GCN Circular 28707
Subject
GRB 201020A: Swift-XRT refined Analysis
Date
2020-10-20T22:29:25Z (4 years ago)
From
Phil Evans at U of Leicester <pae9@leicester.ac.uk>
A. Tohuvavohu (U. Toronto), B. Sbarufatti (PSU), D.N. Burrows (PSU),
P.A. Evans (U. Leicester), J.P. Osborne (U. Leicester), K.L. Page (U.
Leicester), A. Melandri (INAF-OAB), T. Sbarrato (INAF-OAB), P. D'Avanzo
(INAF-OAB) and E. Ambrosi report on behalf of the Swift-XRT team:
We have analysed 6.9 ks of XRT data for GRB 201020A (Ambrosi et al. GCN
Circ. 28696), from 148 s to 35.3 ks after the BAT trigger. The data
are entirely in Photon Counting (PC) mode. The enhanced XRT position
for this burst was given by Osborne et al. (GCN Circ. 28698