[vsnet-grb-info 17324] GRB151212A: Swift/UVOT observations
GCN Circulars
gcncirc at capella2.gsfc.nasa.gov
Mon Dec 14 03:52:18 JST 2015
TITLE: GCN CIRCULAR
NUMBER: 18689
SUBJECT: GRB151212A: Swift/UVOT observations
DATE: 15/12/13 18:49:23 GMT
FROM: Massimiliano de Pasquale at IASF-Palermo <m.depasquale at ucl.ac.uk>
M. De Pasquale (PSU) and P. Evans (U. Leicester)
report on behalf of the Swift/UVOT team:
The Swift/UVOT began observing the field of MAXI-detected GRB 151212A
(Nahakira et al., GCN Circ. 18685) 42183 s after the trigger.
No optical afterglow consistent with the XRT source given by Evans
et al. (GCN Circ 18687) is detected in the UVOT exposures.
Preliminary 3-sigma upper limits using the UVOT photometric system
(Breeveld et al. 2011, AIP Conf. Proc. 1358, 373) for the summed UVOT
exposures is:
Filter T_start(s) T_stop(s) Exp(s) Mag
u 42183 48392 2939 >21.4
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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