NOTE: uvot_fluxes_wget.pl vrs. 2024-08-27 fem at 251018d18h47m43s379003usUT NOTE: Source region spec. is: 282.04183 -37.02840 3" NOTE: Used archived uvot source position of 282.04183 -37.02840 3.00 NOTE: position reference is GCN_Circ_42343 NOTE: A UVOT position was reported in GCN_Circ_42343 NOTE: Possible detection in wh at T+83.7 =========== Draft Upper Limit Circular ======== GRB 251018A: Swift/UVOT Upper Limits ***UBS*** (***INSTITUTION***) and Gupta (NASA GSFC) report on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 251018A 84 s after the BAT trigger (Gupta et al., GCN Circ. 42343). No optical afterglow consistent with the XRT position *** POSITION REFERENCE is GCN_Notice *** 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 84 233 147 >18.0 u_FC 296 546 246 >19.8 white 84 4988 363 >19.1 v 626 5303 121 >18.6 b 551 4783 216 >20.4 u 296 4578 442 >19.9 w1 4173 4373 197 >20.0 m2 650 670 19 >18.3 w2 602 5195 216 >19.5 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.101 in the direction of the burst (Schlegel et al. 1998). =========== Draft Detection Circular ======== GRB 251018A: Swift/UVOT Detection ***UBS*** (***INSTITUTION***) and Gupta (NASA GSFC) report on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 251018A 84 s after the BAT trigger (Gupta et al., GCN Circ. 42343). A source consistent with the XRT position *** POSITION REFERENCE is GCN_Notice *** is detected in the initial UVOT exposures. The preliminary UVOT position is: RA (J2000) = 18:48:10.03 = 282.04180 (deg.) Dec (J2000) = -37:01:42.4 = -37.02845 (deg.) with an estimated uncertainty of 0.45 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 84 233 147 18.16 +/- 0.05 v 626 5303 121 >18.6 b 551 4783 216 >20.4 u 296 4578 442 >19.9 w1 4173 4373 197 >20.0 m2 650 670 19 >18.3 w2 602 5195 216 >19.5 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.101 in the direction of the burst (Schlegel et al. 1998).