GCN Circular 43315

R. Caputo (GSFC), J. J. DeLaunay (PSU), K. L. Page (U Leicester) and
M. H. Siegel (PSU) report on behalf of the Neil Gehrels Swift
Observatory Team:

At 05:37:02 UT, the Swift Burst Alert Telescope (BAT) triggered and
located GRB 260104A (trigger=1430212).  Swift slewed immediately to the burst.
The BAT on-board calculated location is 
RA, Dec 337.415, -21.280 which is 
   RA(J2000) = 22h 29m 40s
   Dec(J2000) = -21d 16' 48"
with an uncertainty of 3 arcmin (radius, 90% containment, including 
systematic uncertainty).  The BAT light curve showed a complex
structure with a duration of about 20 sec.  The peak count rate
was ~2400 counts/sec (15-350 keV), at ~0 sec after the trigger.

The XRT began observing the field at 05:38:28.9 UT, 86.1 seconds after
the BAT trigger. Using promptly downlinked data we find an uncatalogued
X-ray source with an enhanced position: RA, Dec 337.39898, -21.29547
which is equivalent to:
   RA(J2000)  = 22h 29m 35.76s
   Dec(J2000) = -21d 17' 43.7"
with an uncertainty of 2.2 arcseconds (radius, 90% containment). This
location is 77 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 gives a column density in excess of the Galactic value (3.40 x
10^20 cm^-2, Willingale et al. 2013), with an excess column of 2.8
(+2.48/-2.16) x 10^21 cm^-2 (90% confidence).

UVOT took a finding chart exposure of 150 seconds with the White filter
starting 90 seconds after the BAT trigger. No credible afterglow candidate has
been found in the initial data products. The 2.7'x2.7' sub-image covers none of
the XRT error circle. The 8'x8' region for the list of sources generated
on-board covers 100% of the XRT error circle. The list of sources is typically
complete to about 18 mag. No correction has been made for the expected
extinction corresponding to E(B-V) of 0.033.

Burst Advocate for this burst is R. Caputo (regina.caputo 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/)