Fourier deconvolution of electronographic images

Details Fourier deconvolution of electronographic images Fourier deconvolution of electronographic images

Jun 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979a%26a....76...46h&link_type=abstract

Astronomy and Astrophysics, vol. 76, no. 1, June 1979, p. 46-49.

Astronomy and Astrophysics

Astronomy

1

Astronomical Photography, Binary Stars, Electronography, Fourier Transformation, Image Processing, Radio Sources (Astronomy), Stellar Magnitude

Scientific paper

The Fourier deconvolution process is discussed with reference to electronographic images. A technique is described for measuring the separation, position angle, and magnitude difference of binary star images and for investigating fine optical structure in galaxy images. The method is used to measure the binary stars HR 5234, HR 5697, HR 5851/2, HR 6236, and H 4707, as well as to analyze the optical-image structure of Cygnus A.

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