NOTE: uvot_fluxes_wget.pl vrs. 2024-08-27 fem at 251206d03h00m28s173505usUT NOTE: Source region spec. is: 200.27223 29.92888 3" NOTE: Used archived uvot source position of 200.27223 29.92888 3.00 NOTE: position reference is GCN_Circ_43005 NOTE: A UVOT position was reported in GCN_Circ_43005 NOTE: Possible detection in w1 at T+685.8 NOTE: Possible detection in wh at T+149.0 NOTE: Possible detection in vv at T+636.5 NOTE: Possible detection in bb at T+562.4 NOTE: Possible detection in uu at T+306.8 =========== Draft Upper Limit Circular ======== GRB 251205A: Swift/UVOT Upper Limits ***UBS*** (***INSTITUTION***) and Lanava (PSU) report on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 251205A 149 s after the BAT trigger (Lanava et al., GCN Circ. 43005). 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 149 299 147 >17.5 u_FC 307 557 246 >16.5 white 149 869 196 >17.3 v 636 829 39 >16.6 b 562 755 39 >17.0 u 307 730 265 >16.5 w1 686 706 19 >15.8 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.014 in the direction of the burst (Schlegel et al. 1998). =========== Draft Detection Circular ======== GRB 251205A: Swift/UVOT Detection ***UBS*** (***INSTITUTION***) and Lanava (PSU) report on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 251205A 149 s after the BAT trigger (Lanava et al., GCN Circ. 43005). 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) = 13:21:05.34 = 200.27223 (deg.) Dec (J2000) = +29:55:44.0 = 29.92890 (deg.) with an estimated uncertainty of 0.43 arc sec. (radius, 90% confidence). Preliminary detections 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 149 299 147 17.61 +/- 0.04 v 636 829 39 16.98 +/- 0.16 b 562 582 20 17.29 +/- 0.15 u 307 557 246 16.58 +/- 0.04 w1 686 706 20 16.19 +/- 0.16 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.014 in the direction of the burst (Schlegel et al. 1998).