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Digital image centering. IIDigital image centering algorithms were compared in a test involving microdensitometer raster scans of a refractor parallax series consisting of 22 stars on 26 plates. The highest accuracy in determining stellar image positions was provided by an algorithm which involved fitting of a symmetric Gaussian curve and a flat background to the image marginal density distributions. Algorithms involving transmission marginals instead of density marginals were found to be less accurate. The repeatability and computational efficiency of the digital image centering technique were also studied.
Document ID
19780053550
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Auer, L. H.
(Yale Univ. Observatory New Haven, CT, United States)
Van Altena, W. F.
(Yale University Observatory, New Haven, Conn., United States)
Date Acquired
August 9, 2013
Publication Date
May 1, 1978
Publication Information
Publication: Astronomical Journal
Volume: 83
Subject Category
Astronomy
Accession Number
78A37459
Funding Number(s)
CONTRACT_GRANT: NSF GP-42008
CONTRACT_GRANT: NSF AST-76-81339
CONTRACT_GRANT: NSF GP-13771
CONTRACT_GRANT: NAS5-23288
CONTRACT_GRANT: NAS5-20841
CONTRACT_GRANT: NSF AST-75-13512
Distribution Limits
Public
Copyright
Other

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