16 - 21 June 2024
Yokohama, Japan
Conference 13099 > Paper 13099-57
Paper 13099-57

ANDES, the high resolution spectrograph for the ELT: RAM strategy during the preliminary design review

On demand | Presented live 17 June 2024

Abstract

RAM analysis is crucial for the success of any measurement campaign and must be implemented at the earliest design phase of building an astronomical instrument. ANDES (ArmazoNes high Dispersion Echelle Spectrograph) currently in phase B will be the high-resolution spectrograph for the ELT formerly known as ELT-HIRES. Its design in the extended version foresees four spectrographs fed by fibers and operating both in seeing and diffraction-limited (adaptive optics assisted) mode. Due to these properties strictly related to flexibility and modularity, a RAM approach focused on different scientific data requirements permits a high availability for the main data acquisition modes. To implement this process, the product tree, active elements, modularity, component duty cycles, and degraded modes were defined in the earlier phases. In this way, RAM requirements contribute to defining design. This process avoids missing the control of particular aspects like maintenance accessibility, cost of operations, and downtime due to maintenance. The paper presents the process and how it is implemented in the ANDES project, thereby suggesting a design solution for the instrument.

Presenter

INAF - Osservatorio Astronomico di Padova (Italy)
The speaker has been working for over twenty years in the design, development, integration, and validation of instruments and telescopes, such as the Italian Telescopio Nazionale Galileo (TNG), the SPHERE spectrograph for VLT, the Cherenkov telescopes MAGIC, LST, and SST for CTA. In this context, the speaker took responsibility for several fields such as Quality Assurance, System Engineering, and Verification and Validation. Currently, he is the Quality Assurance Manager for ANDES@ELT, he is in charge of the RAM program for MORFEO@ELT and he is part of the System Engineering team for the Verification and Validation of the Vera Rubin Telescope.
Application tracks: Astrophotonics
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Univ. degli Studi di Firenze (Italy)