The VIS detector system of SOXS

Rosario Cosentino; Matteo Aliverti; Salvatore Scuderi; Sergio Campana; Riccardo Claudi; Pietro Schipani; Andrea Baruffolo; Sagi Ben-Ami; L. H. Mehrgan; Derek Ives; 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; R. Zanmar Sanchez; Stephen Smartt; Massimo Turatto

doi:10.1117/12.2312539

The VIS detector system of SOXS

Rosario Cosentino, Matteo Aliverti, Salvatore Scuderi, Sergio Campana, Riccardo Claudi, Pietro Schipani, Andrea Baruffolo, Sagi Ben-Ami, L. H. Mehrgan, Derek Ives, Federico Biondi, Anna Brucalassi, Giulio Capasso, Francesco D'Alessio, Paolo D'Avanzo, Oz Diner, Hanindyo Kuncarayakti, Matteo Munari, Adam Rubin, Fabrizio VitaliJani 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, R. Zanmar Sanchez, Stephen Smartt, Massimo Turatto

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

19 Citations (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).

Original language	English
Title of host publication	Ground-based and Airborne Instrumentation for Astronomy VII
Editors	Luc Simard, Luc Simard, Christopher J. Evans, Hideki Takami
Publisher	SPIE
Number of pages	9
ISBN (Print)	9781510619579
DOIs	https://doi.org/10.1117/12.2312539
Publication status	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

Series	Proceedings of SPIE - The International Society for Optical Engineering
Volume	10702
ISSN	0277-786X

Conference

Conference	Ground-based and Airborne Instrumentation for Astronomy VII 2018
Country/Territory	United States
City	Austin
Period	10/6/18 → 14/6/18

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

10.1117/12.2312539

Cite this

Cosentino, R., Aliverti, M., Scuderi, S., Campana, S., Claudi, R., Schipani, P., Baruffolo, A., Ben-Ami, S., Mehrgan, L. H., Ives, D., Biondi, F., Brucalassi, A., Capasso, G., D'Alessio, F., D'Avanzo, P., Diner, O., Kuncarayakti, H., Munari, M., Rubin, A., ... Turatto, M. (2018). The VIS detector system of SOXS. In L. Simard, L. Simard, C. J. Evans, & H. Takami (Eds.), Ground-based and Airborne Instrumentation for Astronomy VII Article 107022J SPIE. https://doi.org/10.1117/12.2312539

@inproceedings{feb78eacacde4f38ac35520527316811,

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 Riccardo Claudi and Pietro Schipani and Andrea Baruffolo and Sagi Ben-Ami and Mehrgan, {L. H.} and Derek Ives 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 {Zanmar Sanchez}, R. and Stephen Smartt and Massimo Turatto",

note = "NA; 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 = "10.1117/12.2312539",

language = "English",

isbn = "9781510619579",

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

publisher = "SPIE",

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

booktitle = "Ground-based and Airborne Instrumentation for Astronomy VII",

address = "United States",

}

Cosentino, R, Aliverti, M, Scuderi, S, Campana, S, Claudi, R, Schipani, P, Baruffolo, A, Ben-Ami, S, Mehrgan, LH, Ives, D, 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, Zanmar Sanchez, R, Smartt, S & Turatto, M 2018, The VIS detector system of SOXS. in L Simard, L Simard, CJ Evans & H Takami (eds), Ground-based and Airborne Instrumentation for Astronomy VII., 107022J, SPIE, Proceedings of SPIE - The International Society for Optical Engineering, vol. 10702, Ground-based and Airborne Instrumentation for Astronomy VII 2018, Austin, Texas, United States, 10/6/18. https://doi.org/10.1117/12.2312539

The VIS detector system of SOXS. / Cosentino, Rosario; Aliverti, Matteo; Scuderi, Salvatore et al.
Ground-based and Airborne Instrumentation for Astronomy VII. ed. / Luc Simard; Luc Simard; Christopher J. Evans; Hideki Takami. SPIE, 2018. 107022J (Proceedings of SPIE - The International Society for Optical Engineering, Vol. 10702).

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

TY - GEN

T1 - The VIS detector system of SOXS

AU - Cosentino, Rosario

AU - Aliverti, Matteo

AU - Scuderi, Salvatore

AU - Campana, Sergio

AU - Claudi, Riccardo

AU - Schipani, Pietro

AU - Baruffolo, Andrea

AU - Ben-Ami, Sagi

AU - Mehrgan, L. H.

AU - Ives, Derek

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 - Zanmar Sanchez, R.

AU - Smartt, Stephen

AU - Turatto, Massimo

N1 - NA

PY - 2018/7/6

Y1 - 2018/7/6

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).

UR - http://www.scopus.com/inward/record.url?scp=85052645444&partnerID=8YFLogxK

U2 - 10.1117/12.2312539

DO - 10.1117/12.2312539

M3 - Conference contribution

AN - SCOPUS:85052645444

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 VIS detector system of SOXS

Abstract

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