[vsnet-grb-info 12858] Swift GRB130206A: late XRT observations.
GCN Circulars
gcncirc at capella2.gsfc.nasa.gov
Fri Feb 15 06:58:28 JST 2013
TITLE: GCN CIRCULAR
NUMBER: 14203
SUBJECT: Swift GRB130206A: late XRT observations.
DATE: 13/02/14 21:58:20 GMT
FROM: MSSL Swift/UVOT team at MSSL/Swift <msslba at googlemail.com>
M. De Pasquale (MSSL-UCL), A. Beardmore (Univ. Leicester) report, on behalf
of the Swift team:
The X-ray source described in GCN circ. 14188 (Beardmore et al. 2013) is not
detected anymore in XRT observations performed between 33 and 550 ks after
the trigger, for a total of 35.2 ks of integration time. The 3 sigma upper
limit is
0.00089 count/s, appreciably lower than the count rate observed in previous
observations.
Because of the fading behaviour of this source, we conclude it was likely
the
X-ray afterglow of GRB130206A.
We also note that successive analysis of late data has reduced the error
circle
radius of the source to 4.6'' (90% confidence level).
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