The development status of the NIR Arm of the new SoXS instrument at the ESO/NTT telescope

23 Dec 2020  ·  F. Vitali, M. Aliverti, G. Capasso, F. D'Alessio, M. Munari, M. Riva, S. Scuderi, R. Zanmar Sanchez, S. Campana, P. Schipani, R. Claudi, A. Baruffolo, S. Ben-Ami, F. Biondi, A. Brucalassi, R. Cosentino, D. Ricci, P. D'Avanzo, H. Kuncarayakti, A. Rubin, J. Achrén, J. A. Araiza-Duran, I. Arcavi, A. Bianco, R. Bruch, E. Cappellaro, M. Colapietro, M. Della Valle, M. De Pascale, R. Di Benedetto, S. D'Orsi, D. Fantinel, A. Gal-Yam, M. Genoni, M. Hernandez, O. Hershko, J. Kotilainen, M. Landoni, G. Li Causi, S. Mattila, G. Pignata, K. Radhakrishnan, M. Rappaport, B. Salasnich, S. Smartt, M. Stritzinger, E. Ventura, D. Young ·

We present here the development status of the NIR spectrograph of the Son Of X-Shooter (SOXS) instrument, for the ESO/NTT telescope at La Silla (Chile). SOXS is a R~4,500 mean resolution spectrograph, with a simultaneously coverage from about 0.35 to 2.00 micron. It will be mounted at the Nasmyth focus of the NTT. The two UV-VIS-NIR wavelength ranges will be covered by two separated arms. The NIR spectrograph is a fully cryogenic echelle-dispersed spectrograph, working in the range 0.80-2.00 micron, equipped with a Hawaii H2RG IR array from Teledyne. The whole spectrograph will be cooled down to about 150 K (but the array at 40 K), to lower the thermal background, and equipped with a thermal filter to block any thermal radiation above 2.0 micron. In this work, we will show the advanced phase of integration of the NIR spectrograph.

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Instrumentation and Methods for Astrophysics