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A&A 449, 79-88 (2006)
DOI: 10.1051/0004-6361:20054317
Constraining the GRB collimation with a survey for orphan afterglows
A. Rau1, J. Greiner1 and R. Schwarz21 Max-Planck-Institut für extraterrestrische Physik, Giessenbachstrasse, 85748 Garching, Germany
e-mail: arau@mpe.mpg.de
2 Astrophysikalisches Institut Potsdam, An der Sternwarte 16, 14482 Potsdam, Germany
(Received 7 October 2005 / Accepted 22 November 2005)
Abstract
Gamma-ray bursts are believed to be produced in
highly-relativistic collimated outflows. Support for this comes among
others from the association of the times of detected breaks in the
decay of afterglow light curves with the collimation angle of the
jets. An alternative approach to estimate a limit on the collimation
angle uses GRB afterglows without detected prompt-emission
counterparts. Here we report on the analysis of a dedicated survey
for the search of these orphan afterglows using the Wide Field Imager
at the 2.2 m MPI/ESO telescope at La Silla, Chile. We monitored
~12 deg2 in up to 25 nights typically spaced by one to two
nights with a limiting magnitude of R=23. Four previously unknown
optical transients were discovered and three of these associated with
a flare star, a cataclysmic variable and a dwarf nova. The fourth
source shows indications for an extragalactic origin but the sparse
sampling of the light curve prevents a reliable classification. We
discuss the results in the context of the collimation of GRBs.
Key words: gamma rays: bursts -- surveys
SIMBAD Objects
© ESO 2006
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