TITLE: GCN GRB OBSERVATION REPORT NUMBER: 4107 SUBJECT: GRB 051016B: Swift/UVOT detection DATE: 05/10/17 13:45:59 GMT FROM: Alexander Blustin at MSSL-UCL A. J. Blustin (UCL-MSSL), A. Parsons (GSFC), S. T. Holland (GSFC), P. Meszaros, M. Chester (PSU), N. Gehrels (GSFC) on behalf of the Swift/UVOT team report: The Swift/UVOT began taking a settled exposure of the field of GRB 051016B 78 s after the trigger (Parsons et al. GCN 4103). A faint optical/UV source (not visible in the DSS) is detected in summed images at the position reported by Chen et al. (GCN 4105) at greater than 3 sigma in four of the UVOT filters; the magnitudes and upper limits are as follows: Filter T_range(sec) Exp(sec) Mag/3-sig upper limit V 78-29720 2418 20.5 (upper limit) B 445-28020 2748 22.0 +/- 0.5 U 391-35505 2507 20.9 +/- 0.3 UVW1 337-34740 2796 21.7 +/- 0.4 UVM2 283-33833 2798 21.0 (upper limit) UVW2 554-28928 2748 22.8 +/- 0.6 The detection in UVW2 would imply that the redshift of the source is less than ~1.3. There was a further uncatalogued nearby UV-only source at (J2000 08:48:27.7 +13:39:12.0), outside the XRT error circle, with the following magnitudes: Filter Mag UVW1 21.9 +/- 0.4 UVM2 22.3 +/- 0.4 UVW2 22.0 +/- 0.3 Further data will be required to tell whether either source is variable. _______________________________________________ Uvot_cal mailing list Uvot_cal@phoenix.astro.psu.edu https://phoenix.astro.psu.edu/mailman/listinfo/uvot_cal