NOTE: uvot_fluxes_wget.pl vrs. 2024-08-27 fem at 241010d18h01m07s262947usUT NOTE: Source region spec. is: 153.38141 11.53429 3" NOTE: Used archived uvot source position of 153.38141 11.53429 3.00 NOTE: position reference is GCN_Circ_37755 NOTE: A UVOT position was reported in GCN_Circ_37755 NOTE: Possible detection in wh at T+105.4 NOTE: Possible detection in uu at T+317.3 NOTE: Possible detection in w1 at T+4883.1 sum =========== Draft Upper Limit Circular ======== GRB 241010A: Swift/UVOT Upper Limits ***UBS*** (***INSTITUTION***) and S. Dichiara (PSU) report on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 241010A 105 s after the BAT trigger (Dichiara et al., GCN Circ. 37755). No optical afterglow consistent with the XRT position *** POSITION REFERENCE is GCN_Circulars-37757 *** 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 105 255 147 >18.3 u_FC 317 547 226 >17.9 white 105 4263 344 >18.9 v 647 4673 216 >18.9 u 317 5128 265 >18.0 w1 696 5083 216 >18.6 m2 4678 4878 197 >18.9 w2 4269 4468 197 >19.3 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.039 in the direction of the burst (Schlegel et al. 1998). =========== Draft Detection Circular ======== GRB 241010A: Swift/UVOT Detection ***UBS*** (***INSTITUTION***) and S. Dichiara (PSU) report on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 241010A 105 s after the BAT trigger (Dichiara et al., GCN Circ. 37755). A source consistent with the XRT position *** POSITION REFERENCE is GCN_Circulars-37757 *** is detected in the initial UVOT exposures. The preliminary UVOT position is: RA (J2000) = 10:13:31.55 = 153.38145 (deg.) Dec (J2000) = +11:32:03.3 = 11.53424 (deg.) with an estimated uncertainty of 0.49 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 105 255 147 18.56 +/- 0.09 v 647 4673 216 >18.9 u 317 547 226 18.31 +/- 0.15 w1 696 5083 216 19.30 +/- 0.32 m2 4678 4878 197 >18.9 w2 4269 4468 197 >19.3 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.039 in the direction of the burst (Schlegel et al. 1998).