Swift and XMM observations of the dark GRB 050326.

Authors :: Moretti, A.
De Luca, A.
Malesani, D.
Campana, S.
Tiengo, A.
Reeves, J. N.
Capalbi, M.
Chincarini, G.
Covino, S.
Cusumano, G.
Giommi, P.
La Parola, V.
Mangano, V.
Mineo, T.
Perri, M.
Romano, P.
Tagliaferri, G.
Source :: AIP Conference Proceedings; 2006, Vol. 836 Issue 1, p285-288, 4p, 3 Graphs
Publication Year :: 2006
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. © 2006 American Institute of Physics [ABSTRACT FROM AUTHOR]