NOTE: uvot_fluxes_wget.pl vrs. 2020-11-03a fem at 220404d05h32m41s196250usUT NOTE: Source region spec. is: 191.47207 89.18518 3" NOTE: Used archived uvot source position of 191.47207 89.18518 3.00 NOTE: position reference is GCN_Circ_31820 NOTE: A UVOT position was reported in GCN_Circ_31820 NOTE: Possible detection in uu at T+317.6 NOTE: Possible detection in wh at T+105.3 WARNING: Did not recognize UBS name. =========== Draft Upper Limit Circular ======== GRB 220403B: Swift/UVOT Upper Limits Klingler (***INSTITUTION***) reports on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 220403B 105 s after the BAT trigger (Klingler et al., GCN Circ. 31820). 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 105 255 147 >19.5 u_FC 318 567 246 >19.4 white 105 1023 334 >19.6 v 647 1074 58 >18.6 b 573 766 39 >19.3 u 318 741 265 >19.4 w1 697 716 19 >18.9 w2 797 1049 39 >19.9 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.208 in the direction of the burst (Schlegel et al. 1998). =========== Draft Detection Circular ======== GRB 220403B: Swift/UVOT Detection Klingler (***INSTITUTION***) reports on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 220403B 105 s after the BAT trigger (Klingler et al., GCN Circ. 31820). 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) = 12:45:53.46 = 191.47274 (deg.) Dec (J2000) = +89:11:06.5 = 89.18515 (deg.) with an estimated uncertainty of 0.52 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 105 255 147 19.86 +/- 0.12 v 647 1074 58 >18.6 b 573 766 39 >19.3 u 318 741 265 19.93 +/- 0.22 w1 697 716 19 >18.9 w2 797 1049 39 >19.9 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.208 in the direction of the burst (Schlegel et al. 1998).