Algorithm for astronomical, extended source, signal-to-noise radio calculations

Details Algorithm for astronomical, extended source, signal-to-noise radio calculations Algorithm for astronomical, extended source, signal-to-noise radio calculations

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984aaes.book.....j&link_type=abstract

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Astronomy and Astrophysics

Astronomy

Algorithms, Computer Programs, Hubble Space Telescope, Nonpoint Sources, Signal To Noise Ratios, Spaceborne Astronomy, Background Radiation, Black Body Radiation, Cameras, Charge Coupled Devices

Scientific paper

An algorithm was developed to simulate the expected signal-to-noise ratio as a function of observation time in the charge coupled device detector plane of an optical telescope located outside the Earth's atmosphere for an extended, uniform astronomical source embedded in a uniform cosmic background. By choosing the appropriate input values, the expected extended source signal-to-noise ratios can be computed for the Hubble Space Telescope using the Wide Field/Planetary Camera science instrument.

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