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Title: FERMI observations of high-energy gamma-ray emission from GRB 090217A

Journal Article · · The Astrophysical Journal. Letters
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The Fermi observatory is advancing our knowledge of gamma-ray bursts (GRBs) through pioneering observations at high energies, covering more than seven decades in energy with the two on-board detectors, the Large Area Telescope (LAT) and the Gamma-ray Burst Monitor (GBM). Here, we report on the observation of the long GRB 090217A which triggered the GBM and has been detected by the LAT with a significance greater than 9σ. We present the GBM and LAT observations and on-ground analyses, including the time-resolved spectra and the study of the temporal profile from 8 keV up to ~1 GeV. All spectra are well reproduced by a Band model. We compare these observations to the first two LAT-detected, long bursts GRB 080825C and GRB 080916C. These bursts were found to have time-dependent spectra and exhibited a delayed onset of the high-energy emission, which are not observed in the case of GRB 090217A. We discuss some theoretical implications for the high-energy emission of GRBs.

Research Organization:
SLAC National Accelerator Lab., Menlo Park, CA (United States)
Sponsoring Organization:
USDOE
Contributing Organization:
The Fermi LAT Collaboration
Grant/Contract Number:
AC02-76SF00515
OSTI ID:
1357545
Journal Information:
The Astrophysical Journal. Letters, Vol. 717, Issue 2; ISSN 2041-8205
Publisher:
Institute of Physics (IOP)Copyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 26 works
Citation information provided by
Web of Science

References (16)

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conference January 2009
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Cited By (5)

Bulk Lorentz factors of gamma-ray bursts journal January 2018
“SELF-ABSORBED” GeV LIGHT CURVES OF GAMMA-RAY BURST AFTERGLOWS journal May 2014
Bayesian Time-resolved Spectroscopy of GRB Pulses journal November 2019
"Self-absorbed" GeV light-curves of Gamma-Ray Burst afterglows text January 2013
Bulk Lorentz factors of Gamma-Ray Bursts text January 2017

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