Published March 2012 | Version Published
Journal Article Open

An Optical Pointing Telescope for Radio Astronomy

  • 1. ROR icon California Institute of Technology

Abstract

Design details are given for a stable optical pointing telescope for radio astronomy. The telescope is a 100 mm f/15 refractor with the objective glued to a ring of three blade flexures, an insulated and vented Invar tube mounted on flexures, and an axially symmetric camera mount. For a pair of identical telescopes, the rms differential pointing stability is 0.1" hr^(-1) over 2 hr, 0.05" day^(-1) over 3 days, 0.03" K^(-1), and 0.1″ after a 90° change in elevation.

Additional Information

© 2012 The Astronomical Society of the Pacific. Received 2012 January 9; accepted 2012 January 31; published 2012 February 21. This work was supported by the John B. and Nelly Kilroy Foundation.

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Identifiers

Eprint ID
30405
Resolver ID
CaltechAUTHORS:20120501-073000156

Related works

Funding

John B. and Nelly Kilroy Foundation

Dates

Created
2012-05-01
Created from EPrint's datestamp field
Updated
2021-11-09
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