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The Design of Modern Meridian Circles for the Observation of Faint Objects
Published online by Cambridge University Press: 04 August 2017
Abstract
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Definitions of Instantaneous Instrumental Coordinates and Local Horizontal Coordinates of the photoelectric meridian circle of Tokyo Astronomical Observatory are given, and a method to determine the positions of stars by using a scanning double slits micrometer are presented. It is found that stars up to 12.2 mag are observable by making a composite photon intensity. Discussions on the application of observations of faint objects by meridian circles are presented.
- Type
- VI. Transit Circles and Astrolabes
- Information
- Symposium - International Astronomical Union , Volume 109: Astrometric Techniques , 1986 , pp. 449 - 458
- Copyright
- Copyright © Reidel 1986
References
Helmer, L., Fabricius, C., Einicke, O.H., and Thoburn, C., 1983, Astron. Astrophys. Suppl. Ser., 53, pp. 223.Google Scholar
Johnston, K.J., Spencer, J.H., Kaplan, G.H., Klepczynski, W.J., and McCarthy, D.D., 1980, Cele. Mech., 22, pp. 143.Google Scholar
Yoshizawa, M., and Yasuda, H., 1982, Ann. Tokyo Astron. Obs., Sec. Series, 18, pp. 205.Google Scholar
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