MOONS: The multi-object optical and near-infrared spectrograph for the vlt

M. Cirasuolo; J. Afonso; M. Carollo; H. Flores; R. Maiolino; E. Oliva; S. Paltani; Leonardo Vanzi; Christopher Evans; M. Abreu; David Atkinson; C. Babusiaux; Steven Beard; F. Bauer; M. Bellazzini; Ralf Bender; P. Best; N. Bezawada; P. Bonifacio; A. Bragaglia; I. Bryson; D. Busher; A. Cabral; K. Caputi; M. Centrone; F. Chemla; A. Cimatti; M. R. Cioni; G. Clementini; J. Coelho; D. Crnojevic; E. Daddi; J. Dunlop; S. Eales; S. Feltzing; A. Ferguson; M. Fisher; A. Fontana; J. Fynbo; B. Garilli; G. Gilmore; A. Glauser; I. Guinouard; F. Hammer; P. Hastings; A. Hess; R. Ivison; P. Jagourel; M. Jarvis; L. Kaper; G. Kauffman; A. T. Kitching; A. Lawrence; D. Lee; B. Lemasle; G. Licausi; S. Lilly; D. Lorenzetti; D. Lunney; F. Mannucci; R. McLure; D. Minniti; D. Montgomery; B. Muschielok; K. Nandra; R. Navarro; P. Norberg; S. Oliver; L. Origlia; N. Padilla; J. Peacock; F. Pedicini; J. Peng; L. Pentericci; J. Pragt; M. Puech; S. Randich; P. Rees; A. Renzini; N. Ryde; M. Rodrigues; I. Roseboom; F. Royer; R. Saglia; A. Sanchez; R. Schiavon; H. Schnetler; D. Sobral; R. Speziali; D. Sun; R. Stuik; A. Taylor; S. Todd; E. Tolstoy; M. Torres; M. Tosi; E. Vanzella; L. Venema; F. Vitali; M. Wegner; M. Wells; V. Wild; G. Wright; G. Zamorani; M. Zoccali

doi:10.1117/12.2056012

MOONS: The multi-object optical and near-infrared spectrograph for the vlt

M. Cirasuolo, J. Afonso, M. Carollo, H. Flores, R. Maiolino, E. Oliva, S. Paltani, Leonardo Vanzi, Christopher Evans, M. Abreu, David Atkinson, C. Babusiaux, Steven Beard, F. Bauer, M. Bellazzini, Ralf Bender, P. Best, N. Bezawada, P. Bonifacio, A. BragagliaI. Bryson, D. Busher, A. Cabral, K. Caputi, M. Centrone, F. Chemla, A. Cimatti, M. R. Cioni, G. Clementini, J. Coelho, D. Crnojevic, E. Daddi, J. Dunlop, S. Eales, S. Feltzing, A. Ferguson, M. Fisher, A. Fontana, J. Fynbo, B. Garilli, G. Gilmore, A. Glauser, I. Guinouard, F. Hammer, P. Hastings, A. Hess, R. Ivison, P. Jagourel, M. Jarvis, L. Kaper, G. Kauffman, A. T. Kitching, A. Lawrence, D. Lee, B. Lemasle, G. Licausi, S. Lilly, D. Lorenzetti, D. Lunney, F. Mannucci, R. McLure, D. Minniti, D. Montgomery, B. Muschielok, K. Nandra, R. Navarro, P. Norberg, S. Oliver, L. Origlia, N. Padilla, J. Peacock, F. Pedicini, J. Peng, L. Pentericci, J. Pragt, M. Puech, S. Randich, P. Rees, A. Renzini, N. Ryde, M. Rodrigues, I. Roseboom, F. Royer, R. Saglia, A. Sanchez, R. Schiavon, H. Schnetler, D. Sobral, R. Speziali, D. Sun, R. Stuik, A. Taylor, S. Todd, E. Tolstoy, M. Torres, M. Tosi, E. Vanzella, L. Venema, F. Vitali, M. Wegner, M. Wells, V. Wild, G. Wright, G. Zamorani, M. Zoccali

Facultad Ciencias Exactas

Producción científica: Contribución a los tipos de informe/libro › Contribución a la conferencia › revisión exhaustiva

