GCN Circular 40224

S. B. Cenko (GSFC), V. D'Elia (SSDC & INAF-OAR), J. J. DeLaunay (PSU),
R. Gupta (NASA GSFC), A. Melandri (INAF-OAR), K. L. Page (U Leicester)
and M. H. Siegel (PSU) report on behalf of the Neil Gehrels Swift
Observatory Team:

At 06:52:28.51 UT, the Swift Burst Alert Telescope (BAT) triggered and
located GRB 250424A (trigger=1306404). Swift slewed immediately to the burst.
The BAT on-board calculated location is RA, Dec 217.513, -35.022 which is 
   RA(J2000) = 14h 30m 03s
   Dec(J2000) = -35d 01' 19"
with an uncertainty of 3 arcmin (radius, 90% containment, including 
systematic uncertainty).  The BAT light curve showed a single peak
structure with a duration of about 30 sec.  The peak count rate
was ~25000 counts/sec (15-350 keV), at ~15 sec before the trigger.

The XRT began observing the field at 06:56:39.3 UT, 250.9 seconds after
the BAT trigger. Using promptly downlinked data we find an uncatalogued
X-ray source with an enhanced position: RA, Dec 217.50010, -35.02493
which is equivalent to:
   RA(J2000)  = 14h 30m 00.03s
   Dec(J2000) = -35d 01' 29.7"
with an uncertainty of 1.9 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. 

A power-law fit to a spectrum formed from promptly downlinked event
data does not constrain the column density.

UVOT took a finding chart exposure of 150 seconds with the White filter
starting 254 seconds after the BAT trigger. There is a candidate afterglow in
the rapidly available 2.7'x2.7' sub-image at
  RA(J2000)  =	14:29:60.00 = 217.49998
  DEC(J2000) = -35:01:30.6  = -35.02518
with a 90%-confidence error radius of about 0.63 arc sec. This position is 1
arc sec. from the center of the XRT error circle. The estimated magnitude is
18.80 with a 1-sigma error of about  0.15. No correction has been made for the
expected extinction corresponding to E(B-V) of 0.064.

Burst Advocate for this burst is S. B. Cenko (brad.cenko AT nasa.gov).
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/)