TITLE: GCN CIRCULAR NUMBER: 40825 SUBJECT: GRB 250625A: Swift detection of a burst DATE: 25/06/25 16:20:37 GMT FROM: David Palmer at LANL <palmer@lanl.gov> M. Ferro (INAF-OAB), R. Brivio (INAF-OAB), J. J. DeLaunay (PSU), R. Gupta (NASA GSFC), J. A. Kennea (PSU), D. M. Palmer (LANL), B. Sbarufatti (INAF-OAB) and M. H. Siegel (PSU) report on behalf of the Neil Gehrels Swift Observatory Team: At 16:04:56 UT, the Swift Burst Alert Telescope (BAT) triggered and located GRB 250625A (trigger=1327910). Swift slewed immediately to the burst. The BAT on-board calculated location is RA, Dec 261.519, +22.265 which is RA(J2000) = 17h 26m 04s Dec(J2000) = +22d 15' 55" 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 8 sec. The peak count rate was ~2200 counts/sec (15-350 keV), at ~2 sec after the trigger. The XRT began observing the field at 16:06:56.2 UT, 119.8 seconds after the BAT trigger. Using promptly downlinked data we find an uncatalogued X-ray source with an enhanced position: RA, Dec 261.50871, 22.26763 which is equivalent to: RA(J2000) = 17h 26m 02.09s Dec(J2000) = +22d 16' 03.5" with an uncertainty of 1.9 arcseconds (radius, 90% containment). This location is 35 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 https://www.swift.ac.uk/sper. We cannot determine whether the source is fading at the present time. A power-law fit to a spectrum formed from promptly downlinked event data gives a column density in excess of the Galactic value (5.47 x 10^20 cm^-2, Willingale et al. 2013), with an excess column of 8 (+10.81/-7.26) x 10^21 cm^-2 (90% confidence). UVOT took a finding chart exposure of 150 seconds with the White filter starting 124 seconds after the BAT trigger. No credible 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 typical 3-sigma upper limit has been about 19.6 mag. The 8'x8' region for the list of sources generated on-board covers 100% of the XRT error circle. The list of sources is typically complete to about 18 mag. No correction has been made for the expected extinction corresponding to E(B-V) of 0.055. This is co-detection with Fermi/GBM (GCN #40824). Burst Advocate for this burst is M. Ferro (matteo.ferro AT inaf.it). 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/) View this GCN Circular online at https://gcn.nasa.gov/circulars/40825. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0LW...