Poster + Paper
25 August 2022 Modeling wide-field telescopes in presence of misalignments: an application to the Vera C. Rubin Observatory
Author Affiliations +
Conference Poster
Abstract
An accurate alignment of the optical surfaces of a telescope is essential to guarantee an optimal image quality since even small displacements introduce aberrations increasing towards the edges of the field. This effect is especially detrimental in wide-field imagers. This work proposes the derivation of a fully analytical model of the wavefront error as a function of the most likely system misalignments. An accurate response of the telescope under a predefined set of misaligned conditions is obtained through simulations in Zemax OpticStudio. The resulting data is combined through an integrated modeling approach, obtaining a map of the aberrations as a function of a vector of perturbations applied to the optical system. The analytical wavefront error allows for a quick and accurate assessment of the theoretical PSF across the entire image field. As a case study, the example of the Rubin Observatory is adopted, featuring an 8.4m primary mirror and a large field of view.
© (2022) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Salvatore Savarese, Pietro Schipani, Giuliana Fiorentino, Laura Schreiber, Giacomo Basile, Giulio Capasso, Mirko Colapietro, Sergio D'Orsi, Laurent Marty, and Francesco Perrotta "Modeling wide-field telescopes in presence of misalignments: an application to the Vera C. Rubin Observatory", Proc. SPIE 12187, Modeling, Systems Engineering, and Project Management for Astronomy X, 1218719 (25 August 2022); https://doi.org/10.1117/12.2630248
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KEYWORDS
Telescopes

Wavefronts

Point spread functions

Data modeling

Error analysis

Zemax

Active optics

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