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SOXS: Effects on optical performances due to gravity flexures, temperature variations, and subsystems alignment

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arxiv 2012.12680 v1 pith:FMMNMBWU submitted 2020-12-23 astro-ph.IM

SOXS: Effects on optical performances due to gravity flexures, temperature variations, and subsystems alignment

Ricardo Zanmar Sanchez , Matteo Aliverti , Matteo Munari , Sergio Campana , Riccardo Claudi , Pietro Schipani , Andrea Baruffolo , Sagi Ben-Ami
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Federico Biondi Giulio Capasso Rosario Cosentino Francesco D'Alessio Paolo D'Avanzo Ofir Hershko Hanindyo Kuncarayakti Marco Landoni Giuliano Pignata Adam Rubin Salvatore Scuderi Fabrizio Vitali David Young Jani Achr\'en Jos\'e Antonio Araiza-Duran Iair Arcavi Anna Brucalassi Rachel Bruch Enrico Cappellaro Mirko Colapietro Massimo Della Valle Marco de Pascale Rosario di Benedetto Sergio D'Orsi Avishay Gal-Yam Matteo Genoni Marcos Hernandez Jari Kotilainen Gianluca Li Causi Seppo Mattila Michael Rappaport Kalyan Radhakrishnan Davide Ricci Marco Riva Bernardo Salasnich Stephen Smartt Maximilian Stritzinger Hector Ventura
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keywords opticalsoxsalignmenteffectsperformancestemperaturewillaimed
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SOXS (Son Of X-Shooter) is the new medium resolution wide-band spectrograph to be installed at the 3.6m New Technology Telescope (NTT) in La Silla. SOXS will offer simultaneous wavelength coverage from 0.35 to 2.0 {\mu}m and will be dedicated to the study of transient and variable sources. While nominal optical performances of the system were presented in previous proceedings (arXiv:1809.01521), we here present a set of further analyses aimed to identify and quantify optical effects, due to changes in temperature and orientation of the instrument during alignment and operations.

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