XMM-Newton Observations of Gamma-Ray Burst Afterglows

Details XMM-Newton Observations of Gamma-Ray Burst Afterglows XMM-Newton Observations of Gamma-Ray Burst Afterglows

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aipc..727..229s&link_type=abstract

GAMMA-RAY BURSTS: 30 YEARS OF DISCOVERY: Gamma-Ray Burst Symposium. AIP Conference Proceedings, Volume 727, pp. 229-232 (2004).

Computer Science

Gamma-Ray Sources, Gamma-Ray Bursts, X-Ray Sources, X-Ray Bursts, Spaceborne And Space Research Instruments, Apparatus, And Components

Scientific paper

XMM-Newton observes X-ray afterglows of Gamma-Ray Bursts (GRB) with a reaction time of the order of 10 hours. Scientific highlights are the detection of an afterglow 67 days after the GRB occurred, Dark Bursts and the detection of soft X-ray emission lines. Based on the established reaction time and on the obtained results scientific objectives of future XMM-Newton observations of GRB afterglows are formulated.

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