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4MOST: 4-meter Multi-Object Spectroscopic Telescope

Research output: Contribution to Journal/MagazineJournal article

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4MOST: 4-meter Multi-Object Spectroscopic Telescope. / 4MOST Consortium.
In: EPJ Web of Conferences, Vol. 19, 09004, 2012.

Research output: Contribution to Journal/MagazineJournal article

Harvard

4MOST Consortium 2012, '4MOST: 4-meter Multi-Object Spectroscopic Telescope', EPJ Web of Conferences, vol. 19, 09004. https://doi.org/10.1051/epjconf/20121909004

APA

4MOST Consortium (2012). 4MOST: 4-meter Multi-Object Spectroscopic Telescope. EPJ Web of Conferences, 19, [09004]. https://doi.org/10.1051/epjconf/20121909004

Vancouver

4MOST Consortium. 4MOST: 4-meter Multi-Object Spectroscopic Telescope. EPJ Web of Conferences. 2012;19:09004. doi: 10.1051/epjconf/20121909004

Author

4MOST Consortium. / 4MOST : 4-meter Multi-Object Spectroscopic Telescope. In: EPJ Web of Conferences. 2012 ; Vol. 19.

Bibtex

@article{c46c271df3e5438e976ddbe02971180a,
title = "4MOST: 4-meter Multi-Object Spectroscopic Telescope",
abstract = "The 4MOST consortium aims to provide the ESO community with a fibre-fed spectroscopic survey facility on a 4m-class telescope with a large enough field-of-view (FoV) to survey a large fraction of the southern sky in a few years, a multiplex and spectral resolution high enough to detect chemical and kinematic substructure in the stellar halo, bulge and thin and thick discs of the Milky Way, and enough wavelength coverage (> 1.5 octave) to secure velocities of extra-galactic objects over a large range in redshift. 4MOST will run permanently on the selected telescope to perform a 5 year public survey yielding more than 7 million (goal > 25 million) spectra at resolution R ∼ 5000 and more than 1 million spectra at R 20, 000. Such an exceptional facility enables many science goals, but our design is especially intended to complement three key all-sky, space-based observatories of prime European interest: Gaia, eROSITA and Euclid.",
author = "Andreas Koch and {4MOST Consortium}",
year = "2012",
doi = "10.1051/epjconf/20121909004",
language = "English",
volume = "19",
journal = "EPJ Web of Conferences",
issn = "2100-014X",
publisher = "EDP Sciences",

}

RIS

TY - JOUR

T1 - 4MOST

T2 - 4-meter Multi-Object Spectroscopic Telescope

AU - Koch, Andreas

AU - 4MOST Consortium

PY - 2012

Y1 - 2012

N2 - The 4MOST consortium aims to provide the ESO community with a fibre-fed spectroscopic survey facility on a 4m-class telescope with a large enough field-of-view (FoV) to survey a large fraction of the southern sky in a few years, a multiplex and spectral resolution high enough to detect chemical and kinematic substructure in the stellar halo, bulge and thin and thick discs of the Milky Way, and enough wavelength coverage (> 1.5 octave) to secure velocities of extra-galactic objects over a large range in redshift. 4MOST will run permanently on the selected telescope to perform a 5 year public survey yielding more than 7 million (goal > 25 million) spectra at resolution R ∼ 5000 and more than 1 million spectra at R 20, 000. Such an exceptional facility enables many science goals, but our design is especially intended to complement three key all-sky, space-based observatories of prime European interest: Gaia, eROSITA and Euclid.

AB - The 4MOST consortium aims to provide the ESO community with a fibre-fed spectroscopic survey facility on a 4m-class telescope with a large enough field-of-view (FoV) to survey a large fraction of the southern sky in a few years, a multiplex and spectral resolution high enough to detect chemical and kinematic substructure in the stellar halo, bulge and thin and thick discs of the Milky Way, and enough wavelength coverage (> 1.5 octave) to secure velocities of extra-galactic objects over a large range in redshift. 4MOST will run permanently on the selected telescope to perform a 5 year public survey yielding more than 7 million (goal > 25 million) spectra at resolution R ∼ 5000 and more than 1 million spectra at R 20, 000. Such an exceptional facility enables many science goals, but our design is especially intended to complement three key all-sky, space-based observatories of prime European interest: Gaia, eROSITA and Euclid.

U2 - 10.1051/epjconf/20121909004

DO - 10.1051/epjconf/20121909004

M3 - Journal article

VL - 19

JO - EPJ Web of Conferences

JF - EPJ Web of Conferences

SN - 2100-014X

M1 - 09004

ER -