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

Resultado de la investigación: Conference contribution

4 Citas (Scopus)

Resumen

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.

Idioma originalEnglish
Título de la publicación alojadaGround-based and Airborne Instrumentation for Astronomy VII
EditoresLuc Simard, Luc Simard, Christopher J. Evans, Hideki Takami
EditorialSPIE
ISBN (versión impresa)9781510619579
DOI
EstadoPublished - 1 ene 2018
EventoGround-based and Airborne Instrumentation for Astronomy VII 2018 - Austin, United States
Duración: 10 jun 201814 jun 2018

Serie de la publicación

NombreProceedings of SPIE - The International Society for Optical Engineering
Volumen10702
ISSN (versión impresa)0277-786X
ISSN (versión digital)1996-756X

Conference

ConferenceGround-based and Airborne Instrumentation for Astronomy VII 2018
PaísUnited States
CiudadAustin
Período10/06/1814/06/18

Huella dactilar

Spectrographs
Spectrograph
spectrographs
Telescopes
Telescope
telescopes
Echelle
Thermal Radiation
Chile
Heat radiation
thermal radiation
European Southern Observatory
Range of data
Coverage
Wavelength
Filter
filters
wavelengths

ASJC Scopus subject areas

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

Citar esto

Vitali, F., Aliverti, M., Capasso, G., D'Alessio, F., Munari, M., Riva, M., ... Turatto, M. (2018). The NIR spectrograph for the new SOXS instrument at the NTT. En L. Simard, L. Simard, C. J. 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. https://doi.org/10.1117/12.2311466
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, J. A. ; 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. / The NIR spectrograph for the new SOXS instrument at the NTT. Ground-based and Airborne Instrumentation for Astronomy VII. editor / Luc Simard ; Luc Simard ; Christopher J. Evans ; Hideki Takami. SPIE, 2018. (Proceedings of SPIE - The International Society for Optical Engineering).
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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, Near Infrared, NTT, 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",
year = "2018",
month = "1",
day = "1",
doi = "10.1117/12.2311466",
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",

}

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. En L Simard, 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.; 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, J. A.; 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.

Ground-based and Airborne Instrumentation for Astronomy VII. ed. / Luc Simard; Luc Simard; Christopher J. Evans; Hideki Takami. SPIE, 2018. 1070228 (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 10702).

Resultado de la investigación: Conference contribution

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 - 2018/1/1

Y1 - 2018/1/1

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 - Near Infrared

KW - NTT

KW - SOXS

KW - Spectrograph

KW - Transient

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

U2 - 10.1117/12.2311466

DO - 10.1117/12.2311466

M3 - Conference contribution

AN - SCOPUS:85052636448

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 - Simard, Luc

A2 - Evans, Christopher J.

A2 - Takami, Hideki

PB - SPIE

ER -

Vitali F, Aliverti M, Capasso G, D'Alessio F, Munari M, Riva M y otros. The NIR spectrograph for the new SOXS instrument at the NTT. En Simard L, Simard L, Evans CJ, Takami H, editores, Ground-based and Airborne Instrumentation for Astronomy VII. SPIE. 2018. 1070228. (Proceedings of SPIE - The International Society for Optical Engineering). https://doi.org/10.1117/12.2311466