Stellar speckle image reconstruction by the shift-and-add method

Details Stellar speckle image reconstruction by the shift-and-add method Stellar speckle image reconstruction by the shift-and-add method

May 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apopt..24.1403b&link_type=abstract

Applied Optics (ISSN 0003-6935), vol. 24, May 15, 1985, p. 1403-1405.

Physics

Optics

6

Astronomical Photography, Binary Stars, Image Processing, Image Reconstruction, Speckle Patterns, Cassegrain Optics, Imaging Techniques, Interferometry, Spectral Sensitivity

Scientific paper

In the simple shift-and-add method proposed by Bates and Cady (1980), the brightest point in each speckle image is shifted to the center of image space, and the translated image is added to all other speckle images that have been similarly processed. This method is presently used in the reconstruction of a binary star, Alpha Com, which was observed in wide bandwidth light.

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