Hostname: page-component-7479d7b7d-t6hkb Total loading time: 0 Render date: 2024-07-16T03:11:31.475Z Has data issue: false hasContentIssue false

Design Characteristics of the 1.56 m Astrometric Telescope and its Usage in Astrometry

Published online by Cambridge University Press:  04 August 2017

Wan Lai
Affiliation:
Shanghai Observatory, Academia Sinica
Zhu Neng-Hong
Affiliation:
Shanghai Observatory, Academia Sinica
Wang Lan-Juan
Affiliation:
Shanghai Observatory, Academia Sinica
Yang Zheng-Hua
Affiliation:
Shanghai Observatory, Academia Sinica
Zheng Yi-Jin
Affiliation:
Shanghai Observatory, Academia Sinica

Extract

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.

The 1.56m astrometric telescope (Fig. 1) is designed mainly for determining trigonometric parallaxes of faint stars.

In order to keep the design as simple as possible, the telescope has only a Ritchey-Chretien focus and will accomodate plates 200 × 200 mm. We also plan to design several pieces of auxiliary equipment such as a medium dispersion grating spectrograph, a photometer, a reducing camera, and an electrographic camera, all of which are in the second stage of engineering. The whole project consists of four parts.

Type
III. Photographic Astrometry
Copyright
Copyright © Reidel 1986