Avanzo e, A. Antonelli h, V. D’Elia h, G. Chincarini e, F. Fiore h, and S. B. Pandey i	a Centre for Research and Exploration in Space Science and Technology, NASA/GSFC, Greenbelt, MD 20771, USA b Universities Space Research Association, 10211 Winicopin Circle, Columbia, MD 21044, USA c Code 660.1, NASA/GSFC, Greenbelt, MD 20771, USA d Mullard Space Science Laboratory, University College London, Holmbury, St Mary, Dorking, Surrey, RH5 6NT, UK e INAF‐Osservatorio Astronomico di Brera, Via Emilio Bianchi 46, I‐23807 Merate (LC), Italy f Joint Centre for Astrophysics, University of Maryland, Baltimore County, 1000 Hilltop Circle, Baltimore, MD 21250, USA g Max‐Planck Institut fur Extraterrestrische Physik, Giessenbachstraße, 85748 Garching, Germany h INAF‐Osservatorio Astronomico di Roma, Via de Frascati 33, I‐00040 Monteporzio Catone (Roma), Italy i Randall Laboratory of Physics, University of Michigan, 450 Church St, Ann Arbor, MI 48109‐1040, USA	© 2011 American Institute of Physics	10.1063/1.3621754	Employee	a Centre for Research and Exploration in Space Science and Technology, NASA/GSFC, Greenbelt, MD 20771, USA c Code 660.1, NASA/GSFC, Greenbelt, MD 20771, USA	No	We acknowledge the use of public data from the Swift Data Archive. This work is based in part on observations taken with the ROTSE-IIIc telescope in Namibia, the REM telescope at la Silla Observatory, and with ESO Telescopes at the Paranal Observatories.
Journal of Geophysical Research: Space Physics (1978–2012) > Vol 88 Issue A7	Jul-83	Factors controlling the location of the Venus bow shock	1) M. TATRALLYAY AND C. T. RUSSELL; 2) J. D. MIHALOV AND A. BARNES	1) Institute of Geophysics and Planetary Physics, University of California, LosAngeles, California 90024; 2) NASA/Ames Research Center, Moffett Field, California 94035	Copyright 1983 by the American Geophysical Union.	10.1029/JA088iA07p05613	Employee	2) NASA/Ames Research Center, Moffett Field, California 94035	No	Acknowledgments. We are grateful to R. C. Elphic, J. G. Luhmann, J. A. Slavin, and T. I. Gombosi for useful discussions of this work. We are also grateful to L. H. Brace, who not only shared his ideas but freely exchanged with us his observations of the location of the bow shock for cross checking with ours. This work was supported by the National Aeronautics and Space Administration under contract NAS5-9491
The Astrophysical journal	Sep-90	Velocity-resolved far-infrared spectra of forbidden Fe II - Evidence for mixing and clumping in SN 1987A				10.1086/169115	No Access
Proc. SPIE 4360, Thermosense XXIII, 616	Mar-01	Synchronized electronic shutter system (SESS) for thermal nondestructive evaluation	Joseph N. Zalameda	Army Research Lab./NASA Langley Research Ctr. (USA)	© 2001 SPIE	10.1117/12.421044	Employee	Army Research Lab./NASA Langley Research Ctr. (USA)	No	N/A
Journal of Geophysical Research: Space Physics (1978–2012) > Vol 109 Issue A12	Dec-04	Postmidnight storm-time enhancement of tens-of-keV proton flux	Y. Ebihara 1,3 andM.-C. Fok 2	1 Universities Space Research Association, NASA Goddard Space Flight Center, Greenbelt, Maryland, USA 2 NASA Goddard Space Flight Center, Greenbelt, Maryland, USA 3 On leave from National Institute of Polar Research, Tokyo, Japan	Copyright 2004 by the American Geophysical Union	10.1029/2004JA010523	Employee	2 NASA Goddard Space Flight Center, Greenbelt, Maryland, USA	No	The authors would like to gratefullyacknowledge Donald G. Mitchell, Pontus C:son Brandt, and Edmo ndC. Roelof for providing us the valuable IMAGE/HENA data, RichardA. Wolf, Robert W. Spiro, Stanislav Y. Sazykin, and Joe D. Perez forfruitful discussions and supporting computer programs, and the NASA/GSFC/NSSDC for the use of the CDAWeb data. The authors also thankNorman F. Ness and David J. McComas for providing us the ACE data and Daniel R. Weimer for providing us his computer code. Dst and SYMindices were provided from the World Data Center for Geomagnetism,Kyoto. This work was supported by the NASA office of Space ScienceSun-Earth Connection Guest Investigator Program, under RTOP grant 370-16-00-11.
Journal of heat transfer	2004	Visualization of Wettability Effects on Microchannel Two-Phase Flow Resistance				10.1115/1.1811717	No Access
The Astrophysical Journal, Volume 627, Number 1	2005	Chandra High-Resolution X-Ray Spectroscopy of the Fe K Line in the Seyfert 1 Galaxy NGC 3783	T. Yaqoob 1,2, J. N. Reeves 1,2,3, A. Markowitz 2,4, P. J. Serlemitsos 2, and U. Padmanabhan 1	1 Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD 21218 2 Laboratory for High Energy Astrophysics, NASA Goddard Space Flight Center, Greenbelt, MD 20771 3 Universities Space Research Association 4 NAS/NRC Research Associate	© 2005. The American Astronomical Society. All rights reserved	10.1086/430404	Employee	2 Laboratory for High Energy Astrophysics, NASA Goddard Space Flight Center, Greenbelt, MD 20771	No	The authors thank Ian George, Jane Turner, and Barry McKernan for valuable discussions, and S. Watanabe for use of his Comptonized line model. T. Y. gratefully acknowledges support from NASA grants NNG04GB78A, NAG5-10769, and AR4-5009X, the latter issued by the Chandra X-Ray Observatory Center, which is operated by the Smithsonian Astrophysical Observatory for and on behalf of NASA under contract NAS8-39073. This research made use of the HEASARC online data archive services, supported by NASA/GSFC. This research has made use of the NASA/IPAC Extragalactic Database (NED), which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with NASA. The authors are grateful to the Chandra instrument and operations teams for making these observations possible.
Journal of climate and applied meteorology	Feb-84	Thunderstorm Cloud Height–Rainfall Rate Relations for Use with Satellite Rainfall Estimation Techniques				10.1175/1520-0450(1984)023<0280:TCHRRF>2.0.CO;2	No Access
AIAA journal	Aug-80	Asymptotic features of shock-wave boundary-layer interaction				10.2514/3.7705	No Access
1992 22nd European Microwave Conference Year: 1992, Volume: 2	Sep-92	Front-End Topologies for Phased Array Radiometry	1) M. K. Sonmez, R. J. Trew; 2) C. P. Hearn	1) High Frequency Electronics Laboratory, Department of Electrical and Computer Engineering, North Carolina State University, Raleigh, North Carolina 27695-7911; 2) NASA-Langley Research Center, Hampton, VA	N/A	10.1109/EUMA.1992.335876	Employee	2) NASA-Langley Research Center, Hampton, VA	No	This work was supported by NASA-Langley Research Center on Grant NAG-1-943.
2005 IEEE Aerospace Conference	Mar-05	Analysis and Numerical Modeling of Error Sources in SIM Star Light Phase Detection	1) M.W. Regehr, M. Milman	1) Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Dr, m/s 171-113 Pasadena, CA 91109	© 2005 IEEE	10.1109/AERO.2005.1559530	Contractor	1) Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Dr, m/s 171-113 Pasadena, CA 91109	No	The research described in this publication was performed at the Jet Propulsion Laboratory of the California Institute of Technology, under contract with the National Aeronautics and Space Administration. The authors would like to thank TsaePyng Shen and Joseph Catanzarite for their assistance in obtaining and processing data from the MAM testbed.
Science 20 Aug 2010: Vol. 329, Issue 5994, pp. 936-940	Aug-10	Evidence of Recent Thrust Faulting on the Moon Revealed by the Lunar Reconnaissance Orbiter Camera	Thomas R. Watters 1, Mark S. Robinson 2, Ross A. Beyer 3,4, Maria E. Banks 1, James F. Bell III 5, Matthew E. Pritchard 6, Harald Hiesinger 7,8, Carolyn H. van der Bogert 7, Peter C. Thomas 9, Elizabeth P. Turtle 10, Nathan R. Williams 6	1 Center for Earth and Planetary Studies, Smithsonian Institution, Washington, DC 20560, USA. 2 School of Earth and Space Exploration, Arizona State University, Tempe, AZ 85251, USA. 3 Carl Sagan Center, SETI Institute, Mountain View, CA 94043, USA. 4 NASA Ames Research Center, Moffett Field, CA 94035–0001, USA. 5 Department of Astronomy, Cornell University, Ithaca, NY 14853, USA. 6 Department of Earth and Atmospheric Sciences, Cornell University, Ithaca, NY 14853, USA. 7 Institut für Planetologie, Westfälische Wilhelms-Universität, 48149 Münster, Germany. 8 Department of Geological Sciences, Brown University, Box 1846, Providence, RI 02912, USA. 9 Center for Radiophysics and Space Research, Cornell University, Ithaca, NY 14853, USA. 10 Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723, USA.	Copyright © 2010, American Association for the Advancement of Science	10.1126/science.1189590	Employee	1 Center for Earth and Planetary Studies, Smithsonian Institution, Washington, DC 20560, USA. 4 NASA Ames Research Center, Moffett Field, CA 94035–0001, USA.	No	We thank the three anonymous reviewers for helpful comments that improved the manuscript. We gratefully acknowledge the Lunar Orbiter Laser Altimeter team for the lunar topographic model and the LRO and LROC engineers and technical support personnel. This work was supported by the LRO Project, NASA grants NNX08AM73G and NNG07EK00C, and through Deutsches Zentrum für Luft- und Raumfahrt grant 50 OW 0901.
AIAA journal	Jun-89	Integrated structural electromagnetic shape control of large space anatenna reflectors				10.2514/3.10183	No Access
Journal of Climate; Boston 22.17 (Sep 1, 2009): 4459-4464,4466-4480	Sep-09	African Easterly Jet: Structure and Maintenance	1) MAN-LI C. WU; 2) ORESTE REALE; 3) SIEGFRIED D. SCHUBERT, MAX J. SUAREZ, RANDY D. KOSTER, AND PHILIP J. PEGION	1) Global Modeling and Assimilation Office, NASA Goddard Space Flight Center, Greenbelt, Maryland; 2) Laboratory for Atmospheres, NASA Goddard Space Flight Center, Greenbelt, Maryland; 3) Global Modeling and Assimilation Office, NASA Goddard Space Flight Center, Greenbelt, Maryland	Copyright American Meteorological Society Sep 1, 2009	10.1175/2009JCLI2584.1	Employee	1) Global Modeling and Assimilation Office, NASA Goddard Space Flight Center, Greenbelt, Maryland; 2) Laboratory for Atmospheres, NASA Goddard Space Flight Center, Greenbelt, Maryland; 3) Global Modeling and Assimilation Office, NASA Goddard Space Flight Center, Greenbelt, Maryland	No	This work was supported by the NASA Earth Science Enterprise's Global Modeling and Analysis Program.
IEEE Transactions on Antennas and Propagation Year: 1993, Volume: 41, Issue: 2	Feb-93	Study of some practical issues in inversion with the Born iterative method using time-domain data	1) M. Moghadtiam; 2) W. C. Chew	1) Jet Propulsion Laboratory, Califomia Institute of Technology, Pasadena, CA 91109; 2) Department of Electrical and Computer Engineering, University of Illinois at Urbana-Champaign, Urbana, IL 61801.	© 1993 IEEE	10.1109/8.214608	Contractor	1) Jet Propulsion Laboratory, Califomia Institute of Technology, Pasadena, CA 91109;	No	This work was supported by the Army Research Office under contract DAALO3-87-K0006 to the University of Illinois Advanced Construction Technology Center, by the Office of Naval Research under grant NOOO14-89-5-1286, and by the National Science Foundation under grant NSF ECS-85291. The computation time was provided by the National Center for Supercomputing Applications (NCSA) at the University of Illinois, Urbana-Champaign.
