TITLE: GCN CIRCULAR NUMBER: 20575 SUBJECT: GRB 170202A: Swift detection of a burst with an optical afterglow DATE: 17/02/02 18:53:46 GMT FROM: Scott Barthelmy at NASA/GSFC J. L. Racusin (NASA/GSFC), S. D. Barthelmy (GSFC), S. B. Cenko (GSFC), A. Cholden-Brown (PSU), J. A. Kennea (PSU), H. A. Krimm (CRESST/NSF/USRA), F. E. Marshall (NASA/GSFC), K. L. Page (U Leicester), D. M. Palmer (LANL) and M. H. Siegel (PSU) report on behalf of the Swift Team: At 18:28:02 UT, the Swift Burst Alert Telescope (BAT) triggered and located GRB 170202A (trigger=736407). Swift slewed immediately to the burst. The BAT on-board calculated location is RA, Dec 152.529, +5.002 which is RA(J2000) = 10h 10m 07s Dec(J2000) = +05d 00' 06" with an uncertainty of 3 arcmin (radius, 90% containment, including systematic uncertainty). The BAT light curve shows 4 main peaks with a total duration of about 40 sec. The peak count rate was ~4800 counts/sec (15-350 keV), at ~16 sec after the trigger. The XRT began observing the field at 18:29:14.8 UT, 72.5 seconds after the BAT trigger. Using promptly downlinked data we find a bright, uncatalogued X-ray source located at RA, Dec 152.51422, 5.01213 which is equivalent to: RA(J2000) = 10h 10m 03.41s Dec(J2000) = +05d 00' 43.7" with an uncertainty of 3.7 arcseconds (radius, 90% containment). This location is 64 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. No spectrum from the promptly downlinked event data is yet available to determine the column density. The initial flux in the 2.5 s image was 2.21e-09 erg cm^-2 s^-1 (0.2-10 keV). UVOT took a finding chart exposure of 150 seconds with the White filter starting 83 seconds after the BAT trigger. There is a candidate afterglow in the rapidly available 2.7'x2.7' sub-image at RA(J2000) = 10:10:03.49 = 152.51455 DEC(J2000) = +05:00:41.8 = 5.01161 with a 90%-confidence error radius of about 0.75 arc sec. This position is 0.5 arc sec. from the center of the XRT error circle. The estimated magnitude is 18.46 with a 1-sigma error of about 0.15. No correction has been made for the expected extinction corresponding to E(B-V) of 0.02. Burst Advocate for this burst is J. L. Racusin (judith.racusin 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/too.html.)