B. B. Jones
Stanford University
10 Papers
33 Citations
B. B. Jones is an academic researcher from Stanford University. The author has contributed to research in topics: Egret & Gamma ray. The author has an hindex of 7, co-authored 10 publications.
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Papers
•Book
The Third Egret Catalog of High-Energy Gamma-Ray Sources
R. C. Hartman,D. L. Bertsch,Steven D. Bloom,Steven D. Bloom,A. W. Chen,P. Deines-Jones,J. A. Esposito,C. E. Fichtel,D. P. Friedlander,D. P. Friedlander,Stanley D. Hunter,L. M. McDonald,L. M. McDonald,P. Sreekumar,D. J. Thompson,B. B. Jones,Yiing Lin,Peter F. Michelson,P. L. Nolan,W. F. Tompkins,Gottfried Kanbach,H. A. Mayer-Hasselwander,A. Mücke,A. Mücke,Martin Pohl,Martin Pohl,Olaf Reimer,D. A. Kniffen,E. J. Schneid,C. von Montigny,Reshmi Mukherjee,Brenda Dingus +31 more
- 06 Aug 2013
TL;DR: The third catalog of high-energy gamma-ray sources detected by the EGRET telescope on the Compton Gamma Ray Observatory includes data from 1991 April 22 to 1995 October 3 (cycles 1, 2, 3, and 4 of the mission).
Beam Test of Gamma-ray Large Area Space Telescope Components
W. B. Atwood,Steven Ritz,P.L. Anthony,Elliott D. Bloom,P. E. Bosted,J. Bourotte,C. Chaput,X. Chen,D.L. Chenette,D. Engovatov,R. Erickson,T. Fieguth,P. Fleury,R. Gearhart,G.L. Godfrey,J. E. Grove,J.A. Hernando,M. Hirayama,S. Jaggar,R. P. Johnson,W. N. Johnson,B. B. Jones,W. Kroeger,Y. C. Lin,C. Meetre,Peter F. Michelson,Peter Milne,A. A. Moiseev,P. L. Nolan,J. P. Norris,M. J. Oreglia,Jonathan F. Ormes,Bernard F. Phlips,A. Pocar,Z. M. Szalata,D. J. Thompson,W. F. Tompkins +36 more
TL;DR: A beam test of GLAST (Gamma-ray Large Area Space Telescope) components was performed at the Stanford Linear Accelerator Center in October, 1997 as discussed by the authors, where the performance of the tracker, calorimeter, and anti-coincidence charged particle veto were evaluated.
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The pulsar contribution to the diffuse galactic gamma-ray emission
TL;DR: In this paper, it was shown that pulsars contribute very little to the diffuse emission at lower energies, whereas above 1 GeV they can account for 18% of the observed intensity in selected regions for a reasonable number of directly observable γ-ray pulsars (~14).
22
EGRET Gamma-Ray Observations of the Crab P2/P1 Ratio
TL;DR: This paper showed that the high-energy gamma-ray light curve has changed little over the lifetime of the Energetic Gamma-Ray Experiment Telescope (EGRET) on the Compton Gamma Ray Observatory.
13
EGRET Gamma-Ray Observations of the Crab P2/P1 Ratio
TL;DR: In this paper, the Energetic Gamma-Ray Experiment Telescope (EGRET) on the Compton Gamma Ray Observatory (COS-B) showed that the high-energy gamma-ray light curve has changed little over the lifetime of the instrument.
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