Abstract
We present a catalog of X-ray afterglows observed by BeppoSAX, XMM-Newton and Chandra. We observe a temporal evolution of the afterglow properties, that we link with a jet effect. We then investigate on the Sako and Rutledge method to detect X-ray lines within the afterglow spectra, and find that this method can be improved.
Original language | English |
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Pages (from-to) | 1485-1486 |
Number of pages | 2 |
Journal | Nuovo Cimento della Societa Italiana di Fisica B |
Volume | 121 |
Issue number | 12 |
DOIs | |
State | Published - Dec 2006 |