The Swift Gamma-Ray Burst Mission:. First Results

Details The Swift Gamma-Ray Burst Mission:. First Results The Swift Gamma-Ray Burst Mission:. First Results

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ebhe.conf..119g&link_type=abstract

ENERGY BUDGET IN THE HIGH ENERGY UNIVERSE . Proceedings of the International Workshop. Held 22-24 February 2006 in Kashiwa, Japa

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Since its launch on 20 November 2004, the Swift mission is detecting ~100 new gamma-ray bursts (GRBs) each year, and immediately (within two minutes) starting simultaneous X-ray and UV/optical observations of the afterglow. It has already collected am impressive database of bursts, including prompt emission to higher sensitivity than BATSE, uniform monitoring of afterglows, and rapid follow-up by other observatories notified through the GCN.

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