GCN Circular 7268
Subject
GRB080207: Swift/UVOT refined analysis
Date
2008-02-08T07:18:30Z (17 years ago)
From
Antonino Cucchiara at PSU <cucchiara@astro.psu.edu>
A. Cucchiara (PSU), J. Racusin (PSU)
report on behalf of the Swift-UVOT team:
The Swift/UVOT observed the field of GRB080207 (trigger #302728)
starting 55 sec days after the BAT detection (Racusin et
al. 2008, GCN Circ. 7264). We do not find any new source in any
of the UVOT coadded observations inside the XRT enhanced error
circle (Beardmore et al. 2008, GCN Circ. 7265).
The 3-sigma upper limits (in the UVOT photometric system,
Breeveld et al., GCN Circ. 6614) are listed.
Filter Tstart Tstop Exp Upper limit
(s) (s) (s)
white 55 11428 1167 22.40
v 4733 13063 1097 20.50
b 5553 16909 983 21.53
u 5347 6982 393 20.57
uvw1 5143 6777 393 20.75
uvm2 4937 6572 393 20.58
uvw2 5963 12334 1082 21.62
The values quoted above are not corrected for the expected Galactic
extinction corresponding to a reddening of E_{B-V} = 0.02 mag in the
direction of the burst (Schlegel et al. 1998).