The Theory of Optimizing Your Telescope to Detect the Faintest Stars

Details The Theory of Optimizing Your Telescope to Detect the Faintest Stars The Theory of Optimizing Your Telescope to Detect the Faintest Stars

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986javso..15..269z&link_type=abstract

The Journal of the American Association of Variable Star Observers, vol. 15, no. 2, p. 269-274

Physics

Scientific paper

The theory of optical imaging of point and extended sources is used to
develop formulae describing object-to-sky contrast ratios. Study of
these formulae will allow one to discover how to optimize an instrument
for a particular observing program.

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