GCN Circular 17452
Subject
GRB 150212A: Swift-XRT afterglow detection
Date
2015-02-12T11:58:35Z (10 years ago)
From
Phil Evans at U of Leicester <pae9@leicester.ac.uk>
P.A. Evans (U. Leicester) reports on behalf of the Swift-XRT team:
The XRT began observing the field at 11:03:12.7 UT, 353.7 seconds after
the BAT trigger. Due to passage of the spacecraft through the South
Atlantic Anomaly, no XRT data were collected until T0+1805 s.
Using promptly downlinked data we find an uncatalogued
X-ray source located at RA, Dec 285.48092, 47.36602 which is equivalent
to:
RA(J2000) = 19h 01m 55.42s
Dec(J2000) = +47d 21' 57.7"
with an uncertainty of 4.3 arcseconds (radius, 90% containment). This
location is 176 arcseconds from the BAT onboard position, within the
BAT error circle. This position may be improved as more data are
received; the latest position is available at
http://www.swift.ac.uk/sper. We cannot determine whether the source is
fading at the present time.
A power-law fit to a spectrum formed from promptly downlinked event
data gives a column density consistent with the Galactic value of 5.20
x 10^20 cm^-2 (Willingale et al. 2013).
This circular is an official product of the Swift-XRT team.