The status of the NIR arm of the SOXS Instrument toward the PAE
: Vitali, Fabrizio; Genoni, Matteo; Aliverti, Matteo; Radhakrishnan, Kalyan; Battaini, Federico; D'Avanzo, Paolo; D'Alessio, Francesco; Pariani, Giorgio; Oggioni, Luca; Scuderi, Salvatore; Ricci, Davide; Martinetti, Eugenio; Micciche, Antonio; Nicotra, Gaetano; Colapietro, Mirko; D'Orsi, Sergio; Munari, Matteo; Lessio, Luigi; Di Filippo, Simone; Scaudo, Andrea; Bellassai, Giancarlo; Di Benedetto, Rosario; Occhipinti, Giovanni; Landoni, Marco; Accardo, Matteo; Mehrgan, Leander; Ives, Derek; Scire, Carlotta; Campana, Sergio; Schipani, Pietro; Claudia, Riccardo; Capasso, Giulio; Rival, Marco; Sanchez, Ricardo Zanmar; Araiza-Duran, Jose Antonio; Arcavi, Iair; Baruffolo, Andrea; Ben-Ami, Sagi; Brucalassi, Anna; Bruch, Rachel; Cappellaro, Enrico; Cosentino, Rosario; De Pascale, Marco; Della Valle, Massimo; Gal-Yam, Avishay; Diaz, Marcos Hernandez; Hershko, Ofir; Kotilainen, Jan; Kuncarayakti, Hanindyo; Li Causi, Gianluca; Marty, Laurent; Mattila, Seppo; Ventura, Hector Perez; Pignata, Giuliano; Rappaport, Michael; Rubin, Adam; Salasnich, Bernardo; Smartt, Stephen; Stritzinger, Maximilian; Young, David
: Bryant, Julia J.; Motohara, Kentaro; Vernet, Joël R. D.
: SPIE Astronomical Telescopes + Instrumentation
Publisher: SPIE-INT SOC OPTICAL ENGINEERING
: BELLINGHAM
: 2024
: Proceedings of SPIE : the International Society for Optical Engineering
: Ground-based and Airborne Instrumentation for Astronomy X
: PROC SPIE
: 130962V
: Proceedings of SPIE
: 13096
: 8
: 978-1-5106-7515-5
: 978-1-5106-7516-2
: 0277-786X
: 1996-756X
DOI: https://doi.org/10.1117/12.3017072
: https://doi.org/10.1117/12.3017072
The Son Of X-Shooter (SOXS) is a single object spectrograph, built by an international consortium for the 3.58-m ESO New Technology Telescope at the La Silla Observatory [1]. It offers a simultaneous spectral coverage over 350-2000 nm, with two separate spectrographs. In this paper we present the status of the Near InfraRed (NIR) cryogenic echelle crossdispersed spectrograph [1], in the range 0.80-2.00 mu m with 15 orders, equipped with an 2k x 2k Hawaii H2RG IR array from Teledyne, working at 40K, that is currently assembled and tested on the SOXS instrument, in the premises of INAF in Padova. We describe the different tests and results of the cryo, vacuum, opto-mechanics and detector subsystems that finally will be part of the PAE by ESO.
