TITLE:   GCN CIRCULAR
NUMBER:  26045
SUBJECT: GRB 191019A: Swift-XRT refined Analysis
DATE:    19/10/20 15:32:57 GMT
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),
J. D. Gropp (PSU), A. Tohuvavohu (U. Toronto), J.A. Kennea (PSU), P.A.
Evans (U. Leicester), J.P. Osborne (U. Leicester), K.L. Page (U.
Leicester) and K.K. Simpson report on behalf of the Swift-XRT team:

We have analysed 3.9 ks of XRT data for GRB 191019A (Simpson et al. GCN
Circ. 26031), from 3.3 ks to 17.2 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. 26043). The
results of the XRT-team automatic analysis are available at
http://www.swift.ac.uk/xrt_products/00930285.

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