The mechanical design of SOXS for the NTT

Matteo Aliverti, Oz Diner, Anna Brucalassi, Hanindyo Kuncarayakti, Andrea Bianco, Sergio Campana, Riccardo U. Claudi, Pietro Schipani, Andrea Baruffolo, Sagi Ben-ami, Federico Biondi, Giulio Capasso, Rosario Cosentino, Francesco D'alessio, Paolo D'avanzo, Matteo Munari, Adam Rubin, Salvatore Scuderi, Fabrizio Vitali, Jani AchrénJosé Antonio Araiza-durán, Iair Arcavi, Enrico Cappellaro, Massimo Della Valle, Sergio D'orsi, Daniela Fantinel, Avishay Gal-yam, Matteo Genoni, Mika Hirvonen, Jari Kotilainen, Tarun Kumar, Marco Landoni, Jussi Lehti, Johan Fynbo, Gianluca Li Causi, Luca Marafatto, Seppo Mattila, Giorgio Pariani, Giuliano Pignata, Michael Rappaport, Davide Ricci, Marco Riva, Bernardo Salasnich, Stephen Smartt, Massimo Turatto, Ricardo Zanmar Sanchez, Mirko Colapietro, Ofir Hershko, Hideki Takami, Christopher J. Evans, Luc Simard

8 Citationer (Scopus)

Abstract

SOXS (Son of X-shooter) is a wide band, medium resolution spectrograph for the ESO NTT with a first light expected in early 2021. The instrument will be composed by five semi-independent subsystems: a pre-slit Common Path (CP), an Acquisition Camera (AC), a Calibration Unit (CU), the NIR spectrograph, and the UV-VIS spectrograph. In this paper, we present the mechanical design of the subsystems, the kinematic mounts developed to simplify the final integration procedure and the maintenance. The concept of the CP and NIR optomechanical mounts developed for a simple pre- alignment procedure and for the thermal compensation of reflective and refractive elements will be shown.

OriginalsprogEngelsk
TidsskriftProceedings of the SPIE
Vol/bind10702
Sider (fra-til)110
ISSN0277-786X
DOI
StatusUdgivet - 2018
BegivenhedGround-based and Airborne Instrumentation for Astronomy VII - Austin, United States
Varighed: 10 jun. 201815 jun. 2018

Konference

KonferenceGround-based and Airborne Instrumentation for Astronomy VII
LokationAustin, United States
Periode10/06/201815/06/2018

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