Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/26520
 Title: The X-ray afterglow of GRB 020322 Authors: Watson, D.Reeves, J. N.Osborne, J. P.Tedds, Jonathan A.O'Brien, P. T.Tomas, L.Ehle, M. First Published: 1-Nov-2002 Publisher: EDP Sciences for European Southern Observatory (ESO) Citation: Astronomy & Astrophysics, 2002, 395 (2), pp. L41-L45 Abstract: The spectrum of the afterglow of GRB 020322 is the highest-quality X-ray spectrum of a GRB afterglow available to date. It was detected by XMM-Newton in an observation starting fifteen hours after the GRB with a mean 0.2-10.0 keV observed flux of $3.5\pm0.2\times10^{-13}$ erg cm -2 s -1, making it the brightest X-ray afterglow observed so far with XMM-Newton. The source faded; its lightcurve was well fit by a power-law with a decay index of $1.26\pm0.23$. The spectrum is adequately fit with a power-law absorbed with neutral or ionised gas significantly in excess of the foreground Galactic column, at redshift 1.8-1.1+1.0 or with low metal abundances. No spectral line or edge features are detected at high significance, in particular, a thermal emission model fits the data poorly, the upper limit on its contribution to the spectrum is $3.7\times10^{-14}$ erg cm -2 s -1, or ~10% of the total flux. No spectral variability is observed. DOI Link: 10.1051/0004-6361:20021501 ISSN: 0004-6361 Links: http://hdl.handle.net/2381/26520http://www.aanda.org/articles/aa/abs/2002/44/aaei272/aaei272.html Version: Publisher Version Status: Peer-reviewed Type: Journal Article Rights: Copyright © 2002 ESO. Reproduced with permission from Astronomy & Astrophysics, © ESO. Appears in Collections: Published Articles, Dept. of Physics and Astronomy

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