[vsnet-grb-info 18483] GRB 160917A: Swift/UVOT Detection
GCN Circulars
gcncirc at capella2.gsfc.nasa.gov
Sun Sep 18 08:55:21 JST 2016
TITLE: GCN CIRCULAR
NUMBER: 19931
SUBJECT: GRB 160917A: Swift/UVOT Detection
DATE: 16/09/17 23:54:38 GMT
FROM: Paul Kuin at MSSL <npkuin at gmail.com>
N. P. M. Kuin (UCL-MSSL) and J. L. Racusin (NASA/GSFC)
report on behalf of the Swift/UVOT team:
The Swift/UVOT began settled observations of the field of GRB 160917A
100 s after the BAT trigger (Racusin et al., GCN Circ. 19926). The
refined XRT position (Evans et al. GCN Circ. 19927) is close to a
bright star. However, a faint GRB candidate has been found at an
offset of 6.5 arcsec to the south east from the bright star in the
u exposures.
The UVOT candidate position is: RA, Dec = 295.66687, 46.40368 (J2000)
which is :
RA = 19:42:40.049
Dec = +46:24:13.25
with an estimated accuracy of 1.5 arcsec.
Preliminary detections 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 100 224 123 >21.01
b 4222 4422 100 >20.64
u 4017 5545 146 20.47 +- 0.36
v 3402 5038 200 >19.77
uvw1 3812 5448 200 >20.16
uvm2 3606 5242 100 >19.97
uvw2 4633 4833 200 >19.70
The magnitudes in the table are not corrected for the Galactic extinction
due to the reddening of E(B-V) = 0.16 in the direction of the burst
(Schlegel et al. 1998).
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