AIP Conference Proceedings 1531, 752 (2013)	May-13	Trends in severe storms from nine years of AIRS data	1) H. H. Aumann and A. Ruzmaikin	1) California Institute of Technology, Jet Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena CA 91109, USA	© 2013 AIP Publishing LLC	10.1063/1.4804879	Contractor	1) California Institute of Technology, Jet Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena CA 91109, USA	No	This research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under contract with NASA.
Journal of Geophysical Research: Solid Earth (1978–2012) > Vol 96 Issue B13	Dec-91	Models of recurrent strike-slip earthquake cycles and the state of crustal stress	1) GREGORY A. LYZENGA, ARTHUR RAEFSKY, AND STEPHANIE G. MULLIGAN	1) Jet Propulsion Laboratory, California Institute of Technology, Pasadena	Copyright 1991 by the American Geophysical Union	10.1029/91JB02260	Contractor	1) Jet Propulsion Laboratory, California Institute of Technology, Pasadena	No	The research in this publication was carried out by the Jet Propulsion Lal•oratory, California Institute of Tech- nology, under a contract with the National Aeronautics and Space Administration. Support for [his research was provided through the NASA Geodynamics Program. The authors wish to acknowledge the use of the computational facilities of the JPL/Caltech Cray X-MP/I 8, and the Ames Research Center's Numerical Aerodynamic Simulation Program Cray Y-MP in performing the calculations. We gratefully acknowledge the helpful and insightful comments pro- vided by Eugene Humphreys, Franqois Sauqier, and an anonymous reviewer, which led to significant improvements in the paper
Atmos. Chem. Phys., 12, 9097-9111, 2012	May-12	Radiative impacts of cloud heterogeneity and overlap in an atmospheric General Circulation Model	L. Oreopoulos 1, D. Lee 1,2,3, Y. C. Sud 1, and M. J. Suarez 1	1 NASA Goddard Space Flight Center, Greenbelt, MD, USA 2 University Space Research Association, Columbia, MD, USA 3 Seoul National University, Seoul, South Korea	© Author(s) 2012. This work is distributed under the Creative Commons Attribution 3.0 License.	10.5194/acp-12-9097-2012	Employee	1 NASA Goddard Space Flight Center, Greenbelt, MD, USA	No	The authors gratefully acknowledge support by the NASA Modeling Analysis and Prediction and CloudSat/CALIPSO Science Team Recompete programs managed by David Considine. Computational resources and support were provided from the NASA Center for Climate Simulation (NCCS). We would also like to thank M. Iacono and E. Mlawer of AER for their assistance in implementing RRTMG into GEOS-5.
Proc. SPIE 3356, Space Telescopes and Instruments V, 653	Aug-98	Space Infrared Telescope Facility (SIRTF) enters development	1) Michael D. Bicay; 2) Michael W. Werner, Larry L. Simmons; 3) William B. Latter	1) Jet Propulsion Lab. and California Institute of Technology (USA); 2) Jet Propulsion Lab. (USA); 3) California Institute of Technology (USA)	© (1998) COPYRIGHT SPIE--The International Society for Optical Engineering.	10.1117/12.324432	Contractor	1) Jet Propulsion Lab. and California Institute of Technology (USA); 2) Jet Propulsion Lab. (USA);	No	This work was carried out at the Jet Propulsion Laboratoiy, California Institute of Technology, under contract with the National Aeronautics and Space Administration.
Applied Optics Vol. 20, Issue 12, pp. 2153-2165	1981	Two-photon excitation of nitric oxide fluorescence as a temperature indicator in unsteady gasdynamic processes	1) R. L. McKenzie; 2) K. P. Gross	1 NASA Ames Research Center, Moffett Field, California 94035 USA 2 Stanford University, Department of Aeronautical and Astronomical Engineering, Stanford, California 94305 USA	© 1981 Optical Society of America	10.1364/AO.20.002153	Employee	1 NASA Ames Research Center, Moffett Field, California 94035 USA	No	The authors are grateful for the assistance of J. O. Arnold and for the calculations he made to evaluate the effects of fluorescence self-absorption on the absorptivity measurement. One of us (KPG) acknowledges support through NASA contract NAS2-10351.
Journal of Electronic Materials October 1994, Volume 23, Issue 10, pp 1007–1013	Oct-94	Coarsening of three-dimensional droplets by two-dimensional diffusion: Part II. Theory	V. E. Fradkov 1 S. S. Mani 1 M. E. Glicksman 1 J. R. Rogers 2 J. P. Downey 3 W. K. Witherow 3 B. R. Facemire 3 D. O. Frazier 3	1. Rensselaer Polytechnic InstituteTroy 2. National Research Council, Space Science LaboratoryNASA Marshall Space Flight CenterHuntsville 3. Space Science LaboratoryNASA Marshall Space Flight CenterHuntsville	© The Metallurgical of Society of AIME 1994	10.1007/BF02650368	Employee	2. National Research Council, Space Science LaboratoryNASA Marshall Space Flight CenterHuntsville 3. Space Science LaboratoryNASA Marshall Space Flight CenterHuntsville	No	N/A
Science 20 Feb 2015: Vol. 347, Issue 6224	Feb-15	Black hole feedback in the luminous quasar PDS 456	E. Nardini 1, J. N. Reeves 1,2, J. Gofford 1,2, F. A. Harrison 3, G. Risaliti 4,5, V. Braito 6, M. T. Costa 1, G. A. Matzeu 1, D. J. Walton 3,7, E. Behar 8, S. E. Boggs 9, F. E. Christensen 10, W. W. Craig 11, C. J. Hailey 12, G. Matt 13, J. M. Miller 14, P. T. O’Brien 15, D. Stern 7, T. J. Turner 16,17, M. J. Ward 18	1 Astrophysics Group, School of Physical and Geographical Sciences, Keele University, Keele, Staffordshire ST5 5BG, UK. 2 Center for Space Science and Technology, University of Maryland Baltimore County, 1000 Hilltop Circle, Baltimore, MD 21250, USA. 3 Cahill Center for Astronomy and Astrophysics, California Institute of Technology, Pasadena, CA 91125, USA. 4 Istituto Nazionale di Astrofisica, Osservatorio Astrofisico di Arcetri, Largo Enrico Fermi 5, I-50125 Firenze, Italy. 5 Harvard–Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA. 6 INAF, Osservatorio Astronomico di Brera, Via Bianchi 46, I-23807 Merate (LC), Italy. 7 Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA. 8 Department of Physics, Technion, Haifa 32000, Israel. 9 Space Science Laboratory, University of California, Berkeley, CA 94720, USA. 10 Danmarks Tekniske Universitet Space–National Space Institute, Technical University of Denmark, Elektrovej 327, 2800 Lyngby, Denmark. 11 Lawrence Livermore National Laboratory, Livermore, CA 94550, USA. 12 Columbia Astrophysics Laboratory, Columbia University, New York, NY 10027, USA. 13 Dipartimento di Matematica e Fisica, Università degli Studi Roma Tre, Via della Vasca Navale 84, I-00146 Roma, Italy. 14 Department of Astronomy, University of Michigan, Ann Arbor, MI 48109, USA. 15 Department of Physics and Astronomy, University of Leicester, University Road, Leicester LE1 7RH, UK. 16 Physics Department, University of Maryland Baltimore County, 1000 Hilltop Circle, Baltimore, MD 21250, USA. 17 Eureka Scientific Inc., 2452 Delmer Street Suite 100, Oakland, CA 94602, USA. 18 Department of Physics, University of Durham, South Road, Durham DH1 3LE, UK.	N/A	10.1126/science.1259202	National Lab; Contractor	7 Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA. 11 Lawrence Livermore National Laboratory, Livermore, CA 94550, USA.	No	This research was supported under the U.K. Science and Technology Facilities Council grant ST/J001384/1 and is based on x-ray observations obtained with the XMM-Newton and NuSTAR satellites. XMM-Newton is a European Space Agency (ESA) science mission with instruments and contributions directly funded by ESA member states and the National Aeronautics and Space Administration. The NuSTAR mission is a project led by the California Institute of Technology, managed by the Jet Propulsion Laboratory, and funded by NASA. We thank the NuSTAR Operations, Software, and Calibration teams for support with execution and analysis of these observations. We also acknowledge financial support from the Italian Space Agency under grant ASI-INAF I/037/12/0 (G.R. and G.M.); the Italian National Institute for Astrophysics under grant PRIN-INAF 2012 (G.R.); the I-CORE program of the Planning and Budgeting Committee, the Israel Science Foundation under grants 1937/12 and 1163/10, Israel’s Ministry of Science and Technology (E.B.); and NASA under grants NNX11AJ57G and NNG08FD60C (T.J.T.). The data are stored in the science archives of the two x-ray observatories involved and will become publicly available on 25 March 2015 (XMM-Newton) and with the upcoming DR6 data release (NuSTAR).
Geophysical Research Letters > Vol 25 Issue 16	Aug-98	The impact of upper tropospheric humidity from microwave limb sounder on the midlatitude greenhouse effect	1) Hua Hu andW. Timothy Liu	1) Jet Propulsion Laboratory, California Institute of Technology, Pasadena	Copyright 1998 by the American Geophysical Union	10.1029/98GL02252	Contractor	1) Jet Propulsion Laboratory, California Institute of Technology, Pasadena	No	The authors thank Drs. Joe Waters and Bill Read in the Jet Propulsion Laboratory's MLS group for providing the MLS upper tropospheric water vapor data. The authors also thank the Data Assimila- tion Office and the Distributed Active Archive Center at the NASA Goddard Space Flight Center, for producing and distributing the data. This study was conducted at the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration (NASA). This research was supported by the NASA Earth Observing System (EOS) Interdisciplinary Science Investigatio
Journal of Geophysical Research: Atmospheres (1984–2012) > Vol 94 Issue D9	Aug-89	Trace gases in the Antarctic atmosphere	1) L. E. Heidt; 2) J. F. Vedder; 3) W. H. Pollock, R. A. Lueb, B. E. Henry	1) National Center for Atmospheric Research Boulder, Colorado; 2) NASA Ames Research Center, Moffett Fields California; 3) National Center for Atmospheric Research, Boulder, Colorado	Copyright 1989 by the American Geophysical Union.	10.1029/JD094iD09p11599	Employee	1) National Center for Atmospheric Research Boulder, Colorado; 2) NASA Ames Research Center, Moffett Fields California; 3) National Center for Atmospheric Research, Boulder, Colorado	No	This work was supported by contract 87-23 through Robert Watson and James Margitan of the National Aeronautics and Space Administration. We wish to acknowledge the cooperation and professionalism of the entire staff of the aircraft operations division (both ER-2 and DC-8) at NASA Ames, who were involved in this mission. We are indebted to the Project Scientist, Adrian Tuck, and the Project Manager, Estelle Condon, for valuable advice and support. Roland Chan (NASA Ames) freely provided the MMS data and Dan Murphy (NOAA Aeronomy Laboratory) calculated potential temperatures from that data. S. W. Bowen (NASA Ames) guided the design of the inlet probe. Michael Coffey and William Mankin of NCAR contributed generously of their time by collecting our samples aboard the DC-8. Ralph Cicerone exemplified the NCAR contribution to this mission with his support and advice. The National Center for Atmospheric Research is sponsored by the National Science Foundation.
