CUBES, the Cassegrain U-Band Efficient Spectrograph

S. Cristiani; J. M. Alcalá; S. H.P. Alencar; S. A. Balashev; N. Bastian; B. Barbuy; U. Battino; A. Calcines; G. Calderone; P. Cambianica; R. Carini; B. Carter; S. Cassisi; B. V. Castilho; G. Cescutti; N. Christlieb; R. Cirami; I. Coretti; R. Cooke; S. Covino; G. Cremonese; K. Cunha; G. Cupani; A. R. da Silva; V. De Caprio; A. De Cia; H. Dekker; V. D’Elia; G. De Silva; M. Diaz; P. Di Marcantonio; D. D’Auria; V. D’Odorico; A. Fitzsimmons; H. Ernandes; C. Evans; M. Franchini; M. Genoni; B. Gänsicke; R. E. Giribaldi; C. Gneiding; A. Grazian; C. J. Hansen; F. La Forgia; M. Landoni; M. Lazzarin; D. Lunney; W. Maciel; W. Marcolino; M. Marconi; A. Migliorini; C. Miller; P. Noterdaeme; C. Opitom; G. Pariani; B. Pilecki; S. Piranomonte; A. Quirrenbach; E. M.A. Redaelli; C. B. Pereira; S. Randich; S. Rossi; R. Sanchez-Janssen; W. Seifert; R. Smiljanic; C. Snodgrass; I. Stilz; J. Stürmer; E. Vanzella; P. Ventura; O. Verducci; C. Waring; S. Watson; M. Wells; D. Wright; T. Zafar; A. Zanutta

doi:10.1117/12.2629990

CUBES, the Cassegrain U-Band Efficient Spectrograph

S. Cristiani
, J. M. Alcalá
, S. H.P. Alencar
, S. A. Balashev
, N. Bastian
, B. Barbuy
, U. Battino
, A. Calcines
, G. Calderone
, P. Cambianica
, R. Carini
, B. Carter
, S. Cassisi
, B. V. Castilho
, G. Cescutti
, N. Christlieb
, R. Cirami
, I. Coretti
, R. Cooke
, S. Covino

G. Cremonese, K. Cunha, G. Cupani, A. R. da Silva, V. De Caprio, A. De Cia, H. Dekker, V. D’Elia, G. De Silva, M. Diaz, P. Di Marcantonio, D. D’Auria, V. D’Odorico, A. Fitzsimmons, H. Ernandes, C. Evans, M. Franchini, M. Genoni, B. Gänsicke, R. E. Giribaldi, C. Gneiding, A. Grazian, C. J. Hansen, F. La Forgia, M. Landoni, M. Lazzarin, D. Lunney, W. Maciel, W. Marcolino, M. Marconi, A. Migliorini, C. Miller, P. Noterdaeme, C. Opitom, G. Pariani, B. Pilecki, S. Piranomonte, A. Quirrenbach, E. M.A. Redaelli, C. B. Pereira, S. Randich, S. Rossi, R. Sanchez-Janssen, W. Seifert, R. Smiljanic, C. Snodgrass, I. Stilz, J. Stürmer, E. Vanzella, P. Ventura, O. Verducci, C. Waring, S. Watson, M. Wells, D. Wright, T. Zafar, A. Zanutta

Steward Observatory

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

2 Scopus citations

Abstract

In the era of Extremely Large Telescopes, the current generation of 8-10m facilities are likely to remain competitive at ground-UV wavelengths for the foreseeable future. The Cassegrain U-Band Efficient Spectrograph (CUBES) has been designed to provide high-efficiency (> 40%) observations in the near UV (305-400 nm requirement, 300-420 nm goal) at a spectral resolving power of R > 20, 000 (with a lower-resolution, sky-limited mode of R ∼ 7, 000). With the design focusing on maximizing the instrument throughput (ensuring a Signal to Noise Ratio (SNR)∼ 20 per high-resolution element at 313 nm for U ∼ 18.5 mag objects in 1h of observations), it will offer new possibilities in many fields of astrophysics, providing access to key lines of stellar spectra: a tremendous diversity of iron-peak and heavy elements, lighter elements (in particular Beryllium) and light-element molecules (CO, CN, OH), as well as Balmer lines and the Balmer jump (particularly important for young stellar objects). The UV range is also critical in extragalactic studies: the circumgalactic medium of distant galaxies, the contribution of different types of sources to the cosmic UV background, the measurement of H₂ and primordial Deuterium in a regime of relatively transparent intergalactic medium, and follow-up of explosive transients. The CUBES project completed a Phase A conceptual design in June 2021 and has now entered the detailed design and construction phase. First science operations are planned for 2028.

