F. Vitali, M. Aliverti, G. Capasso, F. D'Alessio, M. Munari, M. Riva, S. Scuderi, R. Z. Sánchez, S. Campana, P. Schipani, R. Claudi, A. Baruffolo, S. Ben-Ami, F. Biondi, A. Brucalassi, R. Cosentino, Davide Ricci, P. D’Avanzo, H. Kuncarayakti, A. Rubin, J. Achr'en, J. A. Araiza-Durán, I. Arcavi, A. Bianco, R. Bruch, E. Cappellaro, M. Colapietro, M. Valle, M. D. Pascale, R. D. Benedetto, S. D'orsi, D. Fantinel, A. Gal-yam, M. Genoni, M. Hernández, O. Hershko, J. Kotilainen, M. Landoni, G. Causi, S. Mattila, G. Pignata, K. Radhakrishnan, M. Rappaport, B. Salasnich, S. Smartt, M. Stritzinger, E. Ventura, D. Young
{"title":"The development status of the NIR Arm of the new SoXS instrument at the ESO/NTT telescope","authors":"F. Vitali, M. Aliverti, G. Capasso, F. D'Alessio, M. Munari, M. Riva, S. Scuderi, R. Z. Sánchez, S. Campana, P. Schipani, R. Claudi, A. Baruffolo, S. Ben-Ami, F. Biondi, A. Brucalassi, R. Cosentino, Davide Ricci, P. D’Avanzo, H. Kuncarayakti, A. Rubin, J. Achr'en, J. A. Araiza-Durán, I. Arcavi, A. Bianco, R. Bruch, E. Cappellaro, M. Colapietro, M. Valle, M. D. Pascale, R. D. Benedetto, S. D'orsi, D. Fantinel, A. Gal-yam, M. Genoni, M. Hernández, O. Hershko, J. Kotilainen, M. Landoni, G. Causi, S. Mattila, G. Pignata, K. Radhakrishnan, M. Rappaport, B. Salasnich, S. Smartt, M. Stritzinger, E. Ventura, D. Young","doi":"10.1117/12.2562147","DOIUrl":null,"url":null,"abstract":"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 μm. 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 μm, 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 μm. In this work, we will show the advanced phase of integration of the NIR spectrograph.","PeriodicalId":215000,"journal":{"name":"Ground-based and Airborne Instrumentation for Astronomy VIII","volume":"42 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2020-12-13","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"6","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Ground-based and Airborne Instrumentation for Astronomy VIII","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1117/12.2562147","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 6
Abstract
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 μm. 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 μm, 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 μm. In this work, we will show the advanced phase of integration of the NIR spectrograph.
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