NOTE: A UVOT position was reported in GCN_Circulars-xxxxx NOTE: Possible detection in wh at T+33589.9 =========== Draft Upper Limit Circular ======== GRB 150523A: 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 150523A 32968 s after the LAT trigger (***Author*** et al., GCN Circ. ????). No optical afterglow consistent with the XRT position (Beardmore et al. GCN Circ. 17866) 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 33590 39627 1150 >21.2 v 34212 40619 1433 >20.5 u 32968 44748 2077 >20.5 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.30 in the direction of the burst (Schlegel et al. 1998). =========== Draft Detection Circular ======== GRB 150523A: 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 150523A 32968 s after the LAT trigger (***Author*** et al., GCN Circ. ????). A source consistent with the XRT position (Beardmore et al. GCN Circ. 17866) 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 33590 39627 1150 21.83 +/- 0.24 v 34212 40619 1433 >20.5 u 32968 44748 2077 >20.5 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.30 in the direction of the burst (Schlegel et al. 1998).