NOTE: uvot_fluxes_wget.pl vrs. 2018-01-16 fem at 180824d12h46m52s715669usUT NOTE: Source region spec. is: 210.35583 14.89244 4" NOTE: Used archived XRT position of 210.35583 14.89244 4.00 NOTE: position reference is GCN_Circulars-23170 NOTE: Possible detection in vv at T+4686.3 =========== Draft Upper Limit Circular ======== GRB 180823A: Swift/UVOT Upper Limits S. Sebzda (PSU) and B. Sbarufatti (PSU) report on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 180823A 381 s after the BAT trigger (Sbarufatti et al., GCN Circ. 23169). No optical afterglow consistent with the XRT position (Goad et al. GCN Circ. 23170) 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 initial exposures are: Filter T_start(s) T_stop(s) Exp(s) Mag white 381 4476 380 >20.9 v 4686 10356 927 >19.2 b 4071 4271 197 >19.7 u 3866 4066 197 >19.8 m2 10361 10803 435 >19.8 w2 4482 4681 197 >20.0 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.02 in the direction of the burst (Schlegel et al. 1998). =========== Draft Detection Circular ======== GRB 180823A: Swift/UVOT Detection S. Sebzda (PSU) and B. Sbarufatti (PSU) report on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 180823A 381 s after the BAT trigger (Sbarufatti et al., GCN Circ. 23169). A source consistent with the XRT position (Goad et al. GCN Circ. 23170) 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 381 4476 380 >20.9 v 4686 4729 42 18.05 +/- 0.32 b 4071 4271 197 >19.7 u 3866 4066 197 >19.8 m2 10361 10803 435 >19.8 w2 4482 4681 197 >20.0 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.02 in the direction of the burst (Schlegel et al. 1998).