NOTE: uvot_fluxes_wget.pl vrs. 2024-08-27 fem at 241113d15h04m45s562336usUT NOTE: Source region spec. is: 16.56521 -22.67164 4" NOTE: Used archived XRT position of 16.56521 -22.67164 4.00 NOTE: position reference is GCN_Circulars-38198 NOTE: Possible detection in wh at T+82.0 =========== Draft Upper Limit Circular ======== GRB 241113A: Swift/UVOT Upper Limits A. A. Breeveld (UCL-MSSL) and M. H. Siegel (PSU) report on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 241113A 82 s after the BAT trigger (Siegel et al., GCN Circ. 38194). No optical afterglow consistent with the XRT position *** POSITION REFERENCE is GCN_Circulars-38198 *** 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 initial exposures are: Filter T_start(s) T_stop(s) Exp(s) Mag white 82 183 100 >15.8 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.030 in the direction of the burst (Schlegel et al. 1998). =========== Draft Detection Circular ======== GRB 241113A: Swift/UVOT Detection A. A. Breeveld (UCL-MSSL) and M. H. Siegel (PSU) report on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 241113A 82 s after the BAT trigger (Siegel et al., GCN Circ. 38194). A source consistent with the XRT position *** POSITION REFERENCE is GCN_Circulars-38198 *** is detected in the initial UVOT exposures. The preliminary UVOT position is: RA (J2000) = 01:06:15.64 = 16.56518 (deg.) Dec (J2000) = -22:40:18.6 = -22.67182 (deg.) with an estimated uncertainty of 0.42 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 82 183 100 15.90 +/- 0.03 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.030 in the direction of the burst (Schlegel et al. 1998).