GLAST: physics goals and instrument status (original) (raw)

ADS

Abstract

The Gamma-ray Large Area Space Telescope (GLAST) is a space-based observatory scheduled to launch in October 2007 with two instruments: (1) the GLAST Burst Monitor (GBM), sensitive to photon energies between 8 keV and 25 MeV and optimized to detect gamma-ray bursts, and (2) the Large Area Telescope (LAT), sensitive to gamma rays between 20 MeV and 300 GeV and designed to survey the gamma-ray sky with unprecedented sensitivity. We describe the LAT and the GBM. We then focus on the LAT's capabilities for studying active galactic nuclei.

Publication:

Journal of Physics Conference Series

Pub Date:

March 2007

DOI:

10.1088/1742-6596/60/1/020

10.48550/arXiv.astro-ph/0610960

arXiv:

arXiv:astro-ph/0610960

Bibcode:

2007JPhCS..60..115C

Keywords:

E-Print:

to appear in Proceedings of TeV Particle Astrophysics II, 28-31 August 2006, Madison, WI, USA