TITLE: GCN CIRCULAR NUMBER: 6401 SUBJECT: GRB 070510: Swift detection of a possible burst DATE: 07/05/10 06:44:48 GMT FROM: Scott Barthelmy at NASA/GSFC P. Schady (MSSL-UCL), S. D. Barthelmy (GSFC), P. A. Evans (U Leicester), O. Godet (U Leicester), T. Mineo (INAF-IASFPA), P. T. O'Brien (U Leicester), C. Pagani (PSU), K. L. Page (U Leicester), D. M. Palmer (LANL) and E. Troja (INAF-IASFPA) report on behalf of the Swift Team: At 05:56:40 UT, the Swift Burst Alert Telescope (BAT) triggered and located possible GRB 070510 (trigger=278987) as it was approaching the South Atlantic Anomaly (SAA), with a processing delay of approximately 1 minute due to the data backlog from the high count rates. Swift slewed immediately to the burst. The BAT on-board calculated location is RA, DEC 343.014, +47.933 which is RA(J2000) = 22h 52m 03s Dec(J2000)= +47d 56' 00" with an uncertainty of 3 arcmin (radius, 90% containment, including systematic uncertainty). The BAT light curve shows a single short peak of ~1000 counts/s at the time of the trigger, but the elevated background (4x normal) makes it difficult to characterize the burst using only the TDRSS data. The data is terminated by entrance into the SAA at T+17 s. The XRT began taking data at 05:58:50 UT, 131 seconds after the BAT trigger. The XRT on-board centroid algorithm did not find a source in the image and no prompt position is available due to the spacecraft entering the SAA during the slew. We are waiting for down-linked data to detect and determine a position for the source. UVOT took a finding chart exposure of 100 seconds with the White (160-650nm) filter starting 1361 seconds after the BAT trigger. No afterglow candidate has been found in the initial data products. The typical 3-sigma upper limit has been about 18.5 mag. No correction has been made for the expected extinction corresponding to E(B-V) of 0.20 magnitudes.