[vsnet-grb-info 15330] GRB 140709B: Swift/UVOT Upper Limits
GCN Circulars
gcncirc at capella2.gsfc.nasa.gov
Wed Jul 23 20:23:35 JST 2014
TITLE: GCN CIRCULAR
NUMBER: 16622
SUBJECT: GRB 140709B: Swift/UVOT Upper Limits
DATE: 14/07/23 11:23:28 GMT
FROM: Craig Swenson at PSU/Swift <cswenson at astro.psu.edu>
C. A. Swenson (PSU) reports on behalf of the Swift/UVOT team:
The Swift/UVOT began settled observations of the field of GRB 140709B
97 s after the BAT trigger (Swenson et al., GCN Circ. 16551).
No optical afterglow consistent with the XRT position
(Goad et al. GCN Circ. 16556)
is detected in the initial UVOT exposures.
Preliminary 3-sigma upper limits using the UVOT photometric system
(Breeveld et al. 2011, AIP Conf. Proc. 1358, 373) for the first
finding chart (FC) exposure and subsequent exposures are:
Filter T_start(s) T_stop(s) Exp(s) Mag
white_FC 4835 4985 147 >20.8
u_FC 97 346 246 >20.6
white 4835 6626 541 >21.7
v 633 7037 491 >20.5
b 352 6422 534 >20.9
u 97 6216 668 >21.2
w1 683 11259 922 >20.8
m2 1087 7230 440 >21.2
w2 758 6832 471 >20.6
The magnitudes in the table are not corrected for the Galactic extinction
due to the reddening of E(B-V) = 0.04 in the direction of the burst
(Schlegel et al. 1998).
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