NOTE: uvot_fluxes_wget.pl vrs. 2023-03-23 fem at 230510d20h48m26s643022usUT NOTE: Source region spec. is: 318.13671 34.44306 4" NOTE: Used archived XRT position of 318.13671 34.44306 4.00 NOTE: position reference is GCN_Circulars-33756 NOTE: Possible detection in bb at T+4208.5 NOTE: Possible detection in wh at T+72.0 NOTE: Possible detection in uu at T+284.1 =========== Draft Upper Limit Circular ======== GRB 230510A: Swift/UVOT Upper Limits A. Belles (PSU) and Eyles-Ferris (U. Leicester) report on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 230510A 72 s after the BAT trigger (Eyles-Ferris et al., GCN Circ. 33752). No optical afterglow consistent with the XRT position *** POSITION REFERENCE is GCN_Circulars-33756 *** 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 72 222 147 >18.9 white 72 4613 344 >19.2 v 4824 5023 197 >18.9 b 4208 5690 242 >19.6 u 284 5638 229 >18.6 w1 5233 5433 197 >18.8 m2 5028 5228 197 >19.5 w2 4619 4819 197 >19.3 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.144 in the direction of the burst (Schlegel et al. 1998). =========== Draft Detection Circular ======== GRB 230510A: Swift/UVOT Detection A. Belles (PSU) and Eyles-Ferris (U. Leicester) report on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 230510A 72 s after the BAT trigger (Eyles-Ferris et al., GCN Circ. 33752). A source consistent with the XRT position *** POSITION REFERENCE is GCN_Circulars-33756 *** is detected in the initial UVOT exposures. The preliminary UVOT position is: RA (J2000) = 21:12:32.90 = 318.13710 (deg.) Dec (J2000) = +34:26:35.8 = 34.44328 (deg.) with an estimated uncertainty of 0.55 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 72 222 147 19.14 +/- 0.10 v 4824 5023 197 >18.9 b 4208 4408 197 20.04 +/- 0.29 u 284 5638 229 19.08 +/- 0.18 w1 5233 5433 197 >18.8 m2 5028 5228 197 >19.5 w2 4619 4819 197 >19.3 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.144 in the direction of the burst (Schlegel et al. 1998).