TITLE: GCN CIRCULAR NUMBER: 29420 SUBJECT: GRB 210207B: Swift detection of a burst with a bright optical counterpart DATE: 21/02/07 22:03:29 GMT FROM: Scott Barthelmy at NASA/GSFC A. Y. Lien (GSFC/UMBC), E. Ambrosi (INAF-IASFPA), S. D. Barthelmy (GSFC), A. D'Ai (INAF-IASFPA), V. D'Elia (SSDC), J.D. Gropp (PSU), J. A. Kennea (PSU), N. P. M. Kuin (UCL-MSSL), S. Laha (GSFC/UMBC/CRESST), F. E. Marshall (NASA/GSFC), D. M. Palmer (LANL), A. Tohuvavohu (U Toronto) and E. Troja (NASA/GSFC/UMCP) report on behalf of the Neil Gehrels Swift Observatory Team: At 21:52:08 UT, the Swift Burst Alert Telescope (BAT) triggered and located GRB 210207B (trigger=1031297). Swift slewed immediately to the burst. The BAT on-board calculated location is RA, Dec 270.582, +53.694 which is RA(J2000) = 18h 02m 20s Dec(J2000) = +53d 41' 39" 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 ~2500 counts/sec (15-350 keV), at ~45 sec after the trigger. The XRT began observing the field at 21:53:22.0 UT, 73.9 seconds after the BAT trigger. XRT found a bright, uncatalogued X-ray source located at RA, Dec 270.6356, 53.6836 which is equivalent to: RA(J2000) = 18h 02m 32.54s Dec(J2000) = +53d 41' 01.0" with an uncertainty of 4.7 arcseconds (radius, 90% containment). This location is 120 arcseconds from the BAT onboard position, within the BAT error circle. No event data are yet available to determine the column density using X-ray spectroscopy. The initial flux in the 2.5 s image was 1.09e-08 erg cm^-2 s^-1 (0.2-10 keV). UVOT took a finding chart exposure of 150 seconds with the White filter starting 82 seconds after the BAT trigger. There is a candidate afterglow in the rapidly available 2.7'x2.7' sub-image at RA(J2000) = 18:02:32.40 = 270.63501 DEC(J2000) = +53:40:56.0 = 53.68223 with a 90%-confidence error radius of about 0.74 arc sec. This position is 5.1 arc sec. from the center of the XRT error circle. The estimated magnitude is 13.72 with a 1-sigma error of about 0.14. No correction has been made for the expected extinction corresponding to E(B-V) of 0.041. Burst Advocate for this burst is A. Y. Lien (amy.y.lien 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/)