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SOXS AIT: a paradigm for system engineering of a medium class telescope instrument

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arxiv 2209.07209 v1 pith:BUEQESHB submitted 2022-09-15 astro-ph.IM

SOXS AIT: a paradigm for system engineering of a medium class telescope instrument

Riccardo Claudi , Kalyan Radhakrishnan , Federico Battaini , Sergio Campana , Pietro Schipani , Matteo Aliverti , Jose Antonio Araiza-Duran , Andrea Baruffolo
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Sagi Ben-Ami Anna Brucalassi Giulio Capasso Mirko Colapietro Rosario Cosentino Francesco D'Alessio Paolo D'Avanzo Rosario Di Benedetto Sergio D'Orsi Matteo Genoni Ofir Hershko Hanindyo Kuncarayakti Marco Landoni Matteo Munari Giuliano Pignata Michael Rappaport Davide Ricci Adam Rubin Salvo Scuderi Stephen Smartt Fabrizio Vitali David Young Ricardo Zanmar Sanchez Jani Achren Iair Arcavi Rachel Bruch Enrico Cappellaro Massimo Della Valle Avishay Gal-Yam Gianluca Li Causi Luca Marafatto Seppo Matila Marco Riva Bernardo Salasnich Maximilian Stritzinger
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classification astro-ph.IM
keywords soxsinstrumentspectrographsystemengineeringintegrationoverviewscientific
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SOXS (SOn of X-Shooter) is a high-efficiency spectrograph with a mean Resolution-Slit product of 3500 over the entire band capable of simultaneously observing the complete spectral range 350-2000 nm. It consists of three scientific arms (the UV-VIS Spectrograph, the NIR Spectrograph and the Acquisition Camera) connected by the Common Path system to the NTT, and the Calibration Unit. We present an overview of the flow from the scientific to the technical requirements, and the realization of the sub-systems. Further, we give an overview of the methodologies used for planning and managing the assembly of the sub-systems, their integration and tests before the acceptance of the instrument in Europe (PAE) along with the plan for the integration of SOXS to the NTT. SOXS could be used as an example for the system engineering of an instrument of moderate complexity, with a large geographic spread of the team.

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