CUBES: cassegrain U-band Brazil-ESO spectrograph

Abstract CUBES is a high-efficiency, medium-resolution (R∼20,000) ground based UV (300–400 nm) spectrograph, to be installed in the cassegrain focus of one of ESO’s VLT unit telescopes in 2017/18. The CUBES project is a joint venture between ESO and IAG/USP, and LNA/MCTI. CUBES will provide access t...
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Autor*in:	Barbuy, B. [verfasserIn] Bawden Macanhan, V. Bristow, P. Castilho, B. Dekker, H. Delabre, B. Diaz, M. Gneiding, C. Kerber, F. Kuntschner, H. La Mura, G. Maciel, W. Meléndez, J. Pasquini, L. Pereira, C. B. Petitjean, P. Reiss, R. Siqueira-Mello, C. Smiljanic, R. Vernet, J.

Format:	Artikel
Sprache:	Englisch

Erschienen:	2014

Schlagwörter:	Spectrograph High spectral resolution

Anmerkung:	© Springer Science+Business Media Dordrecht 2014

Übergeordnetes Werk:	Enthalten in: Astrophysics and space science - Springer Netherlands, 1968, 354(2014), 1 vom: 09. Juli, Seite 191-204
Übergeordnetes Werk:	volume:354 ; year:2014 ; number:1 ; day:09 ; month:07 ; pages:191-204

