Swift and XMM observations of the dark GRB 050326

Author(s)
Moretti, A.
de Luca, A.
Malesani, D.
Capalbi, Milvia
Date Issued
2006-05-01
Mission(s)
Abstract
We present a detailed analysis of the GRB 050326 prompt and afterglow emission. The combined capabilities of Swift (which sampled the light curve for a relatively long time span) and XMM (which ensured a large statistics) allowed to obtain a thorough characterization of the afterglow properties.
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