[vsnet-grb-info 17912] GRB 160422A: XRT Afterglow Confirmation
GCN Circulars
gcncirc at capella2.gsfc.nasa.gov
Thu Apr 28 22:39:11 JST 2016
TITLE: GCN CIRCULAR
NUMBER: 19359
SUBJECT: GRB 160422A: XRT Afterglow Confirmation
DATE: 16/04/28 13:38:27 GMT
FROM: Alessandro Maselli at INAF/IASF Palermo <maselli at ifc.inaf.it>
A. Maselli (INAF-IASFPA), D. Malesani (DARK/NBI), K.L. Page 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
Fermi-detected burst GRB 160422A (Yassine et al., GCN Circ. 19329; Burns
et al., GCN Circ. 19331), extending from T0+400 ks to T0+470 ks after
the Fermi/GBM trigger.
At the position of the candidate afterglow reported by Maselli et al.
(GCN Circ. 19334) no source is detected in the new observation, with a
three sigma upper limit of 2.6e-3 ct/s. This confirms that it was the
X-ray afterglow of GRB 160422A.
The results of the full analysis of the XRT observations are available
at http://www.swift.ac.uk/xrt_products/00020605
This circular is an official product of the Swift-XRT team.
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