Links:	Volltext

DOI / URN:	10.1007/s10509-014-2039-z

Katalog-ID:	OLC2066276014

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520			\|a Abstract CUBES is a high-efficiency, medium-resolution (R∼20,000) ground based UV (300–400 nm) spectrograph, to be installed in the cassegrain focus of one of ESO’s VLT unit telescopes in 2017/18. The CUBES project is a joint venture between ESO and IAG/USP, and LNA/MCTI. CUBES will provide access to a wealth of new and relevant information for stellar as well as extragalactic sources. Main science cases include the study of beryllium and heavy elements in metal-poor stars, the direct determination of carbon, nitrogen and oxygen abundances by study of molecular bands in the UV range, as well as the study of active galactic nuclei and the quasar absorption lines. With a streamlined modern instrument design, high efficiency dispersing elements and UV-sensitive detectors, it will give a significant gain in sensitivity over existing ground based medium-high resolution spectrographs, enabling vastly increased sample sizes accessible to the astronomical community. We present here a brief overview of the project including the status, science cases and a discussion of the design options.
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spelling	10.1007/s10509-014-2039-z doi (DE-627)OLC2066276014 (DE-He213)s10509-014-2039-z-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Barbuy, B. verfasserin aut CUBES: cassegrain U-band Brazil-ESO spectrograph 2014 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media Dordrecht 2014 Abstract CUBES is a high-efficiency, medium-resolution (R∼20,000) ground based UV (300–400 nm) spectrograph, to be installed in the cassegrain focus of one of ESO’s VLT unit telescopes in 2017/18. The CUBES project is a joint venture between ESO and IAG/USP, and LNA/MCTI. CUBES will provide access to a wealth of new and relevant information for stellar as well as extragalactic sources. Main science cases include the study of beryllium and heavy elements in metal-poor stars, the direct determination of carbon, nitrogen and oxygen abundances by study of molecular bands in the UV range, as well as the study of active galactic nuclei and the quasar absorption lines. With a streamlined modern instrument design, high efficiency dispersing elements and UV-sensitive detectors, it will give a significant gain in sensitivity over existing ground based medium-high resolution spectrographs, enabling vastly increased sample sizes accessible to the astronomical community. We present here a brief overview of the project including the status, science cases and a discussion of the design options. Spectrograph High spectral resolution Bawden Macanhan, V. aut Bristow, P. aut Castilho, B. aut Dekker, H. aut Delabre, B. aut Diaz, M. aut Gneiding, C. aut Kerber, F. aut Kuntschner, H. aut La Mura, G. aut Maciel, W. aut Meléndez, J. aut Pasquini, L. aut Pereira, C. B. aut Petitjean, P. aut Reiss, R. aut Siqueira-Mello, C. aut Smiljanic, R. aut Vernet, J. aut Enthalten in Astrophysics and space science Springer Netherlands, 1968 354(2014), 1 vom: 09. Juli, Seite 191-204 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:354 year:2014 number:1 day:09 month:07 pages:191-204 https://doi.org/10.1007/s10509-014-2039-z lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4012 AR 354 2014 1 09 07 191-204
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language	English
source	Enthalten in Astrophysics and space science 354(2014), 1 vom: 09. Juli, Seite 191-204 volume:354 year:2014 number:1 day:09 month:07 pages:191-204
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authorswithroles_txt_mv	Barbuy, B. @@aut@@ Bawden Macanhan, V. @@aut@@ Bristow, P. @@aut@@ Castilho, B. @@aut@@ Dekker, H. @@aut@@ Delabre, B. @@aut@@ Diaz, M. @@aut@@ Gneiding, C. @@aut@@ Kerber, F. @@aut@@ Kuntschner, H. @@aut@@ La Mura, G. @@aut@@ Maciel, W. @@aut@@ Meléndez, J. @@aut@@ Pasquini, L. @@aut@@ Pereira, C. B. @@aut@@ Petitjean, P. @@aut@@ Reiss, R. @@aut@@ Siqueira-Mello, C. @@aut@@ Smiljanic, R. @@aut@@ Vernet, J. @@aut@@
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author	Barbuy, B.
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title	CUBES: cassegrain U-band Brazil-ESO spectrograph
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title_full	CUBES: cassegrain U-band Brazil-ESO spectrograph
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author_browse	Barbuy, B. Bawden Macanhan, V. Bristow, P. Castilho, B. Dekker, H. Delabre, B. Diaz, M. Gneiding, C. Kerber, F. Kuntschner, H. La Mura, G. Maciel, W. Meléndez, J. Pasquini, L. Pereira, C. B. Petitjean, P. Reiss, R. Siqueira-Mello, C. Smiljanic, R. Vernet, J.
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title_sort	cubes: cassegrain u-band brazil-eso spectrograph
title_auth	CUBES: cassegrain U-band Brazil-ESO spectrograph
abstract	Abstract CUBES is a high-efficiency, medium-resolution (R∼20,000) ground based UV (300–400 nm) spectrograph, to be installed in the cassegrain focus of one of ESO’s VLT unit telescopes in 2017/18. The CUBES project is a joint venture between ESO and IAG/USP, and LNA/MCTI. CUBES will provide access to a wealth of new and relevant information for stellar as well as extragalactic sources. Main science cases include the study of beryllium and heavy elements in metal-poor stars, the direct determination of carbon, nitrogen and oxygen abundances by study of molecular bands in the UV range, as well as the study of active galactic nuclei and the quasar absorption lines. With a streamlined modern instrument design, high efficiency dispersing elements and UV-sensitive detectors, it will give a significant gain in sensitivity over existing ground based medium-high resolution spectrographs, enabling vastly increased sample sizes accessible to the astronomical community. We present here a brief overview of the project including the status, science cases and a discussion of the design options. © Springer Science+Business Media Dordrecht 2014
abstractGer	Abstract CUBES is a high-efficiency, medium-resolution (R∼20,000) ground based UV (300–400 nm) spectrograph, to be installed in the cassegrain focus of one of ESO’s VLT unit telescopes in 2017/18. The CUBES project is a joint venture between ESO and IAG/USP, and LNA/MCTI. CUBES will provide access to a wealth of new and relevant information for stellar as well as extragalactic sources. Main science cases include the study of beryllium and heavy elements in metal-poor stars, the direct determination of carbon, nitrogen and oxygen abundances by study of molecular bands in the UV range, as well as the study of active galactic nuclei and the quasar absorption lines. With a streamlined modern instrument design, high efficiency dispersing elements and UV-sensitive detectors, it will give a significant gain in sensitivity over existing ground based medium-high resolution spectrographs, enabling vastly increased sample sizes accessible to the astronomical community. We present here a brief overview of the project including the status, science cases and a discussion of the design options. © Springer Science+Business Media Dordrecht 2014
abstract_unstemmed	Abstract CUBES is a high-efficiency, medium-resolution (R∼20,000) ground based UV (300–400 nm) spectrograph, to be installed in the cassegrain focus of one of ESO’s VLT unit telescopes in 2017/18. The CUBES project is a joint venture between ESO and IAG/USP, and LNA/MCTI. CUBES will provide access to a wealth of new and relevant information for stellar as well as extragalactic sources. Main science cases include the study of beryllium and heavy elements in metal-poor stars, the direct determination of carbon, nitrogen and oxygen abundances by study of molecular bands in the UV range, as well as the study of active galactic nuclei and the quasar absorption lines. With a streamlined modern instrument design, high efficiency dispersing elements and UV-sensitive detectors, it will give a significant gain in sensitivity over existing ground based medium-high resolution spectrographs, enabling vastly increased sample sizes accessible to the astronomical community. We present here a brief overview of the project including the status, science cases and a discussion of the design options. © Springer Science+Business Media Dordrecht 2014
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title_short	CUBES: cassegrain U-band Brazil-ESO spectrograph
url	https://doi.org/10.1007/s10509-014-2039-z
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author2	Bawden Macanhan, V. Bristow, P. Castilho, B. Dekker, H. Delabre, B. Diaz, M. Gneiding, C. Kerber, F. Kuntschner, H. La Mura, G. Maciel, W. Meléndez, J. Pasquini, L. Pereira, C. B. Petitjean, P. Reiss, R. Siqueira-Mello, C. Smiljanic, R. Vernet, J.
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