Hostname: page-component-76fb5796d-45l2p Total loading time: 0 Render date: 2024-04-27T21:49:48.904Z Has data issue: false hasContentIssue false
  • English
  • Français

An Optical Design for an Antarctic 2 m Telescope with a Near IR Imager

Published online by Cambridge University Press:  05 March 2013

P. R. Gillingham
P. R. Gillingham*
Affiliation:
Anglo-Australian Observatory, PO Box 296, Epping, NSW 1710, Australia; pg@aaoepp.aoo.gov.au
Rights & Permissions [Opens in a new window]

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 study has been made of the optical performance to be expected from an Antarctic Ritchey Chrétien telescope with a 2 m diameter primary mirror imaging directly onto a detector array in the K and L infrared windows. Near diffraction limited performance is provided across a flat 30 arcmin diameter field by compensating the astigmatism and field curvature with a meniscus lens which also serves as the Dewar window. With baffling inside and Narcissus mirrors outside the Dewar, extraneous radiation can be kept to a low level.

Keywords

telescopesinfrared: generalinstrumentation: photometersmethods: observational
Type
Research Article
Information
Publications of the Astronomical Society of Australia , Volume 19 , Issue 3 , 2002 , pp. 301 - 305
Copyright
Copyright © Astronomical Society of Australia 2002

References

Ashley, M. C. B., et al. 1996, PASP, 721 CrossRefGoogle Scholar
Gascoigne, S. C. B. 1965, Obs, 85, 79 Google Scholar
Hidas, M. G., Burton, M. G., Chamberlain, M. A., & Storey, J. W. V. 2000, PASA, 17, 260 CrossRefGoogle Scholar
Nguyen, H. T., et al. 1996, PASP, 108, 718 CrossRefGoogle Scholar
Phillips, A., et al. 1999, ApJ, 527, 1009 CrossRefGoogle Scholar