Some of them have collaborations or are entirely dedicated to Kuiper belt object observations. The same statements can be made for SNe search. Even if this SNe search is not ready yet, it is a clear extension of the movers search. All the data processing of fast movers has to take place very rapidly after the image acquisition, in order to be able to react quickly to any interesting object detection. CFHT is then the ideal place for running WISP, as the data flow is available in real time.
Many tasks have to be automated.
As the project is quite young, we are far from the most efficient data flow and processing, but each large field imaging run is an opportunity for progress in various areas, as you can see by browsing the pages of WISP on the WEB 1 .