Swift and XMM observations of the dark GRB 050326

Details Swift and XMM observations of the dark GRB 050326 Swift and XMM observations of the dark GRB 050326

May 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aipc..836..285m&link_type=abstract

GAMMA-RAY BURSTS IN THE SWIFT ERA: Sixteenth Maryland Astrophysics Conference. AIP Conference Proceedings, Volume 836, pp. 285-

Astronomy and Astrophysics

Astrophysics

Gamma-Ray Sources, Gamma-Ray Bursts, X-Ray Sources, X-Ray Bursts

Scientific paper

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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