C. Chaput
Stanford University
6 Papers
42 Citations
C. Chaput is an academic researcher from Stanford University. The author has contributed to research in topics: Beam (structure) & Linear particle accelerator. The author has an hindex of 3, co-authored 6 publications.
Chat about Author
Papers
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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Beam test of gamma-ray large area space telescope components
W. B. Atwood,W. B. Atwood,S. Ritz,P. 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. Godfrey,J. E. Grove,J.A. Hernando,M. Hirayama,S. Jaggar,R. P. Johnson,W. N. Johnson,B.B. Jones,W. Kröger,Yiing Lin,C. Meetre,Peter F. Michelson,Peter Milne,A. A. Moiseev,A. A. Moiseev,P. L. Nolan,Jay P. Norris,M. J. Oreglia,Jonathan F. Ormes,Bernard F. Phlips,Bernard F. Phlips,A. Pocar,Hartmut Sadrozinski,Z. M. Szalata,D. J. Thompson,W. F. Tompkins +40 more
TL;DR: A beam test of Gamma-ray Large Area Space Telescope (GLAST) components was performed at the Stanford Linear Accelerator Center in October 1997 as mentioned in this paper, where the performance of the tracker, calorimeter, and anti-coincidence charged particle veto were evaluated.
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Simulating the Glast satellite with Gismo
TL;DR: This group has been involved primarily with software issues, particularly with an object-oriented Monte Carlo package called Gismo, which has modeled all aspects of the satellite's design and performance.
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•Posted Content
Detection of Galactic Dark Matter by GLAST
A. A. Moiseev,Jonathan F. Ormes,H. Arrighi,Elliott D. Bloom,C. Chaput,S. Digel,D. Engovatov,Jay P. Norris,J. Silvis +8 more
TL;DR: The Gamma-ray Large Area Space Telescope (GLAST) is scheduled for launch in 2005 by NASA and will be capable of searching for these gamma-ray lines in the energy range from 20 GeV to ~500 GeV as mentioned in this paper.
1
A Search for Aperiodic Millisecond Variability in Cygnus X-1
C. Chaput,E. D. Bloom,L. R. Cominsky,L. R. Cominsky,G. Godfrey,Paul Hertz,Jeffrey D. Scargle,G. Shabad,H. Wen,Kent S. Wood,Daryl J. Yentis +10 more
TL;DR: In this article, the authors conducted a search for aperiodic millisecond variability in the integrated 1-25 keV X-ray region of Cyg X-1 and found no evidence for excess power above 25 Hz in the HEAO A-1 data.