Published March 2012
| Version Published
Journal Article
Open
An Optical Pointing Telescope for Radio Astronomy
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.Attached Files
Published - Assawaworrarit2012p17891Publ_Astron_Soc_Pac.pdf
Files
Assawaworrarit2012p17891Publ_Astron_Soc_Pac.pdf
Additional details
Identifiers
- Eprint ID
- 30405
- Resolver ID
- CaltechAUTHORS:20120501-073000156
Related works
- Describes
- http://www.jstor.org/stable/10.1086/664969 (URL)
Funding
- John B. and Nelly Kilroy Foundation
Dates
- Created
-
2012-05-01Created from EPrint's datestamp field
- Updated
-
2021-11-09Created from EPrint's last_modified field