Method of determining the transfer functions of photo-optical systems under natural conditions

Details Method of determining the transfer functions of photo-optical systems under natural conditions Method of determining the transfer functions of photo-optical systems under natural conditions

Mar 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976opmep..43...15z&link_type=abstract

(Optiko-Mekhanicheskaia Promyshlennost', vol. 43, Mar. 1976, p. 15-18.) Soviet Journal of Optical Technology, vol. 43, Mar. 1976

Astronomy and Astrophysics

Astrophysics

Astronomical Photometry, Optical Transfer Function, Telescopes, Cinetheodolites, Fourier Transformation, Luminous Intensity, Modulation Transfer Function, Point Sources, Spectral Line Width

Scientific paper

An astrophotometric method of determining the transfer functions of photo-optical systems under natural conditions is discussed. The method is based on an analysis of the spread function of an infinitely narrow luminous line, the image of which is obtained through the exposure of a point light source - a star - that is moving because of the rotation of the earth with respect to the stationary instrument. The results of a determination of the transfer function of a high-speed cinetelescope are presented.

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