GCN Circular 5757
Subject
GRB061025: Swift/UVOT observations
Date
2006-10-26T14:09:09Z (18 years ago)
From
Shashi Pandey at MSSL <sbp2@mssl.ucl.ac.uk>
S. B. Pandey (UCL-MSSL) & M. Stamatikos (NASA-GSFC), on behalf of the
Swift UVOT team.
The Swift/UVOT began observing the field of long duration GRB 061025
around ~1.5 hours after the INTEGRAL trigger at 18:35:50 UT on October 25
(Mereghetti et al., GCN 5751). We do not find any source in the co-added
UVOT observations within the XRT position reported by Mineo et al. (GCN
5753).
Following are the 3-sigma magnitude upper limits from the observations.
Filter T_start T_stop Exposure (s) mag, 3 sigma UL
V 11282 39711 875 20.5
B 11112 38644 1082 21.4
U 9302 38427 1267 21.2
UVW1 8875 38210 2581 21.4
UVM2 11318 40316 2468 22.0
UVW2 11150 39494 3524 22.4
T_start and T_stop are calculated from the time of the burst. The upper
limits are not corrected for Galactic extinction E(B-V) = 0.047 mag along
the line of sight to the burst.
[GCN OPS NOTE(26oct06): Per author's request, the typo 'Minoe' was changed
to 'Mineo'.]