Classical and Quantum Gravity, Volume 29, Number 12	Jun-12	Non-sky-averaged sensitivity curves for space-based gravitational-wave observatories	1) Michele Vallisneri and Chad R Galley	1) Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA	© 2012 IOP Publishing Ltd	10.1088/0264-9381/29/12/124015	Contractor	1) Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA	No	MV is grateful to J Armstrong, F Estabrook and M Tinto for teaching him about TDI and sensitivity calculations. This work was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. MV was supported by the LISA Mission Science Office and by the JPL RTD program. CG was supported by an appointment to the NASA Postdoctoral Program at the JPL administered by Oak Ridge Associated Universities through a contract with NASA. Copyright 2012 California Institute of Technology.
Geophysical Research Letters > Vol 27 Issue 17	Sep-00	El Niño, water vapor, and the global positioning system	James Foster 1, Michael Bevis 1, Thomas Schroeder 1, Mark Merrifield 1, Steven Businger 1, Susanne Dorn 1, Steven Marcus 2, Jean Dickey 2 andYoaz Bar-Sever 2	1 SOEST, University of Hawaii, Honolulu, HI 96822, USA 2 Jet Propulsion Laboratory, Pasadena, CA 91109	Copyright 2000 by the American Geophysical Union	10.1029/2000GL011429	Contractor	2 Jet Propulsion Laboratory, Pasadena, CA 91109	No	We thank Dr. Bin Wang for use- ful discussions and Seth Gutman and an anonymous reviewer for their comments. GPS data are from the IGS combined tropo- spheric solutions where available, augmented with data from JPL and the Pacific GPS Facility. Interpolated OLR data provided by the NOAA-CIRES Climate Diagnostics Center, Boulder, Col- orado, from their web site at http://www.cdc.noaa.gov. SST data are from the National Meteorological Data Center. Rainfall data provided by Ray Tanabe. E1 Nifio indices are from the NOAA Climate Prediction Center.
Radio Science > Vol 38 Issue 5	Oct-03	Theoretical description of a bistatic system for ocean altimetry using the GPS signal	1) George A. Hajj andCinzia Zuffada	1) Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA	Copyright 2003 by the American Geophysical Union	10.1029/2002RS002787	Contractor	1) Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA	No	We thank Brooks Thomas of JPLfor many insightful discussions. This work was performed atthe Jet Propulsion Laboratory, California Institute of Technol-ogy, under a contract with the National Aeronautic and SpaceAdministration.
General Relativity and Gravitation March 1988, Volume 20, Issue 3, pp 201–220	Mar-88	Energy-momentum tensor of fields in the standard cosmology	Philip D. Mannheim 1 Demosthenes Kazanas 2	1.Department of PhysicsUniversity of ConnecticutStorrs 2.Laboratory for High Energy AstrophysicsNASA/Goddard Space Flight CenterGreenbelt	© 1988 Plenum Publishing Corporation	10.1007/BF00759181	Employee	2.Laboratory for High Energy AstrophysicsNASA/Goddard Space Flight CenterGreenbelt	No	We would like to thank Professor S. Nussinov for his enthusiastic support and for many fruitful discussions. One of us (P.D.M.) would like to thank the National Aeronautics and Space Administration for the award of a NASA/ASEE Summer Faculty Fellowship, which enabled him to spend the summer of 1985 at the Goddard Space Flight Center, and in particular to thank Professor F. P. Emad for his kind invitation to participate in the NASA program. He would also like to thank Professors R. Ramaty and F. Stecker for their interest and the kind hospitality of the high-energy astrophysics theory group at the Goddard Space Flight Center. This work has also been supported in part (P.D.M.) by the U.S. Department of Energy under Grant No. DE-AC02-79ER10336.A.
IEEE Transactions on Antennas and Propagation Year: 1979, Volume: 27, Issue: 3	May-79	Wave tilt sounding of a linearly inhomogeneous layered half-space	1) L. WARNE, D. EVANS, AND C. ELACHI	1) Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91103	© 1979 IEEE	10.1109/TAP.1979.1142103	Contractor	1) Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91103	No	N/A
Applied Composite Materials August 2016, Volume 23, Issue 4, pp 523–535	Aug-16	Simulation of Lightning-Induced Delamination in Un-protected CFRP Laminates	P. Naghipour 1 E. J. Pineda 2 S. M. Arnold 2	1.Ohio Aerospace InstituteClevelandUSA 2.NASA Glenn Research CenterClevelandUSA	© Springer Science+Business Media Dordrecht (outside the USA) 2016	10.1007/s10443-016-9472-9	Employee	2.NASA Glenn Research CenterClevelandUSA	No	The authors would like to thank George Szatkowski and Kenneth Dudley from NASA LaRC for providing the experimental data used in this manuscript. This work was funded under the NASA Atmospheric Environment Safety Technologies (AEST) Project.
he Journal of Chemical Physics 84, 5025 (1986)	Jan-86	Theoretical study of the dipole moments of selected alkaline‐earth halides	1) Stephen R. Langhoff and Charles W. Bauschlicher Jr.; 2) Harry Partridge; 3) Reinhart Ahlrichs	1) NASA Ames Research Center, Moffett Field, California 94035; 2) Research Institute for Advanced Computer Science, NASA Ames Research Center, Moffett Field, California 94035; 3) Institut für Physikalische Chemie and Elektrochemie, Lehrstuhl für Theoretische Chemie, Universität Karlsruhe, Kaiserstr. 12, 7500 Karlsruhe, Federal Republic of Germany	© 1986 American Institute of Physics	10.1063/1.450651	Employee	1) NASA Ames Research Center, Moffett Field, California 94035; 2) Research Institute for Advanced Computer Science, NASA Ames Research Center, Moffett Field, California 94035;	No	N/A
Space Science Reviews December 2011, Volume 163, Issue 1–4, pp 3–23	Dec-11	The Dawn Mission to Vesta and Ceres	C. T. Russell 1 C. A. Raymond 2	1.Institute of Geophysics and Planetary Physics, Department of Earth and Space SciencesUniversity of CaliforniaLos AngelesUSA 2.Jet Propulsion LaboratoryCalifornia Institute of TechnologyPasadenaUSA	© Springer Science+Business Media B.V. 2011	10.1007/s11214-011-9836-2	Contractor	2.Jet Propulsion LaboratoryCalifornia Institute of TechnologyPasadenaUSA	No	The preparation of this report was supported by the National Aeronautics and Space Administration under contract NNM05AA86C. A portion of the work was carried out at the Jet Propulsion Laboratory.
The Astrophysical Journal, Volume 724, Number 1	Nov-10	A CHANDRA PERSPECTIVE ON GALAXY-WIDE X-RAY BINARY EMISSION AND ITS CORRELATION WITH STAR FORMATION RATE AND STELLAR MASS: NEW RESULTS FROM LUMINOUS INFRARED GALAXIES	B. D. Lehmer 1,2, D. M. Alexander 3, F. E. Bauer 4,5, W. N. Brandt 6,7, A. D. Goulding 3, L. P. Jenkins 1,2, A. Ptak 2, and T. P. Roberts 3	1 The Johns Hopkins University, Homewood Campus, Baltimore, MD 21218, USA 2 NASA Goddard Space Flight Centre, Code 662, Greenbelt, MD 20771, USA 3 Department of Physics, University of Durham, South Road, Durham, DH1 3LE, UK 4 Pontificia Universidad Catolica de Chile, Departamento de Astronomia y Astrofisica, Casilla 306, Santiago 22, Chile 5 Space Science Institute, 4750 Walnut Street, Suite 205, Boulder, CO 80301, USA 6 Department of Astronomy & Astrophysics, 525 Davey Lab, The Pennsylvania State University, University Park, PA 16802, USA 7 Institute for Gravitation and the Cosmos, The Pennsylvania State University, University Park, PA 16802, USA	© 2010. The American Astronomical Society. All rights reserved. Printed in the U.S.A.	10.1088/0004-637X/724/1/559	Employee	2 NASA Goddard Space Flight Centre, Code 662, Greenbelt, MD 20771, USA	No	We thank the referee for helpful comments that have improved the manuscript. We thank Kazushi Iwasawa for generously sharing data and Lee Armus and Joseph Mazzarella for helpful discussions. We gratefully acknowledge financial support from the Einstein Fellowship Program (B.D.L.), the Royal Society (D.M.A.), the Leverhulme Trust (D.M.A.), Chandra X-ray Center grants G09-0134A (W.N.B.) and G09-0134B (F.E.B.), and NASA ADP grant NNX10AC99G (W.N.B.). This research has made use of the NASA/IPAC Extragalactic Database (NED), which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with NASA.
Journal of Geophysical Research: Space Physics > Vol 119 Issue 8	Aug-14	Structure and dynamics of Mercury's magnetospheric cusp: MESSENGER measurements of protons and planetary ions	Jim M. Raines 1, Daniel J. Gershman 1,2, James A. Slavin 1, Thomas H. Zurbuchen 1, Haje Korth 3, Brian J. Anderson 3 andSean C. Solomon 4,5	1 Department of Atmospheric, Oceanic and Space Sciences, University of Michigan, Ann Arbor, Michigan, USA 2 Geospace Physics Laboratory, NASA Goddard Space Flight Center, Greenbelt, Maryland, USA 3 The Johns Hopkins University Applied Physics Laboratory, Laurel, Maryland, USA 4 Lamont-Doherty Earth Observatory, Columbia University, Palisades, New York, USA 5 Department of Terrestrial Magnetism, Carnegie Institution of Washington, Washington, District of Columbia, USA	©2014. American Geophysical Union. All Rights Reserved.	10.1002/2014JA020120	Unsure	1 Department of Atmospheric, Oceanic and Space Sciences, University of Michigan, Ann Arbor, Michigan, USA 2 Geospace Physics Laboratory, NASA Goddard Space Flight Center, Greenbelt, Maryland, USA	No	The MESSENGER project is supported by the NASA Discovery Program under contracts NAS5-97271 to The Johns Hopkins University Applied Physics Laboratory and NASW-00002 to the Carnegie Institution of Washington. J.M.R. thanks D. Schriver and T. A. Cassidy for discussions helpful to this work. Data used in this study are available from the Planetary Data System.
Journal of Geophysical Research: Space Physics (1978–2012) > Vol 92 Issue A8	Aug-87	The Uranian bow shock: Voyager 2 inbound observations of a high Mach number shock	1) FRAN BAGENAL and JOHN W. BELCHER; 2) EDWARD C. SITTLER, JR., and RONALD P. LEPPING	1) Center for Space Research, Massachusetts Institute of Technology, Cambridge; 2) Laboratory for Extraterrestrial Physics, Goddard Space Flight Center, Greenbelt, Maryland	Copyright 1987 by the American Geophysical Union	10.1029/JA092iA08p08603	Employee	2) Laboratory for Extraterrestrial Physics, Goddard Space Flight Center, Greenbelt, Maryland	No	Work for this paper was supported under JPL/NASA contract number 953733
Journal of Geophysical Research: Space Physics (1978–2012) > Vol 101 Issue A11	Nov-96	Ulysses assessment of the Jovian planetary field	1) M. K. Dougherty, A. Balogh and D. J. Southwood; 2) E. J. Smith	1) The Blackett Laboratory, Imperial College, London, United Kingdom; 2) Jet Propulsion Laboratory, Pasadena, California	Copyright 1996 by the American Geophysical Union	10.1029/96JA02385	Contractor	2) Jet Propulsion Laboratory, Pasadena, California	No	We would like to thank A. F. Lovegrove for initial work carried out on this field modeling problem during a summer project at Imperial College, S. Joy from the UCLA PDS data center for the Voyager 1 and Pioneer 11 data sets, R. J. Forsyth for the description of the calibration and the closest approach data set, and the assistance of the Ulysses spacecraft operations and navigation teams in providing spacecraft position and attitude un- certainties.
