Astronomy and Astrophysics – Astrophysics
Scientific paper
2006-03-11
AIP Conf.Proc.836:414-419,2006
Astronomy and Astrophysics
Astrophysics
11 pages, A&A 449, 79-88
Scientific paper
10.1063/1.2207929
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 2.2m MPI/ESO telescope at La Silla, Chile. We monitored ~12 square degrees. 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.
Greiner Jochen
Rau Arne
Schwarz Robert
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