MAORY: A Multi-conjugate Adaptive Optics RelaY for ELT
Paolo Ciliegi, Guido Agapito, Matteo Aliverti, Francesca Annibali, Carmelo Arcidiacono, Andrea Balestra, Andrea Baruffolo, Maria Bergomi, Andrea Bianco, Marco B… 展开作者
Paolo Ciliegi, Guido Agapito, Matteo Aliverti, Francesca Annibali, Carmelo Arcidiacono, Andrea Balestra, Andrea Baruffolo, Maria Bergomi, Andrea Bianco, Marco Bonaglia, Lorenzo Busoni, Michele Cantiello, Enrico Cascone, Gael Chauvin, Simonetta Chinellato, Vincenzo Cianniello, Jean Jacques Correira, Giuseppe Cosentino, Massimo Dall'Ora, Vincenzo De Caprio, Nicholas Devaney, Ivan Di Antonio, Amico Di Cianno, Ugo Di Giammatteo, Valentina D'Orazi, Gianluca Di Rico, Mauro Dolci, Sylvain Doutè, Cristian Eredia, Jacopo Farinato, Simone Esposito, Daniela Fantinel, Philippe Feautrier, Italo Foppiani, Enrico Giro, Laurance Gluck, Aaron Golden, Alexander Goncharov, Paolo Grani, Marco Gullieuszik, Pierre Haguenauer, Francois Hénault, Zoltan Hubert, Miska Le Louarn, Demetrio Magrin, Elisabetta Maiorano, Filippo Mannucci, Deborah Malone, Luca Marafatto, Estelle Moraux, Matteo Munari, Sylvan Oberti, Giorgio Pariani, Lorenzo Pettazzi, Cedric Plantet, Linda Podio, Elisa Portaluri, Alfio Puglisi, Roberto Ragazzoni, Andrew Rakich, Patrick Rebaut, Edoardo Redaelli, Matt Redman, Marco Riva, Sylvain Rochat, Gabriele Rodeghiero, Bernardo Salasnich, Paolo Saracco, Rosanna Sordo, Marilena Spavone, Marie-Helene Sztefek, Angelo Valentini, Eros Vanzella, Christophe Verinaud, Marco Xompero, Simone Zaggia
MAORY is the adaptive optics module for ELT providing two gravity invariant ports with the same optical quality for two different client instruments. It enable high angular resolution observations in the near infrared over a large field of view (~1 arcmin2 ) by real time compensation of the wavefront distortions due to atmospheric turbulence. Wavefront sensing is performed by laser and natural guide stars while the wavefront sensor compensation is performed by an adaptive deformable mirror in MAORY which works together with the telescope's adaptive and tip tilt mirrors M4 and M5 respectively.
MOSAIC at ELT: Design and First Prototyping of Novel Robotic Optical-Relay Positioners
Ecole Polytechnique Federale de Lausanne (EPFL)（洛桑联邦理工学院）；Haute Ecole du Paysage, d’Ingénierie et d’Architecture de Genève (HEPIA)（日内景观、工程与建筑高等学院）；Durham University（杜伦大学）；University of Sao Paulo（圣保罗大学）；University of Oxford（牛津大学）；STFC RALSpace, Rutherford Appleton Laboratory（英国科技设施委员会RAL空间部，鲁瑟福阿普尔顿实验室）；ASTRON（荷兰射电天文研究所）；Aix Marseille Université（艾克斯-马赛大学）；Univ Toulouse（图卢兹大学）；European Southern Observatory（欧洲南方天文台）；Observatoire de Paris（巴黎天文台）；PSL University（巴黎文理研究大学）；Isaac Newton Group of Telescopes（艾萨克·牛顿望远镜组）；STFC UK Astronomy Technology Centre, Royal Observatory（英国科技设施委员会英国天体物理技术中心，皇家天文台）
INAF Osservatorio Astrofisico di Arcetri（意大利国家天体物理研究所阿切尔西天文台）；ADaptive Optics National laboratory in Italy (ADONI)（意大利自适应光学国家实验室）；Herzberg Astronomy and Astrophysics, National Research Council of Canada（加拿大国家研究委员会赫茨伯格天文学与天体物理学研究所）
INAF Osservatorio Astrofisico di Arcetri（意大利国家天体物理研究所阿切特里天文台）；ADaptive Optics National laboratory in Italy (ADONI)（意大利自适应光学国家实验室）；Herzberg Astronomy and Astrophysics, National Research Council of Canada（加拿大国家研究委员会赫茨伯格天文学与天体物理学研究所）；INAF Osservatorio di Astrofisica e Scienza dello Spazio di Bologna (OAS)（意大利国家天体物理研究所博洛尼亚空间科学与天体物理观测站）；Alma Mater Studiorum - Università di Bologna（博洛尼亚大学）；INAF - Osservatorio Astronomico di Brera（意大利国家天体物理研究所布雷拉天文台）；INAF Osservatorio di Astrofisica e Scienza dello Spazio（意大利国家天体物理研究所空间科学与天体物理观测站）
Istituto Nazionale di Astrofisica (INAF)（意大利国家天体物理研究所）；Institut de Planétologie et d’Astrophysique de Grenoble (IPAG), CNRS, Univ. Grenoble Alpes（格勒诺布尔行星学与天体物理学研究所（CNRS，格勒诺布尔阿尔卑斯大学））
