A Search for Prompt Radio Emission from GRBs

Details A Search for Prompt Radio Emission from GRBs A Search for Prompt Radio Emission from GRBs

Sep 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.231..281g&link_type=abstract

Astrophysics and Space Science, Volume 231, Issue 1-2, pp. 281-284

Astronomy and Astrophysics

Astrophysics

4

Grb Radio Counterparts, Bacodine

Scientific paper

The Cambridge Low Frequency Synthesis Telescope (CLFST) is being used to search for prompt radio emission from GRBs at 151 MHz. For this search a special observing mode has recently been developed; the antennas of the CLFST are split into seven groups which are spaced about 30° apart. When triggered by the real-time signals from the BACODINE system the antennas are slewed to the GRB position, with data being sampled at 1.5 or 3-s intervals. The antennas slew at about 10° per minute, so that an appreciable fraction of the sky can be accessed on timescales of a few minutes - any prompt radio emission from a GRB might be delayed by this timescale due to propagation effects.

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