[vsnet-grb-info 19936] GRB 171010B: Swift-XRT afterglow detection
GCN Circulars
gcncirc at capella2.gsfc.nasa.gov
Wed Oct 18 22:07:39 JST 2017
TITLE: GCN CIRCULAR
NUMBER: 22023
SUBJECT: GRB 171010B: Swift-XRT afterglow detection
DATE: 17/10/18 13:07:12 GMT
FROM: Kim Page at U.of Leicester <kpa at star.le.ac.uk>
A. Melandri (INAF-OAB), D.N. Burrows (PSU), A. Tohuvavohu (PSU), S. J.
LaPorte (PSU), J.P. Osborne (U. Leicester), K.L. Page (U. Leicester),
A.P. Beardmore (U. Leicester), P. D'Avanzo (INAF-OAB), V. D'Elia (ASDC)
and P.A. Evans (U. Leicester) report on behalf of the Swift-XRT team:
Swift-XRT has conducted further observations of the field of the
Swift/BAT-detected burst GRB 171010B (Palmer et al. GCN Circ. 21995).
The observations now extend from T0+91.1 ks to T0+614.5 ks.
Of the sources reported by Sbarufatti et al. (GCN Circ. 22009), "Source
2" is believed to be the afterglow. The position of this source is
RA, Dec=34.1342, -54.3915 which is equivalent to:
RA (J2000): 02:16:32.20
Dec(J2000): -54:23:29.2
with an uncertainty of 5.6 arcsec (radius, 90% confidence). This
position is 71 arcsec from the Swift/BAT position.
The light curve can be modelled with a power-law decay with a decay
index of alpha=0.8 (+0.6, -0.4).
The results of the XRT-team automatic analysis are available at
http://www.swift.ac.uk/xrt_products/00020780.
The results of the full analysis of the XRT observations are available
at http://www.swift.ac.uk/ToO_GRBs/00020780.
This circular is an official product of the Swift-XRT team.
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