So far 6 fields have been scheduled for observations.
Data are available and processed for 5 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.
20429 — 202 s of cleaned data taken between 2014-10-29 08:48:34 and 2014-10-29 10:18:55
20430 — 210 s of cleaned data taken between 2014-10-29 08:52:46 and 2014-10-29 10:14:40
20431 — 107 s of cleaned data taken between 2014-10-29 08:56:46 and 2014-10-29 09:00:05
20432 — 163 s of cleaned data taken between 2014-10-29 09:00:46 and 2014-10-29 10:09:28
20433 — 977 s of cleaned data taken between 2014-10-30 10:18:30 and 2014-10-30 10:34:48
Expected serendipitous sources: ~0.08 [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.