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GCN Circular 38927

Subject
GRB 250114A: Swift detection of a burst with an optical counterpart
Date
2025-01-14T07:50:30Z (8 days ago)
From
K.L. Page at U Leicester <klp5@leicester.ac.uk>
Via
email
N. J. Klingler (GSFC/UMBC/CRESSTII), R. Brivio (INAF-OAB),
J. J. DeLaunay (PSU), K. L. Page (U Leicester),
C. Salvaggio (INAF-OAB), T. Sbarrato (INAF-OAB), M. H. Siegel (PSU)
and A. Tohuvavohu (Caltech) report on behalf of the Neil Gehrels Swift
Observatory Team:

At 07:33:19 UT, the Swift Burst Alert Telescope (BAT) triggered and
located GRB 250114A (trigger=1281241).  Swift slewed immediately to the burst.
The BAT on-board calculated location is 
RA, Dec 166.590, -15.143 which is 
   RA(J2000) = 11h 06m 22s
   Dec(J2000) = -15d 08' 34"
with an uncertainty of 3 arcmin (radius, 90% containment, including 
systematic uncertainty).  The BAT light curve showed a multi-peaked
structure with a duration of about 50 sec.  The peak count rate
was ~875 counts/sec (15-350 keV), at ~3 sec after the trigger.

The XRT began observing the field at 07:35:27.7 UT, 128.3 seconds after
the BAT trigger. Using promptly downlinked data we find a bright,
uncatalogued X-ray source located at RA, Dec 166.57673, -15.11138 which
is equivalent to:
   RA(J2000)  = 11h 06m 18.42s
   Dec(J2000) = -15d 06' 41.0"
with an uncertainty of 3.6 arcseconds (radius, 90% containment). This
location is 122 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. 

A power-law fit to a spectrum formed from promptly downlinked event
data gives a column density in excess of the Galactic value (5.06 x
10^20 cm^-2, Willingale et al. 2013), with an excess column of 3.9
(+3.65/-3.04) x 10^21 cm^-2 (90% confidence). 

The initial flux in the 2.5 s image was 4.84e-09 erg cm^-2 s^-1 (0.2-10
keV).

UVOT took a finding chart exposure of 150 seconds with the White filter
starting 136 seconds after the BAT trigger. There is a candidate afterglow in
the rapidly available 2.7'x2.7' sub-image at
  RA(J2000)  =	11:06:18.43 = 166.57679
  DEC(J2000) = -15:06:41.7  = -15.11159
with a 90%-confidence error radius of about 0.74 arc sec. This position is 3.2
arc sec. from the center of the XRT error circle. The estimated magnitude is
20.35 with a 1-sigma error of about  0.20. No correction has been made for the
expected extinction corresponding to E(B-V) of 0.056.

Burst Advocate for this burst is N. J. Klingler (noelklin AT umbc.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/)


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