NOTE: uvot_fluxes_wget.pl vrs. 2018-11-07 fem at 190627d17h59m11s299044usUT NOTE: Source region spec. is: 244.82788 -5.28912 3" NOTE: Used archived uvot source position of 244.82788 -5.28912 3.00 NOTE: position reference is GCN_Circ_24889 NOTE: A UVOT position was reported in GCN_Circ_24889 NOTE: Possible detection in wh at T+114.5 NOTE: Possible detection in w1 at T+3919.5 NOTE: Possible detection in w2 at T+4740.8 =========== Draft Upper Limit Circular ======== GRB 190627A: Swift/UVOT Upper Limits ***UBS*** (***INSTITUTION***) and E. Sonbas (Adiyaman Univ.) report on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 190627A 114 s after the BAT trigger (Sonbas et al., GCN Circ. 24888). No optical afterglow consistent with the uvot position *** POSITION REFERENCE is GCN_Circ_24889 *** 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 114 144 29 >17.2 w1 3920 5555 393 >18.0 m2 3714 3914 197 >20.1 w2 4741 4941 197 >18.8 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.18 in the direction of the burst (Schlegel et al. 1998). =========== Draft Detection Circular ======== GRB 190627A: Swift/UVOT Detection ***UBS*** (***INSTITUTION***) and E. Sonbas (Adiyaman Univ.) report on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 190627A 114 s after the BAT trigger (Sonbas et al., GCN Circ. 24888). A source consistent with the uvot position *** POSITION REFERENCE is GCN_Circ_24889 *** is detected in the initial UVOT exposures. The preliminary UVOT position is: RA (J2000) = 16:19:18.69 = 244.82788 (deg.) Dec (J2000) = -05:17:20.8 = -5.28912 (deg.) with an estimated uncertainty of 0.46 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 114 144 29 17.43 +/- 0.07 w1 3920 4119 197 18.11 +/- 0.14 m2 3714 3914 197 >20.1 w2 4741 4941 197 19.55 +/- 0.32 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.18 in the direction of the burst (Schlegel et al. 1998).