NOTE: uvot_fluxes_wget.pl vrs. 2018-11-07 fem at 190129d13h16m36s166078usUT NOTE: Source region spec. is: 207.0535 -63.2746 3" NOTE: Used archived uvot source position of 207.05350 -63.27460 3.00 NOTE: position reference is GCN_Notice NOTE: A UVOT position was reported in GCN_Notice_Tue_29_Jan_19_10:46:05_UT NOTE: Possible detection in wh at T+199.4 NOTE: Possible detection in vv at T+1951.5 =========== Draft Upper Limit Circular ======== GRB 190129: 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 190129 199 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 white_FC 199 349 147 >16.5 white 199 349 147 >16.5 v 1952 1971 19 >15.4 m2 1976 1985 9 >17.3 w2 410 430 19 >17.1 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 4.44 in the direction of the burst (Schlegel et al. 1998). =========== Draft Detection Circular ======== GRB 190129: 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 190129 199 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. The preliminary UVOT position is: RA (J2000) = 13:48:12.86 = 207.05357 (deg.) Dec (J2000) = -63:16:28.1 = -63.27448 (deg.) with an estimated uncertainty of 0.44 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 199 349 147 16.61 +/- 0.03 v 1952 1971 20 15.79 +/- 0.13 m2 1976 1985 9 >17.3 w2 410 430 19 >17.1 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 4.44 in the direction of the burst (Schlegel et al. 1998).