Paper
26 September 1989 Wide Spectral Range F/2.3 Prime Focus Spherical Corrector For 3.5m Ritchey-Chretien Telescope
M. Magnani, S. Pieri, A. Romoli
Author Affiliations +
Proceedings Volume 1130, New Technologies for Astronomy; (1989) https://doi.org/10.1117/12.961507
Event: 1989 International Congress on Optical Science and Engineering, 1989, Paris, France
Abstract
This paper deals with the design of a three spherical lenses corrector, able to produce wide flat field at the prime focus with focus ratio F/2.2 - 3.5m of a R-C telescope. The system is corrected over a spectral range extending from 300nm to 1100 nm. The corrector has the following characteristics: reduced size of the optics; all spherical surfaces; resolution better than 1 arcsec within 30 arcmin flat field ; possibility to extend the field up to 1 degree with reduced resolution. The image quality of the corrector is shown by means of Spot Diagrams, Point Spread Function and Encircled Energy Function for different off - axis values and spectral ranges. The paper also includes an analysis of possible alignment errors performed by means of computed interferograms.
© (1989) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
M. Magnani, S. Pieri, and A. Romoli "Wide Spectral Range F/2.3 Prime Focus Spherical Corrector For 3.5m Ritchey-Chretien Telescope", Proc. SPIE 1130, New Technologies for Astronomy, (26 September 1989); https://doi.org/10.1117/12.961507
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KEYWORDS
Astronomy

Error analysis

Spherical lenses

Telescopes

Image quality

Interferometry

Computer simulations

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