The common path of SOXS (Son of X-Shooter)

Riccardo U. Claudi; Matteo Aliverti; Federico Biondi; Matteo Munari; Ricardo Zánmar Sánchez; Sergio Campana; Pietro Schipani; Andrea Baruffolo; Sagi Ben-ami; Anna Brucalassi; Giulio Capasso; Rosario Cosentino; Francesco D'alessio; Paolo D'avanzo; Oz Diner; Hanindyo Kuncarayakti; Adam Rubin; Salvatore Scuderi; Fabrizio Vitali; Jani Achrén; José A. Araiza-durán; Iair Arcavi; Andrea Bianco; Enrico Cappellaro; Mirko Colapietro; Massimo Della Valle; Sergio D'orsi; Daniela Fantinel; Johan Fynbo; Avishay Gal-yam; Matteo Genoni; Mika Hirvonen; Jari Kotilainen; Marco Landoni; Jussi Lehti; Gianluca Li Causi; Luca Marafatto; Seppo Mattila; Giorgio Pariani; Giuliano Pignata; Michael Rappaport; Davide Ricci; Marco Riva; Bernardo Salasnich; Stephen Smartt; Massimo Turatto; T. Kumar; O. Hershko; Hideki Takami; Christopher J. Evans; Luc Simard

doi:10.1117/12.2314576

The common path of SOXS (Son of X-Shooter)

Riccardo U. Claudi, Matteo Aliverti, Federico Biondi, Matteo Munari, Ricardo Zánmar Sánchez, Sergio Campana, Pietro Schipani, Andrea Baruffolo, Sagi Ben-ami, Anna Brucalassi, Giulio Capasso, Rosario Cosentino, Francesco D'alessio, Paolo D'avanzo, Oz Diner, Hanindyo Kuncarayakti, Adam Rubin, Salvatore Scuderi, Fabrizio Vitali, Jani AchrénJosé A. Araiza-durán, Iair Arcavi, Andrea Bianco, Enrico Cappellaro, Mirko Colapietro, Massimo Della Valle, Sergio D'orsi, Daniela Fantinel, Johan Fynbo, Avishay Gal-yam, Matteo Genoni, Mika Hirvonen, Jari Kotilainen, Marco Landoni, Jussi Lehti, Gianluca Li Causi, Luca Marafatto, Seppo Mattila, Giorgio Pariani, Giuliano Pignata, Michael Rappaport, Davide Ricci, Marco Riva, Bernardo Salasnich, Stephen Smartt, Massimo Turatto, T. Kumar, O. Hershko, Hideki Takami, Christopher J. Evans, Luc Simard

The Cosmic Dawn Center

8 Citationer (Scopus)

Abstract

Son of X-Shooter (SOXS) will be a high-efficiency spectrograph with a mean Resolution-Slit product of 4500 (goal 5000) over the entire band capable of simultaneously observing the complete spectral range 350-2000 nm. It consists of three scientific arms (the UV-VIS Spectrograph, the NIR Spectrograph and the Acquisition Camera) connected by the Common Path system to the NTT and the Calibration Unit. The Common Path is the backbone of the instrument and the interface to the NTT Nasmyth focus flange. The light coming from the focus of the telescope is split by the common path optics into the two different optical paths in order to feed the two spectrographs and the acquisition camera. The instrument project went through the Preliminary Design Review in 2017 and is currently in Final Design Phase (with FDR in July 2018). This paper outlines the status of the Common Path system and is accompanied by a series of contributions describing the SOXS design and properties after the instrument Preliminary Design Review.

Originalsprog	Engelsk
Tidsskrift	Proceedings of the SPIE
Vol/bind	10702
Sider (fra-til)	138
ISSN	0277-786X
DOI	https://doi.org/10.1117/12.2314576
Status	Udgivet - 2018
Begivenhed	Ground-based and Airborne Instrumentation for Astronomy VII - Austin, United States Varighed: 10 jun. 2018 → 15 jun. 2018

Konference

Konference	Ground-based and Airborne Instrumentation for Astronomy VII
Lokation	Austin, United States
Periode	10/06/2018 → 15/06/2018

Adgang til dokumentet

10.1117/12.2314576

Citationsformater

Claudi, R. U., Aliverti, M., Biondi, F., Munari, M., Zánmar Sánchez, R., Campana, S., Schipani, P., Baruffolo, A., Ben-ami, S., Brucalassi, A., Capasso, G., Cosentino, R., D'alessio, F., D'avanzo, P., Diner, O., Kuncarayakti, H., Rubin, A., Scuderi, S., Vitali, F., ... Simard, L. (2018). The common path of SOXS (Son of X-Shooter). Proceedings of the SPIE, 10702, 138. https://doi.org/10.1117/12.2314576

Claudi, RU, Aliverti, M, Biondi, F, Munari, M, Zánmar Sánchez, R, Campana, S, Schipani, P, Baruffolo, A, Ben-ami, S, Brucalassi, A, Capasso, G, Cosentino, R, D'alessio, F, D'avanzo, P, Diner, O, Kuncarayakti, H, Rubin, A, Scuderi, S, Vitali, F, Achrén, J, Araiza-durán, JA, Arcavi, I, Bianco, A, Cappellaro, E, Colapietro, M, Della Valle, M, D'orsi, S, Fantinel, D, Fynbo, J, Gal-yam, A, Genoni, M, Hirvonen, M, Kotilainen, J, Landoni, M, Lehti, J, Li Causi, G, Marafatto, L, Mattila, S, Pariani, G, Pignata, G, Rappaport, M, Ricci, D, Riva, M, Salasnich, B, Smartt, S, Turatto, M, Kumar, T, Hershko, O, Takami, H, Evans, CJ & Simard, L 2018, 'The common path of SOXS (Son of X-Shooter)', Proceedings of the SPIE, bind 10702, s. 138. https://doi.org/10.1117/12.2314576