Journal of propulsion and power	Jan-01	Multidisciplinary Approach to Linear Aerospike Nozzle Design				10.2514/2.5712	No Access
IEEE Antennas and Propagation Society International Symposium. 2001 Digest. Held in conjunction with: USNC/URSI National Radio Science Meeting (Cat. No.01CH37229)	Jul-01	Analysis of quarter-wave shorted patch antenna	M.D. Deshpande	NASA Langley Res. Center, Hampton, VA, USA	© 2001 IEEE	10.1109/APS.2001.959821	Employee	NASA Langley Res. Center, Hampton, VA, USA	No	N/A
2010 IEEE AUTOTESTCON	Sep-10	Integrated diagnostic/prognostic experimental setup for capacitor degradation and health monitoring	1) Chetan Kulkarni, Gautam Biswas and Xenofon Koutsoukos; 2) Jose Celaya; 3) Kai Goebel	1) Dept. of EECS, ISIS, Vanderbilt University Nashville, TN, USA; 2) SGT Inc, NASA Ames Research Center, Intelligent Systems Division, Moffett Field, CA, USA; 3) NASA Ames Research Center, Intelligent Systems Division, Moffett Field, CA, USA	©2010 IEEE	10.1109/AUTEST.2010.5613596	Employee	2) SGT Inc, NASA Ames Research Center, Intelligent Systems Division, Moffett Field, CA, USA; 3) NASA Ames Research Center, Intelligent Systems Division, Moffett Field, CA, USA	No	The experiments for this paper were conducted at the Prognostics Center of Excellence, NASA Ames Research.. This project was funded by NASA NRA - NNX07ADIZA, where Vanderbilt has a subcontract from Honeywell Labs, Minneapolis. We thank Raj Bharadwaj (PI), Adam Sweet (COTAR)and Scott Poll of NASA Ames for their helpful suggestions. We would also like to thank Mona Fahimi at the NASA Ames PCoE lab for her help during the experiments and developing the hardware.
Journal of Geophysical Research: Atmospheres (1984–2012) > Vol 103 Issue D6	Mar-98	Role of the quasi-biennial oscillation in the transport of aerosols from the tropical stratospheric reservoir to midlatitudes	Wookap Choi,1 William B. Grant,2 Jae H. Park,2 Kwang-Mog Lee,3 Hyunah Lee,1 and James M. Russell III 4	1 Department of Atmospheric Sciences, Seoul National University, Seoul, Korea 2 Atmospheric Sciences Division, NASA Langley Research Center, Hampton, Virginia 3 Department of Astronomy and Atmospheric Sciences, Kyungpook National University, Taegu, Korea 4 Deptartment of Physics, Hampton University, Hampton, Virgin	Copyright 1998 by the American Geophysical Union	10.1029/97JD03118	Employee	2 Atmospheric Sciences Division, NASA Langley Research Center, Hampton, Virginia	No	The authors thank the HALOE project team for providing the HALOE data and B. Naujokat (Free University of Berlin) for Singapore wind data used in this paper, and J. M. Melnemey (SAIC) for assistance with the graphics. An anonymous reviewer provided insightful and careful comments which made this paper more clear. Support for W. Choi, K.-M. Lee, and H. Lee for time spent at the NASA Langley Research Center was provided by NASA grant NAS1-19656. W. Choi was also supported by the Cray Research, Inc., through the Systems Engineering Research Institute, Korea.
The Astronomical journal	Oct-93	Evolution of the symbiotic binary system AG Pegasi - The slowest classical nova eruption ever recorded				10.1086/116749	No Access
Physical review. B, Condensed matter	Jun-98	Observation and modeling of single-wall carbon nanotube bend junctions				10.1103/PhysRevB.57.14983	No Access
Molecular crystals and liquid crystals (Philadelphia, Pa. : 2003)	Sep-06	The LCPDI: A Compact and Robust Phase-Shifting Point-Diffraction Interferometer Based on Dye-Doped LC Technology				10.1080/15421400600654116	No Access
New Series, Vol. 285, No. 5427	Jul-99	Imaging of Asteroid 433 Eros During NEAR's Flyby Reconnaissance	J. Veverka,1 P. C. Thomas,1 J. F. Bell 111,1 M. Bell, B. Carcich,1 B. Clark,1 A. Harch,1 J. Joseph,1 P. Martin,1 M. Robinson,2 S. Murchie,3 N. Izenberg,3 E. Hawkins,3 J. Warren,3 R. Farquhar,3 A. Cheng,3 D. Dunham,3 C. Chapman,4 W. J. Merline,4 L. McFadden,5 D. Wellnitz,5 M. MaLin,6 W. M. Owen Jr.,7 J. K. Miller,7 B. G. Williams,7 D. K. Yeomans7	1 Space Sciences Building Comell University, Ithaca, NY 14853, USA. 2 Department of Geological Sciences, Northwestem University, 309 Locy Hall, Evanston, IL 60208, USA. 3 Applied Physics Laboratory, 11100 Johns Hopkins Road, Laurel MD 20723, USA. 4 Southwest Research Institute, 1050 Walnut Street, Suite 426, Boulder, CO 80302, USA. 5 Department of Astronomy, University of Maryland, College Park, MD 20742, USA. 6 Malin Space Science Systems Inc., Post Office Box 910148, San Diego, CA 92191, USA. 7 Jet PropuLsion Laboratory, 4800 Oak Grove Drive, Pasadena, CA 91109, USA.	N/A	10.1126/science.285.5427.562	Contractor	7 Jet PropuLsion Laboratory, 4800 Oak Grove Drive, Pasadena, CA 91109, USA.	No	N/A
International journal of modern physics. B, Condensed matter physics, statistical physics, applied physics	Apr-93	QUANTUM STATE CONTROL IN SEMICONDUCTOR p-n JUNCTIONS (I) — SQUEEZED STATE GENERATION IN SEMICONDUCTOR LASERS				10.1142/S021797929300250X	No Access
Geophysical Research Letters > Vol 7 Issue 4	Apr-80	Microwave radar and radiometric remote sensing measurements of lake ice	1) C. T. Swift, W. L. Jones, Jr., R. F. Harrington, J. C. Fedors and R. H. Couch; 2) B. L. Jackson,	1) NASA Langley Research Center, Hampton, Virginia 23665; 2) Old Dominion University, Norfolk, Virginia 23508	This paper is not subject to U.S. copyright. Published in 1980 by the American Geophysical Union.	10.1029/GL007i004p00243	Employee	1) NASA Langley Research Center, Hampton, Virginia 23665;	No	The authors would like to acknowledge the outstanding cooperation received by J. Lindeman and the entire flight crew of the NASA C-130. One of us (CTS) is indebted to T. T. Wilheit and J. Crawford of NASA Goddard for valuable discussions relating to this work.
Journal of Geophysical Research: Atmospheres (1984–2012) > Vol 105 Issue D20	Oct-00	The response of atmospheric circulation to weak solar forcing	1) J. K. Lawrence and A. C. Cadavid; 2) A. Ruzmaiken	1) Department of Physics and Astronomy, California State University, Northridge; 2) Jet Propulsion Laboratory, California Institute of Technology, Pasadena	Copyright 2000 by the American Geophysical Union	10.1029/2000JD900354	Contractor	2) Jet Propulsion Laboratory, California Institute of Technology, Pasadena	No	This work was supported in part by the NASA Solar Influences on Global Change Research and Analysis Program.
Journal of Geophysical Research: Oceans (1978–2012) > Vol 103 Issue C6	Jun-98	Radar-derived interferometric surface currents and their relationship to subsurface current structure	1) Delwyn Moller*, Robert E. Mcintosh and Stephen J. Frasier; 2) David L. Porter	1) Microwave Remote Sensing Laboratory, University of Massachusetts, Amherst; 2) Applied Physics Laboratory, Johns Hopkins University, Laurel, Maryland; *Now at Jet Propulsion Laboratory, Pasadena, California.	Copyright 1998 by the American Geophysical Union	10.1029/98JC00781	False Positive	*Now at Jet Propulsion Laboratory, Pasadena, California.	No	The authors gratefully acknowledge R. Chap- man, D. Thompson, B. Gotwols, M. Jose, and R. Sterner of JHU/APL; M. Sletten of NRL; and J. Eshbaugh and J. Li of UMass for their support in the field and in the laboratory. We acknowledge the Envi- ronmental Research Institute of Michigan and thank Chris Wacker- man for providing comparative measurements from their interfero- metric SAR system. The staff at the Army Corps of Engineers Field Research Facility, whose facilities we utilized, deserve special mention for their logistical support and accommodation. This work was sup- ported by the Office of Naval Research (Remote Sensing) under grant N00014-95-1-0832
Data Mining and Knowledge Discovery March 2012, Volume 24, Issue 2, pp 443–471	Mar-12	Greener aviation with virtual sensors: a case study	Ashok N. Srivastava 1	1.Intelligent Systems DivisionIntelligent Data Understanding Group, NASA Ames Research CenterMoffett FieldUSA	© The Author(s) 2011	10.1007/s10618-011-0240-z	Employee	1.Intelligent Systems DivisionIntelligent Data Understanding Group, NASA Ames Research CenterMoffett FieldUSA	No	The author would like to thank Irving Statler for extremely thoughtful and useful discussions throughout this project. The author also thanks Timothy Woodbury for valuable discussions and Don Simon of NASA Glenn Research Center for providing key references and analytical advice. He would also like to acknowledge Nikunj Oza for valuable discussions and the reviewers for their constructive feedback. The author also thanks our airline partner in providing access to their flight operational data to enable this study. This research was conducted with the support of the NASA Aviation Safety Program’s System-Wide Safety and Assurance project. The code used for many of the algorithms in this paper is available as opensource and can be found on DASHlink at https://c3.nasa.gov/dashlink/projects/7/.
IEEE Transactions on Nuclear Science Year: 1996, Volume: 43, Issue: 3	Jun-96	A content addressable memory for use in CEBAF's CLAS detector level 2 triggering system	1) R.F. Hodson, D.C. Doughty Jr., D.C. Allgood, S.A. Campbell; 2) W.C. Wilson; 3) M.H. Bickley	1) Christopher Newport University, Newport News, VA 23606 ; 2) NASA Langley Research Center, Hampton VA 23681; 3) CEBAF, Newport News, VA 23606	© 1996 IEEE	10.1109/23.507169	Employee	2) NASA Langley Research Center, Hampton VA 23681;	No	Special thanks to Mark Lantz of the National Security Agency and Thomas A. Shull of NASA Langley Research Center for their support on this project. We also greatly appreciate grant contributions made by CEBAF and NASA used for funding faculty and student researchers.
The Astronomical journal	Dec-96	UIT: New Ultraviolet Stellar Photometry and Surface Brightness Profiles of the Globular Cluster M79 (NGC 1904)				10.1086/118230	No Access
Proc. SPIE 9148, Adaptive Optics Systems IV, 91483X	Jul-14	L'-band AGPM vector vortex coronagraph's first light on LBTI/LMIRCam	1) D. Defrère, P. Hinz, A. Skemer, V. Bailey, E. Downey, O. Durney, W. F. Hoffmann, J. Leisenring, M. Montoya; 2) O. Absil, C. Delacroix, C. Gomez, S. Habraken, J, Surdej; 3) J. Kuhn, B. Mennesson, K. Wallace; 4) D. Mawet; 5) P. Forsberg, M. Karlsson; 6) M. Kenworthy; 7) L. Pueyo; 8) M. Skrutskie	1) Steward Observatory, The Univ. of Arizona (United States); 2) Univ. de Liège (Belgium); 3) Jet Propulsion Lab. (United States); 4) European Southern Observatory (Chile); 5) Uppsala Univ. (Sweden); 6) Leiden Observatory (Netherlands); 7) Space Telescope Science Institute (United States); 8) Univ. of Virginia (United States)	© 2014 SPIE	10.1117/12.2057205	Contractor	3) Jet Propulsion Lab. (United States);	No	LBTI is funded by a NASA grant in support of the Exoplanet Exploration Program (NSF 0705296). The LBT is an international collaboration among institutions in the United States, Italy and Germany. LBT Corporation partners are: The University of Arizona on behalf of the Arizona university system; Istituto Nazionale di Astrofisica, Italy; LBT Beteiligungsgesellschaft, Germany, representing the Max-Planck Society, the Astrophysical Institute Potsdam, and Heidelberg University; The Ohio State University, and The Research Corporation, on behalf of The University of Notre Dame, University of Minnesota and University of Virginia. The research leading to these results has received funding from the European Research Council under the European Union’s Seventh Framework Programme (ERC Grant Agreement n.337569) and from the French Community of Belgium through an ARC grant for Concerted Research Actions. O.A. is a Research Associate of the F.R.S.-FNRS (Belgium).
