[vsnet-grb-info 14702] GRB 140320A: Confirmation of a fading X-ray afterglow

GCN Circulars gcncirc at capella2.gsfc.nasa.gov
Fri Mar 21 19:08:19 JST 2014


TITLE:   GCN CIRCULAR
NUMBER:  16016
SUBJECT: GRB 140320A: Confirmation of a fading X-ray afterglow
DATE:    14/03/21 10:08:11 GMT
FROM:    Kim Page at U.of Leicester  <klp5 at leicester.ac.uk>

K.L. Page, C. Pagani, P.A. Evans (U. Leicester) & J.K. Cannizzo
(NASA/UMBC) report on behalf of the Swift-XRT team:

We have now analysed 9.8 ks of Swift-XRT data for GRB 140320A, between 93
s and 33.5 ks after the trigger. The X-ray source given by Page, Pagani &
Cannizzo in GCN Circ. 16010 has now faded, with a 3-sigma upper limit on
the count rate centred at 27 ks after the trigger of 1.2 x 10^-3 count
s^-1. We therefore confirm this source as the X-ray afterglow of GRB
140320A.

This circular is an official product of the Swift-XRT team.


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