So far 4 fields have been scheduled for observations.
Data are available and processed for 4 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.
32609 — 1.6 ks of cleaned data taken between 2012-10-25 14:28:08 and 2012-10-25 22:50:24
32610 — 1.8 ks of cleaned data taken between 2012-10-25 16:05:20 and 2012-10-25 22:37:24
32611 — 1.5 ks of cleaned data taken between 2012-10-25 17:50:54 and 2012-10-25 22:44:46
32612 — 1.6 ks of cleaned data taken between 2012-10-25 16:15:54 and 2012-10-25 22:53:00
Expected serendipitous sources: ~0.6 [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.