ANDES, the high resolution spectrograph for the ELT: evolution of the fiber-link subsystem after the system architecture review

A. Brucalassi; . Tozzi; E. Oliva; J. A. Araiza-Durán; D. Ferruzzi; D. Savio; P. Di Marcantonio; A. Marconi; G. Murray; N. Piskunov; E. Stempels; A. Zanutta

doi:10.1117/12.3018950

18 July 2024 ANDES, the high resolution spectrograph for the ELT: evolution of the fiber-link subsystem after the system architecture review

A. Brucalassi, . Tozzi, E. Oliva, J. A. Araiza-Durán, D. Ferruzzi, D. Savio, P. Di Marcantonio, A. Marconi, G. Murray, N. Piskunov, E. Stempels, A. Zanutta

Author Affiliations +

Proceedings Volume 13096, Ground-based and Airborne Instrumentation for Astronomy X; 130964I (2024) https://doi.org/10.1117/12.3018950
Event: SPIE Astronomical Telescopes + Instrumentation, 2024, Yokohama, Japan

Conference Poster

Abstract

With this work we summarise the design evolution and challenges of the Fiber-Link module for ANDES (ArmazoNes high Dispersion Echelle Spectrograph), the high resolution spectrograph for ESO ELT. The instrument just passed the System Architecture Review of Phase-B1. The Fiber-Link subsystem carries and redistributes the light from the telescope to the spectrometers via several selectable optical paths. The general updated layout for the Fiber-Link module is presented giving element characteristics and obtained performances. First results from laboratory test and prototype activities are also shown. Moreover, we include the reasoning for selected solutions and explaining how requirements are met. Finally, we summarise the compliance against the science top-level requirements and the issues to address moving forward.

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A. Brucalassi, . Tozzi, E. Oliva, J. A. Araiza-Durán, D. Ferruzzi, D. Savio, P. Di Marcantonio, A. Marconi, G. Murray, N. Piskunov, E. Stempels, and A. Zanutta "ANDES, the high resolution spectrograph for the ELT: evolution of the fiber-link subsystem after the system architecture review", Proc. SPIE 13096, Ground-based and Airborne Instrumentation for Astronomy X, 130964I (18 July 2024); https://doi.org/10.1117/12.3018950

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