The Glast Mission and Observability of Supernovae Remnants

Details The Glast Mission and Observability of Supernovae Remnants The Glast Mission and Observability of Supernovae Remnants

Nov 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007auhe.conf..189t&link_type=abstract

ASTROPHYSICS AT ULTRA-HIGH ENERGIES. Proceedings of the 15th Course of the International School of Cosmic Ray Astrophysics . Hel

Astronomy and Astrophysics

Astronomy

Glast, Gamma-Astronomy, Supernovae Remnants, Nasa

Scientific paper

The Gamma-ray Large Area Space Telescope (GLAST) is a collaboration of several countries: France, Germany, Italy, Japan, Sweden and United States of America. GLAST is a satellite-based observatory that will study the Cosmos in the Energy Range 10 keV - 300 GeV and consists of two different instruments: the Large Area Telescope (LAT) and the GLAST Burst Monitor (GBM). The two instruments are ready and now are being tested and integrated with the spacecraft: the launch is scheduled for October 2007. GLAST will improve the knowledge about several astrophysical sources (AGNs, Pulsars, GRBs, etc.). In this paper we will consider the scientific case of gamma-ray emitting Super-novae Remnants (SNRs).

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