NOTE: uvot_fluxes_wget.pl vrs. 2020-11-03a fem at 210217d12h03m35s124487usUT NOTE: Source region spec. is: 277.67275 -6.75439 4" NOTE: Used archived XRT position of 277.67275 -6.75439 4.00 NOTE: position reference is GRB_Auto_Processing NOTE: Possible detection in wh at T+76.8 =========== Draft Upper Limit Circular ======== GRB 210217: Swift/UVOT Upper Limits K. K. Simpson (PSU) and ***BA*** (***BA INSTITUTION***) report on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 210217 77 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 77 227 147 >17.9 white 77 227 147 >17.9 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 1.778 in the direction of the burst (Schlegel et al. 1998). =========== Draft Detection Circular ======== GRB 210217: Swift/UVOT Detection K. K. Simpson (PSU) and ***BA*** (***BA INSTITUTION***) report on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 210217 77 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 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 77 227 147 18.05 +/- 0.07 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 1.778 in the direction of the burst (Schlegel et al. 1998).