Hostname: page-component-586b7cd67f-2plfb Total loading time: 0 Render date: 2024-11-28T23:14:11.083Z Has data issue: false hasContentIssue false
  • English
  • Français

CCD Astrometry with Wide-Field Astrographs

Published online by Cambridge University Press:  07 August 2017

V. S. Gubanov  and
O. E. Shornikov
V. S. Gubanov
Affiliation:
Institute of Applied Astronomy 8, Zhdanovskaya st., St.-Petersburg 197042, Russia
O. E. Shornikov
Affiliation:
Institute of Applied Astronomy 8, Zhdanovskaya st., St.-Petersburg 197042, Russia

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
Symposium - International Astronomical Union , Volume 156: Developments in Astrometry and their Impacts on Astrophysics , 1993 , pp. 125 - 127
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