Journal of Molecular Spectroscopy Volume 280, October 2012, Pages 134–144	Oct-12	Broadband rotational spectroscopy of acrylonitrile: Vibrational energies from perturbations	Zbigniew Kisiel a, Lech Pszczółkowski a, Brian J. Drouin b, Carolyn S. Brauer b, Shanshan Yu b, John C. Pearson b, Ivan R. Medvedev c, Sarah Fortman d, Christopher Neese d	a Institute of Physics, Polish Academy of Sciences, Al. Lotników 32/46, 02-668 Warszawa, Poland b Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109-8099, USA c Department of Physics, Wright State University, 3640 Colonel Glenn Highway, Dayton, OH 45435, USA d Department of Physics, The Ohio State University, 191 W. Woodruff Ave., Columbus, OH 43210, USA	© 2012 Elsevier Inc. All rights reserved.	10.1016/j.jms.2012.06.013	Contractor	b Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109-8099, USA	No	The authors thank Benjamin Moran for assistance with collecting data at Wright State University and Adam Kraśnicki for the ab initio calculations. Financial support from the Army Research Office (OSU) and from the Institute of Physics of the Polish Academy of Sciences (Warsaw) is gratefully acknowledged. This paper presents research carried out at the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.
The Astronomical Journal, Volume 140, Number 5	Oct-10	SIMULTANEOUS X-RAY AND ULTRAVIOLET OBSERVATIONS OF THE SW SEXTANTIS STAR DW URSAE MAJORIS	D. W. Hoard 1,2, Ting-Ni Lu 3, Christian Knigge 4, Lee Homer 5, Paula Szkody 5, M. Still 6, Knox S. Long 7, V. S. Dhillon 8, and S. Wachter 1	1 Spitzer Science Center, California Institute of Technology, MS 220-6, 1200 E. California Blvd., Pasadena, CA 91125, USA 2 Eureka Scientific, Inc., 2452 Delmer Street, Suite 100, Oakland, CA 94602, USA 3 Institute of Astronomy, National Tsing Hua University, Hsinchu 30013, Taiwan 4 School of Physics and Astronomy, University of Southampton, Highfield, Southampton SO17 1BJ, UK 5 Department of Astronomy, University of Washington, Box 351580, Seattle, WA 98195-1580, USA 6 NASA Ames Research Center, Moffett Field, CA 94035, USA 7 Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA 8 Department of Physics and Astronomy, University of Sheffield, Sheffield S3 7RH, UK	© 2010. The American Astronomical Society. All rights reserved.	10.1088/0004-6256/140/5/1313	Employee	6 NASA Ames Research Center, Moffett Field, CA 94035, USA	No	This work was supported by an XMM-Newton Guest Observer grant for program 014297 and is based on observations obtained with XMM-Newton, a European Space Agency (ESA) science mission with instruments and contributions directly funded by ESA Member States and the United States of America (through the National Aeronautics and Space Administration). This work was performed, in part, at the Jet Propulsion Laboratory, California Institute of Technology. We utilized the SIMBAD database, operated at CDS, Strasbourg, France, and NASA’s Astrophysics Data System
Physics of Fluids 11, 627 (1999)	Feb-99	Turbulent force as a diffusive field with vortical sources	1) Jie-Zhi Wu; 2) Ye Zhou; 3) Xi-Yun Lu and Meng Fan	1) The University of Tennessee Space Institute, Tullahoma, Tennessee 37388; 2) Institute for Computer Applications in Science and Engineering, NASA Langley Research Center, Hampton, Virginia 23681 & IBM Research Division, T. J. Watson Research Center, P.O. Box 218, Yorktown Heights, New York 10598; 3) The University of Tennessee Space Institute, Tullahoma, Tennessee 37388	© 1999 American Institute of Physics	10.1063/1.869934	Unsure	2) Institute for Computer Applications in Science and Engineering, NASA Langley Research Center, Hampton, Virginia 23681 & IBM Research Division, T. J. Watson Research Center, P.O. Box 218, Yorktown Heights, New York 10598;	No	The work is supported in part by Office of Naval Research under the Grant W00014-96-1-0452, and the National Aeronautics and Space Administration under NASA Contract No. NAS1-19480 while the first ~J.Z.W. as a summer visitor! and second authors were in residence at the Institute for Computer Applications in Science and Engineering, NASA Langley Research Center. The major numerical computation was performed at NAS Eagle Cray C-90 supercomputer, NASA Ames Research Center. The third and fourth authors are grateful to the financial support of J. M. Wu Research Fund of UTSI and Peking University, Peking, China, respectively, during their stay at UTSI. Valuable discussions with Xiao-Hui Wu, Xie-Yuan Yin, Philippe Spalart, and H. Marmanis are very appreciated.
Geophysical Research Letters > Vol 24 Issue 22	Nov-97	The missing dimension in Magsat and POGO anomaly studies	Michael E. Purucker 1, Terence J. Sabaka 1, Robert A. Langel 2 andNils Olsen 3	1 Hughes-STX, Geodynamics Branch, Goddard Space Flight Center, Greenbelt, Maryland 2 Staff Scientist Emeritus, Goddard Space Flight Center, Greenbelt, Maryland 3 Department of Geophysics, Copenhagen University, Copenhagen, Denmark	Copyright 1997 by the American Geophysical Union	10.1029/97GL52978	Employee	1 Hughes-STX, Geodynamics Branch, Goddard Space Flight Center, Greenbelt, Maryland 2 Staff Scientist Emeritus, Goddard Space Flight Center, Greenbelt, Maryland	No	We thank J. Conrad for program- ming assistance and J. Heirtzler, H. Frey, D. Ravat, and P. Taylor for reviews of the manuscript. AGSO released the digital version of the upward continued map of Australia, kindly provided by Chris Tarlowski. Supported by NASA RTOP 579-31-01.
Geophysical Research Letters > Vol 34 Issue 11	Jun-07	Simultaneous detection/separation of mineral dust and cirrus clouds using MODIS thermal infrared window data	R. A. Hansell 1, S. C. Ou 1, K. N. Liou 1, J. K. Roskovensky 2, S. C. Tsay 3, C. Hsu 3 andQ. Ji 4	1 Department of Atmospheric and Oceanic Sciences, University of California, Los Angeles, California, USA 2 Sandia National Laboratories, Albuquerque, New Mexico, USA 3 NASA Goddard Space Flight Center, Greenbelt, Maryland, USA 4 Earth System Science Interdisciplinary Center, University of Maryland at College Park, College Park, Maryland, USA	Copyright 2007 by the American Geophysical Union	10.1029/2007GL029388	National Lab; Employee	2 Sandia National Laboratories, Albuquerque, New Mexico, USA 3 NASA Goddard Space Flight Center, Greenbelt, Maryland, USA	No	The MODIS cloud-mask read algorithm from S. Nasari/S.W. Seemann 2001 (CIMSS/SSEC) was used in this study and the MODIS data and images were obtained from the NASA LAADS Web site. The NAMMA MPL data was acquired through the NASA Micro-Pulse Lidar Network which is funded by the NASA Earth Observing System and Radiation Sciences Program. Sun-photometer data from the Sir-Bu-Nuair site was provided by the NASA AERONET Program. The AMF MPL data was acquired through the ARM data archive. We are grateful to the following people: J. Campbell for producing the NAMMA MPL plot, R. Coulter for help with the AMF MPL data correction, and to C. Zender and T. Roush for making available the mineral datasets. We are also grateful to the reviewers of this manuscript for their helpful and insightful comments. This research was supported by NASA grants NNC5-712 and NNG04GG91G
Icarus Volume 237, 15 July 2014, Pages 415–418	Jul-14	Convective instabilities during Mars Climate Sounder’s limb staring mode were overestimated	Robert M. Edmonds a, J.R. Murphy a, J.T. Schofield b, N.G. Heavens c	a New Mexico State University, Department of Astronomy, Las Cruces, NM 88003, USA b Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA c Hampton University, Department of Atmospheric and Planetary Sciences, Hampton, VA 23669, USA	© 2014 Elsevier Inc. All rights reserved.	10.1016/j.icarus.2014.04.034	Contractor	b Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA	No	N/A
2006 IEEE International Symposium on Industrial Electronics	Jul-06	High impedance nano charger for on-chip 50nAH rated microbatteries	1) Vinesh Sukumar, Mahmoud Alahmad, Kevin Buck, Mathew Braley, Jasper Nance, Fadi Nessir Zghoul, Herbert Hess, HarryLi, Dave Cox; 2) M.M.Mojarradi, W.C.West, J.F.Whitacre	1) Microelectronics Research and Communications Institute, University ofIdaho, Moscow, Idaho, U.S.A.; 2) Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, U.S.A	© 2006 IEEE	10.1109/ISIE.2006.296043	Contractor	2) Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, U.S.A	No	N/A
IEEE Antennas and Propagation Society International Symposium. 1995 Digest Year: 1995, Volume: 1	Jun-95	Passive EVA tracking system using a pair of 3-element microstrip patch arrays	1) B. Bourgeois, D. Arndt, I. Paz, M. Chavez	1) Div. of Avionic Syst., NASA Johnson Space Center, Houston, TX, USA	© 1995 IEEE	10.1109/APS.1995.529980	Employee	1) Div. of Avionic Syst., NASA Johnson Space Center, Houston, TX, USA	No	N/A
Journal of aircraft	May-04	Transonic Free-to-Roll Analysis of Abrupt Wing Stall on Military Aircraft				10.2514/1.3073	No Access
Journal of aircraft	Nov-94	Forebody flow control on a full-scale F/A-18 aircraft				10.2514/3.46660	No Access
Journal of Geophysical Research: Atmospheres (1984–2012) > Vol 108 Issue D19	Oct-03	Molecular density retrieval and temperature climatology for 40–60 km from SAGE II	S. P. Burton 1 andL. W. Thomason 2	1 Science Applications International Corporation, Hampton, Virginia, USA 2 NASA Langley Research Center, Hampton, Virginia, USA	Copyright 2003 by the American Geophysical Union.	10.1029/2003JD003605	Employee	2 NASA Langley Research Center, Hampton, Virginia, USA	No	S. P. Burton is supported by NASA contract NAS1-02058.
