NOTE: uvot_fluxes_wget.pl vrs. 2024-08-27 fem at 250924d21h33m10s694897usUT NOTE: Source region spec. is: 51.87340 74.65945 3" NOTE: Used archived uvot source position of 51.87340 74.65945 3.00 NOTE: position reference is GCN_Circ_41959 NOTE: A UVOT position was reported in GCN_Circ_41959 NOTE: Possible detection in uu at T+350.9 NOTE: Possible detection in bb at T+606.5 NOTE: Possible detection in wh at T+192.7 =========== Draft Upper Limit Circular ======== GRB 250924A: Swift/UVOT Upper Limits ***UBS*** (***INSTITUTION***) and M. H. Siegel (PSU) report on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 250924A 193 s after the BAT trigger (Siegel et al., GCN Circ. 41959). No optical afterglow consistent with the XRT position *** POSITION REFERENCE is GRB_Auto_Processing *** is detected in the initial UVOT exposures. Preliminary 3-sigma upper limits using the UVOT photometric system (Breeveld et al. 2011, AIP Conf. Proc. 1358, 373) for the first finding chart (FC) exposure and subsequent exposures are: Filter T_start(s) T_stop(s) Exp(s) Mag white_FC 193 342 147 >17.7 u_FC 351 601 246 >17.8 white 193 1184 353 >18.4 v 681 1234 58 >18.4 b 606 1160 58 >18.8 u 351 1135 285 >17.9 w1 730 1110 39 >19.0 m2 1065 1085 19 >17.6 w2 656 1210 78 >19.6 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.315 in the direction of the burst (Schlegel et al. 1998). =========== Draft Detection Circular ======== GRB 250924A: Swift/UVOT Detection ***UBS*** (***INSTITUTION***) and M. H. Siegel (PSU) report on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 250924A 193 s after the BAT trigger (Siegel et al., GCN Circ. 41959). A source consistent with the XRT position *** POSITION REFERENCE is GRB_Auto_Processing *** is detected in the initial UVOT exposures. The preliminary UVOT position is: RA (J2000) = 03:27:29.66 = 51.87358 (deg.) Dec (J2000) = +74:39:34.0 = 74.65945 (deg.) with an estimated uncertainty of 0.43 arc sec. (radius, 90% confidence). Preliminary detections and 3-sigma upper limits using the UVOT photometric system (Breeveld et al. 2011, AIP Conf. Proc. 1358, 373) for the early exposures are: Filter T_start(s) T_stop(s) Exp(s) Mag white 193 342 147 17.80 +/- 0.04 v 681 1234 58 >18.4 b 606 626 19 18.75 +/- 0.30 u 351 601 246 18.03 +/- 0.08 w1 730 1110 39 >19.0 m2 1065 1085 19 >17.6 w2 656 1210 78 >19.6 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.315 in the direction of the burst (Schlegel et al. 1998).