No CrossRef data available.
Article contents
CCD Astrometry with Wide-Field Astrographs
Published online by Cambridge University Press: 07 August 2017
Abstract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
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÷20th magnitudes when observing with the K. Zeiss wide-field astrographs.
- Type
- Ground-Based Optical Astrometry
- Information
- Copyright
- Copyright © Kluwer
References
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.Google Scholar
You have
Access