So far 8 fields have been scheduled for observations.
Data are available and processed for 8 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.
20196 — 694 s of cleaned data taken between 2012-01-10 15:08:50 and 2012-01-10 17:07:50
20197 — 962 s of cleaned data taken between 2012-01-10 15:16:02 and 2012-01-10 17:02:24
20198 — 970 s of cleaned data taken between 2012-01-10 15:23:04 and 2012-01-10 16:41:36
20199 — 566 s of cleaned data taken between 2012-01-10 16:42:34 and 2012-01-10 16:52:00
20201 — 630 s of cleaned data taken between 2012-01-10 21:26:40 and 2012-01-10 23:17:55
20202 — 937 s of cleaned data taken between 2012-01-10 21:31:58 and 2012-01-10 23:24:52
20203 — 957 s of cleaned data taken between 2012-01-10 21:41:57 and 2012-01-10 23:03:38
20204 — 768 s of cleaned data taken between 2012-01-10 21:51:51 and 2012-01-10 23:10:42
Expected serendipitous sources: ~1.3 [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.