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相关论文: The Gaia-ESO Survey: processing of the FLAMES-UVES…

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The Gaia-ESO Public Spectroscopic Survey is an ambitious project designed to obtain astrophysical parameters and elemental abundances for 100,000 stars, including large representative samples of the stellar populations in the Galaxy, and a…

太阳与恒星天体物理 · 物理学 2022-10-19 G. Gilmore , S. Randich , C. C. Worley , A. Hourihane , A. Gonneau , G. G. Sacco , J. R. Lewis , L. Magrini , P. Francois , R. D. Jeffries , S. E. Koposov , A. Bragaglia , E. J. Alfaro , C. Allende Prieto , R. Blomme , A. J. Korn , A. C. Lanzafame , E. Pancino , A. Recio-Blanco , R. Smiljanic , S. Van Eck , T. Zwitter , T. Bensby , E. Flaccomio , M. J. Irwin , E. Franciosini , L. Morbidelli , F. Damiani , R. Bonito , E. D. Friel , J. S. Vink , L. Prisinzano , U. Abbas , D. Hatzidimitriou , E. V. Held , C. Jordi , E. Paunzen , A. Spagna , R. J. Jackson , J. Maiz Apellaniz , M. Asplund , P. Bonifacio , S. Feltzing , J. Binney , J. Drew , A. M. N. Ferguson , G. Micela , I. Negueruela , T. Prusti , H. -W. Rix , A. Vallenari , M. Bergemann , A. R. Casey , P. de Laverny , A. Frasca , V. Hill , K. Lind , L. Sbordone , S. G. Sousa , V. Adibekyan , E. Caffau , S. Daflon , D. K. Feuillet , M. Gebran , J. I. Gonzalez Hernandez , G. Guiglion , A. Herrero , A. Lobel , T. Merle , S. Mikolaitis , D. Montes , T. Morel , G. Ruchti , C. Soubiran , H. M. Tabernero , G. Tautvaisiene , G. Traven , M. Valentini , M. Van der Swaelmen , S. Villanova , C. Viscasillas Vazquez , A. Bayo , K. Biazzo , G. Carraro , B. Edvardsson , U. Heiter , P. Jofre , G. Marconi , C. Martayan , T. Masseron , L. Monaco , N. A. Walton , S. Zaggia , V. Aguirre Borsen-Koch , J. Alves , L. Balaguer-Nunez , P. S. Barklem , D. Barrado , M. Bellazzini , S. R. Berlanas , A. S. Binks , A. Bressan , R. Capuzzo-Dolcetta , L. Casagrande , L. Casamiquela , R. S. Collins , V. D'Orazi , M. L. L. Dantas , V. P. Debattista , E. Delgado-Mena , P. Di Marcantonio , A. Drazdauskas , N. W. Evans , B. Famaey , M. Franchini , Y. Fremat , X. Fu , D. Geisler , O. Gerhard , E. A. Gonzalez Solares , E. K. Grebel , M. L. Gutierrez Albarran , F. Jimenez-Esteban , H. Jonsson , T. Khachaturyants , G. Kordopatis , J. Kos , N. Lagarde , H. -G. Ludwig , L. Mahy , M. Mapelli , E. Marfil , S. L. Martell , S. Messina , A. Miglio , I. Minchev , A. Moitinho , J. Montalban , M. J. P. F. G. Monteiro , C. Morossi , N. Mowlavi , A. Mucciarelli , D. N. A. Murphy , N. Nardetto , S. Ortolani , F. Paletou , J. Palous , J. C. Pickering , A. Quirrenbach , P. Re Fiorentin , J. I. Read , D. Romano , N. Ryde , N. Sanna , W. Santos , G. M. Seabroke , L. Spina , M. Steinmetz , E. Stonkute , E. Sutorius , F. Thevenin , M. Tosi , M. Tsantaki , N. Wright , R. F. G. Wyse , M. Zoccali , J. Zorec , D. B. Zucker

The Gaia-ESO Survey is obtaining high-quality spectroscopic data for about 10^5 stars using FLAMES at the VLT. UVES high-resolution spectra are being collected for about 5000 FGK-type stars. These UVES spectra are analyzed in parallel by…

The Gaia-ESO survey is a large public spectroscopic survey aimed at investigating the origin and formation history of our Galaxy by collecting spectroscopy of representative samples (about 10^5 Milky Way stars) of all Galactic stellar…

In the last 15 years different ground-based spectroscopic surveys have been started (and completed) with the general aim of delivering stellar parameters and elemental abundances for large samples of Galactic stars, complementing Gaia…

