NOTE: uvot_fluxes_wget.pl vrs. 2024-08-27 fem at 250808d09h10m47s834433usUT NOTE: Source region spec. is: 51.44829 -47.88782 3" NOTE: Used archived uvot source position of 51.44829 -47.88782 3.00 NOTE: position reference is GCN_Circ_41262 NOTE: A UVOT position was reported in GCN_Circ_41262 NOTE: Possible detection in wh at T+111.2 NOTE: Possible detection in uu at T+323.2 =========== Draft Upper Limit Circular ======== GRB 250807A: Swift/UVOT Upper Limits ***UBS*** (***INSTITUTION***) and N. J. Klingler (GSFC/UMBC/CRESSTII) report on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 250807A 111 s after the BAT trigger (Klingler et al., GCN Circ. 41262). No optical afterglow consistent with the XRT position *** POSITION REFERENCE is GCN_Circulars-41270 *** 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 111 261 147 >17.9 u_FC 323 573 246 >18.9 white 111 1719 411 >18.8 v 653 1769 136 >19.1 b 579 1695 117 >19.3 u 323 1841 361 >19.3 w1 702 1818 117 >19.0 w2 801 821 19 >18.7 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.011 in the direction of the burst (Schlegel et al. 1998). =========== Draft Detection Circular ======== GRB 250807A: Swift/UVOT Detection ***UBS*** (***INSTITUTION***) and N. J. Klingler (GSFC/UMBC/CRESSTII) report on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 250807A 111 s after the BAT trigger (Klingler et al., GCN Circ. 41262). A source consistent with the XRT position *** POSITION REFERENCE is GCN_Circulars-41270 *** is detected in the initial UVOT exposures. The preliminary UVOT position is: RA (J2000) = 03:25:47.60 = 51.44832 (deg.) Dec (J2000) = -47:53:16.0 = -47.88777 (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 111 261 147 17.99 +/- 0.04 v 653 1769 136 >19.1 b 579 1695 117 >19.3 u 323 573 246 19.32 +/- 0.15 w1 702 1818 117 >19.0 w2 801 821 19 >18.7 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.011 in the direction of the burst (Schlegel et al. 1998).