Shack-Hartmann analysis of the 3.5-m primary mirror of the Galileo telescope

Rajiv K. Bhatia; Adriana Ciani; Piero Rafanelli

doi:10.1117/12.167955

1 February 1994 Shack-Hartmann analysis of the 3.5-m primary mirror of the Galileo telescope

Rajiv K. Bhatia, Adriana Ciani, Piero Rafanelli

Author Affiliations +

Proceedings Volume 1994, Advanced Optical Manufacturing and Testing IV; (1994) https://doi.org/10.1117/12.167955
Event: SPIE's 1993 International Symposium on Optics, Imaging, and Instrumentation, 1993, San Diego, CA, United States

Abstract

We present here the results obtained from a Shack-Hartmann analysis of the optical quality of the primary mirror of the Telescopio Nazionale Galileo. We compare our results with those obtained from Zeiss from interferometry, finding a good agreement. The 80% encircled energy is found to be within a diameter of 0.14 arc sec. Calculations of the MTF, EE and PSF and comparison with diffraction theory show a remarkable agreement, indicating that the mirror quality is very near the diffraction limit.

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Rajiv K. Bhatia, Adriana Ciani, and Piero Rafanelli "Shack-Hartmann analysis of the 3.5-m primary mirror of the Galileo telescope", Proc. SPIE 1994, Advanced Optical Manufacturing and Testing IV, (1 February 1994); https://doi.org/10.1117/12.167955

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