The NIR spectrograph for the new SOXS instrument at the NTT

F. Vitali; M. Aliverti; G. Capasso; F. D'Alessio; M. Munari; M. Riva; S. Scuderi; R. Zanmar Sanchez; S. Campana; P. Schipani; R. Claudi; A. Baruffolo; S. Ben-Ami; F. Biondi; A. Brucalassi; R. Cosentino; D. Ricci; P. D'Avanzo; O. Diner; H. Kuncarayakti; A. Rubin; J. Achrén; J. A. Araiza-Duran; I. Arcavi; A. Bianco; E. Cappellaro; M. Colapietro; M. Della Valle; 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; B. Salasnich; S. Smartt; M. Turatto

doi:https://doi.org/10.1117/12.2311466

The NIR spectrograph for the new SOXS instrument at the NTT

F. Vitali, M. Aliverti, G. Capasso, F. D'Alessio, M. Munari, M. Riva, S. Scuderi, R. Zanmar Sanchez, S. Campana, P. Schipani, R. Claudi, A. Baruffolo, S. Ben-Ami, F. Biondi, A. Brucalassi, R. Cosentino, D. Ricci, P. D'Avanzo, O. Diner, H. KuncarayaktiA. Rubin, J. Achrén, J. A. Araiza-Duran, I. Arcavi, A. Bianco, E. Cappellaro, M. Colapietro, M. Della Valle, 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, 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

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
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	13
ISBN (Print)	9781510619579
DOIs	https://doi.org/10.1117/12.2311466
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

Cryogenics
H2RG
NTT
Near Infrared
SOXS
Spectrograph
Transient

All Science Journal Classification (ASJC) codes

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

UN SDGs

This output contributes to the following UN Sustainable Development Goals (SDGs)

Access to Document

https://doi.org/10.1117/12.2311466

https://arxiv.org/abs/1809.01511License: Other

Cite this

Vitali, F., Aliverti, M., Capasso, G., D'Alessio, F., Munari, M., Riva, M., Scuderi, S., Zanmar Sanchez, R., Campana, S., Schipani, P., Claudi, R., Baruffolo, A., Ben-Ami, S., Biondi, F., Brucalassi, A., Cosentino, R., Ricci, D., D'Avanzo, P., Diner, O., ... Turatto, M. (2018). The NIR spectrograph for the new SOXS instrument at the NTT. In L. Simard, C. J. Evans, & H. Takami (Eds.), Ground-based and Airborne Instrumentation for Astronomy VII Article 1070228 (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 10702). SPIE. https://doi.org/10.1117/12.2311466

@inproceedings{68ab160b268f4d92a007fbc30e3d7275,

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.",

keywords = "Cryogenics, H2RG, NTT, Near Infrared, SOXS, Spectrograph, Transient",

author = "F. Vitali and M. Aliverti and G. Capasso and F. D'Alessio and M. Munari and M. Riva and S. Scuderi and {Zanmar Sanchez}, R. and S. Campana and P. Schipani and R. Claudi and A. Baruffolo and S. Ben-Ami and F. Biondi and A. Brucalassi and R. Cosentino and D. Ricci and P. D'Avanzo and O. Diner and H. Kuncarayakti and A. Rubin and J. Achr{\'e}n and Araiza-Duran, {J. A.} and I. Arcavi and A. Bianco and E. Cappellaro and M. Colapietro and {Della Valle}, M. 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 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 = "https://doi.org/10.1117/12.2311466",

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",

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

address = "الولايات المتّحدة",

}

Vitali, F, Aliverti, M, Capasso, G, D'Alessio, F, Munari, M, Riva, M, Scuderi, S, Zanmar Sanchez, R, Campana, S, Schipani, P, Claudi, R, Baruffolo, A, Ben-Ami, S, Biondi, F, Brucalassi, A, Cosentino, R, Ricci, D, D'Avanzo, P, Diner, O, Kuncarayakti, H, Rubin, A, Achrén, J, Araiza-Duran, 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, Salasnich, B, Smartt, S & Turatto, M 2018, The NIR spectrograph for the new SOXS instrument at the NTT. in L Simard, CJ Evans & H Takami (eds), Ground-based and Airborne Instrumentation for Astronomy VII., 1070228, 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/10.1117/12.2311466

The NIR spectrograph for the new SOXS instrument at the NTT. / Vitali, F.; Aliverti, M.; Capasso, G. et al.
Ground-based and Airborne Instrumentation for Astronomy VII. ed. / Luc Simard; Christopher J. Evans; Hideki Takami. SPIE, 2018. 1070228 (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 10702).

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

TY - GEN

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

AU - Vitali, F.

AU - Aliverti, M.

AU - Capasso, G.

AU - D'Alessio, F.

AU - Munari, M.

AU - Riva, M.

AU - Scuderi, S.

AU - Zanmar Sanchez, R.

AU - Campana, S.

AU - Schipani, P.

AU - Claudi, R.

AU - Baruffolo, A.

AU - Ben-Ami, S.

AU - Biondi, F.

AU - Brucalassi, A.

AU - Cosentino, R.

AU - Ricci, D.

AU - D'Avanzo, P.

AU - Diner, O.

AU - Kuncarayakti, H.

AU - Rubin, A.

AU - Achrén, J.

AU - Araiza-Duran, J. A.

AU - Arcavi, I.

AU - Bianco, A.

AU - Cappellaro, E.

AU - Colapietro, M.

AU - Della Valle, M.

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 - Salasnich, B.

AU - Smartt, S.

AU - Turatto, M.

PY - 2018/7/6

Y1 - 2018/7/6

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.

KW - Cryogenics

KW - H2RG

KW - NTT

KW - Near Infrared

KW - SOXS

KW - Spectrograph

KW - Transient

UR - http://www.scopus.com/inward/record.url?scp=85052636448&partnerID=8YFLogxK

U2 - https://doi.org/10.1117/12.2311466

DO - https://doi.org/10.1117/12.2311466

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 NIR spectrograph for the new SOXS instrument at the NTT

Abstract

Publication series

Conference

Keywords

All Science Journal Classification (ASJC) codes

UN SDGs

Access to Document

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