Moretti, A.A.Morettide Luca, A.A.de LucaMalesani, D.D.MalesaniCapalbi, MilviaMilviaCapalbiGiommi, PaoloPaoloGiommiPerri, MatteoMatteoPerri2020-09-172020-09-172006-05-01https://hdl.handle.net/20.500.13025/467GAMMA-RAY BURSTS IN THE SWIFT ERA Sixteenth Maryland Astrophysics Conference. AIP Conference Proceedings, Volume 836, pp. 285-288 (2006).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.Swift and XMM observations of the dark GRB 05032610.1063/1.2207903http://adsabs.harvard.edu/abs/2006AIPC..836..285M2006AIPC..836..285M