Paper
1 November 1997 Using the Shack-Hartmann system for a complete analysis of optical telescopes
Rajiv K. Bhatia, Adriana Ciani
Author Affiliations +
Abstract
We have developed a SHack-Hartmann system, which has been extensively used to test various telescope around the world over the past 5 years. In this paper we describe the instrument and the software, and indicate how they have been used to measure the optical aberrations in terms of coma, spherical aberration etc. We also show how our system can be used to identify less obvious problems like telescope support errors and dome and mirror seeing.
© (1997) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Rajiv K. Bhatia and Adriana Ciani "Using the Shack-Hartmann system for a complete analysis of optical telescopes", Proc. SPIE 3134, Optical Manufacturing and Testing II, (1 November 1997); https://doi.org/10.1117/12.295155
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CITATIONS
Cited by 3 scholarly publications.
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KEYWORDS
Mirrors

Telescopes

Monochromatic aberrations

Wavefronts

Wavefront sensors

Charge-coupled devices

Optical telescopes

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