Corpus ID: 118805311

The Gaia-ESO Public Spectroscopic Survey

  title={The Gaia-ESO Public Spectroscopic Survey},
  author={G. Gilmore and S. Randich and M. Asplund and J. Binney and P. Bonifacio and J. Drew and S. Feltzing and A. Ferguson and R. Jeffries and G. Micela and I. Negueruela and T. Prusti and H. Rix and A. Vallenari and E. Alfaro and C. Allende-Prieto and C. Babusiaux and T. Bensby and R. Blomme and A. Bragaglia and E. Flaccomio and P. François and M. Irwin and Sergey E. Koposov and A. Korn and A. Lanzafame and E. Pancino and E. Paunzen and A. Recio-Blanco and G. Sacco and R. Smiljanic and S. Eck and N. Walton and D. Ad'en and C. Aerts and L. Affer and J. Alcala' and G. Altavilla and J. Alves and T. Antoja and Fr{\'e}d{\'e}ric Arenou and C. Argiroffi and A. Ramos and C. Bailer-Jones and L. Balaguer-N{\'u}{\~n}ez and A. Bayo and B. Barbuy and G. Barisevicius and D. B. Y. Navascu{\'e}s and C. Battistini and I. B. Velidis and M. Bellazzini and V. Belokurov and M. Bergemann and G. Bertelli and K. Biazzo and O. Bienaym{\'e} and J. Bland-Hawthorn and C. Boeche and S. Bonito and S. Boudreault and J. Bouvier and I. Brand{\~a}o and Anthony G. A. Brown and J. Bruijne and M. Burleigh and J. Caballero and E. Caffau and F. Calura and R. Capuzzo-Dolcetta and M. Caramazza and G. Carraro and L. Casagrande and S. Casewell and S. Chapman and C. Chiappini and Y. Chorniy and N. Christlieb and M. Cignoni and G. Cocozza and M. Colless and R. Collet and M. Collins and M. Correnti and E. Covino and D. Crnojevi{\'c} and M. Cropper and M. Cunha and F. Damiani and M. David and A. Delgado and S. Duffau and B. Edvardsson and J. Eldridge and H. Enke and K. Eriksson and N. Evans and L. Eyer and B. Famaey and M. Fellhauer and I. Ferreras and F. Figueras and G. Fiorentino and C. Flynn and D. Folha and E. Franciosini and A. Frasca and K. Freeman and Y. Fr{\'e}mat and E. Friel and B. Gaensicke and J. Gameiro and F. Garz{\'o}n and S. Geier and D. Geisler and O. Gerhard and B. Gibson and A. Gomboc and A. G{\'o}mez and C. Gonz{\'a}lez-Fern{\'a}ndez and J. Hern{\'a}ndez and E. Gosset and E. Grebel and R. Greimel and M. Groenewegen and F. Grundahl and M. Guarcello and B. Gustafsson and P. Hadrava and D. Hatzidimitriou and N. Hambly and P. Hammersley and C. Hansen and M. Haywood and U. Heber and U. Heiter and E. Held and A. Helmi and G. Hensler and A. Herrero and V. Hill and S. Hodgkin and N. Hu{\'e}lamo and A. Huxor and R. Ibata and R. Jackson and R. D. Jong and P. Jonker and S. Jordan and C. Jordi and A. Jorissen and D. Katz and D. Kawata and S. Keller and N. Kharchenko and R. Klement and A. Klutsch and J. Knude and A. Koch and O. Kochukhov and M. Kontizas and P. Koubsk{\'y} and R. Lallement and P. D. Laverny and F. V. Leeuwen and B. Lemasle and G. Lewis and K. Lind and H. Lindstr{\o}m and A. Lobel and J. Santiago and P. Lucas and H. Ludwig and T. Lueftinger and L. Magrini and J. M. Apell{\'a}niz and J. Maldonado and G. Marconi and A. Marino and C. Martayan and I. Martinez-Valpuesta and G. Matijevi{\vc} and R. McMahon and S. Messina and M. Meyer and A. Miglio and {\vS}. Mikolaitis and I. Minchev and D. Minniti and A. Moitinho and Y. Momany and L. Monaco and M. Montalto and M. F. G. Monteiro and R. Monier and D. Montes and A. Mora and E. Moraux and T. Morel and N. Mowlavi and A. Mucciarelli and U. Munari and R. Napiwotzki and N. Nardetto and T. Naylor and Y. Naz{\'e} and G. Nelemans and S. Okamoto and S. Ortolani and G. Pace and F. Palla and J. Palou{\vs} and R. Parker and J. Pe{\~n}arrubia and I. Pillitteri and G. Piotto and H. Posbic and L. Prisinzano and E. Puzeras and A. Quirrenbach and S. Ragaini and J. Read and M. Read and C. Reyl{\'e} and J. Ridder and N. Robichon and A. Robin and S. Roeser and D. Romano and F. Royer and G. Ruchti and A. Rů{\vz}i{\vc}ka and S. Ryan and N. Ryde and N. Santos and J. S. Forcada and L. S. Baro and L. Sbordone and E. Schilbach and S. Schmeja and O. Schnurr and R. Schoenrich and R. Scholz and G. Seabroke and Sanjib Sharma and G. D. Silva and M. Smith and E. Solano and R. Sordo and C. Soubiran and S. Sousa and A. Spagna and M. Steffen and M. Steinmetz and B. Stelzer and E. Stempels and H. Tabernero and G. Tautvai{\vs}ienė and F. Th{\'e}venin and J. Torra and M. Tosi and E. Tolstoy and C. Turon and M. Walker and J. Wambsganss and C. Worley and K. Venn and J. Vink and R. Wyse and S. Zaggia and W. Zeilinger and M. Zoccali and J. Zorec and D. Zucker and T. Zwitter},
  journal={The Messenger},
The Gaia-ESO Public Spectroscopic Survey has begun and will obtain high quality spectroscopy of some 100000 Milky Way stars, in the field and in open clusters, down to magnitude 19, systematically ... 

