Conceptual opto-mechanical design of SHARP: a near-infrared multi-mode spectrograph conceived for the next-generation telescopes

The next generation of Extremely Large Telescopes (ELTs), with their wide apertures and advanced multi-conjugate adaptive optics (MCAO) systems, will provide unprecedented sharp and deep observations, even surpassing the capabilities of the James Webb Space Telescope. SHARP, a near-infrared (0.95 to 2.45 μm) spectrograph, is designed to optimally exploit the collecting area and angular resolution of these forthcoming ELTs and specifically optimized for the MCAO unit MORFEO at the ELT. SHARP includes two main units: NEXUS, a multi-object spectrograph, and VESPER, a multi-integral field unit. We outline the opto-mechanical design of SHARP based on the scientific requirements of the project. The optical design is engineered to meet project specifications, featuring a compact mechanical structure that minimizes the required cryogenic power while ensuring ease of access for maintenance and straightforward assembly procedures.

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Publication Details

Journal
Journal of Astronomical Telescopes Instruments and Systems
Published
2025-07-24
DOI
https://doi.org/10.1117/1.jatis.11.3.035002
Primary Topic
Astronomy and Astrophysical Research
Type
article
Field-Weighted Citation Impact
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article

Conceptual opto-mechanical design of SHARP: a near-infrared multi-mode spectrograph conceived for the next-generation telescopes

Vincenzo Cianniello, Ivan Di Antonio, Vincenzo De Caprio, P. Franzetti et al.
Journal of Astronomical Telescopes Instruments and Systems
Astronomy and Astrophysical Research
article

Conceptual opto-mechanical design of SHARP: a near-infrared multi-mode spectrograph conceived for the next-generation telescopes

Vincenzo Cianniello, Ivan Di Antonio, Vincenzo De Caprio, P. Franzetti, P. Saracco, Marcello Agostino Scalera, Bortolino Saggin, Davide Greggio, Elisa Portaluri, Carmelo Arcidiacono, E. Cascone, Christian Eredia, Ilaria Arosio, E. Molinari, P. Conconi, M. Fumana, Benedetta Di Francesco, Hossein Mahmoodzadeh, Diego Scaccabarozzi, Marco Riva, Gianluca Di Rico
article en

Abstract

The next generation of Extremely Large Telescopes (ELTs), with their wide apertures and advanced multi-conjugate adaptive optics (MCAO) systems, will provide unprecedented sharp and deep observations, even surpassing the capabilities of the James Webb Space Telescope. SHARP, a near-infrared (0.95 to 2.45 μm) spectrograph, is designed to optimally exploit the collecting area and angular resolution of these forthcoming ELTs and specifically optimized for the MCAO unit MORFEO at the ELT. SHARP includes two main units: NEXUS, a multi-object spectrograph, and VESPER, a multi-integral field unit. We outline the opto-mechanical design of SHARP based on the scientific requirements of the project. The optical design is engineered to meet project specifications, featuring a compact mechanical structure that minimizes the required cryogenic power while ensuring ease of access for maintenance and straightforward assembly procedures.

Journal of Astronomical Telescopes Instruments and SystemsVol. 11(03)
Astronomical Observatory of Capodimonte (IT), Brera Astronomical Observatory (IT), Istituto di Astrofisica Spaziale e Fisica Cosmica di Milano (IT), Collurania Teramo Observatory (IT), Osservatorio Astronomico di Padova (IT), National Institute for Astrophysics (IT), Politecnico di Milano (IT)
Openalex Percentile: Top 82%
Astronomy and Astrophysical Research
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