A Statistical Study of the Redshifts of Long Gamma-Ray Bursts

Details A Statistical Study of the Redshifts of Long Gamma-Ray Bursts A Statistical Study of the Redshifts of Long Gamma-Ray Bursts

Feb 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006sgrb.confe...5b&link_type=abstract

Presented at the KITP Conference: Supernova and Gamma-Ray Burst Remnants, Feb 10, 2006, Kavli Institute for Theoretical Physics,

Physics

Scientific paper

The directly measured redshifts of the long gamma-ray bursts - obtained from the afterglow data - are separated into two samples. The bursts detected first by the Swift satellite gives the "Swift-sample"; th eremaining ones forms the "non-Swift-sample". We perfored five statistical tests to compare the redshifts in these two samples. All these tests show that in the Swift sample the redshifts are on average larger.

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