Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..312..201b&link_type=abstract
Third Rome Workshop on Gamma-Ray Bursts in the Afterglow Era ASP Conference Series, Volume 312, Proceedings of the conference he
Astronomy and Astrophysics
Astronomy
Scientific paper
We failed to detect a counterpart source to the short/hard GRB 020531, which was discovered by the HETE satellite. We present observations in the X-rays made with Chandra in 2 epochs. We also summarize observations made in the optical with the Subaru telescope, with Magellan, and with 2 orbits of Hubble STIS. The X-ray afterglow flux must have been fainter than 2× 10-15 erg cm-2 s-1 5.27 days after the GRB. The source must have faded faster than t-2.1 in the optical.
Burles Scott
Butler Nat
Dullighan Allyn
Ebeling Harald
Ford Patrick
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