GCN Circular 8514
Subject
GRB 081025: Swift-XRT further analysis
Date
2008-11-10T17:05:33Z (15 years ago)
From
Jirong Mao at INAF-OAB <jirong.mao@brera.inaf.it>
J. Mao (INAF-OAB) on behalf of the Swift-XRT team reports:
Swift-XRT re-observed the Swift-BATSS GRB 081025 (Copete et al., GCN
8409) from 12.9 days after the burst with an exposure time of 6.9 ks.
We did not detect any source in the field. The 3-sigma upper limit is
1.7e-3 count/s. We compared this result with the previous observation
(Mao et al., GCN 8411). Thus we confirm that XRT observed the fading
afterglow of GRB 081025.
This circular is an official product of the Swift-XRT team.