TITLE: GCN CIRCULAR NUMBER: 32240 SUBJECT: Swift Detection of MAXI J0655-013 DATE: 22/06/21 15:47:48 GMT FROM: David Palmer at LANL J.D. Gropp (PSU), N. J. Klingler (GSFC/UMBC/CRESSTII), A. Y. Lien (U Tampa), T. M. Parsotan (GSFC/UMBC/CRESSTII) and M. H. Siegel (PSU) report on behalf of the Neil Gehrels Swift Observatory Team: At 15:19:30 UT, the Swift Burst Alert Telescope (BAT) located the source MAXI J0655-013 (trigger=1111242). Due to observing constraints, Swift could not slew to the location. The BAT on-board calculated location is RA, Dec 103.829, -1.479 which is RA(J2000) = 06h 55m 19s Dec(J2000) = -01d 28' 43" with an uncertainty of 3 arcmin (radius, 90% containment, including systematic uncertainty). As is usual for an image trigger, the immediately available lightcurve does not show clear variation due to this source. Due to a Sun observing constraint, Swift cannot slew to the BAT position until 19:28 UT on 2022 August 19. There will thus be no XRT or UVOT data for this trigger before this time. This source, MAXI J0655-013 (GCN #32223; ATEL #15442, #15443), has been seen by BAT multiple times in 64s or longer image triggers. These include 2022-06-18T10:59 2022-06-18T15:43 2022-06-18T18:46 2022-06-18T20:24 2022-06-19T10:33 2022-06-19T15:34 2022-06-20T12:14 The strength of the source is ~100-200 mCrab during the above detections. The average location of these detections is RA, Dec 103.806, -1.491 with a standard deviation of ~1.5 arcmin in each coordinate.