NOTE: uvot_fluxes_wget.pl vrs. 2023-03-23 fem at 240621d09h32m51s037304usUT NOTE: Source region spec. is: 162.39442 17.28292 4" NOTE: Used archived XRT position of 162.39442 17.28292 4.00 NOTE: position reference is GCN_Circulars-36721 NOTE: Possible detection in uu at T+740635456.8 NOTE: Possible detection in wh at T+740636273.2 WARNING: t_start for light curve (740635457) and t_start from the exposure report (0) do not agree. Replace ??? in draft Circular with correct value. =========== Draft Upper Limit Circular ======== GRB ??????: 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 ?????? ***???*** s after the BAT trigger (***Author*** et al., GCN Circ. ????). No optical afterglow consistent with the XRT position *** POSITION REFERENCE is GCN_Circulars-36721 *** 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 initial exposures are: Filter T_start(s) T_stop(s) Exp(s) Mag white 740636273 740636911 628 >19.5 v 740637090 740637173 81 >18.5 u 740635457 740641426 1071 >18.8 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.029 in the direction of the burst (Schlegel et al. 1998). =========== Draft Detection Circular ======== GRB ??????: 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 ?????? ***???*** s after the BAT trigger (***Author*** et al., GCN Circ. ????). A source consistent with the XRT position *** POSITION REFERENCE is GCN_Circulars-36721 *** is detected in the initial UVOT exposures. The preliminary UVOT position is: RA (J2000) = 10:49:34.72 = 162.39467 (deg.) Dec (J2000) = +17:16:58.6 = 17.28295 (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 740636273 740636911 628 19.69 +/- 0.08 v 740637090 740637173 81 >18.5 u 740635457 740636267 797 19.15 +/- 0.14 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.029 in the direction of the burst (Schlegel et al. 1998).