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

2); A. Tiengo (1; Cambridge; (5) XMM-SOC; E. Rossi (4); G. Ghirlanda (1); G. Ghisellini (3); Merate; (4) IoA; Milano; (2) Milano Univ.; (3) OAB; N. Schartel (5) ((1) IASF; S. Mereghetti (1)

arxiv: astro-ph/0403648 · v1 · submitted 2004-03-29 · 🌌 astro-ph

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

A. Tiengo (1 , 2) , S. Mereghetti (1) , G. Ghisellini (3) , E. Rossi (4) , G. Ghirlanda (1) , N. Schartel (5) ((1) IASF , Milano; (2) Milano Univ.; (3) OAB

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Merate; (4) IoA Cambridge; (5) XMM-SOC Vilspa)

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keywords x-rayafterglowearlyemissiongrb030329xmm-newtonanalysisbrightness

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

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