Translator Disclaimer
Paper
8 August 2016 Optical parametric evaluation model for a broadband high resolution spectrograph at E-ELT (E-ELT HIRES)
Author Affiliations +
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.
© (2016) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
M. Genoni, M. Riva, G. Pariani, M. Aliverti, and 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 VII, 99112L (8 August 2016); https://doi.org/10.1117/12.2233978
PROCEEDINGS
9 PAGES


SHARE
Advertisement
Advertisement
RELATED CONTENT

The design of the WEAVE spectrograph
Proceedings of SPIE (July 24 2014)
The G-CLEF spectrograph optical design
Proceedings of SPIE (July 28 2014)
VIRUS W commissioning and first year results of a...
Proceedings of SPIE (September 24 2012)
The Endue Of Grating Spectrographs
Proceedings of SPIE (January 09 1984)
The design of the MOONS-VLT spectrometer
Proceedings of SPIE (September 24 2012)

Back to Top