NOTE: uvot_fluxes_wget.pl vrs. 2020-11-03a fem at 220413d01h30m42s492902usUT NOTE: Source region spec. is: 123.96728 +30.34269 3" NOTE: Used archived opt source position of 123.96728 30.34269 3.00 NOTE: position reference is GCN_Circ-31882 NOTE: Possible detection in wh at T+863.2 =========== Draft Upper Limit Circular ======== GRB 220412A: Swift/UVOT Upper Limits A. A. Breeveld (UCL-MSSL) and N. J. Klingler (GSFC/UMBC/CRESSTII) report on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 220412A 127 s after the BAT trigger (Klingler et al., GCN Circ. 31881). No optical afterglow consistent with the optical position *** POSITION REFERENCE is GCN_Circ-31882 *** 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 127 276 147 >20.9 u_FC 285 534 246 >20.4 white 127 1013 295 >20.7 u 285 534 246 >20.4 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.037 in the direction of the burst (Schlegel et al. 1998). =========== Draft Detection Circular ======== GRB 220412A: Swift/UVOT Detection A. A. Breeveld (UCL-MSSL) and N. J. Klingler (GSFC/UMBC/CRESSTII) report on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 220412A 127 s after the BAT trigger (Klingler et al., GCN Circ. 31881). A source consistent with the optical position *** POSITION REFERENCE is GCN_Circ-31882 *** 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 863 1013 147 20.87 +/- 0.32 u 285 534 246 >20.4 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.037 in the direction of the burst (Schlegel et al. 1998).