Observational difference between gamma and X-ray properties of optically dark and bright GRBs

Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics

Scientific paper

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Santa Fe proc

Scientific paper

10.1063/1.2943506

Using the discriminant analysis of the multivariate statistical analysis we
compared the distribution of the physical quantities of the optically dark and
bright GRBs, detected by the BAT and XRT on board of the Swift Satellite. We
found that the GRBs having detected optical transients (OT) have systematically
higher peak fluxes and lower HI column densities than those without OT.

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