6533b7dbfe1ef96bd126fc2e

RESEARCH PRODUCT

The Gaia-ESO Public Spectroscopic Survey

G. GilmoreS. RandichM. AsplundJ. BinneyP. BonifacioJ. DrewS. FeltzingA. FergusonR. JeffriesG. MicelaI. NegueruelaT. PrustiH. -W RixA. VallenariE. AlfaroC. Allende-prietoC. BabusiauxT. BensbyR. BlommeA. BragagliaE. FlaccomioP. FrançoisM. IrwinS. KoposovA. KornA. LanzafameE. PancinoE. PaunzenA. Recio-blancoG. SaccoR. SmiljanicS. EckN. WaltonD. AdenC. AertsL. AfferJ. -M AlcalaG. AltavillaJ. AlvesT. AntojaF. ArenouCostanza ArgiroffiA. Asensio RamosC. Bailer-jonesL. Balaguer-nunezA. BayoB. BarbuyG. BariseviciusD. Barrado Y NavascuesC. BattistiniI. Bellas VelidisM. BellazziniV. BelokurovM. BergemannG. BertelliK. BiazzoO. BienaymeJ. Bland-hawthornC. BoecheS. BonitoS. BoudreaultJ. BouvierI. BrandaoA. BrownJ. BruijneM. BurleighJ. CaballeroE. CaffauF. CaluraR. Capuzzo-dolcettaM. CaramazzaG. CarraroL. CasagrandeS. CasewellS. ChapmanC. ChiappiniY. ChorniyN. ChristliebM. CignoniG. CocozzaM. CollessR. ColletM. CollinsM. CorrentiE. CovinoD. CrnojevicM. CropperM. CunhaF. DamianiM. DavidA. DelgadoS. DuffauB. EdvardssonJ. EldridgeH. EnkeK. ErikssonN. W. EvansL. EyerB. FamaeyM. FellhauerI. FerrerasF. FiguerasG. FiorentinoC. FlynnD. FolhaE. FranciosiniA. FrascaK. FreemanY. FrematE. FrielB. GaensickeJ. GameiroF. GarzonS. GeierD. GeislerO. GerhardB. GibsonA. GombocA. GomezC. Gonzalez-fernandezJ. Gonzalez HernandezE. GossetE. GrebelR. GreimelM. GroenewegenF. GrundahlM. GuarcelloB. GustafssonP. HadravaD. HatzidimitriouN. HamblyP. HammersleyC. HansenM. HaywoodU. HeberU. HeiterE. HeldA. HelmiG. HenslerA. HerreroV. HillS. HodgkinN. HuelamoA. HuxorR. IbataR. JacksonR. JongP. JonkerS. JordanC. JordiA. JorissenD. KatzD. KawataS. KellerN. KharchenkoR. KlementA. KlutschJ. KnudeA. KochO. KochukhovM. KontizasP. KoubskyR. LallementP. LavernyF. LeeuwenB. LemasleG. LewisK. LindH. P. E. LindstromA. LobelJ. Lopez SantiagoP. LucasH. LudwigT. LueftingerL. MagriniJ. Maiz ApellanizJ. MaldonadoG. MarconiA. MarinoC. MartayanI. Martinez-valpuestaG. MatijevicR. McmahonS. MessinaM. MeyerA. MiglioS. MikolaitisI. MinchevD. MinnitiA. MoitinhoY. MomanyL. MonacoM. MontaltoM. J. MonteiroR. MonierD. MontesA. MoraE. MorauxT. MorelN. MowlaviA. MucciarelliU. MunariR. NapiwotzkiN. NardettoT. NaylorY. NazeG. NelemansS. OkamotoS. OrtolaniG. PaceF. PallaJ. PalousR. ParkerJ. PenarrubiaI. PillitteriG. PiottoH. PosbicL. PrisinzanoE. PuzerasA. QuirrenbachS. RagainiJ. ReadM. ReadC. ReyleJ. RidderN. RobichonA. RobinS. RoeserD. RomanoF. RoyerG. RuchtiA. RuzickaS. RyanN. RydeN. SantosJ. Sanz ForcadaL. M. Sarro BaroL. SbordoneE. SchilbachS. SchmejaO. SchnurrR. SchoenrichR. -D ScholzG. SeabrokeS. SharmaG. SilvaM. SmithE. SolanoR. SordoC. SoubiranS. SousaA. SpagnaM. SteffenM. SteinmetzB. StelzerE. StempelsH. TaberneroG. TautvaisieneF. TheveninJ. TorraM. TosiE. TolstoyC. TuronM. WalkerJ. WambsganssC. WorleyK. VennJ. VinkR. WyseS. ZaggiaW. ZeilingerM. ZoccaliJ. ZorecD. ZuckerT. ZwitterGaia-eso Survey Team

subject

spectroscopy stars kinematics abundancesSettore FIS/05 - Astronomia E AstrofisicaAstrophysics::Instrumentation and Methods for AstrophysicsAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics::Galaxy Astrophysics

description

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 covering all the major components of the Milky Way. This survey will provide the first homogeneous overview of the distributions of kinematics and chemical element abundances in the Galaxy. The motivation, organisation and implementation of the Gaia-ESO Survey are described, emphasising the complementarity with the ESA Gaia mission. Spectra from the very first observing run of the survey are presented.

yearjournalcountryeditionlanguage
2012-03-01
https://ui.adsabs.harvard.edu/#abs/2012Msngr.147...25G