Abstract
A principle of a CCD-Tracking System for wide-field astrographs is proposed. This system can be used for precise relative positioning of fixed and moving, bright and very faint optical objects with respect to reference stars. Estimates of the positioning accuracy are given for objects of the \( 10 \div 20th \) magnitudes when observing with the K. Zeiss wide-field astrographs.
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Gubanov, V., Kumkova, I. and Malakhov, E. (1990), “Precision estimate of positional CCD observations’, Kinematics and Physics of Celestial Bodies, Allerton Press, New York (English translation), 6,No.2, 83–90
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© 1993 Springer Science+Business Media Dordrecht
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Gubanov, V.S., Shornikov, O.E. (1993). CCD Astrometry with Wide-Field Astrographs. In: Mueller, I.I., Kołaczek, B. (eds) Developments in Astrometry and Their Impact on Astrophysics and Geodynamics. International Astronomical Union / Union Astronomique Internationale, vol 156. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-1711-1_22
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DOI: https://doi.org/10.1007/978-94-011-1711-1_22
Publisher Name: Springer, Dordrecht
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