The transfer function, signal-to-noise ratio, and limiting magnitude in stellar speckle interferometry

Details The transfer function, signal-to-noise ratio, and limiting magnitude in stellar speckle interferometry The transfer function, signal-to-noise ratio, and limiting magnitude in stellar speckle interferometry

Dec 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974mnras.169..631d&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 169, Dec. 1974, p. 631-641.

Astronomy and Astrophysics

Astronomy

28

Interferometry, Signal To Noise Ratios, Speckle Patterns, Stellar Luminosity, Transfer Functions, Binary Stars, Diffraction Patterns, Fourier Transformation, Point Sources

Scientific paper

Abstract image available at:
http://adsabs.harvard.edu/abs/1974MNRAS.169..631D

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