Physics Today 46, 5, 91 (1993)	May-93	Solar Cycle's Effect on How High Hubble Flies	Greg Davidson	NASA, Washington, DC	N/A	10.1063/1.2808920	Employee	NASA, Washington, DC	No	N/A
The European Physical Journal B - Condensed Matter and Complex Systems June 2000, Volume 15, Issue 4, pp 739–764	Jun-00	A wavelet-based method for multifractal image analysis. II. Applications to synthetic multifractal rough surfaces	N. Decoster 1 S.G. Roux 1,2 A. Arnéodo 1	1.Centre de Recherche Paul Pascal, Avenue Schweitzer, 33600 Pessac, FranceFR 2.Climate & Radiation Branch, NASA's Goddard Space Flight Center, Greenbelt, Maryland 20771, USAFR	© Societ`a Italiana di Fisica Springer-Verlag 2000	10.1007/s100510051179	Unsure	1.Centre de Recherche Paul Pascal, Avenue Schweitzer, 33600 Pessac, FranceFR 2.Climate & Radiation Branch, NASA's Goddard Space Flight Center, Greenbelt, Maryland 20771, USAFR	No	We are very grateful to E. Bacry, A. Davis and J.F. Muzy for helpful discussions and technical assistance. This work was supported by NATO (Grant no CRG 960176) and was performed while S.G. Roux held a National Research Council NASA/GSFC Research Associateship.
Monthly weather review	Sep-82	Equatorial Response to Northeasterly Cold Surges as Inferred from Satellite Cloud Imagery				10.1175/1520-0493(1982)110<1306:ERTNCS>2.0.CO;2	No Access
Environment and Planning B: Urban Analytics and City Science Vol 37, Issue 2	Apr-10	The Impact of Urbanization on Current and Future Coastal Precipitation: A Case Study for Houston	1) J Marshall Shepherd, Michael Carter; 2) Michael Manyin; 3) Dmitry Messen; 4) Steve Burian	1) Atmospheric Sciences Program, Department of Geography, University of Georgia, Athens, GA 30602, USA; 2) Science Systems Applications Inc., NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA; 3) Houston-Galveston Area Council, 555 Timmons Lane, Suite 120, Houston, TX 77027, USA; 4) 122 South Central Campus, Civil and Environmental Engineering, University of Utah, Salt Lake City, UT 84112, USA;	© 2010 Pion Ltd and its Licensors	10.1068/b34102t	Employee	2) Science Systems Applications Inc., NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA;	No	The authors acknowledge the support of NASA's Precipitation Measurement Missions program under grant number NNX07AF39G. We acknowledge the helpful comments of the anonymous reviewers and editor.
Proc. SPIE 8860, UV/Optical/IR Space Telescopes and Instruments: Innovative Technologies and Concepts VI, 88600E	Sep-13	Wide-Field InfraRed Survey Telescope (WFIRST) 2.4-meter mission study	1) D. Content, J. Kruk, M. Melton, J. Ruffa; 2) K. Aaron, K. Anderson, R. Capps, Z. Chang, J. Dooley, R. Goullioud, D. Klein, G. Kuan, M. Underhill, D. Van Buren; 3) L. Abplanalp, R. Egerman	1) NASA Goddard Space Flight Ctr. (United States); 2) Jet Propulsion Lab. (United States); 3) Exelis Inc. (United States)	© 2013 SPIE	10.1117/12.2027717	Employee	1) NASA Goddard Space Flight Ctr. (United States);	No	This work is adapted, with slight updates, from the April 2013 final report jointly written by the SDT and WFIRST project team. We gratefully acknowledge that any work such as this is a product of the combined efforts of a large team. Particularly we want to thank the current WFIRST SDT, and project support staff. This work was funded by the National Aeronautics and Space Administration (NASA); Part of this research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with NASA.
Phys. Rev. B 32, 6207	Nov-85	Reassessment of the theory of stimulated Raman scattering	1) G. C. Fralick; 2) R. T. Deck	1) NASA Lewis Research Center, Cleveland, Ohio 44135; 2) Department of Physics and Astronomy, The University of Toledo, Toledo, Ohio 43606	©1985 American Physical Society	10.1103/PhysRevB.32.6207	Employee	1) NASA Lewis Research Center, Cleveland, Ohio 44135;	No	Certain of the graphs presented here were produced with the assistance of Larry Oberle and Howard Reichle of NASA Lewis Laboratory, who we wish to thank
Journal of propulsion and power	Nov-94	Production and Use of Metals and Oxygen for Lunar Propulsion				10.2514/3.51397	No Access
Earth and Planetary Science Letters Volume 285, Issues 3–4, 15 August 2009, Pages 340–346	Aug-09	Mercury's internal magnetic field: Constraints on large- and small-scale fields of crustal origin	Michael E. Purucker a, Terence J. Sabaka a, Sean C. Solomon b, Brian J. Anderson c, Haje Korth c, Maria T. Zuber d, Gregory A. Neumann e	a Raytheon at Planetary Geodynamics Laboratory, Code 698, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA b Department of Terrestrial Magnetism, Carnegie Institution of Washington, Washington, DC 20015, USA c Johns Hopkins University Applied Physics Laboratory, 11100 Johns Hopkins Road, Laurel, MD 20723, USA d Department of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139, USA e Planetary Geodynamics Laboratory, Code 698, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA	© 2009 Elsevier B.V. All rights reserved.	10.1016/j.epsl.2008.12.017	Employee	a Raytheon at Planetary Geodynamics Laboratory, Code 698, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA e Planetary Geodynamics Laboratory, Code 698, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA	No	We thank Mario Acuña and two anonymous reviewers for a critical reading of the manuscript. Figures were produced using the GMT package of Wessel and Smith. The manuscript was written in coordination with that by Uno et al. (2009-this issue), and we thank Catherine Johnson for ongoing discussions and a review of an early draft of our paper. MP and TS were supported by the MESSENGER Participating Scientist grant NNH08CC05C. The MESSENGER project is supported by the NASA Discovery Program through contracts NASW-00002 with the Carnegie Institution of Washington and NAS5-97271 with the Johns Hopkins University Applied Physics Laboratory
Journal of Applied Meteorology and Climatology	Aug-84	Infrared Parameterization and Simple Climate Models	1) David Short, Gerald North; 2) T. Dale Bess, G. Louis Smith	1) NASA Goddard Space Center; 2) NASA Langley Research Center	N/A	10.1175/1520-0450(1984)023<1222:IPASCM>2.0.CO;2	Employee	1) NASA Goddard Space Center; 2) NASA Langley Research Center	No	N/A
JOURNAL OF GUIDANCE, CONTROL, AND DYNAMICS Vol. 29, No. 2	Apr-06	System Identification of a Nonlinear Mode for the Shuttle Radar Topography Mission	1) Paul B. Brugarolas, David S. Bayard, John T. Spanos, and William G. Breckenridge	1) Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California 90012	Copyright © 2005 by the American Institute of Aeronautics and Astronautics, Inc	10.2514/1.6989	Contractor	1) Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California 90012	No	The U.S. Government has a royalty-free license to exercise all rights under the copyright claimed herein for Governmental purposes. All other rights are reserved by the copyright owner. Copies of this paper may be made for personal or internal use, on condition that the copier pay the $10.00 per-copy fee to the Copyright Clearance Center, Inc., 222 Rosewood Drive, Danvers, MA 01923; include the code 0731-5090/06 $10.00 in correspondence with the CCC.
IEEE Transactions on Geoscience and Remote Sensing Year: 1995, Volume: 33, Issue: 3	May-95	Observations of radar backscatter at Ku and C bands in the presence of large waves during the Surface Wave Dynamics Experiment	1) S. V. Nghiem, F. K. Li, S. H. Lou, and G. Neumann; 2) R. E. McIntosh, S. C. Carson, and J. R. Carswell; 3) E. J. Walsh; 4) M. A. Donelan and W. M. Drennan	1) Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109 USA; 2) Department of Electrical Engineering, University of Massachusetts, Amherst, MA 01003 USA; 3) NASA Goddard Space Flight Center, Observational Science Branch, Laboratory for Hydrospheric Processes, Wallops Flight Facility, Wallops Island, VA; 4) National Water Research Institute, Burlington, ON, Canada.	© 1995 IEEE	10.1109/36.387586	Employee	3) NASA Goddard Space Flight Center, Observational Science Branch, Laboratory for Hydrospheric Processes, Wallops Flight Facility, Wallops Island, VA;	No	This research was carried out by the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration. This work was supported in part by the Office of Naval Research under Grant "14-88-J-1028.
Phys. Rev. Lett. 65, 1953	Oct-90	Bioconvective patterns, synchrony, and survival	David A. Noever	NASA Marshall Space Flight Center, ES-76, Huntsville, Alabama 35812	© 1990 The American Physical Society	10.1103/PhysRevLett.65.1953	Employee	NASA Marshall Space Flight Center, ES-76, Huntsville, Alabama 35812	No	N/A
Journal of Geophysical Research: Space Physics > Vol 120 Issue 9	Sep-15	Ion beams in the plasma sheet boundary layer	J. Birn 1,2, M. Hesse 3, A. Runov 4 andX.-Z. Zhou 5	1 Space Science Institute, Boulder, Colorado, USA 2 Los Alamos National Laboratory, Los Alamos, New Mexico, USA 3 NASA Goddard Space Flight Center, Greenbelt, Maryland, USA 4 Department of Earth, Planetary, and Space Sciences, University of California, Los Angeles, California, USA 5 School of Earth and Space Sciences, Peking University, Beijing, China	©2015. American Geophysical Union. All Rights Reserved.	10.1002/2015JA021573	National Lab; Employee	2 Los Alamos National Laboratory, Los Alamos, New Mexico, USA 3 NASA Goddard Space Flight Center, Greenbelt, Maryland, USA	No	The simulation work was performed at Los Alamos under the auspices of the U.S. Department of Energy, supported by NASA grants NNX13AD10G, NNX13AD21G, and NSF grant 1203711. THEMIS data analysis was supported by NASA grants NAS5-0299 and NNX13AF81G. We thank V. Angelopoulos for the use of data from the THEMIS Mission; C.W. Carlson and J.P. McFadden for use of ESA data; D. Larson and R.P. Lin for use of SST data; D.L. Turner and P. Cruce for help with SST data calibration, K.-H. Glassmeier, U. Auster, and W. Baumjohann for the use of FGM data provided with financial support through the DLR contract 50 OC 0302. This work also grew out of a workshop on jet fronts at the International Space Science Institute (ISSI), Bern, Switzerland, and we thank ISSI for its support. Data necessary to understand, evaluate, replicate, and build upon the reported research will be made available upon request.
2013 IEEE International Geoscience and Remote Sensing Symposium - IGARSS	Jul-13	Aquarius salinity and wind retrieval using the CAP algorithm and application to water cycle observation in the Indian Ocean and subcontinent	1) Simon Yueh, Wenqing Tang, Alexander Fore, Julian Chaubell Akiko Hayashi; 2) Gary Lagerloef; 3) Thomas Jackson, and Rajat Bindlish	1) Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA; 2) Earth and Space Research, Seattle, WA, USA; 3) US Department of Agriculture ARS, USA	©2013 IEEE	10.1109/IGARSS.2013.6723146	Contractor; Employee	1) Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA; 3) US Department of Agriculture ARS, USA	No	The work described in this paper was carried out by the Jet Propulsion Laboratory, California Institute of Technology under a contract with the National Aeronautics and Space Administration. USDA is an equal opportunity provider and employer.
