[vsnet-grb-info 18617] GRB 161015A: Swift/UVOT observations
GCN Circulars
gcncirc at capella2.gsfc.nasa.gov
Tue Oct 18 04:48:55 JST 2016
TITLE: GCN CIRCULAR
NUMBER: 20065
SUBJECT: GRB 161015A: Swift/UVOT observations
DATE: 16/10/17 19:48:19 GMT
FROM: Massimiliano de Pasquale at IASF-Palermo <m.depasquale at ucl.ac.uk>
M. De Pasquale (MSSL-UCL) and J. Cannizzo (NASA/UMBC) report on
behalf of the Swift/UVOT team:
The Swift/UVOT report started to observe the field of the putative X-ray
afterglow of GRB 161015A, the Fermi/LAT burst (Ohno et al. GCN
Circ. 20054, D'Avanzo et al. GCN Circ. 20057), 38 ks after the
LAT trigger.
No optical counterpart to this source is found. The 3 sigma upper limit
is given in the table below.
T_start (s) T_end (s) Exposure Time (s) filter 3s UL
37991 45608 1210 u >20.35
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).
--
Dr. Massimiliano De Pasquale
Research associate - Swift UVOT scientist
Mullard Space Science Laboratory, University College London
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