So far 9 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.
20607 — 258 s of cleaned data taken between 2016-05-09 10:55:10 and 2016-05-09 10:59:28
20608 — 250 s of cleaned data taken between 2016-05-09 11:00:11 and 2016-05-09 11:04:22
20609 — 258 s of cleaned data taken between 2016-05-09 11:05:09 and 2016-05-09 11:09:28
20610 — 275 s of cleaned data taken between 2016-05-09 11:10:04 and 2016-05-09 11:14:40
20611 — 255 s of cleaned data taken between 2016-05-09 11:15:09 and 2016-05-09 11:19:25
20612 — 230 s of cleaned data taken between 2016-05-09 11:19:59 and 2016-05-09 11:23:50
20613 — 155 s of cleaned data taken between 2016-05-09 11:24:38 and 2016-05-09 11:27:13
Probable afterglow details
A source was found which matches the afterglow criteria.
Expected serendipitous sources: ~0.00×10+0 [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: ~0.00×10+0 [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.