NOTE: uvot_fluxes_wget.pl vrs. 2024-08-27 fem at 260118d15h26m11s468316usUT NOTE: Source region spec. is: 170.2386 -61.9161 4" NOTE: Used archived XRT position of 170.23860 -61.91610 4.00 NOTE: position reference is GCN_Notice NOTE: Possible detection in uu at T+189.0 WARNING: t_start for light curve (189) and t_start from the exposure report (107) do not agree. Replace ??? in draft Circular with correct value. =========== Draft Upper Limit Circular ======== GRB 260118: Swift/UVOT Upper Limits ***UBS*** (***INSTITUTION***) and ***BA*** (***BA INSTITUTION***) report on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 260118 ***???*** s after the BAT trigger (***Author*** et al., GCN Circ. ????). 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 u_FC 189 439 246 >12.7 u 189 1024 393 >12.7 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 3.080 in the direction of the burst (Schlegel et al. 1998). =========== Draft Detection Circular ======== GRB 260118: Swift/UVOT Detection ***UBS*** (***INSTITUTION***) and ***BA*** (***BA INSTITUTION***) report on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 260118 ***???*** s after the BAT trigger (***Author*** et al., GCN Circ. ????). A source consistent with the XRT position *** POSITION REFERENCE is GCN_Notice *** is detected in the initial UVOT exposures. Preliminary detections 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 u 189 439 246 12.72 +/- 0.02 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 3.080 in the direction of the burst (Schlegel et al. 1998).