The motivation behind the Wise Observatory fast photometry project
is to use a non-frame-transfer CCD for fast photometry of
The system takes images and performs aperture photometry
with cycle of (>3) seconds and integration times
of (=cycle - 3 sec).
On the Wise observatory 1m telescope 6 sec. exposure
is needed to obtain S/N of about 20 for 15 mag star.
Detailed description + Software
Download the paper (PostScript)
The WET project
Constructed: November 1998, Eran Ofek