You will find hereafter some information on the program I started here as my own research activity done on the time left by my  duties as resident astronomer at CFHT.  Part of that program is made in collaboration with DAO (D. Balam) and University of Victoria  (Chris Aikman)

It is made in addition to WISP (Wide field Imaging Symbiotic Program), using Discretionnary and Allocated Time on two different instruments,  CFH12K at the Prime Focus, and MOS in imaging mode at the Cassegrain focus. UH8K has also been used at the beginning of the program