Original language	English (US)
Title of host publication	Ground-based and Airborne Instrumentation for Astronomy IX
Editors	Christopher J. Evans, Julia J. Bryant, Kentaro Motohara
Publisher	SPIE
ISBN (Electronic)	9781510653498
DOIs	https://doi.org/10.1117/12.2629990
State	Published - 2022
Event	Ground-based and Airborne Instrumentation for Astronomy IX 2022 - Montreal, Canada Duration: Jul 17 2022 → Jul 22 2022

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	12184
ISSN (Print)	0277-786X
ISSN (Electronic)	1996-756X

Conference

Conference	Ground-based and Airborne Instrumentation for Astronomy IX 2022
Country/Territory	Canada
City	Montreal
Period	7/17/22 → 7/22/22

Keywords

CUBES
ELT
VLT
efficient U-band spectrograph

ASJC Scopus subject areas

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

Access to Document

10.1117/12.2629990

Cite this

Cristiani, S., Alcalá, J. M., Alencar, S. H. P., Balashev, S. A., Bastian, N., Barbuy, B., Battino, U., Calcines, A., Calderone, G., Cambianica, P., Carini, R., Carter, B., Cassisi, S., Castilho, B. V., Cescutti, G., Christlieb, N., Cirami, R., Coretti, I., Cooke, R., ... Zanutta, A. (2022). CUBES, the Cassegrain U-Band Efficient Spectrograph. In C. J. Evans, J. J. Bryant, & K. Motohara (Eds.), Ground-based and Airborne Instrumentation for Astronomy IX Article 121840A (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 12184). SPIE. https://doi.org/10.1117/12.2629990

CUBES, the Cassegrain U-Band Efficient Spectrograph. / Cristiani, S.; Alcalá, J. M.; Alencar, S. H.P. et al.
Ground-based and Airborne Instrumentation for Astronomy IX. ed. / Christopher J. Evans; Julia J. Bryant; Kentaro Motohara. SPIE, 2022. 121840A (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 12184).

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

Cristiani, S, Alcalá, JM, Alencar, SHP, Balashev, SA, Bastian, N, Barbuy, B, Battino, U, Calcines, A, Calderone, G, Cambianica, P, Carini, R, Carter, B, Cassisi, S, Castilho, BV, Cescutti, G, Christlieb, N, Cirami, R, Coretti, I, Cooke, R, Covino, S, Cremonese, G, Cunha, K, Cupani, G, da Silva, AR, De Caprio, V, De Cia, A, Dekker, H, D’Elia, V, De Silva, G, Diaz, M, Di Marcantonio, P, D’Auria, D, D’Odorico, V, Fitzsimmons, A, Ernandes, H, Evans, C, Franchini, M, Genoni, M, Gänsicke, B, Giribaldi, RE, Gneiding, C, Grazian, A, Hansen, CJ, La Forgia, F, Landoni, M, Lazzarin, M, Lunney, D, Maciel, W, Marcolino, W, Marconi, M, Migliorini, A, Miller, C, Noterdaeme, P, Opitom, C, Pariani, G, Pilecki, B, Piranomonte, S, Quirrenbach, A, Redaelli, EMA, Pereira, CB, Randich, S, Rossi, S, Sanchez-Janssen, R, Seifert, W, Smiljanic, R, Snodgrass, C, Stilz, I, Stürmer, J, Vanzella, E, Ventura, P, Verducci, O, Waring, C, Watson, S, Wells, M, Wright, D, Zafar, T & Zanutta, A 2022, CUBES, the Cassegrain U-Band Efficient Spectrograph. in CJ Evans, JJ Bryant & K Motohara (eds), Ground-based and Airborne Instrumentation for Astronomy IX., 121840A, Proceedings of SPIE - The International Society for Optical Engineering, vol. 12184, SPIE, Ground-based and Airborne Instrumentation for Astronomy IX 2022, Montreal, Canada, 7/17/22. https://doi.org/10.1117/12.2629990

