Overview of current status of the UVEX survey
This is the status of UVEX as of September 30, 2012. A total fraction of 76% of the fields has been observed at least once. As can be seen a strong concentration towards the early Plane is visible, which is due to a larger observational coverage during the La Palma summer months.
From the imaging performed in the first two years we have constructed a seeing histogram in the four filters used, shown below
Here is the status per field (Sep 2012), organized
by Constellation along the Galactic Plane (as in the figure above), and
by year of IPHAS observation of the given field.