GCN Circular 4773
Subject
Swift UVOT observations of GRB060213
Date
2006-02-17T21:59:50Z (19 years ago)
From
Massimiliano de Pasquale at MSSL-UCL <mdp@mssl.ucl.ac.uk>
M. De Pasquale (MSSL-UCL), D. Morris (PSU) and P. Roming (PSU)
on the behalf of the Swift UVOT/team:
The Swift/UVOT began taking data on the field of GRB 060213
at 13:35:41 UT on 2006-02-15, 48.41 hours after the GRB
(Pal'shin et al. GCN 4762).
The UVOT field does not cover the whole IPN error box, but it
encompasses the field of the uncatalogued source detected
by the XRT (Morris et al. GCN 4770). No optical afterglow
candidate is detected in the summed images of each of the
UVOT filters down to the following 3-sigma magnitude
upper limits:
Filter T_range (sec) Exp(sec) 3 sigma u.l.
V 180203 - 187038 1020 20.1
B 185073 - 185982 849 21
UW1 175186 - 176088 878 20.4
UM2 174272 - 180401 1620 20.7
UW2 179290 - 186897 1705 21.1
The quoted values have not been corrected for Galactic extinction.