Marco Bonaglia,1 Guido Agapito,1 Matteo Alivertihttps://orcid.org/0000-0002-2525-3202,2 Nicolò Azzarolihttps://orcid.org/0000-0002-7270-7860,1 Runa Briguglio,1 Lorenzo Busoni,1 Giulio Capasso,3 Luca Carbonaro,1 Mirko Colapietro,3 Ciro Del Vecchiohttps://orcid.org/0000-0001-6486-3903,1 Sergio D'Orsi,3 Simone Doniselli,2 Paolo Grani,1 Davide Greggio,4 Tommaso Lapucci,1 Cédric Plantet,1 Enrico Pinna,1 Alfio Puglisi,1 Fabio Rossi,1 Salvatore Savarese,3 Pietro Schipani,3 Chiara Selmi,1 Valentina Viotto,4 François Rigaut5
1INAF, Osservatorio Astrofisico di Arcetri (Italy) 2INAF, Osservatorio Astronomico di Brera (Italy) 3INAF, Osservatorio Astronomico di Capodimonte (Italy) 4INAF, Osservatorio Astronomico di Padova (Italy) 5The Australian National Univ. (Australia)
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The paper describes the design of the NGS WFS sub-module of MAVIS, an instrument for the VLT UT4 that aims to provide diffraction limited imaging and spectroscopy at visible wavelengths. In this framework the NGS WFS provides means for the tomographic measurement of the lower-orders of the atmospheric turbulence allowing MAVIS to reach the required performances in terms of sky coverage and resolution. We present the optical design and performance of the NGS WFS probes and acquisition camera, the actuators embedded in the subsystem and their control hardware. Finally, we show the mechanical arrangement of the submodule.
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