The X-ray afterglow of GRB030329 at early and late times

Details The X-ray afterglow of GRB030329 at early and late times The X-ray afterglow of GRB030329 at early and late times

2004-03-29

arxiv.org/abs/astro-ph/0403648v1

Astronomy and Astrophysics

Astrophysics

4 pages, 2 figures, to appear in the Santa Fe GRB Conference Proceedings, 2003

Scientific paper

10.1063/1.1810855

Thanks to its extraordinary brightness, the X-ray afterglow of GRB030329 could be studied by XMM-Newton up to two months after the prompt Gamma-ray emission. We present the results of two XMM-Newton observations performed on May 5 and 29, as well as an analysis of the Rossi-XTE data of the early part of the afterglow, discussing in particular the stability of the X-ray spectrum and presenting upper limits on the presence of X-ray emission lines.

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