Is there a significant fraction of GRBs located in dusty environs?

Astronomy and Astrophysics – Astronomy

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Gamma-Ray Sources (Astronomical), Redshift, X-Ray Spectra, Gamma-Ray Sources, Gamma-Ray Bursts, Distances, Redshifts, Radial Velocities, Spatial Distribution Of Galaxies, Photometric, Polarimetric, And Spectroscopic Instrumentation

Scientific paper

We discuss to what extent the current sample of Swift bursts with OA spectroscopy is a biased subsample of all Swift detected GRBs. For that purpose we define an X-ray selected statistical sample of Swift bursts with optimal conditions for ground-based follow up from the period March 2005 to September 2008; 146 bursts fulfill our sample criteria. We derive the redshift distribution for the statistical sample and conclude that less than 18% of Swift bursts can be at z>7. Finally, by splitting the sample into three subsamples we conclude that the sample of GRBs with OA spectroscopy is not representative for all Swift bursts, most likely due to a bias against the most dusty sight-lines. This should be taken into account when determining, e.g., the redshift or metallicity distribution of GRBs and when using GRBs as a probe of star formation.

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