Optical afterglows of gamma-ray bursts: a bimodal distribution?"

Abstract

The luminosities of the optical afterglows of Gamma Ray Bursts, 12 hours (rest frame time) after the trigger, show a surprising clustering, with a minority of events being at a significant smaller luminosity. If real, this dichotomy would be a crucial clue to understand the nature of optically dark afterglows, i.e. bursts that are detected in the X-ray band, but not in the optical. We investigate this issue by studying bursts of the pre-Swift era, both detected and undetected in the optical. The limiting magnitudes of the undetected ones are used to construct the probability that a generic bursts is observed down to a given magnitude limit. Then, by simulating a large number of bursts with pre-assigned characteristics, we can compare the properties of the observed optical luminosity distribution with the simulated one. Our results suggest that the hints of bimodality present in the observed distribution reflects a real bimodality: either the optical luminosity distributions of bursts is intrinsically bimodal, or there exists a population of bursts with a quite significant grey absorption, i.e. wavelength independent extinction. This population of intrinsically weak or grey-absorbed events can be associated to dark bursts.

arXiv comment10 pages, 5 figures, accepted for publication in MNRAS

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• Afterglow rebrightenings as a signature of a long-lasting central engine activity? The emblematic case of GRB 100814A
• Optical afterglow luminosities in the Swift epoch: confirming clustering and bimodality
• On Some Properties of the Beta Normal Distribution
• Are GRB optical afterglows relatively brighter at high z?