86 Citas (Scopus)

Resumen

MOONS is a new Multi-Object Optical and Near-infrared Spectrograph selected by ESO as a third generation instrument for the Very Large Telescope (VLT). The grasp of the large collecting area offered by the VLT (8.2m diameter), combined with the large multiplex and wavelength coverage (optical to near-IR: 0.8μm - 1.8μm) of MOONS will provide the European astronomical community with a powerful, unique instrument able to pioneer a wide range of Galactic, Extragalactic and Cosmological studies and provide crucial follow-up for major facilities such as Gaia, VISTA, Euclid and LSST. MOONS has the observational power needed to unveil galaxy formation and evolution over the entire history of the Universe, from stars in our Milky Way, through the redshift desert, and up to the epoch of very first galaxies and re-ionization of the Universe at redshift z>8-9, just few million years after the Big Bang. On a timescale of 5 years of observations, MOONS will provide high quality spectra for >3M stars in our Galaxy and the local group, and for 1-2M galaxies at z>1 (SDSS-like survey), promising to revolutionise our understanding of the Universe. The baseline design consists of ∼1000 fibers deployable over a field of view of ∼500 square arcmin, the largest patrol field offered by the Nasmyth focus at the VLT. The total wavelength coverage is 0.8μm-1.8μm and two resolution modes: medium resolution and high resolution. In the medium resolution mode (R∼4,000-6,000) the entire wavelength range 0.8μm-1.8μm is observed simultaneously, while the high resolution mode covers simultaneously three selected spectral regions: one around the CaII triplet (at R∼8,000) to measure radial velocities, and two regions at R∼20,000 one in the J-band and one in the H-band, for detailed measurements of chemical abundances.

Idioma original	Inglés
Título de la publicación alojada	Ground-Based and Airborne Instrumentation for Astronomy V
Editores	Suzanne K. Ramsay, Ian S. McLean, Hideki Takami
Editorial	SPIE
ISBN (versión digital)	9780819496157
DOI	https://doi.org/10.1117/12.2056012
Estado	Publicada - 2014
Evento	Ground-Based and Airborne Instrumentation for Astronomy V - Montreal, Canadá Duración: 22 jun. 2014 → 26 jun. 2014

Serie de la publicación

Nombre	Proceedings of SPIE - The International Society for Optical Engineering
Volumen	9147
ISSN (versión impresa)	0277-786X
ISSN (versión digital)	1996-756X

Otros

Otros	Ground-Based and Airborne Instrumentation for Astronomy V
País/Territorio	Canadá
Ciudad	Montreal
Período	22/06/14 → 26/06/14

Áreas temáticas de ASJC Scopus

Materiales electrónicos, ópticos y magnéticos
Física de la materia condensada
Informática aplicada
Matemáticas aplicadas
Ingeniería eléctrica y electrónica

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10.1117/12.2056012

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Cirasuolo, M., Afonso, J., Carollo, M., Flores, H., Maiolino, R., Oliva, E., Paltani, S., Vanzi, L., Evans, C., Abreu, M., Atkinson, D., Babusiaux, C., Beard, S., Bauer, F., Bellazzini, M., Bender, R., Best, P., Bezawada, N., Bonifacio, P., ... Zoccali, M. (2014). MOONS: The multi-object optical and near-infrared spectrograph for the vlt. En S. K. Ramsay, I. S. McLean, & H. Takami (Eds.), Ground-Based and Airborne Instrumentation for Astronomy V Artículo 91470N (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 9147). SPIE. https://doi.org/10.1117/12.2056012

@inproceedings{857db3fd9b4d44a493ff866ba8f05b10,

title = "MOONS: The multi-object optical and near-infrared spectrograph for the vlt",

abstract = "MOONS is a new Multi-Object Optical and Near-infrared Spectrograph selected by ESO as a third generation instrument for the Very Large Telescope (VLT). The grasp of the large collecting area offered by the VLT (8.2m diameter), combined with the large multiplex and wavelength coverage (optical to near-IR: 0.8μm - 1.8μm) of MOONS will provide the European astronomical community with a powerful, unique instrument able to pioneer a wide range of Galactic, Extragalactic and Cosmological studies and provide crucial follow-up for major facilities such as Gaia, VISTA, Euclid and LSST. MOONS has the observational power needed to unveil galaxy formation and evolution over the entire history of the Universe, from stars in our Milky Way, through the redshift desert, and up to the epoch of very first galaxies and re-ionization of the Universe at redshift z>8-9, just few million years after the Big Bang. On a timescale of 5 years of observations, MOONS will provide high quality spectra for >3M stars in our Galaxy and the local group, and for 1-2M galaxies at z>1 (SDSS-like survey), promising to revolutionise our understanding of the Universe. The baseline design consists of ∼1000 fibers deployable over a field of view of ∼500 square arcmin, the largest patrol field offered by the Nasmyth focus at the VLT. The total wavelength coverage is 0.8μm-1.8μm and two resolution modes: medium resolution and high resolution. In the medium resolution mode (R∼4,000-6,000) the entire wavelength range 0.8μm-1.8μm is observed simultaneously, while the high resolution mode covers simultaneously three selected spectral regions: one around the CaII triplet (at R∼8,000) to measure radial velocities, and two regions at R∼20,000 one in the J-band and one in the H-band, for detailed measurements of chemical abundances.",

