Presented at the 84th
AAVSO Annual Meeting, October 28, 1995; revised April 5, 1996
A system for performing CCD
photometry employing an ST6 attached to a 2-inch f/3.6 lens is described. The
system's advantages and problem areas are discussed, its performance is
described based on over 4500 CCD images of eclipsing binary stars, and its
prospects for photometry on more than one variable per image are explored.