The VIS detector system of SOXS

Rosario Cosentino; Matteo Aliverti; Salvatore Scuderi; Sergio Campana; Riccardo U. Claudi; Pietro Schipani; Andrea Baruffolo; Sagi Ben-ami; Federico Biondi; Anna Brucalassi; Giulio Capasso; Francesco D'alessio; Paolo D'avanzo; Oz Diner; Hanindyo Kuncarayakti; Matteo Munari; Adam Rubin; Fabrizio Vitali; Jani Achrén; José Antonio 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; Tarun Kumar; 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; Ricardo Zánmar Sánchez; Leander H. Mehrgan; Derek Ives; Hideki Takami; Christopher J. Evans; Luc Simard

doi:10.1117/12.2312539

The VIS detector system of SOXS

Rosario Cosentino, Matteo Aliverti, Salvatore Scuderi, Sergio Campana, Riccardo U. Claudi, Pietro Schipani, Andrea Baruffolo, Sagi Ben-ami, Federico Biondi, Anna Brucalassi, Giulio Capasso, Francesco D'alessio, Paolo D'avanzo, Oz Diner, Hanindyo Kuncarayakti, Matteo Munari, Adam Rubin, Fabrizio Vitali, Jani Achrén, José Antonio Araiza-duránIair 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, Tarun Kumar, 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, Ricardo Zánmar Sánchez, Leander H. Mehrgan, Derek Ives, Hideki Takami, Christopher J. Evans, Luc Simard

The Cosmic Dawn Center

8 Citationer (Scopus)

Abstract

SOXS will be a unique spectroscopic facility for the ESO NTT telescope able to cover the optical and NIR bands thanks to two different arms: the UV-VIS (350-850 nm), and the NIR (800-1800 nm). In this article, we describe the design of the visible camera cryostat and the architecture of the acquisition system. The UV-VIS detector system is based on a e2v CCD 44-82, a custom detector head coupled with the ESO continuous flow cryostats (CFC) cooling system and the NGC CCD controller developed by ESO. This paper outlines the status of the system and describes the design of the different parts that made up the UV-VIS arm and is accompanied by a series of contributions describing the SOXS design solutions (Ref. 1-12).

Originalsprog	Engelsk
Tidsskrift	Proceedings of the SPIE
Vol/bind	10702
Sider (fra-til)	92
ISSN	0277-786X
DOI	https://doi.org/10.1117/12.2312539
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

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10.1117/12.2312539

Citationsformater

Cosentino, R., Aliverti, M., Scuderi, S., Campana, S., Claudi, R. U., Schipani, P., Baruffolo, A., Ben-ami, S., Biondi, F., Brucalassi, A., Capasso, G., D'alessio, F., D'avanzo, P., Diner, O., Kuncarayakti, H., Munari, M., Rubin, A., Vitali, F., Achrén, J., ... Simard, L. (2018). The VIS detector system of SOXS. Proceedings of the SPIE, 10702, 92. https://doi.org/10.1117/12.2312539

Cosentino, R, Aliverti, M, Scuderi, S, Campana, S, Claudi, RU, Schipani, P, Baruffolo, A, Ben-ami, S, Biondi, F, Brucalassi, A, Capasso, G, D'alessio, F, D'avanzo, P, Diner, O, Kuncarayakti, H, Munari, M, Rubin, A, 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, 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, Zánmar Sánchez, R, Mehrgan, LH, Ives, D, Takami, H, Evans, CJ & Simard, L 2018, 'The VIS detector system of SOXS', Proceedings of the SPIE, bind 10702, s. 92. https://doi.org/10.1117/12.2312539