@inproceedings{5e49cffcc51c4319a9d82c4b1ed1530a,

title = "CUBES, the Cassegrain U-Band Efficient Spectrograph",

abstract = "In the era of Extremely Large Telescopes, the current generation of 8-10m facilities are likely to remain competitive at ground-UV wavelengths for the foreseeable future. The Cassegrain U-Band Efficient Spectrograph (CUBES) has been designed to provide high-efficiency (> 40\%) observations in the near UV (305-400 nm requirement, 300-420 nm goal) at a spectral resolving power of R > 20, 000 (with a lower-resolution, sky-limited mode of R ∼ 7, 000). With the design focusing on maximizing the instrument throughput (ensuring a Signal to Noise Ratio (SNR)∼ 20 per high-resolution element at 313 nm for U ∼ 18.5 mag objects in 1h of observations), it will offer new possibilities in many fields of astrophysics, providing access to key lines of stellar spectra: a tremendous diversity of iron-peak and heavy elements, lighter elements (in particular Beryllium) and light-element molecules (CO, CN, OH), as well as Balmer lines and the Balmer jump (particularly important for young stellar objects). The UV range is also critical in extragalactic studies: the circumgalactic medium of distant galaxies, the contribution of different types of sources to the cosmic UV background, the measurement of H2 and primordial Deuterium in a regime of relatively transparent intergalactic medium, and follow-up of explosive transients. The CUBES project completed a Phase A conceptual design in June 2021 and has now entered the detailed design and construction phase. First science operations are planned for 2028.",

keywords = "CUBES, ELT, VLT, efficient U-band spectrograph",

author = "S. Cristiani and Alcal{\'a}, \{J. M.\} and Alencar, \{S. H.P.\} and Balashev, \{S. A.\} and N. Bastian and B. Barbuy and U. Battino and A. Calcines and G. Calderone and P. Cambianica and R. Carini and B. Carter and S. Cassisi and Castilho, \{B. V.\} and G. Cescutti and N. Christlieb and R. Cirami and I. Coretti and R. Cooke and S. Covino and G. Cremonese and K. Cunha and G. Cupani and \{da Silva\}, \{A. R.\} and \{De Caprio\}, V. and \{De Cia\}, A. and H. Dekker and V. D{\textquoteright}Elia and \{De Silva\}, G. and M. Diaz and \{Di Marcantonio\}, P. and D. D{\textquoteright}Auria and V. D{\textquoteright}Odorico and A. Fitzsimmons and H. Ernandes and C. Evans and M. Franchini and M. Genoni and B. G{\"a}nsicke and Giribaldi, \{R. E.\} and C. Gneiding and A. Grazian and Hansen, \{C. J.\} and \{La Forgia\}, F. and M. Landoni and M. Lazzarin and D. Lunney and W. Maciel and W. Marcolino and M. Marconi and A. Migliorini and C. Miller and P. Noterdaeme and C. Opitom and G. Pariani and B. Pilecki and S. Piranomonte and A. Quirrenbach and Redaelli, \{E. M.A.\} and Pereira, \{C. B.\} and S. Randich and S. Rossi and R. Sanchez-Janssen and W. Seifert and R. Smiljanic and C. Snodgrass and I. Stilz and J. St{\"u}rmer and E. Vanzella and P. Ventura and O. Verducci and C. Waring and S. Watson and M. Wells and D. Wright and T. Zafar and A. Zanutta",

note = "Publisher Copyright: {\textcopyright} 2022 SPIE.; Ground-based and Airborne Instrumentation for Astronomy IX 2022 ; Conference date: 17-07-2022 Through 22-07-2022",

year = "2022",

doi = "10.1117/12.2629990",

language = "English (US)",

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

publisher = "SPIE",

editor = "Evans, \{Christopher J.\} and Bryant, \{Julia J.\} and Kentaro Motohara",

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

}

TY - GEN

T1 - CUBES, the Cassegrain U-Band Efficient Spectrograph

AU - Cristiani, S.

AU - Alcalá, J. M.

AU - Alencar, S. H.P.

AU - Balashev, S. A.

AU - Bastian, N.

AU - Barbuy, B.

AU - Battino, U.

AU - Calcines, A.

AU - Calderone, G.

AU - Cambianica, P.

AU - Carini, R.

AU - Carter, B.

AU - Cassisi, S.

AU - Castilho, B. V.

AU - Cescutti, G.

AU - Christlieb, N.

AU - Cirami, R.

AU - Coretti, I.

AU - Cooke, R.

AU - Covino, S.

AU - Cremonese, G.

AU - Cunha, K.

AU - Cupani, G.

AU - da Silva, A. R.

AU - De Caprio, V.

AU - De Cia, A.

AU - Dekker, H.

AU - D’Elia, V.

AU - De Silva, G.

AU - Diaz, M.

AU - Di Marcantonio, P.

AU - D’Auria, D.

AU - D’Odorico, V.

AU - Fitzsimmons, A.

AU - Ernandes, H.

AU - Evans, C.

AU - Franchini, M.

AU - Genoni, M.

AU - Gänsicke, B.

AU - Giribaldi, R. E.

AU - Gneiding, C.

AU - Grazian, A.

