So far 8 fields have been scheduled for observations.
Data are available and processed for 7 of these.
The list gives the exposure time used in source detection. If any individual sources
were selected for follow-up observations, the source detection is not repeated for the follow up
observations and the table below is not updated.
20456 — 912 s of cleaned data taken between 2014-12-29 14:50:11 and 2014-12-29 18:31:16
20457 — 955 s of cleaned data taken between 2014-12-29 14:56:40 and 2014-12-29 18:35:43
20458 — 955 s of cleaned data taken between 2014-12-29 15:03:12 and 2014-12-29 18:26:46
20459 — 937 s of cleaned data taken between 2014-12-29 15:09:38 and 2014-12-29 18:22:05
20460 — 942 s of cleaned data taken between 2014-12-29 15:15:32 and 2014-12-29 18:17:19
20461 — 925 s of cleaned data taken between 2014-12-29 15:21:23 and 2014-12-29 18:12:10
20462 — 937 s of cleaned data taken between 2014-12-29 15:26:56 and 2014-12-29 18:07:21
Probable afterglow details
A source was found which matches the afterglow criteria.
Expected serendipitous sources: ~0.2 [What is this?]
1 Radius, 90% confidence. 2 Indicates how likely the source is to be real. See the 1SXPS documentation. * The position was enhanced using astrometry derived from the Swift UVOT. † The position was astrometrically corrected using the XRT sources and the 2MASS catalogue.
Expected serendipitous sources: ~0.2 [What is this?]
1 Radius, 90% confidence. 2 Indicates how likely the source is to be real. See the 1SXPS documentation. * The position was enhanced using astrometry derived from the Swift UVOT. † The position was astrometrically corrected using the XRT sources and the 2MASS catalogue.