NOTE: uvot_fluxes_wget.pl vrs. 2020-11-03a fem at 220408d11h00m39s285860usUT NOTE: Source region spec. is: 202.41548 47.06931 3" NOTE: Used archived uvot source position of 202.41548 47.06931 3.00 NOTE: position reference is GCN_Circ_31848 NOTE: A UVOT position was reported in GCN_Circ_31848 NOTE: Possible detection in wh at T+112.5 =========== Draft Upper Limit Circular ======== GRB 220408A: Swift/UVOT Upper Limits S. R. Oates (U.Birmingham) and Caputo (GSFC) report on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 220408A 112 s after the BAT trigger (Caputo et al., GCN Circ. 31848). 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 112 262 147 >20.0 u_FC 325 575 246 >20.1 white 112 799 186 >20.2 b 581 774 39 >20.1 u 325 575 246 >20.1 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.042 in the direction of the burst (Schlegel et al. 1998). =========== Draft Detection Circular ======== GRB 220408A: Swift/UVOT Detection S. R. Oates (U.Birmingham) and Caputo (GSFC) report on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 220408A 112 s after the BAT trigger (Caputo et al., GCN Circ. 31848). A source consistent with the XRT position *** POSITION REFERENCE is GCN_Notice *** 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 112 262 147 20.49 +/- 0.17 b 581 774 39 >20.1 u 325 575 246 >20.1 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.042 in the direction of the burst (Schlegel et al. 1998).