GCN Circular 22708
Subject
GRB 180510B: Swift-XRT refined Analysis
Date
2018-05-11T21:22:02Z (6 years ago)
From
Phil Evans at U of Leicester <pae9@leicester.ac.uk>
B. Sbarufatti (INAF-OAB/PSU), D.N. Burrows (PSU), P.A. Evans (U.
Leicester), S.L. Gibson (U. Leicester), Z. Liu (NAOC / U. Leicester),
A. Melandri (INAF-OAB), P. D'Avanzo (INAF-OAB), V. D'Elia (ASDC) and A.
Tohuvavohu report on behalf of the Swift-XRT team:
We have analysed 2.6 ks of XRT data for GRB 180510B (Tohuvavohu et al.
GCN Circ. 22696), from 3.0 ks to 10.2 ks after the BAT trigger. The
data are entirely in Photon Counting (PC) mode. The enhanced XRT
position for this burst was given by Beardmore et al. (GCN Circ.
22698