The Astrophysical Journal Letters, Volume 504, Number 1	Jul-98	Low-Mass X-Ray Binaries, Millisecond Radio Pulsars, and the Cosmic Star Formation Rate	Nicholas E. White 1 and Pranab Ghosh 1,2,3	1 Laboratory for High Energy Astrophysics, NASA Goddard Space Flight Center, Greenbelt, MD 20771 2 Senior NAS/NRC Resident Research Associate 3 On leave from the Tata Institute of Fundamental Research, Bombay 400 005, India	© 1998. The American Astronomical Society. All rights reserved. Printed in U.S.A.	10.1086/311568	Employee	1 Laboratory for High Energy Astrophysics, NASA Goddard Space Flight Center, Greenbelt, MD 20771	No	N/A
Journal of spacecraft and rockets	Sep-99	Low-speed aerodynamics of a planetary entry capsule				10.2514/2.3498	No Access
Opt. Eng. 42(2), 494-509	Feb-03	Operations and calibration of the solid-state imaging system during the Galileo extended mission at Jupiter	1) Kenneth P. Klaasen, H. Herbert Breneman, Greg C. Levanas; 2) Amy A. Simon-Miller; 3) Donald Banfield	1) California Institute of Technology, Jet Propulsion Laboratory, Mail Stop 230-260, 4800 Oak Grove Drive, Pasadena, California?91109-8099; 2) NASA/Goddard Space Flight Center, Mailstop 693.0, Greenbelt, Maryland?20771; 3) Cornell University, 420 Space Sciences, Ithaca, New York?14853	© 2003 Society of Photo-Optical Instrumentation Engineers	10.1117/1.1534590	Employee	2) NASA/Goddard Space Flight Center, Mailstop 693.0, Greenbelt, Maryland?20771;	No	We acknowledge the major contribution of George Wells of the Jet Propulsion Laboratory ~JPL! in the development of the data-descrambling algorithm that enabled eventual recovery of the majority of the high-resolution Io science images from that encounter. Tom Elliott of JPL provided the motivation for obtaining the end-of-mission warm temperature dark current frames to assess CCD radiation damage and assisted in analyzing that data. A portion of the work described herein was performed at the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.
The Astrophysical Journal, Volume 608, Number 2	2004	The Gamma-Ray Bright BL Lacertae Object RX J1211+2242	V. Beckmann 1, P. Favre 2, F. Tavecchio 3, T. Bussien 4, J. Fliri 5, and A. Wolter 6	1 NASA Goddard Space Flight Center, Code 661, Greenbelt, MD 20771; and Joint Center for Astrophysics, Department of Physics, University of Maryland, Baltimore County, MD 21250 2 INTEGRAL Science Data Centre, Chemin d' Écogia 16, CH-1290 Versoix Switzerland; and Observatoire de Genève, 51 Chemin des Maillettes, CH-1290 Sauverny, Switzerland 3 Osservatorio Astronomico di Brera, via Bianchi 46, I-23807 Merate, Italy 4 École Polytechnique Fédérale de Lausanne, CH-1015 Lausanne, Switzerland 5 Universitäts-Sternwarte München, Scheinerstraße 1, D-81679 München, Germany 6 Osservatorio Astronomico di Brera, via Brera 28, I-20121 Milano, Italy	© 2004. The American Astronomical Society. All rights reserved. Printed in U.S.A.	10.1086/420815	Unsure	1 NASA Goddard Space Flight Center, Code 661, Greenbelt, MD 20771; and Joint Center for Astrophysics, Department of Physics, University of Maryland, Baltimore County, MD 21250	No	This research has made use of the NASA/IPAC Extragalactic Database (NED), which is operated by the Jet Propulsion Laboratory, and of the SIMBAD Astronomical Database, which is operated by the Centre de Donne´es astronomiques de Strasbourg. We thank Laura Maraschi for fruitful discussions and Steve Sturner for proof reading the manuscript. This work has received partial financial support from the Italian Space Agency and from COFIN grant 2001 028773-007.
Visualization '97., Proceedings	Oct-97	UFLIC: a line integral convolution algorithm for visualizing unsteady flows	1) Han-Wei Shen; 2) David L. Kao	1) MRJ Technology Solutions & NASA Ames Research Center; 2) NASA Ames Research Center	N/A	10.1109/VISUAL.1997.663898	Employee	2) NASA Ames Research Center	No	This work was supported in part by NASA contract NAS2-14303. We would like to thank Neal Chaderjian, Ken Gee, Shigeru Obayashi, and Ravi Samtaney for providing their data sets. We also thank Tim Sandstrom, Gail Felchle, Chris Henze, and other members in the Data Analysis Group at NASA Ames Research Center for their helpful comments, suggestions, and technical support.
The Astrophysical Journal, Volume 542, Number 2	2000	A Study of the Physics and Chemistry of L134N	J. E. Dickens 1,2, W. M. Irvine 1, R. L. Snell 1, E. A. Bergin 1,3, F. P. Schloerb 1, P. Pratap 1,4, and M. P. Miralles 1,3	1 Five College Radio Astronomy Observatory, 619 Lederle Graduate Research Center, University of Massachusetts, Amherst, MA 01003 2 Present Address: MS 169-506, Jet Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena, CA 91109 3 Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 4 MIT Haystack Observatory, Route 40, Westford, MA 01886	© 2000. The American Astronomical Society. All rights reserved. Printed in U.S.A.	10.1086/317040	False Positive	2 Present Address: MS 169-506, Jet Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena, CA 91109	No	We acknowledge support from NSF grant AST-9420159 and NASA grants NAGW-436, NAG5-3653, and NAG5- 8718. We would like to thank the sta† at FCRAO and Haystack for their help with the observations and Joe Santoro for helping with the observations and NH3 analysis. We are very grateful to an anonymous referee for many helpful suggestions with the manuscript.
The Astrophysical journal	Feb-88	Infrared radiative transfer in dense disks around young stars				10.1086/166000	No Access
IEEE Transactions on Software Engineering Year: 1983, Volume: SE-9, Issue: 4	Jul-83	Control of a Heterogeneous Two-Server Exponential Queueing System	1) R.L. Larsen; 2) A.K. Agrawala	1) National Aeronautics and Space Administration; 2) Department of Computer Science, University of Maryland, College Park, MD 20742.	© 1983 IEEE	10.1109/TSE.1983.234960	Employee	1) National Aeronautics and Space Administration;	No	N/A
Experimental astronomy Vol. 27 No. 1-2	Dec-09	X-ray interferometry with transmissive beam combiners for ultra-high angular resolution astronomy	1) G. K. Skinner; 2) J. F. Krizmanic	1) NASA-GSFC & CRESST, Greenbelt, Md 20771, USA, & Dept. of Astronomy, Univ, Md, College Park, Md 20742, USA; 2) NASA-GSFC & CRESST, Greenbelt, Md 20771, USA, & Universities Space Research Association	N/A	10.1007/s10686-009-9175-4	Unsure	1) NASA-GSFC & CRESST, Greenbelt, Md 20771, USA, & Dept. of Astronomy, Univ, Md, College Park, Md 20742, USA; 2) NASA-GSFC & CRESST, Greenbelt, Md 20771, USA, & Universities Space Research Association	No	The authors are is grateful to K. Gendreau, Z. Arzoumanian and the team responsible for the development of the GSFC 600 m interferometry test bed and to 3M Optical Service Division and Microsharp Corporation Ltd., U.K. for providing film samples.
Monthly weather review Vol. 129 No. 9	Sep-93	A Mesoscale Gravity-Wave Event Observed during CCOPE. Part IV: Stability Analysis and Doppler-derived Wave Vertical Structure	1) Steven Koch, F. Einaudi, Gerald Heymsfield; 2) Paul Dorian; 3) Stephen Lang	1) NASA, Goddard Space Flight Center; 2) General Sciences Corporation; 3) SSAI	© American Meterological Society	10.1175/1520-0493(1993)121<2483:AMGWEO>2.0.CO;2	Employee	1) NASA, Goddard Space Flight Center;	No	N/A
The Astrophysical Journal, Volume 799, Number 1	Jan-15	NEAR-INFRARED PHOTOMETRY OF Y DWARFS: LOW AMMONIA ABUNDANCE AND THE ONSET OF WATER CLOUDS	S. K. Leggett1 , Caroline V. Morley 2, M. S. Marley 3, and D. Saumon 4	1 Gemini Observatory, Northern Operations Center, 670 N. A'ohoku Place, Hilo, HI 96720, USA 2 Department of Astronomy and Astrophysics, University of California, Santa Cruz, CA 95064, USA 3 NASA Ames Research Center, Mail Stop 245-3, Moffett Field, CA 94035, USA 4 Los Alamos National Laboratory, P.O. Box 1663, MS F663, Los Alamos, NM 87545, USA	© 2015. The American Astronomical Society. All rights reserved.	10.1088/0004-637X/799/1/37	National Lab; Employee	3 NASA Ames Research Center, Mail Stop 245-3, Moffett Field, CA 94035, USA 4 Los Alamos National Laboratory, P.O. Box 1663, MS F663, Los Alamos, NM 87545, USA	No	D.S. is supported by NASA Origins NNH12AT89I. Based on observations obtained at the Gemini Observatory, which is operated by the Association of Universities for Research in Astronomy, Inc., under a cooperative agreement with the NSF on behalf of the Gemini partnership: the National Science Foundation (United States), the Science and Technology Facilities Council (United Kingdom), the National Research Council (Canada), CONICYT (Chile), the Australian Research Council (Australia), Ministério da Ciência, Tecnologia e Inovação (Brazil) and Ministerio de Ciencia, Tecnología e Innovación Productiva (Argentina). S.K.L.'s research is supported by Gemini Observatory. This publication makes use of data products from the Wide-field Infrared Survey Explorer, which is a joint project of the University of California, Los Angeles, and the Jet Propulsion Laboratory/California Institute of Technology, funded by the National Aeronautics and Space Administration. This research has made use of the NASA/IPAC Infrared Science Archive, which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. This research has made use of the Keck Observatory Archive (KOA), which is operated by the W. M. Keck Observatory and the NASA Exoplanet Science Institute (NExScI), under contract with the National Aeronautics and Space Administration.
AIAA JOURNAL Vol. 49, No. 4	Apr-11	Reply by the Authors to G. E. Dorrington	1) Arnab Samanta, Daniel Appelö, and Tim Colonius; 2) Julian Nott; 3) Jeffrey Hall	1) California Institute of Technology, Pasadena, California 91125; 2) Nott Technology, LLC, Santa Barbara, California 93101; 3) Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California 91011	Copyright © 2010 by Arnab Samanta. Published by the American Institute of Aeronautics and Astronautics, Inc., with permission.	10.2514/1.J050961	Contractor	3) Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California 91011	No	N/A
Astrobiology. July 2004, 3(2)	Jul-04	The Catalytic Potential of Cosmic Dust: Implications for Prebiotic Chemistry in the Solar Nebula and Other Protoplanetary Systems	1) Hugh G.M. Hill; 2) Joseph A. Nuth	1) International Space University, Strasbourg Central Campus, Illkirch-Graffenstaden, France; 2) Laboratory for Extraterrestrial Physics, NASA Goddard Space Flight Center, Greenbelt, Maryland	© Mary Ann Liebert, Inc.	10.1089/153110703769016389	Employee	2) Laboratory for Extraterrestrial Physics, NASA Goddard Space Flight Center, Greenbelt, Maryland	No	We thank Mark Iannone, Millersville State University, Millersville, PA, for GCMS analyses of the gases. This research is supported by NASA grants. H.G.M.H. acknowledges funding from the NAS/NRC RRA program.
J. Phys. Chem., 1987, 91 (2), pp 437–440	Jan-87	Photochemistry of diacetylene	1) S. Clicker; 2) H. Okabe	1) Astrochemistry Branch, Goddard Space Fliglt Center, Greenbelt, Maryland 20771; 2) Department of Chemistry, Howard University, Washington, D. C. 20059, and Chemical Kinetics Division, Center for Chemical Physics, National Bureau of Standards. Gaithersburg, Maryland 20899	© 1987 American Chemical Society	10.1021/j100286a036	Employee	1) Astrochemistry Branch, Goddard Space Fliglt Center, Greenbelt, Maryland 20771;	No	We thank the reviewer for numerous constructive comments. H. Okabe thanks Dr. L. Stief for his hospitality during his stay at NASA/GSFC. This research was supported by the NASA Planetary Atmospheres Program.
