GCN Circular 3170
Subject
GRB 050402A: IR Analysis
Date
2005-04-02T10:01:42Z (20 years ago)
From
Josh Bloom at Harvard/CFA <jbloom@cfa.harvard.edu>
H. W. Chen (MIT), J. S. Bloom (UCB), J. X. Prochaska (UCSC) & C. Blake
reports on behalf of a larger collaboration:
"Upon more detailed analysis following GCN #3168 we cannot confirm our
earlier claim of significant variability as suggested. We thus find no
variable or new source to the 2MASS detection levels in J, H, and K
starting ~18 min after the GRB."
This message may be cited.