The Gaia-ESO Public Spectroscopic Survey

By G. Gilmore, S. Randich, Martin Asplund, J. Binney, P. Bonifacio, J. Drew, S. Feltzing, A. Ferguson, R. Jeffries, G. Micela and 265 more. 2012

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Yule-Simpson’s paradox in Galactic Archaeology (2019, methodology): “We expect to get those form the K2 (Howell et al. 2014), TESS (Ricker et al. 2015) and PLATO (Rauer et al. 2014) asteroseismic missions in the near future, as well as isochrone age determination from spectroscopic surveys, such as GALAH (De Silva et al. 2015), Gaia-ESO (Gilmore et al. 2012), APOGEE,”
The age–metallicity structure of the Milky Way disc using APOGEE (2017, background): “…stellar ages are now becoming readily available, due to the advent of modern spectroscopic surveys such as APOGEE (Majewski et al. 2015), Gaia-ESO (Gilmore et al. 2012) and GALAH (Martell et al. 2016), with future instruments aiming to bolster the ESA-Gaia data releases (Gaia Collaboration et al.…”
The Gaia-ESO Survey: the analysis of high-resolution UVES spectra of FGK-type stars (2014, background): “The EWs are available for 1265 stars, out of the 1268 observed by the Gaia-ESO Survey for which atmospheric parameters were determined.”
The structure and dynamical evolution of the stellar disc of a simulated Milky Way-mass galaxy (2016, background): “…surveys of stars in the MW, such as RAVE (Steinmetz et al. 2006), SEGUE (Yanny et al. 2009), APOGEE (Allende Prieto et al. 2008), and Gaia-ESO (Gilmore et al. 2012), one can now combine three-dimensional position, velocity, and chemical abundance information for large samples (for a recent…”
Gaia FGK benchmark stars: Effective temperatures and surface gravities (2015, background): “Examples of such surveys are the Gaia-ESO Public Spectroscopic Survey (Gilmore et al. 2012; Randich et al. 2013), RAVE (Steinmetz et al. 2006), APOGEE (Allende Prieto et al. 2008), and GALAH (De Silva et al. 2015).”
Exploring the Milky Way stellar disk - A detailed elemental abundance study of 714 F and G dwarf stars in the solar neighbourhood (2013, methodology): “APOGEE (Allende Prieto et al. 2008), the Gaia-ESO Survey (Gilmore et al. 2012), the GALAH survey (e.g., Zucker et al. 2012) which together will gather spectra and determine stellar parameters and chemical abundances for several hundreds of thousands of dwarf and red giant stars in the Galactic thin ”
The VST Photometric Hα Survey of the Southern Galactic Plane and Bulge (VPHAS (2014, background): “Conversely in the meantime, VPHAS+ has already begun to assist ambitious wide-field spectroscopy programmes such as the Gaia-ESO Survey (Gilmore et al. 2012) through the provision of the wide-field photometry needed for target selection and field setup.”
PLATO as it is: a legacy mission for Galactic archaeology (2017, unknown): “…et al. 2006), SEGUE-2 (Eisenstein et al. 2011; Yanny et al. 2009), APOGEE (Majewski et al. 2015; Majewski, APOGEE Team, & APOGEE-2016), Gaia-ESO (Gilmore et al. 2012), LAM-OST (Cui et al. 2012), GALAH (De Silva et al. 2015; Martell et al. 2017), WEAVE (Dalton et al. 2014), 4MOST (de Jong et al.…”
The GALAH survey and Gaia DR2: dissecting the stellar disc’s phase space by age, action, chemistry, and location (2018, background): “…by Australian N ational U niversity user on 10 O ctober 2019 (Steinmetz et al. 2006), APOGEE (Majewski et al. 2017), GaiaESO (Gilmore et al. 2012), LAMOST (Deng et al. 2012) – and are now able to exploit the overlap of targets with Gaia DR2 – this is the golden age of…”
The Gaia-ESO Survey : radial metallicity gradients and age-metallicity relation of stars in the Milky Way disk (2014, methodology): “For the analysis of the spectra, several state-of-the-art spectrum analysis codes are used (Gilmore et al. 2012, Randich et al. 2013, Smiljanic et al. in prep).”
The GALAH survey: observational overview and Gaia DR1 companion (2016, methodology): “The Gaia-ESO Survey (GES; Gilmore et al. 2012; Randich et al. 2013) is another ongoing Galactic archaeology survey project, using the GIRAFFE spectrograph (Pasquini et al. 2000) at the Very Large Telescope at the European Southern Observatory in Chile to collect high-resolution (R ∼ 26, 000)…”
The vertical metallicity gradients of mono-age stellar populations in the Milky Way with the RAVE and Gaia data (2017, background): “…et al. 2014), the Apache Point Observatory Galactic Evolution Experiment (SDSS-III/APOGEE; Eisenstein et al. 2011; Majewski et al. 2015), Gaia-ESO (Gilmore et al. 2012), the GALactic Archaeology with HERMES (GALAH; Martell et al. 2017), the 4-metre Multi-Object Spectroscopic Telescope (4MOST; de…”
On the metallicity of open clusters. III. Homogenised sample (2015, background): “We wish to mention the ongoing Gaia-ESO Public Spectroscopic Survey (Gilmore et al. 2012), which has already provided mean abundances for some open clusters.”
Constraining the Milky Way assembly history with Galactic Archaeology (2016, background): “…to obtaining spectroscopic information for a large number of stars, e.g., RAVE ⋆ Corresponding author: iminchev@aip.de (Steinmetz et al., 2006), SEGUE (Yanny et al., 2009), APOGEE (Majewski et al., 2010), HERMES (Freeman, 2010), Gaia-ESO (Gilmore et al., 2012), and LAMOST (Zhao et al., 2006).”
Chemodynamical evolution of the Milky Way disk - I. The solar vicinity (2012, background): “For the young populations, this should be already possible to obtain from the observations of open clusters, e.g., with the ongoing Gaia-ESO or APOGEE surveys.”
Near-Field Cosmology with Extremely Metal-Poor Stars (2015, background): “We refer the reader to Gilmore et al. (2012) for a description of the synergy between Gaia and ground-based facilities that will together provide basic detailed chemical abundances for an unprecedented sample of the Galaxy’s metal-poor stars.”
The Milky Way’s stellar disk (2013, background): “– Gaia-ESO (Gilmore et al. 2012): The Gaia-ESO program, is a 300-night ESO public survey, which commenced in early 2012, and will obtain 100,000 high-resolution spectra with the GIRAFFE and UVES spectrographs at the VLT.”