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arXiv:astro-ph/0403648 (astro-ph)
[Submitted on 29 Mar 2004]

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

Authors: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, Merate; (4) IoA, Cambridge; (5) XMM-SOC, Vilspa)
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Abstract: 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.
Comments: 4 pages, 2 figures, to appear in the Santa Fe GRB Conference Proceedings, 2003
Subjects: Astrophysics (astro-ph)
Cite as: arXiv:astro-ph/0403648
  (or arXiv:astro-ph/0403648v1 for this version)
  https://doi.org/10.48550/arXiv.astro-ph/0403648
Related DOI: https://doi.org/10.1063/1.1810855

Submission history

From: Tiengo Andrea [view email]
[v1] Mon, 29 Mar 2004 08:15:10 UTC (37 KB)
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