NOTE: uvot_fluxes_wget.pl vrs. 2018-01-16 fem at 180312d13h55m59s800846usUT NOTE: Source region spec. is: 275.0895 +7.1832 4" NOTE: Used archived XRT position of 275.08950 7.18320 4.00 NOTE: position reference is GCN_Notice NOTE: Possible detection in uu at T+1616.3 NOTE: Possible detection in wh at T+1837.8 sum NOTE: Possible detection in bb at T+6116.2 NOTE: Possible detection in w1 at T+1764.3 NOTE: Possible detection in vv at T+6731.9 NOTE: Possible detection in w2 at T+1863.1 sum NOTE: Possible detection in m2 at T+1911.9 sum =========== Draft Upper Limit Circular ======== GRB 180312: Swift/UVOT Upper Limits F. E. Marshall (NASA/GSFC) and ***BA*** (***BA INSTITUTION***) report on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 180312 1212 s after the BAT trigger (***Author*** et al., GCN Circ. ????). No optical afterglow consistent with the XRT position *** POSITION REFERENCE is GCN_Notice *** 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 1212 1362 147 >20.0 white 1212 7957 657 >20.8 v 1369 12340 1227 >18.1 b 1469 7751 510 >19.2 u 1444 7546 510 >18.3 w1 1419 13915 1163 >17.7 m2 1394 13245 1206 >17.8 w2 1518 8162 510 >17.8 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.23 in the direction of the burst (Schlegel et al. 1998). =========== Draft Detection Circular ======== GRB 180312: Swift/UVOT Detection F. E. Marshall (NASA/GSFC) and ***BA*** (***BA INSTITUTION***) report on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 180312 1212 s after the BAT trigger (***Author*** et al., GCN Circ. ????). A source consistent with the XRT position *** POSITION REFERENCE is GCN_Notice *** 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 6321 6521 197 20.14 +/- 0.20 v 11433 11733 295 17.93 +/- 0.12 b 6116 6316 197 19.06 +/- 0.15 u 5911 6111 197 18.28 +/- 0.12 w1 1419 2302 117 17.86 +/- 0.18 m2 1394 7136 321 18.20 +/- 0.16 w2 6527 6727 197 18.05 +/- 0.16 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.23 in the direction of the burst (Schlegel et al. 1998).