A Search for Untriggered GRB Afterglows with ROTSE-III

Details A Search for Untriggered GRB Afterglows with ROTSE-III A Search for Untriggered GRB Afterglows with ROTSE-III

2005-06-19

arxiv.org/abs/astro-ph/0506442v1

Astrophys.J.631:1032-1038,2005

Astronomy and Astrophysics

Astrophysics

Seven pages, five figures, uses emulateapj class file. Accepted to Astrophysical Journal

Scientific paper

10.1086/432832

We present the results of a search for untriggered gamma-ray burst (GRB) afterglows with the Robotic Optical Transient Search Experiment-III (ROTSE-III) telescope array. This search covers observations from September 2003 to March 2005. We have an effective coverage of 1.74 deg^2 yr for rapidly fading transients that remain brighter than ~ 17.5 magnitude for more than 30 minutes. This search is the first large area survey to be able to detect typical untriggered GRB afterglows. Our background rate is very low and purely astrophysical. We have found 4 previously unknown cataclysmic variables (CVs) and 1 new flare star. We have not detected any candidate afterglow events or other unidentified transients. We can place an upper limit on the rate of fading optical transients with quiescent counterparts dimmer than ~ 20th magnitude at a rate of less than 1.9 deg^-2 yr-1 with 95% confidence. This places limits on the optical characteristics of off-axis (orphan) GRB afterglows. As a byproduct of this search, we have an effective ~ 52 deg^2 yr of coverage for very slowly decaying transients, such as CVs. This implies an overall rate of outbursts from high galactic latitude CVs of 0.1 deg^2 yr^-1.

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