The NIR spectrograph for the new SOXS instrument at the NTT

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

doi:10.1117/12.2311466

The NIR spectrograph for the new SOXS instrument at the NTT

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

The Cosmic Dawn Center

10 Citations (Scopus)

Abstract

We present the NIR spectrograph of the Son Of XShooter (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 criogenic echelle-dispersed spectrograph, working in the range 0.80- 2.00 μm, equipped with an Hawaii H2RG IR array from Teledyne, working at 40 K. The spectrograph will be cooled down to about 150 K, to lower the thermal background, and equipped with a thermal filter to block any thermal radiation above 2.0 μm. In this poster we will show the main characteristics of the instrument along with the expected performances at the telescope.

Original language	English
Journal	Proceedings of the SPIE
Volume	10702
Pages (from-to)	80
ISSN	0277-786X
DOIs	https://doi.org/10.1117/12.2311466
Publication status	Published - 2018
Event	Proceedings of the SPIE - Orlando, Florida, United States Duration: 7 Feb 2009 → 12 Feb 2009

Conference

Conference	Proceedings of the SPIE
Country/Territory	United States
City	Orlando, Florida
Period	07/02/2009 → 12/02/2009

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Aliverti, M., Capasso, G., D'alessio, F., Munari, M., Riva, M., Scuderi, S., Zánmar Sánchez, R., Campana, S., Schipani, P., Claudi, R. U., Baruffolo, A., Ben-ami, S., Biondi, F., Brucalassi, A., Cosentino, R., D'avanzo, P., Diner, O., Kuncarayakti, H., Rubin, A., ... Simard, L. (2018). The NIR spectrograph for the new SOXS instrument at the NTT. Proceedings of the SPIE, 10702, 80. https://doi.org/10.1117/12.2311466

Aliverti, M, Capasso, G, D'alessio, F, Munari, M, Riva, M, Scuderi, S, Zánmar Sánchez, R, Campana, S, Schipani, P, Claudi, RU, Baruffolo, A, Ben-ami, S, Biondi, F, Brucalassi, A, Cosentino, R, D'avanzo, P, Diner, O, Kuncarayakti, H, Rubin, A, Achrén, J, Araiza-durán, JA, Arcavi, I, Bianco, A, Cappellaro, E, Colapietro, M, Della Valle, M, D'orsi, S, Fynbo, J, Genoni, M, Hirvonen, M, Kotilainen, J, Kumar, T, Landoni, M, Lehti, J, Li Causi, G, Marafatto, L, Mattila, S, Pariani, G, Pignata, G, Rappaport, M, Ricci, D, Salasnich, B, Smartt, S, Turatto, M, Vitali, F, Fantinel, D, Gal-yam, A, Takami, H, Evans, CJ & Simard, L 2018, 'The NIR spectrograph for the new SOXS instrument at the NTT', Proceedings of the SPIE, vol. 10702, pp. 80. https://doi.org/10.1117/12.2311466

@inproceedings{bbb37a561a674f9eb1cd6a387bea9ada,

title = "The NIR spectrograph for the new SOXS instrument at the NTT",

abstract = "We present the NIR spectrograph of the Son Of XShooter (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 criogenic echelle-dispersed spectrograph, working in the range 0.80- 2.00 μm, equipped with an Hawaii H2RG IR array from Teledyne, working at 40 K. The spectrograph will be cooled down to about 150 K, to lower the thermal background, and equipped with a thermal filter to block any thermal radiation above 2.0 μm. In this poster we will show the main characteristics of the instrument along with the expected performances at the telescope.",

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

year = "2018",

doi = "10.1117/12.2311466",

language = "English",

volume = "10702",

pages = "80",

journal = "Proceedings of SPIE - The International Society for Optical Engineering",

issn = "0277-786X",

publisher = "International Society for Optical Engineering",

note = "Proceedings of the SPIE ; Conference date: 07-02-2009 Through 12-02-2009",

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TY - GEN

T1 - The NIR spectrograph for the new SOXS instrument at the NTT

AU - Aliverti, Matteo

AU - Capasso, Giulio

AU - D'alessio, Francesco

AU - Munari, Matteo

AU - Riva, Marco

AU - Scuderi, Salvatore

AU - Zánmar Sánchez, Ricardo

AU - Campana, Sergio

AU - Schipani, Pietro

AU - Claudi, Riccardo U.

AU - Baruffolo, Andrea

AU - Ben-ami, Sagi

AU - Biondi, Federico

AU - Brucalassi, Anna

AU - Cosentino, Rosario

AU - D'avanzo, Paolo

AU - Diner, Oz

AU - Kuncarayakti, Hanindyo

AU - Rubin, Adam

AU - Achrén, Jani

AU - Araiza-durán, José Antonio

AU - Arcavi, Iair

AU - Bianco, Andrea

AU - Cappellaro, Enrico

AU - Colapietro, Mirko

AU - Della Valle, Massimo

AU - D'orsi, Sergio

AU - Fynbo, Johan

AU - Genoni, Matteo

AU - Hirvonen, Mika

AU - Kotilainen, Jari

AU - Kumar, Tarun

AU - Landoni, Marco

AU - Lehti, Jussi

AU - Li Causi, Gianluca

AU - Marafatto, Luca

AU - Mattila, Seppo

AU - Pariani, Giorgio

AU - Pignata, Giuliano

AU - Rappaport, Michael

AU - Ricci, Davide

AU - Salasnich, Bernardo

AU - Smartt, Stephen

AU - Turatto, Massimo

AU - Vitali, Fabrizio

AU - Fantinel, Daniela

AU - Gal-yam, Avishay

AU - Takami, Hideki

AU - Evans, Christopher J.

AU - Simard, Luc

PY - 2018

Y1 - 2018

N2 - We present the NIR spectrograph of the Son Of XShooter (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 criogenic echelle-dispersed spectrograph, working in the range 0.80- 2.00 μm, equipped with an Hawaii H2RG IR array from Teledyne, working at 40 K. The spectrograph will be cooled down to about 150 K, to lower the thermal background, and equipped with a thermal filter to block any thermal radiation above 2.0 μm. In this poster we will show the main characteristics of the instrument along with the expected performances at the telescope.

AB - We present the NIR spectrograph of the Son Of XShooter (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 criogenic echelle-dispersed spectrograph, working in the range 0.80- 2.00 μm, equipped with an Hawaii H2RG IR array from Teledyne, working at 40 K. The spectrograph will be cooled down to about 150 K, to lower the thermal background, and equipped with a thermal filter to block any thermal radiation above 2.0 μm. In this poster we will show the main characteristics of the instrument along with the expected performances at the telescope.

U2 - 10.1117/12.2311466

DO - 10.1117/12.2311466

M3 - Conference article

SN - 0277-786X

VL - 10702

SP - 80

JO - Proceedings of SPIE - The International Society for Optical Engineering

JF - Proceedings of SPIE - The International Society for Optical Engineering

T2 - Proceedings of the SPIE

Y2 - 7 February 2009 through 12 February 2009

ER -

The NIR spectrograph for the new SOXS instrument at the NTT

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Conference

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