Figures from this paper

Broadening of spectral lines in the Gaia-ESO survey
Analyzing stellar spectra plays a big role in understanding the evolution of our galaxy. Having good data for spectral line properties is very important when analyzing these spectra. One part of thExpand
The Gaia-ESO Survey: the N/O abundance ratio in the Milky Way
9 pages, 7 figures (Appendix not available in the current version), accepted for publication on A&A. Reproduced with permission from Astronomy & Astrophysics. © 2018 ESO
The thick disc according to Gaia-ESO
Abstract In the era of large spectroscopic surveys, it is vital that selection effects are taken into account when making conclusions about the stellar populations of the Galaxy. Here we use theExpand
Gaia FGK benchmark stars: new candidates at low metallicities
Context. We have entered an era of large spectroscopic surveys in which we can measure, through automated pipelines, the atmospheric parameters and chemical abundances for large numbers of stars. CExpand
Open clusters in the Gaia-ESO Survey tracing the chemical history of the Milky Way
The Gaia-ESO Survey (GES) is a large public spectroscopic survey that aims at observing with FLAMES@VLT the main stellar components of our Galaxy. The study of the population of open clusters is oneExpand
The TESS-HERMES survey data release 1 : high-resolution spectroscopy of the TESS southern continuous viewing zone
The Transiting Exoplanet Survey Satellite (TESS) will provide high-precision time series photometry for millions of stars with at least a half-hour cadence. Of particular interest are the circular ...
The GALAH survey and Gaia DR2: dissecting the stellar disc's phase space by age, action, chemistry, and location
We use the second data releases of the European Space Agency Gaia astrometric survey and the high-resolution Galactic Archaeology with HERMES (GALAH) spectroscopic survey to analyse the structure oExpand
FORS2/VLT survey of Milky Way globular clusters I. Description of the method for derivation of metal abundances in the optical and application to NGC 6528, NGC 6553, M 71, NGC 6558, NGC 6426, and Terzan 8
We are grateful to Paula Coelho for useful discussions. B.D. acknowledges financial support from CNPq and ESO. B.B. acknowledges partial financial support from CNPq and Fapesp.
OCCASO – II. Physical parameters and Fe abundances of red clump stars in 18 open clusters
Open clusters have long been used to study the chemodynamical evolution of the Galactic disc. This requires a homogeneously analysed sample covering a wide range of ages and distances. In this papeExpand
Double, triple and quadruple-line spectroscopic binary candidates within the Gaia-ESO Survey
Abstract The Gaia-ESO Survey (GES, Gilmore et al. 2012) provides a unique opportunity to detect spectroscopically multiplicity among different populations of the Galaxy using the cross-correlationExpand