NOTE: uvot_fluxes_wget.pl vrs. 2023-03-23 fem at 240113d03h42m57s470971usUT NOTE: Source region spec. is: 270.64414 24.48923 3" NOTE: Used archived uvot source position of 270.64414 24.48923 3.00 NOTE: position reference is GCN_Circ_35522 NOTE: A UVOT position was reported in GCN_Circ_35522 NOTE: Possible detection in w1 at T+3929.6 NOTE: Possible detection in bb at T+4339.5 NOTE: Possible detection in uu at T+4134.4 NOTE: Possible detection in wh at T+120.7 =========== Draft Upper Limit Circular ======== GRB 240112C: Swift/UVOT Upper Limits N. P. M. Kuin (UCL-MSSL) and Eyles-Ferris (U. Leicester) report on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 240112C 121 s after the BAT trigger (Eyles-Ferris et al., GCN Circ. 35522). No optical afterglow consistent with the XRT position *** POSITION REFERENCE is GCN_Circulars-35522 *** 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 121 236 113 >16.9 white 121 4744 310 >17.9 v 4955 5126 169 >18.6 b 4340 4539 197 >18.9 u 4134 4334 197 >18.7 w1 3930 4129 197 >18.5 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.108 in the direction of the burst (Schlegel et al. 1998). =========== Draft Detection Circular ======== GRB 240112C: Swift/UVOT Detection N. P. M. Kuin (UCL-MSSL) and Eyles-Ferris (U. Leicester) report on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 240112C 121 s after the BAT trigger (Eyles-Ferris et al., GCN Circ. 35522). A source consistent with the XRT position *** POSITION REFERENCE is GCN_Circulars-35522 *** is detected in the initial UVOT exposures. The preliminary UVOT position is: RA (J2000) = 18:02:34.58 = 270.64410 (deg.) Dec (J2000) = +24:29:21.3 = 24.48925 (deg.) with an estimated uncertainty of 0.43 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 121 236 113 16.98 +/- 0.04 v 4955 5126 169 >18.6 b 4340 4539 197 19.35 +/- 0.16 u 4134 4334 197 19.11 +/- 0.18 w1 3930 4129 197 19.13 +/- 0.24 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.108 in the direction of the burst (Schlegel et al. 1998).