GCN Circular 24934

T. N. Ukwatta (LANL), A. P. Beardmore (U Leicester),
N. J. Klingler (PSU), H. A. Krimm (NSF), F. E. Marshall (NASA/GSFC),
K. L. Page (U Leicester) and A. Tohuvavohu (PSU) report on behalf of
the Neil Gehrels Swift Observatory Team:

At 09:45:20 UT, the Swift Burst Alert Telescope (BAT) triggered and
located GRB 190701A (trigger=912310).  Swift slewed immediately to the burst. 
The BAT on-board calculated location is 
RA, Dec 28.063, +58.906 which is 
   RA(J2000) = 01h 52m 15s
   Dec(J2000) = +58d 54' 23"
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 100 sec.  The peak count rate
was ~800 counts/sec (15-350 keV), at ~37 sec after the trigger. 

The XRT began observing the field at 09:47:41.9 UT, 141.1 seconds after
the BAT trigger. Using promptly downlinked data we find a fading,
uncatalogued X-ray source located at RA, Dec 28.08019, 58.91005 which
is equivalent to:
   RA(J2000)  = 01h 52m 19.25s
   Dec(J2000) = +58d 54' 36.2"
with an uncertainty of 3.7 arcseconds (radius, 90% containment). This
location is 35 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. 

A power-law fit to a spectrum formed from promptly downlinked event
data gives a column density consistent with the Galactic value of 6.36
x 10^21 cm^-2 (Willingale et al. 2013). 

UVOT took a finding chart exposure of 150 seconds with the White filter
starting 144 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 100% of
the XRT error circle. The typical 3-sigma upper limit has been about 19.6 mag. 
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 large, but uncertain, extinction expected. 

Burst Advocate for this burst is T. N. Ukwatta (tilan.ukwatta AT gmail.com). 
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/)