GCN Circular 4516
Subject
GRB 060115: Swift/UVOT upper limits
Date
2006-01-16T00:13:52Z (18 years ago)
From
Patricia Schady at MSSL/Swift <ps@mssl.ucl.ac.uk>
P. Schady (UCL-MSSL/PSU), A. Cucchiara (PSU), M. De Pasquale (UCL-MSSL), F.
Marshall (GSFC), N. Gehrels (GSFC) on behalf of the Swift/UVOT team
The Swift/UVOT began observing the field of GRB 060115 at 13:09:59 on
2006-01-15 whilst settling on the target, 119 s after the BAT trigger
(Tagliagerri et al., GCN 4509). No new source is detected either at the XRT
position (Perri et al., GCN 4514) or at the position of the candidate afterglow
reported by Yanagisawa et al. (GCN 4510) in coadded images with any of the
filters. The following 3-sigma magnitude upper limits are not corrected for
Galactic extinction; E(B-V) = 0.133.
Filter T_range(s) Exp(s) 3sigUL(mag)
V 104-1585 488.1 19.5
B 326-1042 199.7 20.4
U 651-1657 99.0 19.3
W1 627-1788 105.9 19.4
M2 603-1777 118.8 19.5
W2 556-1730 99.0 19.7
White 531-1705 99.0 19.8
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