AU - Hansen, C. J.

AU - La Forgia, F.

AU - Landoni, M.

AU - Lazzarin, M.

AU - Lunney, D.

AU - Maciel, W.

AU - Marcolino, W.

AU - Marconi, M.

AU - Migliorini, A.

AU - Miller, C.

AU - Noterdaeme, P.

AU - Opitom, C.

AU - Pariani, G.

AU - Pilecki, B.

AU - Piranomonte, S.

AU - Quirrenbach, A.

AU - Redaelli, E. M.A.

AU - Pereira, C. B.

AU - Randich, S.

AU - Rossi, S.

AU - Sanchez-Janssen, R.

AU - Seifert, W.

AU - Smiljanic, R.

AU - Snodgrass, C.

AU - Stilz, I.

AU - Stürmer, J.

AU - Vanzella, E.

AU - Ventura, P.

AU - Verducci, O.

AU - Waring, C.

AU - Watson, S.

AU - Wells, M.

AU - Wright, D.

AU - Zafar, T.

AU - Zanutta, A.

PY - 2022

Y1 - 2022

N2 - In the era of Extremely Large Telescopes, the current generation of 8-10m facilities are likely to remain competitive at ground-UV wavelengths for the foreseeable future. The Cassegrain U-Band Efficient Spectrograph (CUBES) has been designed to provide high-efficiency (> 40%) observations in the near UV (305-400 nm requirement, 300-420 nm goal) at a spectral resolving power of R > 20, 000 (with a lower-resolution, sky-limited mode of R ∼ 7, 000). With the design focusing on maximizing the instrument throughput (ensuring a Signal to Noise Ratio (SNR)∼ 20 per high-resolution element at 313 nm for U ∼ 18.5 mag objects in 1h of observations), it will offer new possibilities in many fields of astrophysics, providing access to key lines of stellar spectra: a tremendous diversity of iron-peak and heavy elements, lighter elements (in particular Beryllium) and light-element molecules (CO, CN, OH), as well as Balmer lines and the Balmer jump (particularly important for young stellar objects). The UV range is also critical in extragalactic studies: the circumgalactic medium of distant galaxies, the contribution of different types of sources to the cosmic UV background, the measurement of H2 and primordial Deuterium in a regime of relatively transparent intergalactic medium, and follow-up of explosive transients. The CUBES project completed a Phase A conceptual design in June 2021 and has now entered the detailed design and construction phase. First science operations are planned for 2028.

AB - In the era of Extremely Large Telescopes, the current generation of 8-10m facilities are likely to remain competitive at ground-UV wavelengths for the foreseeable future. The Cassegrain U-Band Efficient Spectrograph (CUBES) has been designed to provide high-efficiency (> 40%) observations in the near UV (305-400 nm requirement, 300-420 nm goal) at a spectral resolving power of R > 20, 000 (with a lower-resolution, sky-limited mode of R ∼ 7, 000). With the design focusing on maximizing the instrument throughput (ensuring a Signal to Noise Ratio (SNR)∼ 20 per high-resolution element at 313 nm for U ∼ 18.5 mag objects in 1h of observations), it will offer new possibilities in many fields of astrophysics, providing access to key lines of stellar spectra: a tremendous diversity of iron-peak and heavy elements, lighter elements (in particular Beryllium) and light-element molecules (CO, CN, OH), as well as Balmer lines and the Balmer jump (particularly important for young stellar objects). The UV range is also critical in extragalactic studies: the circumgalactic medium of distant galaxies, the contribution of different types of sources to the cosmic UV background, the measurement of H2 and primordial Deuterium in a regime of relatively transparent intergalactic medium, and follow-up of explosive transients. The CUBES project completed a Phase A conceptual design in June 2021 and has now entered the detailed design and construction phase. First science operations are planned for 2028.

KW - CUBES

KW - ELT

KW - VLT

KW - efficient U-band spectrograph

UR - https://www.scopus.com/pages/publications/85140088830

UR - https://www.scopus.com/pages/publications/85140088830#tab=citedBy

U2 - 10.1117/12.2629990

DO - 10.1117/12.2629990

M3 - Conference contribution

AN - SCOPUS:85140088830

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

BT - Ground-based and Airborne Instrumentation for Astronomy IX

A2 - Evans, Christopher J.

A2 - Bryant, Julia J.

A2 - Motohara, Kentaro

PB - SPIE

T2 - Ground-based and Airborne Instrumentation for Astronomy IX 2022

Y2 - 17 July 2022 through 22 July 2022

ER -

CUBES, the Cassegrain U-Band Efficient Spectrograph

Abstract

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Keywords

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