NOTE: uvot_fluxes_wget.pl vrs. 2020-11-03a fem at 201111d14h00m33s541063usUT NOTE: Source region spec. is: 277.67371 -6.75478 4" NOTE: Used archived XRT position of 277.67371 -6.75478 4.00 NOTE: position reference is GRB_Auto_Processing NOTE: Possible detection in uu at T+267.3 NOTE: Possible detection in wh at T+55.0 NOTE: Possible detection in bb at T+695.2 NOTE: Possible detection in vv at T+596.7 =========== Draft Upper Limit Circular ======== GRB 201111: 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 201111 55 s after the BAT trigger (***Author*** et al., GCN Circ. ????). No optical afterglow consistent with the XRT position *** POSITION REFERENCE is GRB_Auto_Processing *** 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 55 205 147 >18.2 u_FC 267 517 246 >18.3 white 55 1542 392 >18.4 v 597 1767 136 >16.9 b 523 1691 117 >18.0 u 267 1666 362 >18.4 w1 646 1641 117 >19.2 w2 572 1742 136 >19.9 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 1.78 in the direction of the burst (Schlegel et al. 1998). =========== Draft Detection Circular ======== GRB 201111: 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 201111 55 s after the BAT trigger (***Author*** et al., GCN Circ. ????). A source consistent with the XRT position *** POSITION REFERENCE is GRB_Auto_Processing *** is detected in the initial UVOT exposures. 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 55 205 147 18.46 +/- 0.08 v 597 1243 78 17.26 +/- 0.17 b 523 1342 78 18.37 +/- 0.17 u 267 517 246 18.66 +/- 0.15 w1 646 1641 117 >19.2 w2 572 1742 136 >19.9 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 1.78 in the direction of the burst (Schlegel et al. 1998).