TITLE: GCN CIRCULAR NUMBER: 6654 SUBJECT: GRB 070724: Swift detection of a burst DATE: 07/07/24 11:22:00 GMT FROM: Scott Barthelmy at NASA/GSFC H. Ziaeepour (UCL-MSSL), S. D. Barthelmy (GSFC), A. P. Beardmore (U Leicester), D. N. Burrows (PSU), M. De Pasquale (UCL-MSSL), P. A. Evans (U Leicester), N. Gehrels (NASA/GSFC), S. T. Holland (CRESST/GSFC/USRA), H. A. Krimm (GSFC/USRA), V. Mangano (INAF-IASFPA), F. E. Marshall (NASA/GSFC), P. T. O'Brien (U Leicester), J. P. Osborne (U Leicester), C. Pagani (PSU), K. L. Page (U Leicester), D. M. Palmer (LANL), A. M. Parsons (GSFC), P. Romano (Univ. Bicocca & INAF-OAB), B. Sbarufatti (INAF-IASFPA), P. Schady (MSSL-UCL), M. Stamatikos (NASA/ORAU) and R. L. C. Starling (U Leicester) report on behalf of the Swift Team: At 10:53:50 UT, the Swift Burst Alert Telescope (BAT) triggered and located GRB 070724 (trigger=285948). Swift slewed immediately to the burst. The BAT on-board calculated location is RA, Dec 27.818, -18.622 which is RA(J2000) = 01h 51m 16s Dec(J2000) = -18d 37' 17" with an uncertainty of 3 arcmin (radius, 90% containment, including systematic uncertainty). The BAT light curve showed a strong spike about one second long at T+0 sec. The peak count rate was ~2700 counts/sec (15-350 keV), at ~0 sec after the trigger. This could be a short burst although the spectrum is not hard. The XRT began observing the field at 10:54:56 UT, 67 seconds after the BAT trigger. Using prompt downlinked data, we find a variable, uncatalogued X-ray source located at RA, Dec 27.8077, -18.5951 which is RA(J2000) = 01 51 13.86 Dec(J2000) = -18 35 42.4 with an uncertainty of 4.7 arcsec (radius, 90% containment). This location is 102 arcseconds from the BAT on-board position, within the BAT error circle. The initial flux in the 2.5s image was 6.4e-10 erg/cm2/s (0.2-10 keV). UVOT took a finding chart exposure of 100s with the White filter starting 75s after the BAT trigger. No 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 3-sigma upper limit is about 19.2 mag. No correction has been made for the expected reddening of E(B-V) of 0.01. Burst Advocate for this burst is H. Ziaeepour (hz AT mssl.ucl.ac.uk). 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.)