GRB Simulations in GLAST

Conference · Mon Oct 22 04:00:00 EDT 2007 · AIP Conf.Proc.906:1-10,2007

DOI:https://doi.org/10.1063/1.2737401· OSTI ID:918542

Omodei, Nicola; Battelino, Milan; Komin, Nukri; Longo, Francesco; McEnery, Julie; Ryde, Felix

The Gamma-ray Large Area Space Telescope (GLAST), scheduled to be launched in fall of 2007, is the next generation satellite for high-energy gamma-ray astronomy. The Large Area Telescope (LAT) is a pair conversion telescope built with a high precision silicon tracker, a segmented CsI electromagnetic calorimeter and a plastic anticoincidence shield. The LAT will survey the sky in the energy range between 20 MeV to more than 300 GeV, shedding light on many issues left open by its highly successful predecessor EGRET. LAT will observe Gamma-Ray Bursts (GRB) in an energy range never explored before; to tie these frontier observations to the better-known properties at lower energies, a second instrument, the GLAST Burst Monitor (GBM) will provide important spectra and timing in the 10 keV to 30 MeV range. We briefly present the instruments onboard the GLAST satellite, their synergy in the GRB observations and the work done so far by the collaboration in simulation, analysis, and GRB sensitivity estimation.

• Research Organization: Stanford Linear Accelerator Center (SLAC)
• Sponsoring Organization: USDOE
• DOE Contract Number: AC02-76SF00515
• OSTI ID: 918542
• Report Number(s): SLAC-PUB-12904
• Conference Information: Journal Name: AIP Conf.Proc.906:1-10,2007 Journal Volume: 906
• Country of Publication: United States
• Language: English

Related Subjects

71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ANTICOINCIDENCE
Astrophysics
Instrumentation
ASTRO
INST
CALORIMETERS
COSMIC GAMMA BURSTS
ENERGY RANGE
GAMMA ASTRONOMY
MEV RANGE
MONITORS
SATELLITES
SENSITIVITY
SILICON
SIMULATION
SKY
SPECTRA
TELESCOPES