TITLE: GCN CIRCULAR NUMBER: 18875 SUBJECT: GRB 160117B: Swift detection of a burst with optical counterpart DATE: 16/01/17 14:14:09 GMT FROM: David Palmer at LANL E. Sonbas (Adiyaman Univ.), J. A. Kennea (PSU), F. E. Marshall (NASA/GSFC), K. L. Page (U Leicester) and D. M. Palmer (LANL) report on behalf of the Swift Team: At 13:59:27 UT, the Swift Burst Alert Telescope (BAT) triggered and located GRB 160117B (trigger=670800). Swift slewed immediately to the burst. The BAT on-board calculated location is RA, Dec 132.190, -16.340 which is RA(J2000) = 08h 48m 46s Dec(J2000) = -16d 20' 23" 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 60 sec. The peak count rate was ~1300 counts/sec (15-350 keV), at ~7 sec after the trigger. The XRT began observing the field at 14:00:22.5 UT, 55.0 seconds after the BAT trigger. Using promptly downlinked data we find a bright, uncatalogued X-ray source with an enhanced position: RA, Dec 132.1953, -16.3668 which is equivalent to: RA(J2000) = 08h 48m 46.88s Dec(J2000) = -16d 22' 00.4" with an uncertainty of 2.2 arcseconds (radius, 90% containment). This location is 98 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. 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 consistent with the Galactic value of 5.71 x 10^20 cm^-2 (Willingale et al. 2013). 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 63 seconds after the BAT trigger. There is a candidate afterglow in the rapidly available 2.7'x2.7' sub-image at RA(J2000) = 08:48:46.76 = 132.19484 DEC(J2000) = -16:21:59.9 = -16.36664 with a 90%-confidence error radius of about 0.62 arc sec. This position is 3.2 arc sec. from the center of the XRT error circle. The estimated magnitude is 18.32 with a 1-sigma error of about 0.14. No correction has been made for the expected extinction corresponding to E(B-V) of 0.07. Burst Advocate for this burst is E. Sonbas (edasonbas AT yahoo.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/too.html.) [GCN OPS NOTE(17jan16): Per N.Cucchiara's request, the Trigger number in the first paragraph was changed from 670793 to 670800.]