1. MAORY: A Multi-conjugate Adaptive Optics RelaY for ELT
- Author
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Ciliegi, Paolo, Agapito, Guido, Aliverti, Matteo, Annibali, Francesca, Arcidiacono, Carmelo, Balestra, Andrea, Baruffolo, Andrea, Bergomi, Maria, Bianco, Andrea, Bonaglia, Marco, Busoni, Lorenzo, Cantiello, Michele, Cascone, Enrico, Chauvin, Gael, Chinellato, Simonetta, Cianniello, Vincenzo, Correira, Jean Jacques, Cosentino, Giuseppe, Dall'Ora, Massimo, De Caprio, Vincenzo, Devaney, Nicholas, Di Antonio, Ivan, Di Cianno, Amico, Di Giammatteo, Ugo, D'Orazi, Valentina, Di Rico, Gianluca, Dolci, Mauro, Doutè, Sylvain, Eredia, Cristian, Farinato, Jacopo, Esposito, Simone, Fantinel, Daniela, Feautrier, Philippe, Foppiani, Italo, Giro, Enrico, Gluck, Laurance, Golden, Aaron, Goncharov, Alexander, Grani, Paolo, Gullieuszik, Marco, Haguenauer, Pierre, Hénault, Francois, Hubert, Zoltan, Louarn, Miska Le, Magrin, Demetrio, Maiorano, Elisabetta, Mannucci, Filippo, Malone, Deborah, Marafatto, Luca, Moraux, Estelle, Munari, Matteo, Oberti, Sylvan, Pariani, Giorgio, Pettazzi, Lorenzo, Plantet, Cedric, Podio, Linda, Portaluri, Elisa, Puglisi, Alfio, Ragazzoni, Roberto, Rakich, Andrew, Rebaut, Patrick, Redaelli, Edoardo, Redman, Matt, Riva, Marco, Rochat, Sylvain, Rodeghiero, Gabriele, Salasnich, Bernardo, Saracco, Paolo, Sordo, Rosanna, Spavone, Marilena, Sztefek, Marie-Helene, Valentini, Angelo, Vanzella, Eros, Verinaud, Christophe, Xompero, Marco, and Zaggia, Simone
- Subjects
Astrophysics::Instrumentation and Methods for Astrophysics ,FOS: Physical sciences ,Physics::Optics ,Astrophysics - Instrumentation and Methods for Astrophysics ,Instrumentation and Methods for Astrophysics (astro-ph.IM) - Abstract
The Multi-conjugate Adaptive Optics RelaY (MAORY) is the adaptive optics (AO) module for the Extremely Large Telescope (ELT) that will provide two gravity-invariant ports with the same optical quality for two different client instruments. It will enable high-angular-resolution observations in the near-infrared over a large field of view (~ 1 arcminute2) by real-time compensation of the wavefront distortions caused by atmospheric turbulence. Wavefront sensing is performed using laser and natural guide stars while the wavefront sensor compensation is performed by an adaptive deformable mirror (DM) in MAORY which works together with the telescope’s adaptive and tip-tilt mirrors M4 and M5 respectively., Published in The Messenger vol. 182, pp. 13-16, March 2021.
- Published
- 2021
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