[vsnet-grb-info 10946] GRB 110918A: INT optical detection of Swift candidate afterglow
GCN Circulars
gcncirc at capella2.gsfc.nasa.gov
Tue Sep 20 22:53:41 JST 2011
TITLE: GCN CIRCULAR
NUMBER: 12365
SUBJECT: GRB 110918A: INT optical detection of Swift candidate afterglow
DATE: 11/09/20 13:53:36 GMT
FROM: Nial Tanvir at U.Leicester <nrt3 at star.le.ac.uk>
N.R. Tanvir, K. Wiersema (U. Leicester), A.J. Levan, S. Greiss,Â
B. Gaensicke (U. Warwick) report on behalf of a larger collaboration:Â
We observed the field of IPN burst GRB 110918A (Hurley et al. GCN
12357) with the Isaac Newton Telescope on La Palma, using the Wide
Field Camera starting at 20-Sep-2011 02:22 UT, roughly 29 hours
post-burst. Â Close to the location of the X-ray source reported by Mangano
et al. (GCN 12364) we detect a bright optical point-source which is not
visible in the DSS2 images of the region.
Very provisional calibration gives a magnitude R~19.0-19.5 (well above the
DSS2 limit) and a position:Â
RA(2000)=02 10 09.39Â
dec(2000)=-27 06 19.6Â
accurate to ~0.5" in each coordinate. Â We cannot yet assess variability.
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