Broad band observation of gamma-ray burst afterglows to constrain the fireball p

Details Broad band observation of gamma-ray burst afterglows to constrain the fireball p Broad band observation of gamma-ray burst afterglows to constrain the fireball p

Oct 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009xmm..prop...20g&link_type=abstract

XMM-Newton Proposal ID #06506101

Physics

Supernovae, Supernova Remnants, Diffuse (Galactic) Emission And Isolated Neutron Stars, Grb#1

Scientific paper

We propose a broad band observation of one gamma-ray burst afterglow in order to constrain the physics of the fireball that produce the burst, the density profile and composition of the surrounding environment of the burst, and deduce properties about the stellar progenitor of the burst. This observation will be performed in co-ordination with ESO APEX and optical telescopes. We request one observations of 50 kiloseconds, starting 70 kiloseconds after the start of the burst, using the EPIC MOS and PN cameras. This proposal is the continuation of the proposal 60140, accepted during AO08.

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