NOTE: uvot_fluxes_wget.pl vrs. 2024-08-27 fem at 250905d01h41m55s463058usUT NOTE: Source region spec. is: 84.38046 3.58444 4" NOTE: Used archived XRT position of 84.38046 3.58444 4.00 NOTE: position reference is GCN_Circulars-41711 NOTE: Possible detection in wh at T+85.7 =========== Draft Upper Limit Circular ======== GRB 250904A: Swift/UVOT Upper Limits ***UBS*** (***INSTITUTION***) and C. Salvaggio (INAF-OAB) report on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 250904A 86 s after the BAT trigger (Salvaggio et al., GCN Circ. 41704). No optical afterglow consistent with the XRT position *** POSITION REFERENCE is GCN_Circulars-41711 *** 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 86 235 147 >19.5 white 86 235 147 >19.5 u 298 441 141 >18.6 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.305 in the direction of the burst (Schlegel et al. 1998). =========== Draft Detection Circular ======== GRB 250904A: Swift/UVOT Detection ***UBS*** (***INSTITUTION***) and C. Salvaggio (INAF-OAB) report on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 250904A 86 s after the BAT trigger (Salvaggio et al., GCN Circ. 41704). A source consistent with the XRT position *** POSITION REFERENCE is GCN_Circulars-41711 *** is detected in the initial UVOT exposures. 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 86 235 147 20.12 +/- 0.25 u 298 441 141 >18.6 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.305 in the direction of the burst (Schlegel et al. 1998).