J. Phys. Chem. A, 2015, 119 (47), pp 11623–11631	Nov-15	Structure, Anharmonic Vibrational Frequencies, and Intensities of NNHNN+	Qi Yu†, Joel M. Bowman*†, Ryan C. Fortenberry*‡, John S. Mancini†, Timothy J. Lee¶, T. Daniel Crawford§, William Klemperer∥, and Joseph S. Francisco⊥	† Department of Chemistry and Cherry L. Emerson Center for Scientific Computation, Emory University, Atlanta, Georgia 30322, United States ‡ Department of Chemistry, Georgia Southern University, Statesboro, Georgia 30460, United States ¶ NASA Ames Research Center, Moffett Field, California 94035-1000, United States § Department of Chemistry, Virginia Tech, Blacksburg, Virginia 24061, United States ∥ Department of Chemistry, Harvard University, Cambridge, Massachusetts 02138, United States ⊥ Department of Chemistry, University of Nebraska—Lincoln, Lincoln, Nebraska 68588, United States	Copyright © 2015 American Chemical Society	10.1021/acs.jpca.5b09682	Employee	¶ NASA Ames Research Center, Moffett Field, California 94035-1000, United States	No	The National Science Foundation grant No. CHE-1463552 supported the work done by J.M.B., Q.Y., and J.S.M. R.C.F. acknowledges Georgia Southern University for providing start-up funds utilized in this work. T.D.C. acknowledges support from the U.S. National Science Foundation (NSF) through award CHE-1058420 and by NSF Multi-User Chemistry Research Instrumentation and Facility (CRIF:MU) award CHE-0741927, which provided the computer hardware employed. This work is also supported by the National Aeronautics and Space Administration through the NASA Astrobiology Institute under Cooperative Agreement Notice NNH13ZDA017C issued through the Science Mission Directorate.
Journal of Quantitative Spectroscopy and Radiative Transfer Volume 101, Issue 3, October 2006, Pages 394–403	Oct-06	Particle size effect on the opposition spike and negative polarization	Andrey A. Ovcharenko a, Sergey Yu. Bondarenko a, Eugeniy S. Zubko a, Yuriy G. Shkuratov a, Gorden Videen b, Robert M. Nelson c, William D. Smythe c	a Astronomical Institute of Kharkov National University, 35 Sumskaya Street, Kharkov 61022, Ukraine b Army Research Laboratory AMSRL-CI-EM, 2800 Powder Mill Road, Adelphi Maryland 20783 USA c Jet Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena, CA 91101, USA	Published by Elsevier Ltd.	10.1016/j.jqsrt.2006.02.036	Contractor; Employee	b Army Research Laboratory AMSRL-CI-EM, 2800 Powder Mill Road, Adelphi Maryland 20783 USA c Jet Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena, CA 91101, USA	No	This work was supported by the TechBase Program on Chemical and Biological Defense and by the Battlefield Environment Directorate under the auspices of the U.S. Army Research Office Scientific Services Program administered by Battelle (Delivery Order 291, Contract. no. DAAD19-02-D-0001). We (RMN and WDS) also appreciate the support from NASA’s Planetary Geology and Geophysics Program.
The Astrophysical Journal Letters, Volume 721, Number 2	Sep-10	ERRATUM: "VERITAS OBSERVATIONS OF A VERY HIGH ENERGY γ-RAY FLARE FROM THE BLAZAR 3C 66A"	V. A. Acciari1, E. Aliu2, T. Arlen3, M. Beilicke4, W. Benbow5, M. Böttcher6, S. M. Bradbury7, J. H. Buckley4, V. Bugaev4, Y. Butt8, K. Byrum9, A. Cannon10, O. Celik3, A. Cesarini11, Y. C. Chow3, L. Ciupik12, P. Cogan13, W. Cui14, M. K. Daniel7,30, R. Dickherber4, T. Ergin8, A. Falcone15, S. J. Fegan3, J. P. Finley14, P. Fortin16, L. Fortson12, A. Furniss17, D. Gall14, K. Gibbs5, G. H. Gillanders11, S. Godambe18, J. Grube10, R. Guenette13, G. Gyuk12, D. Hanna13, E. Hays19, J. Holder2, D. Horan20, C. M. Hui18, T. B. Humensky21, A. Imran22, P. Kaaret23, N. Karlsson12, M. Kertzman24, D. Kieda18, J. Kildea5, A. Konopelko25, H. Krawczynski4, F. Krennrich22, M. J. Lang11, S. LeBohec18, G. Maier13, A. McCann13, M. McCutcheon13, J. Millis26, P. Moriarty1, R. Mukherjee16, T. Nagai22, R. A. Ong3, A. N. Otte17, D. Pandel23, J. S. Perkins5,31, D. Petry27, F. Pizlo14, M. Pohl22, J. Quinn10, K. Ragan13, L. C. Reyes28, P. T. Reynolds29, E. Roache5, H. J. Rose7, M. Schroedter22, G. H. Sembroski14, A. W. Smith9, D. Steele12, S. P. Swordy21, M. Theiling5, J. A. Toner11, A. Varlotta14, V. V. Vassiliev3, R. G. Wagner9, S. P. Wakely21, J. E. Ward10, T. C. Weekes5, A. Weinstein3, D. A. Williams17, S. Wissel21, M. Wood3, and B. Zitzer14	1 Department of Life and Physical Sciences, Galway-Mayo Institute of Technology, Dublin Road, Galway, Republic of Ireland 2 Department of Physics and Astronomy and the Bartol Research Institute, University of Delaware, Newark, DE 19716, USA 3 Department of Physics and Astronomy, University of California, Los Angeles, CA 90095, USA 4 Department of Physics, Washington University, St. Louis, MO 63130, USA 5 Fred Lawrence Whipple Observatory, Harvard-Smithsonian Center for Astrophysics, Amado, AZ 85645, USA 6 Astrophysical Institute, Department of Physics and Astronomy, Ohio University, Athens, OH 45701, USA 7 School of Physics and Astronomy, University of Leeds, Leeds, LS2 9JT, UK 8 Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA 9 Argonne National Laboratory, 9700 S. Cass Avenue, Argonne, IL 60439, USA 10 School of Physics, University College Dublin, Belfield, Dublin 4, Republic of Ireland 11 School of Physics, National University of Ireland, Galway, Republic of Ireland 12 Astronomy Department, Adler Planetarium and Astronomy Museum, Chicago, IL 60605, USA 13 Physics Department, McGill University, Montreal, QC H3A 2T8, Canada 14 Department of Physics, Purdue University, West Lafayette, IN 47907, USA 15 Department of Astronomy and Astrophysics, 525 Davey Lab, Pennsylvania State University, University Park, PA 16802, USA 16 Department of Physics and Astronomy, Barnard College, Columbia University, NY 10027, USA 17 Santa Cruz Institute for Particle Physics and Department of Physics, University of California, Santa Cruz, CA 95064, USA 18 Physics Department, University of Utah, Salt Lake City, UT 84112, USA 19 NASA/Goddard Space-Flight Center, Code 661, Greenbelt, MD 20771, USA 20 Laboratoire Leprince-Ringuet, Ecole Polytechnique, CNRS/IN2P3, F-91128 Palaiseau, France 21 Enrico Fermi Institute, University of Chicago, Chicago, IL 60637, USA 22 Department of Physics and Astronomy, Iowa State University, Ames, IA 50011, USA 23 Department of Physics and Astronomy, University of Iowa, Van Allen Hall, Iowa City, IA 52242, USA 24 Department of Physics and Astronomy, DePauw University, Greencastle, IN 46135-0037, USA 25 Department of Physics, Pittsburg State University, 1701 South Broadway, Pittsburg, KS 66762, USA 26 Department of Physics, Anderson University, 1100 East 5th Street, Anderson, IN 46012, USA 27 European Southern Observatory, Karl-Schwarzchild-Strasse 2, 85748 Garching, Germany 28 Kavli Institute for Cosmological Physics, University of Chicago, Chicago, IL 60637, USA 29 Department of Applied Physics and Instrumentation, Cork Institute of Technology, Bishopstown, Cork, Republic of Ireland 30 Now at Department of Physics, Durham University, South Road, Durham, DH1 3LE, UK. 31 Author to whom any correspondence should be addressed.	© 2010. The American Astronomical Society. All rights reserved. Printed in the U.S.A.	10.1088/2041-8205/721/2/L203	National Lab; Employee	9 Argonne National Laboratory, 9700 S. Cass Avenue, Argonne, IL 60439, USA 19 NASA/Goddard Space-Flight Center, Code 661, Greenbelt, MD 20771, USA	No	N/A
Future Generation Computer Systems Volume 13, Issues 2–3, November 1997, Pages 99–115	Nov-97	Data mining and KDD: Promise and challenges	Usama Fayyad a, Paul Stolorz b	a Microsoft Research, One Microsoji Way, Redmond, WA 98052, USA b Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA	© 1997 Published by Elsevier Science B.V. All rights reserved	10.1016/S0167-739X(97)00015-0	Contractor	b Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA	No	N/A
Journal of Fish and Wildlife Management	Dec-15	Prespawning movements and spawning distribution of sockeye salmon in an urbanizing Alaskan lake	1) J.D.M. Ray; 2) S.A. Sethi; 3) J.H. Eiler, J.E. Joyce	1) California Department of Fish and Wildlife, Aquaculture and Bay Management, 619 Second Street, Eureka, California 95501; 2) U.S. Fish and Wildlife Service, Conservation Genetics Laboratory, 1011 E. Tudor Road, Anchorage, Alaska 99503; 3) National Marine Fisheries Service, Ted Stevens Marine Research Institute, 17109 Point Lena Loop Road, Juneau, Alaska 99801	COPYRIGHT 2015 U.S. Fish and Wildlife Service.	10.3996/112014-JFWM-083	Employee	2) U.S. Fish and Wildlife Service, Conservation Genetics Laboratory, 1011 E. Tudor Road, Anchorage, Alaska 99503; 3) National Marine Fisheries Service, Ted Stevens Marine Research Institute, 17109 Point Lena Loop Road, Juneau, Alaska 99801	No	This project was funded under the Alaska Sustainable Salmon Fund with additional contributions from the Alaska Department of Transportation and Public Facilities. Any use of trade, product, or firm names is for descriptive purposes only and does not imply endorsement by the U.S. Government.
Mon Not R Astron Soc (2000) 319 (1)	Nov-00	Differences between the two anomalous X-ray pulsars: variations in the spin-down rate of 1E 1048.1-5937 and an extended interval of quiet spin-down in 1E 2259+586	Altan Baykal,1 Tod Strohmayer,2 Jean Swank,2 M. Ali Alpar,3 and Michael J. Stark,4	1 Physics Department, Middle East Technical University, Ankara 06531, Turkey 2 Laboratory for High Energy Astrophysics NASA/GSFC Greenbelt, MD 20771, USA 3 Department of Physics, Sabancõ University, Istanbul, Turkey 4 Department of Physics and Astronomy, Denison University, Granville, OH 43023, USA	© 2000 RAS	10.1046/j.1365-8711.2000.03845.x	Employee	2 Laboratory for High Energy Astrophysics NASA/GSFC Greenbelt, MD 20771, USA	No	N/A
International Journal of Impact Engineering Volume 16, Issue 3, June 1995, Pages 405–418	Jun-95	Morphology of meteoroid and debris impact craters formed in soft metal targets on the LDEF satellite	Stanley G. Love†, Donald E. Brownlee†, Nichole L. King†, Friedrich Hörz‡	† Department of Astronomy FM-20, University of Washington, Seattle, WA 98195 USA ‡ Solar System Exploration Division SN4, NASA Johnson Space Center Houston, TX 77058, U.S.A.	Elsevier Science Ltd	10.1016/0734-743X(94)00050-7	Employee	‡ Solar System Exploration Division SN4, NASA Johnson Space Center Houston, TX 77058, U.S.A.	No	The authors thank two anonymous referees for their helpful suggestions. This work was supported by NASA.
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