ANDES, the high-resolution spectrograph for the ELT: design of the adaptive optics system

Enrico Pinna; Chiara Selmi; Anne-Laure Cheffot; Nicolò Azzaroli; Edoardo Redaelli; Jean-François Sauvage; Veronica Baldini; Jennifer Dunn; Giorgio Calderone; Guido Agapito; Adrien Simonnin; Pierre Jouve; Jean-Pierre Véran; Nicolas Blind; Matteo Aliverti; André Beaudoin; Philippe Berio; Marco Bonaglia; Runa Briguglio; Luca Carbonaro; Gaël Chauvin; Andrea Chiavassa; Bruno Chazelas; Roberto Cirami; Igor Coretti; Paolo Di Marcantonio; Simone Doniselli; Thierry Fusco; Kathryn Jackson; Alessandro Marconi; Patrice Martinez; Mamadou N'Diaye; Benoit Neichel; Marco Riva; Alain Spang; Esther Soria Hernandez; Jonathan Stocks; Antonio Sulich; Alessio Zanutta

doi:10.1117/12.3018434

27 August 2024 ANDES, the high-resolution spectrograph for the ELT: design of the adaptive optics system

Enrico Pinna, Chiara Selmi, Anne-Laure Cheffot, Nicolò Azzaroli, Edoardo Redaelli, Jean-François Sauvage, Veronica Baldini, Jennifer Dunn, Giorgio Calderone, Guido Agapito, Adrien Simonnin, Pierre Jouve, Jean-Pierre Véran, Nicolas Blind, Matteo Aliverti, André Beaudoin, Philippe Berio, Marco Bonaglia, Runa Briguglio, Luca Carbonaro, Gaël Chauvin, Andrea Chiavassa, Bruno Chazelas, Roberto Cirami, Igor Coretti, Paolo Di Marcantonio, Simone Doniselli, Thierry Fusco, Kathryn Jackson, Alessandro Marconi, Patrice Martinez, Mamadou N'Diaye, Benoit Neichel, Marco Riva, Alain Spang, Esther Soria Hernandez, Jonathan Stocks, Antonio Sulich, Alessio Zanutta

Author Affiliations +

Proceedings Volume 13097, Adaptive Optics Systems IX; 130974W (2024) https://doi.org/10.1117/12.3018434
Event: SPIE Astronomical Telescopes + Instrumentation, 2024, Yokohama, Japan

Conference Poster

Abstract

ANDES,the high resolution spectrograph for the ELT, will work both in seeing limited mode and with Adaptive Optics (AO) correction. ANDES-SCAO is a single conjugated AO system working with natural guide stars, feeding the IFU coupled to the YJH spectrograph. The main science goal of the ANDES AO mode is the characterization of the exo-planet atmosphere in reflected light. Hence, the driving technical requirement for the AO system is the PSF contrast. The level of achieved contrast determines the number of exo-planets on which the instrument will be able to detect bio-signatures. The key challenge for the achievement of high contrast is the control of M4 petalling. Here, we present the current status of the ANDES-SCAO design, approaching the ANDES preliminary design review scheduled in fall 2024.

(2024) Published by SPIE. Downloading of the abstract is permitted for personal use only.

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Enrico Pinna, Chiara Selmi, Anne-Laure Cheffot, Nicolò Azzaroli, Edoardo Redaelli, Jean-François Sauvage, Veronica Baldini, Jennifer Dunn, Giorgio Calderone, Guido Agapito, Adrien Simonnin, Pierre Jouve, Jean-Pierre Véran, Nicolas Blind, Matteo Aliverti, André Beaudoin, Philippe Berio, Marco Bonaglia, Runa Briguglio, Luca Carbonaro, Gaël Chauvin, Andrea Chiavassa, Bruno Chazelas, Roberto Cirami, Igor Coretti, Paolo Di Marcantonio, Simone Doniselli, Thierry Fusco, Kathryn Jackson, Alessandro Marconi, Patrice Martinez, Mamadou N'Diaye, Benoit Neichel, Marco Riva, Alain Spang, Esther Soria Hernandez, Jonathan Stocks, Antonio Sulich, and Alessio Zanutta "ANDES, the high-resolution spectrograph for the ELT: design of the adaptive optics system", Proc. SPIE 13097, Adaptive Optics Systems IX, 130974W (27 August 2024); https://doi.org/10.1117/12.3018434

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