[vsnet-grb-info 15838] GRB 141130: Swift/UVOT Detection
GCN Circulars
gcncirc at capella2.gsfc.nasa.gov
Mon Dec 1 22:27:00 JST 2014
TITLE: GCN CIRCULAR
NUMBER: 17126
SUBJECT: GRB 141130: Swift/UVOT Detection
DATE: 14/12/01 13:26:52 GMT
FROM: Paul Kuin at MSSL <npkuin at gmail.com>
S. R. Oates (IAA-CSIC/UCL-MSSL) and A. Vargas (PSU) report
on behalf of the Swift/UVOT team:
The Swift/UVOT began settled observations of the field of
GRB 141130 95 s after the BAT trigger (Vargas et al., GCN
Circ. 17120). A source consistent with the XRT position
(Goad et al. GCN Circ. 17123) is detected in the initial UVOT
exposures.
The preliminary UVOT position is:
RA (J2000) = 14:51:17.23 = 222.82181 (deg.)
Dec (J2000) = +47:19:07.3 = 47.31870 (deg.)
with an estimated uncertainty of 0.45 arc sec. (radius, 90% confidence).
Preliminary detections and 3-sigma upper limits using the UVOT photometric
system
(Breeveld et al. 2011, AIP Conf. Proc. 1358, 373) for the early exposures
are:
Filter T_start(s) T_stop(s) Exp(s) Mag
white 95 244 147 18.71 +/- 0.06
v 636 655 19 >17.8
b 562 753 39 >20.1
u 306 556 246 18.85 +/- 0.13
w1 684 704 19 >18.7
w2 611 798 34 >19.0
The magnitudes in the table are not corrected for the Galactic extinction
due to the reddening of E(B-V) = 0.02 in the direction of the burst
(Schlegel et al. 1998).
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