NOTE: uvot_fluxes_wget.pl vrs. 2023-03-23 fem at 230819d06h03m47s846052usUT NOTE: Source region spec. is: 285.88796 40.89681 3" NOTE: Used archived opt source position of 285.88796 40.89681 3.00 NOTE: position reference is GCN_Circulars-34476 NOTE: Possible detection in wh at T+144.1 NOTE: Possible detection in bb at T+650.0 sum NOTE: Possible detection in vv at T+551.8 sum =========== Draft Upper Limit Circular ======== GRB 230818A: Swift/UVOT Upper Limits ***UBS*** (***INSTITUTION***) and A. Tohuvavohu (U. Toronto) report on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 230818A 144 s after the BAT trigger (Tohuvavohu et al., GCN Circ. 34479). No optical afterglow consistent with the optical position *** POSITION REFERENCE is GCN_Circulars-34476 *** 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 144 294 147 >18.9 white 144 1536 410 >19.5 v 379 5121 243 >19.1 b 477 1513 117 >19.2 u 452 1487 117 >19.5 w1 428 1463 97 >20.2 w2 1026 4987 255 >20.1 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.101 in the direction of the burst (Schlegel et al. 1998). =========== Draft Detection Circular ======== GRB 230818A: Swift/UVOT Detection ***UBS*** (***INSTITUTION***) and A. Tohuvavohu (U. Toronto) report on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 230818A 144 s after the BAT trigger (Tohuvavohu et al., GCN Circ. 34479). A source consistent with the optical position *** POSITION REFERENCE is GCN_Circulars-34476 *** is detected in the initial UVOT exposures. The preliminary UVOT position is: RA (J2000) = 19:03:33.13 = 285.88806 (deg.) Dec (J2000) = +40:53:49.0 = 40.89695 (deg.) with an estimated uncertainty of 0.48 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 144 294 147 19.09 +/- 0.07 v 379 572 39 18.40 +/- 0.30 b 477 1513 117 19.68 +/- 0.20 u 452 1487 117 >19.5 w1 428 1463 97 >20.2 w2 1026 4987 255 >20.1 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.101 in the direction of the burst (Schlegel et al. 1998).