NOTE: A UVOT position was reported in uvotdetect NOTE: Possible detection in wh at T+89110.6 =========== Draft Upper Limit Circular ======== GRB 130702A: Swift/UVOT Upper Limits B. Porterfield (PSU) and P. D'Avanzo (***BA INSTITUTION***) report on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 130702A 89111 s after the BAT trigger (***Author*** et al., GCN Circ. ????). No optical afterglow consistent with the uvot position *** POSITION REFERENCE is uvotdetect *** 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 89111 89229 117 >18.2 white 89111 100760 4773 >18.4 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.04 in the direction of the burst (Schlegel et al. 1998). =========== Draft Detection Circular ======== GRB 130702A: Swift/UVOT Detection B. Porterfield (PSU) and P. D'Avanzo (***BA INSTITUTION***) report on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 130702A 89111 s after the BAT trigger (***Author*** et al., GCN Circ. ????). A source consistent with the uvot position *** POSITION REFERENCE is uvotdetect *** is detected in the initial UVOT exposures. The preliminary UVOT position is: RA (J2000) = 14:29:14.77 = 217.31155 (deg.) Dec (J2000) = +15:46:26.5 = 15.77403 (deg.) with an estimated uncertainty of 0.50 arc sec. (radius, 90% confidence). 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 89111 89229 117 18.34 +/- 0.05 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.04 in the direction of the burst (Schlegel et al. 1998).