keywords = "instrumentation: VLT spectrograph - galaxies: evolution, stellar content",

author = "M. Cirasuolo and J. Afonso and M. Carollo and H. Flores and R. Maiolino and E. Oliva and S. Paltani and Leonardo Vanzi and Christopher Evans and M. Abreu and David Atkinson and C. Babusiaux and Steven Beard and F. Bauer and M. Bellazzini and Ralf Bender and P. Best and N. Bezawada and P. Bonifacio and A. Bragaglia and I. Bryson and D. Busher and A. Cabral and K. Caputi and M. Centrone and F. Chemla and A. Cimatti and Cioni, {M. R.} and G. Clementini and J. Coelho and D. Crnojevic and E. Daddi and J. Dunlop and S. Eales and S. Feltzing and A. Ferguson and M. Fisher and A. Fontana and J. Fynbo and B. Garilli and G. Gilmore and A. Glauser and I. Guinouard and F. Hammer and P. Hastings and A. Hess and R. Ivison and P. Jagourel and M. Jarvis and L. Kaper and G. Kauffman and Kitching, {A. T.} and A. Lawrence and D. Lee and B. Lemasle and G. Licausi and S. Lilly and D. Lorenzetti and D. Lunney and F. Mannucci and R. McLure and D. Minniti and D. Montgomery and B. Muschielok and K. Nandra and R. Navarro and P. Norberg and S. Oliver and L. Origlia and N. Padilla and J. Peacock and F. Pedicini and J. Peng and L. Pentericci and J. Pragt and M. Puech and S. Randich and P. Rees and A. Renzini and N. Ryde and M. Rodrigues and I. Roseboom and F. Royer and R. Saglia and A. Sanchez and R. Schiavon and H. Schnetler and D. Sobral and R. Speziali and D. Sun and R. Stuik and A. Taylor and S. Todd and E. Tolstoy and M. Torres and M. Tosi and E. Vanzella and L. Venema and F. Vitali and M. Wegner and M. Wells and V. Wild and G. Wright and G. Zamorani and M. Zoccali",

note = "Publisher Copyright: {\textcopyright} 2014 SPIE.; Ground-Based and Airborne Instrumentation for Astronomy V ; Conference date: 22-06-2014 Through 26-06-2014",

