[vsnet-grb-info 27708] GRB 210411C: Swift/UVOT Detection
GCN Circulars
gcncirc at capella2.gsfc.nasa.gov
Tue Apr 13 07:06:14 JST 2021
TITLE: GCN CIRCULAR
NUMBER: 29811
SUBJECT: GRB 210411C: Swift/UVOT Detection
DATE: 21/04/12 22:05:23 GMT
FROM: Paul Kuin at MSSL <npkuin at gmail.com>
N. P. M. Kuin (UCL-MSSL) and Sbarrato (INAF-OAB)
report on behalf of the Swift/UVOT team:
The Swift/UVOT began settled observations of the field of GRB 210411C
66 s after the BAT trigger (Sbarrato et al., GCN Circ. 29794).
A source consistent with the XRT position (Goad et al. GCN Circ. 29800)
is detected in the initial UVOT exposures. Further detections were
reported by Strausbaugh et al. (GCN Circ 29802)
The preliminary UVOT position is:
RA (J2000) = 19:46:26.81 = 296.61170 (deg.)
Dec (J2000) = -39:23:52.2 = -39.39784 (deg.)
with an estimated uncertainty of 0.43 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 66 216 147 17.16 +/- 0.03
v 609 801 39 17.43 +/- 0.18
b 535 555 20 17.82 +/- 0.17
u 279 528 246 17.82 +/- 0.07
w1 658 1280 78 >19.7
m2 633 5836 83 >19.6
w2 584 5600 255 >20.1
The magnitudes in the table are not corrected for the Galactic extinction
due to the reddening of E(B-V) = 0.081 in the direction of the burst
(Schlegel et al. 1998).
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