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title = "The common path of SOXS (Son of X-Shooter)",

abstract = "Son of X-Shooter (SOXS) will be a high-efficiency spectrograph with a mean Resolution-Slit product of 4500 (goal 5000) over the entire band capable of simultaneously observing the complete spectral range 350-2000 nm. It consists of three scientific arms (the UV-VIS Spectrograph, the NIR Spectrograph and the Acquisition Camera) connected by the Common Path system to the NTT and the Calibration Unit. The Common Path is the backbone of the instrument and the interface to the NTT Nasmyth focus flange. The light coming from the focus of the telescope is split by the common path optics into the two different optical paths in order to feed the two spectrographs and the acquisition camera. The instrument project went through the Preliminary Design Review in 2017 and is currently in Final Design Phase (with FDR in July 2018). This paper outlines the status of the Common Path system and is accompanied by a series of contributions describing the SOXS design and properties after the instrument Preliminary Design Review.",

author = "Claudi, {Riccardo U.} and Matteo Aliverti and Federico Biondi and Matteo Munari and {Z{\'a}nmar S{\'a}nchez}, Ricardo and Sergio Campana and Pietro Schipani and Andrea Baruffolo and Sagi Ben-ami and Anna Brucalassi and Giulio Capasso and Rosario Cosentino and Francesco D'alessio and Paolo D'avanzo and Oz Diner and Hanindyo Kuncarayakti and Adam Rubin and Salvatore Scuderi and Fabrizio Vitali and Jani Achr{\'e}n and Araiza-dur{\'a}n, {Jos{\'e} A.} and Iair Arcavi and Andrea Bianco and Enrico Cappellaro and Mirko Colapietro and {Della Valle}, Massimo and Sergio D'orsi and Daniela Fantinel and Johan Fynbo and Avishay Gal-yam and Matteo Genoni and Mika Hirvonen and Jari Kotilainen 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 Marco Riva and Bernardo Salasnich and Stephen Smartt and Massimo Turatto and T. Kumar and O. Hershko and Hideki Takami and Evans, {Christopher J.} and Luc Simard",

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doi = "10.1117/12.2314576",

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journal = "Proceedings of the SPIE",

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AU - Claudi, Riccardo U.

AU - Aliverti, Matteo

AU - Biondi, Federico

AU - Munari, Matteo

AU - Zánmar Sánchez, Ricardo

AU - Campana, Sergio

AU - Schipani, Pietro

AU - Baruffolo, Andrea

AU - Ben-ami, Sagi

AU - Brucalassi, Anna

AU - Capasso, Giulio

AU - Cosentino, Rosario

AU - D'alessio, Francesco

AU - D'avanzo, Paolo

AU - Diner, Oz

AU - Kuncarayakti, Hanindyo

AU - Rubin, Adam

AU - Scuderi, Salvatore

AU - Vitali, Fabrizio

AU - Achrén, Jani

AU - Araiza-durán, José A.

AU - Arcavi, Iair

AU - Bianco, Andrea

AU - Cappellaro, Enrico

AU - Colapietro, Mirko

AU - Della Valle, Massimo

AU - D'orsi, Sergio

AU - Fantinel, Daniela

AU - Fynbo, Johan

AU - Gal-yam, Avishay

AU - Genoni, Matteo

AU - Hirvonen, Mika

AU - Kotilainen, Jari

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 - Riva, Marco

AU - Salasnich, Bernardo

AU - Smartt, Stephen

AU - Turatto, Massimo

AU - Kumar, T.

AU - Hershko, O.

AU - Takami, Hideki

AU - Evans, Christopher J.

AU - Simard, Luc

PY - 2018

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AB - Son of X-Shooter (SOXS) will be a high-efficiency spectrograph with a mean Resolution-Slit product of 4500 (goal 5000) over the entire band capable of simultaneously observing the complete spectral range 350-2000 nm. It consists of three scientific arms (the UV-VIS Spectrograph, the NIR Spectrograph and the Acquisition Camera) connected by the Common Path system to the NTT and the Calibration Unit. The Common Path is the backbone of the instrument and the interface to the NTT Nasmyth focus flange. The light coming from the focus of the telescope is split by the common path optics into the two different optical paths in order to feed the two spectrographs and the acquisition camera. The instrument project went through the Preliminary Design Review in 2017 and is currently in Final Design Phase (with FDR in July 2018). This paper outlines the status of the Common Path system and is accompanied by a series of contributions describing the SOXS design and properties after the instrument Preliminary Design Review.

U2 - 10.1117/12.2314576

DO - 10.1117/12.2314576

M3 - Conference article

SN - 0277-786X

VL - 10702

SP - 138

JO - Proceedings of the SPIE

JF - Proceedings of the SPIE

T2 - Ground-based and Airborne Instrumentation for Astronomy VII

Y2 - 10 June 2018 through 15 June 2018

ER -

The common path of SOXS (Son of X-Shooter)

Abstract

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