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.
20359 — 636 s of cleaned data taken between 2014-02-21 10:14:34 and 2014-02-21 12:32:17
20360 — 674 s of cleaned data taken between 2014-02-21 10:20:52 and 2014-02-21 12:27:10
20361 — 707 s of cleaned data taken between 2014-02-21 10:27:02 and 2014-02-21 12:21:18
20362 — 684 s of cleaned data taken between 2014-02-21 10:33:11 and 2014-02-21 12:14:54
20363 — 681 s of cleaned data taken between 2014-02-21 10:39:18 and 2014-02-21 12:08:50
20364 — 684 s of cleaned data taken between 2014-02-21 10:45:20 and 2014-02-21 11:56:31
20365 — 641 s of cleaned data taken between 2014-02-21 10:51:20 and 2014-02-21 12:02:40
Probable afterglow details
A source was found which matches the afterglow criteria.
Expected serendipitous sources: ~0.03 [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: ~0.03 [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.