Selection Effects on the Observed Redshift Dependence of GRB Jet Opening Angles
arXiv:1110.4943 · doi:10.1088/0004-637X/745/2/168
Abstract
Apparent redshift dependence of the jet opening angles () of gamma-ray bursts (GRBs) is observed from current GRB sample. We investigate whether this dependence can be explained with instrumental selection effects and observational biases by a bootstrapping method. Assuming that (1) the GRB rate follows the star formation history and the cosmic metallicity history and (2) the intrinsic distributions of the jet-corrected luminosity () and are a Gaussian or a power-law function, we generate a mock {\em Swift}/BAT sample by considering various instrumental selection effects, including the flux threshold and the trigger probability of BAT, the probabilities of a GRB jet pointing to the instrument solid angle and the probability of redshift measurement. Our results well reproduce the observed dependence. We find that in case of good consistency between the mock and observed samples can be obtained, indicating that both and are degenerate for a flux-limited sample. The parameter set gives the best consistency for the current {\em Swift} GRB sample. Considering the beaming effect, the derived intrinsic local GRB rate accordingly is Gpc yr, inferring that of Type Ib/c SNe may be accompanied by a GRB.
25pages, 7 figures. ApJ in press
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