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

R. Claudi; M. Aliverti; F. Biondi; M. Munari; R. Zanmar Sanchez; S. Campana; P. Schipani; A. Baruffolo; S. Ben-Ami; A. Brucalassi; G. Capasso; R. Cosentino; F. D'Alessio; P. D'Avanzo; O. Hershko; H. Kuncarayakti; A. Rubin; S. Scuderi; F. Vitali; J. Achrén; J. A. Araiza-Durán; I. Arcavi; A. Bianco; E. Cappellaro; M. Colapietro; M. Della Valle; O. Diner; S. D'Orsi; D. Fantinel; J. Fynbo; A. Gal-Yam; M. Genoni; M. Hirvonen; J. Kotilainen; T. Kumar; M. Landoni; J. Lehti; G. Li Causi; L. Marafatto; S. Mattila; G. Pariani; G. Pignata; M. Rappaport; D. Ricci; M. Riva; B. Salasnich; S. Smartt; M. Turatto

doi:10.1117/12.2314576

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

R. Claudi, M. Aliverti, F. Biondi, M. Munari, R. Zanmar Sanchez, S. Campana, P. Schipani, A. Baruffolo, S. Ben-Ami, A. Brucalassi, G. Capasso, R. Cosentino, F. D'Alessio, P. D'Avanzo, O. Hershko, H. Kuncarayakti, A. Rubin, S. Scuderi, F. Vitali, J. AchrénJ. A. Araiza-Durán, I. Arcavi, A. Bianco, E. Cappellaro, M. Colapietro, M. Della Valle, O. Diner, S. D'Orsi, D. Fantinel, J. Fynbo, A. Gal-Yam, M. Genoni, M. Hirvonen, J. Kotilainen, T. Kumar, M. Landoni, J. Lehti, G. Li Causi, L. Marafatto, S. Mattila, G. Pariani, G. Pignata, M. Rappaport, D. Ricci, M. Riva, B. Salasnich, S. Smartt, M. Turatto

Tel Aviv University, Weizmann Institute of Science

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

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.

Original language	English
Title of host publication	Ground-based and Airborne Instrumentation for Astronomy VII
Editors	Luc Simard, Christopher J. Evans, Hideki Takami
Publisher	SPIE
Number of pages	11
ISBN (Print)	9781510619579
DOIs	https://doi.org/10.1117/12.2314576
State	Published - 6 Jul 2018
Event	Ground-based and Airborne Instrumentation for Astronomy VII 2018 - Austin, United States Duration: 10 Jun 2018 → 14 Jun 2018

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	10702

Conference

Conference	Ground-based and Airborne Instrumentation for Astronomy VII 2018
Country/Territory	United States
City	Austin
Period	10/06/18 → 14/06/18

Keywords

Astronomical Instrumentation
NIR
Spectrograph
Transients
VIS

All Science Journal Classification (ASJC) codes

Electronic, Optical and Magnetic Materials
Condensed Matter Physics
Computer Science Applications
Applied Mathematics
Electrical and Electronic Engineering

Access to Document

10.1117/12.2314576

https://arxiv.org/abs/1808.03272License: Other

Cite this

Claudi, R., Aliverti, M., Biondi, F., Munari, M., Zanmar Sanchez, R., Campana, S., Schipani, P., Baruffolo, A., Ben-Ami, S., Brucalassi, A., Capasso, G., Cosentino, R., D'Alessio, F., D'Avanzo, P., Hershko, O., Kuncarayakti, H., Rubin, A., Scuderi, S., Vitali, F., ... Turatto, M. (2018). The common path of SOXS (Son of X-Shooter). In L. Simard, C. J. Evans, & H. Takami (Eds.), Ground-based and Airborne Instrumentation for Astronomy VII Article 107023T (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 10702). SPIE. https://doi.org/10.1117/12.2314576