year = "2014",

doi = "10.1117/12.2056012",

language = "English",

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

publisher = "SPIE",

editor = "Ramsay, {Suzanne K.} and McLean, {Ian S.} and Hideki Takami",

booktitle = "Ground-Based and Airborne Instrumentation for Astronomy V",

}

Cirasuolo, M, Afonso, J, Carollo, M, Flores, H, Maiolino, R, Oliva, E, Paltani, S, Vanzi, L, Evans, C, Abreu, M, Atkinson, D, Babusiaux, C, Beard, S, Bauer, F, Bellazzini, M, Bender, R, Best, P, Bezawada, N, Bonifacio, P, Bragaglia, A, Bryson, I, Busher, D, Cabral, A, Caputi, K, Centrone, M, Chemla, F, Cimatti, A, Cioni, MR, Clementini, G, Coelho, J, Crnojevic, D, Daddi, E, Dunlop, J, Eales, S, Feltzing, S, Ferguson, A, Fisher, M, Fontana, A, Fynbo, J, Garilli, B, Gilmore, G, Glauser, A, Guinouard, I, Hammer, F, Hastings, P, Hess, A, Ivison, R, Jagourel, P, Jarvis, M, Kaper, L, Kauffman, G, Kitching, AT, Lawrence, A, Lee, D, Lemasle, B, Licausi, G, Lilly, S, Lorenzetti, D, Lunney, D, Mannucci, F, McLure, R, Minniti, D, Montgomery, D, Muschielok, B, Nandra, K, Navarro, R, Norberg, P, Oliver, S, Origlia, L, Padilla, N, Peacock, J, Pedicini, F, Peng, J, Pentericci, L, Pragt, J, Puech, M, Randich, S, Rees, P, Renzini, A, Ryde, N, Rodrigues, M, Roseboom, I, Royer, F, Saglia, R, Sanchez, A, Schiavon, R, Schnetler, H, Sobral, D, Speziali, R, Sun, D, Stuik, R, Taylor, A, Todd, S, Tolstoy, E, Torres, M, Tosi, M, Vanzella, E, Venema, L, Vitali, F, Wegner, M, Wells, M, Wild, V, Wright, G, Zamorani, G & Zoccali, M 2014, MOONS: The multi-object optical and near-infrared spectrograph for the vlt. En SK Ramsay, IS McLean & H Takami (eds.), Ground-Based and Airborne Instrumentation for Astronomy V., 91470N, Proceedings of SPIE - The International Society for Optical Engineering, vol. 9147, SPIE, Ground-Based and Airborne Instrumentation for Astronomy V, Montreal, Canadá, 22/06/14. https://doi.org/10.1117/12.2056012

MOONS: The multi-object optical and near-infrared spectrograph for the vlt. / Cirasuolo, M.; Afonso, J.; Carollo, M. et al.
Ground-Based and Airborne Instrumentation for Astronomy V. ed. / Suzanne K. Ramsay; Ian S. McLean; Hideki Takami. SPIE, 2014. 91470N (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 9147).

Producción científica: Contribución a los tipos de informe/libro › Contribución a la conferencia › revisión exhaustiva

TY - GEN

T1 - MOONS

T2 - Ground-Based and Airborne Instrumentation for Astronomy V

AU - Cirasuolo, M.

AU - Afonso, J.

AU - Carollo, M.

AU - Flores, H.

AU - Maiolino, R.

AU - Oliva, E.

AU - Paltani, S.

AU - Vanzi, Leonardo

AU - Evans, Christopher

AU - Abreu, M.

AU - Atkinson, David

AU - Babusiaux, C.

AU - Beard, Steven

AU - Bauer, F.

AU - Bellazzini, M.

AU - Bender, Ralf

AU - Best, P.

AU - Bezawada, N.

AU - Bonifacio, P.

AU - Bragaglia, A.

AU - Bryson, I.

AU - Busher, D.

AU - Cabral, A.

AU - Caputi, K.

AU - Centrone, M.

AU - Chemla, F.

AU - Cimatti, A.

AU - Cioni, M. R.

AU - Clementini, G.

AU - Coelho, J.

AU - Crnojevic, D.

AU - Daddi, E.

AU - Dunlop, J.

AU - Eales, S.

AU - Feltzing, S.

AU - Ferguson, A.

AU - Fisher, M.

AU - Fontana, A.

AU - Fynbo, J.

AU - Garilli, B.

AU - Gilmore, G.

AU - Glauser, A.

AU - Guinouard, I.

AU - Hammer, F.

AU - Hastings, P.

AU - Hess, A.

AU - Ivison, R.

AU - Jagourel, P.

AU - Jarvis, M.

AU - Kaper, L.

AU - Kauffman, G.

AU - Kitching, A. T.

AU - Lawrence, A.

AU - Lee, D.

AU - Lemasle, B.

AU - Licausi, G.

AU - Lilly, S.

AU - Lorenzetti, D.

AU - Lunney, D.

AU - Mannucci, F.

AU - McLure, R.

AU - Minniti, D.

AU - Montgomery, D.

AU - Muschielok, B.

AU - Nandra, K.

AU - Navarro, R.

AU - Norberg, P.

AU - Oliver, S.

AU - Origlia, L.

AU - Padilla, N.

AU - Peacock, J.

AU - Pedicini, F.

AU - Peng, J.

AU - Pentericci, L.

AU - Pragt, J.

AU - Puech, M.

AU - Randich, S.

AU - Rees, P.

AU - Renzini, A.

AU - Ryde, N.

AU - Rodrigues, M.

AU - Roseboom, I.

AU - Royer, F.

AU - Saglia, R.

AU - Sanchez, A.

AU - Schiavon, R.

AU - Schnetler, H.

AU - Sobral, D.

AU - Speziali, R.

AU - Sun, D.

AU - Stuik, R.

