TITLE: GCN CIRCULAR NUMBER: 37662 SUBJECT: GRB 241002A: Swift detection of a burst DATE: 24/10/02 01:09:25 GMT FROM: K.L. Page at U Leicester R. Caputo (GSFC), R. Gupta (NASA GSFC), M. J. Moss (GSFC), K. L. Page (U Leicester), D. M. Palmer (LANL) and B. Sbarufatti (INAF-OAB) report on behalf of the Neil Gehrels Swift Observatory Team: At 00:50:22 UT, the Swift Burst Alert Telescope (BAT) triggered and located GRB 241002A (trigger=1257556). Swift slewed immediately to the burst. The BAT on-board calculated location is RA, Dec 140.955, +39.854 which is RA(J2000) = 09h 23m 49s Dec(J2000) = +39d 51' 15" 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 20 sec. The peak count rate was ~1900 counts/sec (15-350 keV), at ~0 sec after the trigger. The XRT began observing the field at 00:52:09.0 UT, 106.1 seconds after the BAT trigger. XRT found a bright, uncatalogued X-ray source located at RA, Dec 140.9500, 39.8324 which is equivalent to: RA(J2000) = 09h 23m 48.00s Dec(J2000) = +39d 49' 56.6" with an uncertainty of 5.8 arcseconds (radius, 90% containment). This location is 78 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. UVOT took a finding chart exposure of 150 seconds with the White filter starting 115 seconds after the BAT trigger. No credible afterglow candidate has been found in the initial data products. The 2.7'x2.7' sub-image processing FAILED because of no aspect solution. Data from the list of sources generated on-board are not available at this time. No correction has been made for the expected extinction corresponding to E(B-V) of 0.011. Burst Advocate for this burst is R. Caputo (regina.caputo 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/)