Presented at the 3rd
AAVSO CCD Workshop, June 6, 1993
Abstract
CCDs have had a
revolutionary effect on large, mountain-top astronomy (40-to 160-inch
telescopes), and, more recently, on smaller, urban and suburban university
astronomy research (12- to 200-inch telescopes). This paper explores the
theoretical capabilities of a range of CCD cameras and sites and compares them
to actual results using 3- to 12-inch telescopes. The detection of stars to
16th and 21st magnitudes with these instruments with signal-to-noise ratios of
3 to 10 is documented. The conclusion is that amateur astronomers with 3-inch
telescopes and CCD cameras from suburban sites can make valuable contributions
to AAVSO programs.