AU - Taylor, A.

AU - Todd, S.

AU - Tolstoy, E.

AU - Torres, M.

AU - Tosi, M.

AU - Vanzella, E.

AU - Venema, L.

AU - Vitali, F.

AU - Wegner, M.

AU - Wells, M.

AU - Wild, V.

AU - Wright, G.

AU - Zamorani, G.

AU - Zoccali, M.

PY - 2014

Y1 - 2014

N2 - MOONS is a new Multi-Object Optical and Near-infrared Spectrograph selected by ESO as a third generation instrument for the Very Large Telescope (VLT). The grasp of the large collecting area offered by the VLT (8.2m diameter), combined with the large multiplex and wavelength coverage (optical to near-IR: 0.8μm - 1.8μm) of MOONS will provide the European astronomical community with a powerful, unique instrument able to pioneer a wide range of Galactic, Extragalactic and Cosmological studies and provide crucial follow-up for major facilities such as Gaia, VISTA, Euclid and LSST. MOONS has the observational power needed to unveil galaxy formation and evolution over the entire history of the Universe, from stars in our Milky Way, through the redshift desert, and up to the epoch of very first galaxies and re-ionization of the Universe at redshift z>8-9, just few million years after the Big Bang. On a timescale of 5 years of observations, MOONS will provide high quality spectra for >3M stars in our Galaxy and the local group, and for 1-2M galaxies at z>1 (SDSS-like survey), promising to revolutionise our understanding of the Universe. The baseline design consists of ∼1000 fibers deployable over a field of view of ∼500 square arcmin, the largest patrol field offered by the Nasmyth focus at the VLT. The total wavelength coverage is 0.8μm-1.8μm and two resolution modes: medium resolution and high resolution. In the medium resolution mode (R∼4,000-6,000) the entire wavelength range 0.8μm-1.8μm is observed simultaneously, while the high resolution mode covers simultaneously three selected spectral regions: one around the CaII triplet (at R∼8,000) to measure radial velocities, and two regions at R∼20,000 one in the J-band and one in the H-band, for detailed measurements of chemical abundances.

AB - MOONS is a new Multi-Object Optical and Near-infrared Spectrograph selected by ESO as a third generation instrument for the Very Large Telescope (VLT). The grasp of the large collecting area offered by the VLT (8.2m diameter), combined with the large multiplex and wavelength coverage (optical to near-IR: 0.8μm - 1.8μm) of MOONS will provide the European astronomical community with a powerful, unique instrument able to pioneer a wide range of Galactic, Extragalactic and Cosmological studies and provide crucial follow-up for major facilities such as Gaia, VISTA, Euclid and LSST. MOONS has the observational power needed to unveil galaxy formation and evolution over the entire history of the Universe, from stars in our Milky Way, through the redshift desert, and up to the epoch of very first galaxies and re-ionization of the Universe at redshift z>8-9, just few million years after the Big Bang. On a timescale of 5 years of observations, MOONS will provide high quality spectra for >3M stars in our Galaxy and the local group, and for 1-2M galaxies at z>1 (SDSS-like survey), promising to revolutionise our understanding of the Universe. The baseline design consists of ∼1000 fibers deployable over a field of view of ∼500 square arcmin, the largest patrol field offered by the Nasmyth focus at the VLT. The total wavelength coverage is 0.8μm-1.8μm and two resolution modes: medium resolution and high resolution. In the medium resolution mode (R∼4,000-6,000) the entire wavelength range 0.8μm-1.8μm is observed simultaneously, while the high resolution mode covers simultaneously three selected spectral regions: one around the CaII triplet (at R∼8,000) to measure radial velocities, and two regions at R∼20,000 one in the J-band and one in the H-band, for detailed measurements of chemical abundances.

KW - instrumentation: VLT spectrograph - galaxies: evolution

KW - stellar content

UR - http://www.scopus.com/inward/record.url?scp=84922728112&partnerID=8YFLogxK

U2 - 10.1117/12.2056012

DO - 10.1117/12.2056012

M3 - Conference contribution

AN - SCOPUS:84922728112

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

BT - Ground-Based and Airborne Instrumentation for Astronomy V

A2 - Ramsay, Suzanne K.

A2 - McLean, Ian S.

A2 - Takami, Hideki

PB - SPIE

Y2 - 22 June 2014 through 26 June 2014

ER -

MOONS: The multi-object optical and near-infrared spectrograph for the vlt

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