Some applications of signal-to-noise in photographic stellar photometry

Details Some applications of signal-to-noise in photographic stellar photometry Some applications of signal-to-noise in photographic stellar photometry

Apr 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984asph.conf..269g&link_type=abstract

In Royal Observatory Astron. Phot. 1984 p 269-277 (SEE N85-16102 07-35)

Astronomy and Astrophysics

Astronomy

1

Astronomical Photography, Signal To Noise Ratios, Stellar Spectrophotometry, Luminous Intensity, Photographic Emulsions, Photographic Plates, Stellar Magnitude

Scientific paper

The concept of output signal-to-noise is used to determine the limiting stellar magnitude, the signal-to-noise of stellar images, and the precision of the photometry of faint stars on a given plate taken by a 2-m telescope. Tests of the results show their reasonableness and underline the usefulness of the output signal-to-noise concept in astronomical photography.

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