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GCN Circular 21367

Subject
GRB 170728A: Swift detection of a burst
Date
2017-07-28T07:04:25Z (7 years ago)
From
David Palmer at LANL <palmer@lanl.gov>
J. K. Cannizzo (NASA/UMBC), A. P. Beardmore (U Leicester),
K. L. Page (U Leicester), D. M. Palmer (LANL) and M. H. Siegel (PSU)
report on behalf of the Swift Team:

At 06:53:28 UT, the Swift Burst Alert Telescope (BAT) triggered and
located GRB 170728A (trigger=765008).  Swift slewed immediately to the burst. 
The BAT on-board calculated location is 
RA, Dec 58.898, +12.153 which is 
   RA(J2000) = 03h 55m 35s
   Dec(J2000) = +12d 09' 11"
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 3 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 06:54:39.4 UT, 70.6 seconds after
the BAT trigger. Using promptly downlinked data we find a fading,
uncatalogued X-ray source located at RA, Dec 58.88846, 12.18313 which
is equivalent to:
   RA(J2000)  = 03h 55m 33.23s
   Dec(J2000) = +12d 10' 59.3"
with an uncertainty of 3.7 arcseconds (radius, 90% containment). This
location is 113 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 2.27
x 10^21 cm^-2 (Willingale et al. 2013). 

UVOT took a finding chart exposure of 150 seconds with the White filter
starting 73 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 0.24. 

Burst Advocate for this burst is J. K. Cannizzo (cannizzo AT milkyway.gsfc.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/too.html.)
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