NOTE: uvot_fluxes_wget.pl vrs. 2018-11-07 fem at 190220d14h52m53s554642usUT NOTE: Source region spec. is: 330.16309 -76.68067 3" NOTE: Used archived uvot source position of 330.16309 -76.68067 3.00 NOTE: position reference is GCN_Circ_23908 NOTE: A UVOT position was reported in GCN_Circ_23908 NOTE: Possible detection in wh at T+86.6 =========== Draft Upper Limit Circular ======== GRB 190220A: Swift/UVOT Upper Limits S. J. LaPorte (PSU) and K. L. Page (U. Leicester) report on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 190220A 87 s after the BAT trigger (Page et al., GCN Circ. 23908). No optical afterglow consistent with the XRT position *** POSITION REFERENCE is GRB_Auto_Processing *** 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 87 236 147 >19.1 u_FC 299 548 246 >19.7 white 87 910 219 >19.4 v 628 821 39 >18.9 b 554 747 39 >19.4 u 299 722 265 >19.7 w1 678 871 39 >18.4 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.13 in the direction of the burst (Schlegel et al. 1998). =========== Draft Detection Circular ======== GRB 190220A: Swift/UVOT Detection S. J. LaPorte (PSU) and K. L. Page (U. Leicester) report on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 190220A 87 s after the BAT trigger (Page et al., GCN Circ. 23908). A source consistent with the XRT position *** POSITION REFERENCE is GRB_Auto_Processing *** is detected in the initial UVOT exposures. The preliminary UVOT position is: RA (J2000) = 22:00:39.17 = 330.16322 (deg.) Dec (J2000) = -76:40:50.6 = -76.68073 (deg.) with an estimated uncertainty of 0.50 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 87 236 147 19.44 +/- 0.11 v 628 821 39 >18.9 b 554 747 39 >19.4 u 299 722 265 >19.7 w1 678 871 39 >18.4 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.13 in the direction of the burst (Schlegel et al. 1998).