Laura Schreiber,1 Philippe Feautrier,2 Eric Stadler,2 Patrick Rabou,2 Jean-Jacques Correia,2 Laurence Glück,2 Sylvain Rochat,2 Laurent Jocou,2 Yves Magnard,2 Thibaut Moulin,2 Alain Delboulbé,2 Sylvain Douté,2 Gaël Chauvin,2 Estelle Moraux,2 Sylvain Oberti,3 Christophe Verinaud,3 Fausto Cortecchiahttps://orcid.org/0000-0001-5072-7791,1 Carmelo Arcidiacono,1 Emiliano Diolaiti,1 Paolo Ciliegi,1 Michele Bellazzini,1 Simone Esposito,4 Lorenzo Busoni,4 Roberto Ragazzoni5
1INAF - Osservatorio di Astrofisica e Scienza dello Spazio di Bologna (Italy) 2Univ. Joseph Fourer-Grenoble 1, CNRS-INSU, Institut de Planétologie et d’Astrophysique de Grenoble (France) 3European Southern Observatory (Germany) 4INAF - Osservatorio Astrofisico di Arcetri (Italy) 5INAF - Osservatorio Astronomico di Padova (Italy)
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MAORY will be the multi-adaptive optics module feeding the high resolution camera and spectrograph MICADO at the Extremely Large Telescope (ELT) first light. In order to ensure high and homogeneous image quality over the MICADO field of view and high sky coverage, the baseline is to operate wavefront sensing using six Sodium Laser Guide Stars. The Laser Guide Star Wavefront Sensor (LGS WFS) is the MAORY sub-system devoted to real-time measurement of the high order wavefront distortions. In this paper we describe the MAORY LGS WFS current design, including opto-mechanics, trade-offs and possible future improvements.
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