GCN Circular 21154
Subject
GRB 170526A: Swift-XRT refined Analysis
Date
2017-05-27T04:29:59Z (7 years ago)
From
Phil Evans at U of Leicester <pae9@leicester.ac.uk>
A. D'Ai (INAF-IASFPA), A. Melandri (INAF-OAB), P. D'Avanzo (INAF-OAB),
A. Cholden-Brown (PSU), S. J. LaPorte (PSU), J.A. Kennea (PSU), S.L.
Gibson (U. Leicester), J.P. Osborne (U. Leicester), K.L. Page (U.
Leicester) and B. Sbarufatti report on behalf of the Swift-XRT team:
We have analysed 6.5 ks of XRT data for GRB 170526A (Sbarufatti et al.
GCN Circ. 21149), from 132 s to 46.4 ks after the BAT trigger. The
data are entirely in Photon Counting (PC) mode. The enhanced XRT
position for this burst was given by Goad et al. (GCN Circ. 21151