@inproceedings{fd67bfbff7ab4ce4aa42218fd94969b9,

title = "The VIS detector system of SOXS",

abstract = "SOXS will be a unique spectroscopic facility for the ESO NTT telescope able to cover the optical and NIR bands thanks to two different arms: the UV-VIS (350-850 nm), and the NIR (800-1800 nm). In this article, we describe the design of the visible camera cryostat and the architecture of the acquisition system. The UV-VIS detector system is based on a e2v CCD 44-82, a custom detector head coupled with the ESO continuous flow cryostats (CFC) cooling system and the NGC CCD controller developed by ESO. This paper outlines the status of the system and describes the design of the different parts that made up the UV-VIS arm and is accompanied by a series of contributions describing the SOXS design solutions (Ref. 1-12).",

author = "Rosario Cosentino and Matteo Aliverti and Salvatore Scuderi and Sergio Campana and Claudi, {Riccardo U.} and Pietro Schipani and Andrea Baruffolo and Sagi Ben-ami and Federico Biondi and Anna Brucalassi and Giulio Capasso and Francesco D'alessio and Paolo D'avanzo and Oz Diner and Hanindyo Kuncarayakti and Matteo Munari and Adam Rubin and Fabrizio Vitali 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 Daniela Fantinel and Johan Fynbo and Avishay Gal-yam 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 Marco Riva and Bernardo Salasnich and Stephen Smartt and Massimo Turatto and {Z{\'a}nmar S{\'a}nchez}, Ricardo and Mehrgan, {Leander H.} and Derek Ives and Hideki Takami and Evans, {Christopher J.} and Luc Simard",

year = "2018",

doi = "10.1117/12.2312539",

language = "English",

volume = "10702",

pages = "92",

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

issn = "0277-786X",

publisher = "International Society for Optical Engineering",

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T1 - The VIS detector system of SOXS

AU - Cosentino, Rosario

AU - Aliverti, Matteo

AU - Scuderi, Salvatore

AU - Campana, Sergio

AU - Claudi, Riccardo U.

AU - Schipani, Pietro

AU - Baruffolo, Andrea

AU - Ben-ami, Sagi

AU - Biondi, Federico

AU - Brucalassi, Anna

AU - Capasso, Giulio

AU - D'alessio, Francesco

AU - D'avanzo, Paolo

AU - Diner, Oz

AU - Kuncarayakti, Hanindyo

AU - Munari, Matteo

AU - Rubin, Adam

AU - Vitali, Fabrizio

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 - Fantinel, Daniela

AU - Fynbo, Johan

AU - Gal-yam, Avishay

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 - Riva, Marco

AU - Salasnich, Bernardo

AU - Smartt, Stephen

AU - Turatto, Massimo

AU - Zánmar Sánchez, Ricardo

AU - Mehrgan, Leander H.

AU - Ives, Derek

AU - Takami, Hideki

AU - Evans, Christopher J.

AU - Simard, Luc

PY - 2018

Y1 - 2018

N2 - SOXS will be a unique spectroscopic facility for the ESO NTT telescope able to cover the optical and NIR bands thanks to two different arms: the UV-VIS (350-850 nm), and the NIR (800-1800 nm). In this article, we describe the design of the visible camera cryostat and the architecture of the acquisition system. The UV-VIS detector system is based on a e2v CCD 44-82, a custom detector head coupled with the ESO continuous flow cryostats (CFC) cooling system and the NGC CCD controller developed by ESO. This paper outlines the status of the system and describes the design of the different parts that made up the UV-VIS arm and is accompanied by a series of contributions describing the SOXS design solutions (Ref. 1-12).

AB - SOXS will be a unique spectroscopic facility for the ESO NTT telescope able to cover the optical and NIR bands thanks to two different arms: the UV-VIS (350-850 nm), and the NIR (800-1800 nm). In this article, we describe the design of the visible camera cryostat and the architecture of the acquisition system. The UV-VIS detector system is based on a e2v CCD 44-82, a custom detector head coupled with the ESO continuous flow cryostats (CFC) cooling system and the NGC CCD controller developed by ESO. This paper outlines the status of the system and describes the design of the different parts that made up the UV-VIS arm and is accompanied by a series of contributions describing the SOXS design solutions (Ref. 1-12).

U2 - 10.1117/12.2312539

DO - 10.1117/12.2312539

M3 - Conference article

SN - 0277-786X

VL - 10702

SP - 92

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

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

T2 - Ground-based and Airborne Instrumentation for Astronomy VII

Y2 - 10 June 2018 through 15 June 2018

ER -

The VIS detector system of SOXS

Abstract

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