Recent results from the BATSE/OSSE rapid burst response

Details Recent results from the BATSE/OSSE rapid burst response Recent results from the BATSE/OSSE rapid burst response

Aug 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aipc..384..846m&link_type=abstract

Gamma-ray bursts: 3rd Huntsville symposium. AIP Conference Proceedings, Volume 384, pp. 846-850 (1996).

Computer Science

X- And Gamma-Ray Telescopes And Instrumentation, Gamma-Ray Sources, Gamma-Ray Bursts, Gamma-Ray

Scientific paper

The OSSE and BATSE instrument teams on GRO have implemented a system which allows OSSE to slew promptly (within 2 min) to observe burst positions calculated on-board by BATSE. This enables OSSE to make deep searches of burst error boxes for recurrent burst emission and fading or persistent counterparts in hard X-rays and gamma rays. Detections of, or limits on, such emission may severely constrain burst models. We describe the BATSE and OSSE components of the system and compare the on-board positions to the final BATSE positions calculated on the ground. We summarize the bursts which OSSE has observed and present post-burst flux limits for GRB950809 on a number of time scales.

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