GCN Circular 16451
Subject
GRB 140623A: Swift-XRT and UVOT observations
Event
Date
2014-06-24T15:21:15Z (11 years ago)
From
Valerio D'Elia at ASDC <delia@asdc.asi.it>
V. D'Elia (ASDC), F. E. Marshall (NASA/GSFC), L. Izzo (URoma/ICRA) &
D. Malesani (DARK/NBI) report on behalf of the Swift team:
Following the report of a potential optical afterglow iPTF14cyb
(Bhalerao et al., GCN Circ. 16442) to the Fermi/GBM-detected burst GRB
140623A (von Kienlin, GCN Circ. 16450), Swift began a follow-up
observation of the iPTF field.
We have analyzed all the 3.0 ks of XRT data for GRB 140623A, from
38.7 ks to 49.6 ks after the Fermi/GBM trigger. The data are entirely
in Photon Counting (PC) mode. An X-ray source is detected at a
position consistent with the candidate optical afterglow (Bhalerao et
al., GCN Circ. 16442