What can BeppoSAX tell us about short GRBs: An update from the Subsecond GRB Project

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Proc. 5th Huntsville GRB Symposium

Scientific paper

10.1063/1.1361500

We present some statistical considerations on the BeppoSAX hunt for subsecond GRBs at the Scientific Operation Center. Archive analysis of a BATSE/SAX sub-sample of bursts indicates that the GRB Monitor is sensitive to short (< 2 sec) events, that are in fact about 22% of the total. The non-detection of corresponding prompt X-ray counterparts to short bursts in the Wide Field Cameras, in about 3 years of operations, is discussed: with present data no implications on the X-to-gamma-ray spectra of short vs long GRBs may be inferred. Finally, the status of searching procedures at SOC is reviewed.

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