GCN Circular 8012
Subject
GRB 080723A: Swift/UVOT Upper Limits
Date
2008-07-24T14:32:06Z (16 years ago)
From
Stephen Holland at USRA/NASA/GSFC/SSC <sholland@milkyway.gsfc.nasa.gov>
S. T. Holland (CRESST/GSFC/USRA) and M. Stamatikos (NASA/ORAU) report
on the behalf of the Swift UVOT team:
The Swift/UVOT observed the field of GRB 080723A starting 68 s
after the BAT trigger (Stamatikos et al. 2008, GCN Circ. 8000). We do
not find any source, in any of the UVOT observations, at the
UVOT-enhanced XRT position of the afterglow (Beardmore 2008, GCN
Circ. 8001). The 3-sigma upper limits for detecting a source at this
location in the co-added images are:
Filter T_start T_stop Exp(s) Mag (3-sigma upper limit)
-----------------------------------------------------------------
v 194 6260 1040 >20.1
b 674 7080 451 >20.6
u 649 6874 471 >20.4
uvw1 625 6670 469 >20.3
uvm2 600 6465 467 >20.1
uvw2 704 7468 430 >20.4
white 88 7284 628 >21.4
-----------------------------------------------------------------
The quoted upper limits have not been corrected for the expected
Galactic extinction along the line of sight corresponding to a
reddening of E_{B-V} = 1.3 mag. All photometry is on the UVOT flight
system described in Poole et al. (2008, MNRAS, 383, 627).