Optical parametric evaluation model for a broadband high resolution spectrograph at E-ELT (E-ELT HIRES)

M. Genoni; M. Riva; G. Pariani; M. Aliverti; M. Moschetti

doi:10.1117/12.2233978

8 August 2016 Optical parametric evaluation model for a broadband high resolution spectrograph at E-ELT (E-ELT HIRES)

M. Genoni; M. Riva; G. Pariani; M. Aliverti; M. Moschetti

Author Affiliations +

Proceedings Volume 9911, Modeling, Systems Engineering, and Project Management for Astronomy VI; 99112L (2016) https://doi.org/10.1117/12.2233978
Event: SPIE Astronomical Telescopes + Instrumentation, 2016, Edinburgh, United Kingdom

Abstract

We present the details of a paraxial parametric model of a high resolution spectrograph which can be used as a tool, characterized by good approximation and reliability, at a system engineering level. This model can be exploited to perform a preliminary evaluation of the different parameters as long as different possible architectures of high resolution spectrograph like the one under design for the E-ELT (for the moment called E-ELT HIRES in order to avoid wrong association with the HIRES spectrograph at Keck telescope). The detailed equations flow concerning the first order effects of all the spectrograph components is described; in addition a comparison with the data of a complete physical ESPRESSO spectrograph model is presented as a model proof.

Citation Download Citation

M. Genoni, M. Riva, G. Pariani, M. Aliverti, M. Moschetti, "Optical parametric evaluation model for a broadband high resolution spectrograph at E-ELT (E-ELT HIRES)", Proc. SPIE 9911, Modeling, Systems Engineering, and Project Management for Astronomy VI, 99112L (8 August 2016); doi: 10.1117/12.2233978; https://doi.org/10.1117/12.2233978

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