THE FIRST FERMI-LAT GAMMA-RAY BURST CATALOG
By M. Ackermann, M. Ajello, K. Asano, M. Axelsson, L. Baldini, J. Ballet, G. Barbiellini, D. Bastieri, K. Bechtol, R. Bellazzini and 170 more. 2013
212 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/f5418a3628d0de2779c2b9f7fc831e8d074042b2
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Citations in the corpus
- THE THIRD FERMI GBM GAMMA-RAY BURST CATALOG: THE FIRST SIX YEARS (2016, background): “In addition, the number of Autonomous Repoint Requests (ARRs, described in Section 2.2 below) and GRBs detected by LAT observed with high confidence above 100MeV (and 20MeV) are given (Ackermann et al. 2013).”
- THE SECOND FERMI GBM GAMMA-RAY BURST CATALOG: THE FIRST FOUR YEARS (2014, background): “In addition the numbers of autonomous repoint requests (ARRs, described in Section 2.2 below) and GRBs detected by LAT, observed with high confidence above 100 MeV (and 20 MeV), are given (Ackermann et al. 2013).”
- The physics of gamma-ray bursts & relativistic jets (2014, methodology): “os, 2002a). The same conclusion can be obtained from the Fermi/LAT data alone. The lack of an excess ux at high energies | there is no evidence for departure from a Band function t for most GRBs e.g. Ackermann et al. (2013a) | means that the IC scattering of photons near the peak ( p) into the LAT b”