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OPTICAL CLASSIFICATION OF GAMMA-RAY BURSTS IN THE SWIFT ERA

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A. J. van der Horst1, C. Kouveliotou2, N. Gehrels3, E. Rol4, R. A. M. J. Wijers5, J. K. Cannizzo3,6, J. Racusin7, and D. N. Burrows7

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We propose a new method for the classification of optically dark gamma-ray bursts (GRBs), based on the X-ray and optical-to-X-ray spectral indices of GRB afterglows, and utilizing the spectral capabilities of Swift. This method depends less on model assumptions than previous methods, and can be used as a quick diagnostic tool to identify optically sub-luminous bursts. With this method we can also find GRBs that are extremely bright at optical wavelengths. We show that the previously suggested correlation between the optical darkness and the X-ray/gamma-ray brightness is merely an observational selection effect.


Keywords

gamma rays: bursts


Dates

Issue 2 (2009 July 10)

Received 2009 February 4, accepted for publication 2009 April 29

Published 2009 June 18

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