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Title: LAT Onboard Science: Gamma-Ray Burst Identification

Journal Article · · AIP Conference Proceedings
DOI:https://doi.org/10.1063/1.2757449· OSTI ID:21067312
; ; ;  [1];  [2];  [3];  [2];  [4]
  1. Ohio State University (United States)
  2. NASA Goddard Space Flight Center (United States)
  3. University of Denver (United States)
  4. Stanford Linear Accelerator Center (United States)

The main goal of the Large Area Telescope (LAT) onboard science program is to provide quick identification and localization of Gamma Ray Bursts (GRB) onboard the LAT for follow-up observations by other observatories. The GRB identification and localization algorithm will provide celestial coordinates with an error region that will be distributed via the Gamma ray burst Coordinate Network (GCN). We present results that show our sensitivity to bursts as characterized using Monte Carlo simulations of the GLAST observatory. We describe and characterize the method of onboard track determination and the GRB identification and localization algorithm. Onboard track determination is considerably different than in the on-ground case, resulting in a substantially altered point spread function. The algorithm contains tunable parameters which may be adjusted after launch when real bursts characteristics at very high energies have been identified.

OSTI ID:
21067312
Journal Information:
AIP Conference Proceedings, Vol. 921, Issue 1; Conference: 1. GLAST symposium, Stanford, CA (United States), 5-8 Feb 2007; Other Information: DOI: 10.1063/1.2757449; (c) 2007 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA); ISSN 0094-243X
Country of Publication:
United States
Language:
English

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