NOTE: uvot_fluxes_wget.pl vrs. 2020-11-03a fem at 220101d08h29m03s769306usUT NOTE: Source region spec. is: 1.3533 +31.7690 3" NOTE: Used archived uvot source position of 1.35330 31.76900 3.00 NOTE: position reference is GCN_Notice NOTE: A UVOT position was reported in GCN_Notice_Sat_01_Jan_22_05:27:04_UT NOTE: Possible detection in wh at T+90.0 NOTE: Possible detection in vv at T+4447.6 =========== Draft Upper Limit Circular ======== GRB 220101: Swift/UVOT Upper Limits N. P. M. Kuin (UCL-MSSL) and ***BA*** (***BA INSTITUTION***) report on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 220101 90 s after the BAT trigger (***Author*** et al., GCN Circ. ????). 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 90 240 147 >14.6 white 90 4237 344 >16.1 v 4448 4647 197 >18.2 b 3833 4032 197 >19.8 u 3628 5201 334 >20.1 w1 4858 5057 197 >20.1 m2 4652 4852 197 >20.2 w2 4243 4443 197 >20.4 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.056 in the direction of the burst (Schlegel et al. 1998). =========== Draft Detection Circular ======== GRB 220101: Swift/UVOT Detection N. P. M. Kuin (UCL-MSSL) and ***BA*** (***BA INSTITUTION***) report on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 220101 90 s after the BAT trigger (***Author*** et al., GCN Circ. ????). 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) = 00:05:24.80 = 1.35334 (deg.) Dec (J2000) = +31:46:08.4 = 31.76899 (deg.) with an estimated uncertainty of 0.42 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 90 240 147 14.68 +/- 0.02 v 4448 4647 197 18.70 +/- 0.18 b 3833 4032 197 >19.8 u 3628 5201 334 >20.1 w1 4858 5057 197 >20.1 m2 4652 4852 197 >20.2 w2 4243 4443 197 >20.4 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.056 in the direction of the burst (Schlegel et al. 1998).