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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.",

keywords = "Astronomical Instrumentation, NIR, Spectrograph, Transients, VIS",

author = "R. Claudi and M. Aliverti and F. Biondi and M. Munari and \{Zanmar Sanchez\}, R. and S. Campana and P. Schipani and A. Baruffolo and S. Ben-Ami and A. Brucalassi and G. Capasso and R. Cosentino and F. D'Alessio and P. D'Avanzo and O. Hershko and H. Kuncarayakti and A. Rubin and S. Scuderi and F. Vitali and J. Achr{\'e}n and Araiza-Dur{\'a}n, \{J. A.\} and I. Arcavi and A. Bianco and E. Cappellaro and M. Colapietro and \{Della Valle\}, M. and O. Diner and S. D'Orsi and D. Fantinel and J. Fynbo and A. Gal-Yam and M. Genoni and M. Hirvonen and J. Kotilainen and T. Kumar and M. Landoni and J. Lehti and \{Li Causi\}, G. and L. Marafatto and S. Mattila and G. Pariani and G. Pignata and M. Rappaport and D. Ricci and M. Riva and B. Salasnich and S. Smartt and M. Turatto",

note = "Publisher Copyright: {\textcopyright} 2018 SPIE.; Ground-based and Airborne Instrumentation for Astronomy VII 2018 ; Conference date: 10-06-2018 Through 14-06-2018",

year = "2018",

month = jul,

day = "6",

doi = "10.1117/12.2314576",

language = "الإنجليزيّة",

isbn = "9781510619579",

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

publisher = "SPIE",

editor = "Luc Simard and Evans, \{Christopher J.\} and Hideki Takami",

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Claudi, R, Aliverti, M, Biondi, F, Munari, M, Zanmar Sanchez, R, Campana, S, Schipani, P, Baruffolo, A, Ben-Ami, S, Brucalassi, A, Capasso, G, Cosentino, R, D'Alessio, F, D'Avanzo, P, Hershko, 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, Diner, O, D'Orsi, S, Fantinel, D, Fynbo, J, Gal-Yam, A, 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, Riva, M, Salasnich, B, Smartt, S & Turatto, M 2018, The common path of SOXS (Son of X-Shooter). in L Simard, CJ Evans & H Takami (eds), Ground-based and Airborne Instrumentation for Astronomy VII., 107023T, Proceedings of SPIE - The International Society for Optical Engineering, vol. 10702, SPIE, Ground-based and Airborne Instrumentation for Astronomy VII 2018, Austin, United States, 10/06/18. https://doi.org/10.1117/12.2314576

The common path of SOXS (Son of X-Shooter). / Claudi, R.; Aliverti, M.; Biondi, F. et al.
Ground-based and Airborne Instrumentation for Astronomy VII. ed. / Luc Simard; Christopher J. Evans; Hideki Takami. SPIE, 2018. 107023T (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 10702).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

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AU - Aliverti, M.

AU - Biondi, F.

AU - Munari, M.

AU - Zanmar Sanchez, R.

AU - Campana, S.

AU - Schipani, P.

AU - Baruffolo, A.

AU - Ben-Ami, S.

AU - Brucalassi, A.

AU - Capasso, G.

AU - Cosentino, R.

AU - D'Alessio, F.

AU - D'Avanzo, P.

AU - Hershko, O.

AU - Kuncarayakti, H.

AU - Rubin, A.

AU - Scuderi, S.

AU - Vitali, F.

AU - Achrén, J.

AU - Araiza-Durán, J. A.

AU - Arcavi, I.

AU - Bianco, A.

AU - Cappellaro, E.

AU - Colapietro, M.

AU - Della Valle, M.

AU - Diner, O.

AU - D'Orsi, S.

AU - Fantinel, D.

AU - Fynbo, J.

AU - Gal-Yam, A.

AU - Genoni, M.

AU - Hirvonen, M.

AU - Kotilainen, J.

AU - Kumar, T.

AU - Landoni, M.

AU - Lehti, J.

AU - Li Causi, G.

AU - Marafatto, L.

AU - Mattila, S.

AU - Pariani, G.

AU - Pignata, G.

AU - Rappaport, M.

AU - Ricci, D.

AU - Riva, M.

AU - Salasnich, B.

AU - Smartt, S.

AU - Turatto, M.

PY - 2018/7/6

Y1 - 2018/7/6

N2 - 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.

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.

KW - Astronomical Instrumentation

KW - NIR

KW - Spectrograph

KW - Transients

KW - VIS

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U2 - 10.1117/12.2314576

DO - 10.1117/12.2314576

M3 - منشور من مؤتمر

SN - 9781510619579

T3 - Proceedings of SPIE - The International Society for Optical Engineering

BT - Ground-based and Airborne Instrumentation for Astronomy VII

A2 - Simard, Luc

A2 - Evans, Christopher J.

A2 - Takami, Hideki

PB - SPIE

T2 - Ground-based and Airborne Instrumentation for Astronomy VII 2018

Y2 - 10 June 2018 through 14 June 2018

ER -

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

Abstract

Publication series

Conference

Keywords

All Science Journal Classification (ASJC) codes

Access to Document

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