GCN Circular 17171
Subject
GRB 141212A: Swift-XRT refined Analysis
Date
2014-12-13T00:27:05Z (9 years ago)
From
Phil Evans at U of Leicester <pae9@leicester.ac.uk>
P.A. Evans (U. Leicester), B.P. Gompertz (U. Leicester), V. D'Elia
(ASDC), M. de Pasquale (INAF-IASFPA), A. Maselli (INAF-IASFPA), V.
Mangano (PSU), M.C. Stroh (PSU), D.N. Burrows (PSU), J.P. Osborne (U.
Leicester) and T.N. Ukwatta report on behalf of the Swift-XRT team:
We have analysed 7.9 ks of XRT data for GRB 141212A (Ukwatta et al.
GCN Circ. 17158), from 77 s to 28.9 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. 17164