GCN Circular 38194

M. H. Siegel (PSU), J. J. DeLaunay (PSU), P. A. Evans (U Leicester),
R. Gupta (NASA GSFC), K. L. Page (U Leicester) and T. Sakamoto (AGU)
report on behalf of the Neil Gehrels Swift Observatory Team:

At 07:48:13 UT, the Swift Burst Alert Telescope (BAT) triggered and
located GRB 241113A (trigger=1267501).  Swift slewed immediately to the burst.
The BAT on-board calculated location is 
RA, Dec 16.576, -22.667 which is 
   RA(J2000) = 01h 06m 18s
   Dec(J2000) = -22d 40' 00"
with an uncertainty of 3 arcmin (radius, 90% containment, including 
systematic uncertainty).  The BAT light curve showed a single-peaked 
structure with a duration of about 4 sec.  The peak count rate
was ~2000 counts/sec (15-350 keV), at ~1 sec after the trigger.

The XRT began observing the field at 07:49:31.0 UT, 77.2 seconds after
the BAT trigger. Using promptly downlinked data we find an uncatalogued
X-ray source located at RA, Dec 16.56509, -22.67118 which is equivalent
to:
   RA(J2000)  = 01h 06m 15.62s
   Dec(J2000) = -22d 40' 16.2"
with an uncertainty of 4.6 arcseconds (radius, 90% containment). This
location is 39 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 https://www.swift.ac.uk/sper.  We
cannot determine whether the source is fading at the present time. No
spectrum from the promptly downlinked event data is yet available to
determine the column density.

UVOT took a finding chart exposure of 101 seconds with the White
filter starting 81 seconds after the BAT trigger. An uncatalogued
source is found inside the XRT error circle at
RA, Dec = 16.56518, -22.67177 which is equivalent to: 
   RA(J2000)  = 01h 06m 15.64s 
   Dec(J2000) = -22d 40' 18.4"  
with an estimated uncertainty of 0.7 arcseconds (radius, 90% containment). 
This source is 2.1" from the centre of the XRT error circle. The estimated
magnitude of the source is 15.8.

Burst Advocate for this burst is M. H. Siegel (siegel AT swift.psu.edu).
Please contact the BA by email if you require additional information
regarding Swift followup of this burst. In extremely urgent cases, after
trying the Burst Advocate, you can contact the Swift PI by phone (see
Swift TOO web site for information: http://www.swift.psu.edu/)