NOTE: uvot_fluxes_wget.pl vrs. 2020-11-03a fem at 210213d14h09m46s370728usUT NOTE: Source region spec. is: 277.67338 -6.75422 4" NOTE: Used archived XRT position of 277.67338 -6.75422 4.00 NOTE: position reference is GRB_Auto_Processing NOTE: Possible detection in uu at T+276.0 NOTE: Possible detection in wh at T+64.0 NOTE: Possible detection in bb at T+531.3 NOTE: Possible detection in vv at T+605.2 NOTE: Possible detection in w2 at T+1034.1 sum =========== Draft Upper Limit Circular ======== GRB 210213: 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 210213 64 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 64 214 147 >16.8 u_FC 276 526 246 >17.2 white 64 1374 373 >16.9 v 605 1772 136 >15.9 b 531 1698 117 >16.9 u 276 1673 363 >17.3 w1 654 1648 117 >18.4 w2 581 1575 117 >18.2 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 1.777 in the direction of the burst (Schlegel et al. 1998). =========== Draft Detection Circular ======== GRB 210213: 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 210213 64 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 64 214 147 16.92 +/- 0.03 v 605 625 20 15.94 +/- 0.14 b 531 551 20 16.97 +/- 0.13 u 276 526 246 17.43 +/- 0.07 w1 654 1648 117 >18.4 w2 581 1575 117 18.84 +/- 0.29 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 1.777 in the direction of the burst (Schlegel et al. 1998).