星系天体物理 · 物理学 2022-10-26 S. Randich , G. Gilmore , L. Magrini , G. G. Sacco , R. J. Jackson , R. D. Jeffries , C. C. Worley , A. Hourihane , A. Gonneau , C. Viscasillas Vàzquez , E. Franciosini , J. R. Lewis , E. J. Alfaro , C. Allende Prieto , T. Bensby R. Blomme , A. Bragaglia , E. Flaccomio , P. François , M. J. Irwin , S. E. Koposov , A. J. Korn , A. C. Lanzafame , E. Pancino , A. Recio-Blanco , R. Smiljanic , S. Van Eck , T. Zwitter , M. Asplund , P. Bonifacio , S. Feltzing , J. Binney , J. Drew , A. M. N. Ferguson , G. Micela , I. Negueruela , T. Prusti , H. -W. Rix , A. Vallenari , A. Bayo , M. Bergemann , K. Biazzo , G. Carraro , A. R. Casey , F. Damiani , A. Frasca , U. Heiter , V. Hill , P. Jofré , P. de Laverny , K. Lind , G. Marconi , C. Martayan , T. Masseron , L. Monaco , L. Morbidelli , L. Prisinzano , L. Sbordone , S. G. Sousa , S. Zaggia , V. Adibekyan , R. Bonito , E. Caffau , S. Daflon , D. K. Feuillet , M. Gebran , J. I. González Hernández , G. Guiglion , A. Herrero , A. Lobel , J. Maíz Apellániz , T. Merle , S. Mikolaitis , D. Montes , T. Morel , C. Soubiran , L. Spina , H. M. Tabernero , G. Tautvaišienė , G. Traven , M. Valentini , M. Van der Swaelmen , S. Villanova , N. J. Wright , U. Abbas , V. Aguirre Børsen-Koch , J. Alves , L. Balaguer-Núnez , P. S. Barklem , D. Barrado , S. R. Berlanas , A. S. Binks , A. Bressan , R. Capuzzo--Dolcetta , L. Casagrande , L. Casamiquela , R. S. Collins , V. D'Orazi , M. L. L. Dantas , V. P. Debattista , E. Delgado-Mena , P. Di Marcantonio , A. Drazdauskas , N. W. Evans , B. Famaey , M. Franchini , Y. Frémat , E. D. Friel , X. Fu , D. Geisler , O. Gerhard , E. A. González Solares , E. K. Grebel , M. L. Gutiérrez Albarrán , D. Hatzidimitriou , E. V. Held , F. Jiménez-Esteban , H. Jönsson , C. Jordi , T. Khachaturyants , G. Kordopatis , J. Kos , N. Lagarde , L. Mahy , M. Mapelli , E. Marfil , S. L. Martell , S. Messina , A. Miglio , I. Minchev , A. Moitinho , J. Montalban , M. J. P. F. G. Monteiro , C. Morossi , N. Mowlavi , A. Mucciarelli , D. N. A. Murphy , N. Nardetto , S. Ortolani , F. Paletou , J. Palouus , E. Paunzen , J. C. Pickering , A. Quirrenbach , P. Re Fiorentin , J. I. Read , D. Romano , N. Ryde , N. Sanna , W. Santos , G. M. Seabroke , A. Spagna , M. Steinmetz , E. Stonkuté , E. Sutorius , F. Thévenin , M. Tosi , M. Tsantaki , J. S. Vink , N. Wright , R. F. G. Wyse , M. Zoccali , J. Zorec , D. B. Zucker , N. A. Walton

The Gaia-ESO Survey (GES) is a large public spectroscopic survey that has collected, over a period of 6 years, spectra of ~ 10^5 stars. This survey provides not only the reduced spectra, but also the stellar parameters and abundances…

The Gaia-ESO Survey was designed to target all major Galactic components (i.e., bulge, thin and thick discs, halo and clusters), with the goal of constraining the chemical and dynamical evolution of the Milky Way. This paper presents the…

The Gaia-ESO Survey (GES) is a public, high-resolution spectroscopic survey with FLAMES@VLT. GES targeted in particular a large sample of open clusters (OCs) of all ages. The different kinds of OCs are useful to reach the main science…

Gaia is a space mission currently measuring the five astrometric parameters as well as spectrophotometry of at least 1 billion stars to G = 20.7 mag with unprecedented precision. The sixth parameter in phase space (radial velocity) is also…

The Gaia-ESO Survey is a wide field spectroscopic survey recently started with the FLAMES@VLT in Cerro Paranal, Chile. It will produce radial velocities more accurate than Gaia's for faint stars (down to V~18), and astrophysical parameters…

星系天体物理 · 物理学 2019-08-15 E. Pancino

The Gaia-ESO survey (GES) is now in its fifth and last year of observations, and has already produced tens of thousands of high-quality spectra of stars in all Milky Way components. This paper presents the strategy behind the selection of…

太阳与恒星天体物理 · 物理学 2017-01-25 E. Pancino , the Gaia-ESO Survey collaboration

The Gaia-ESO Survey (GES) is a large public spectroscopic survey that was carried out using the multi-object FLAMES spectrograph at the Very Large Telescope. The survey provides accurate radial velocities, stellar parameters, and elemental…

The Gaia Data Release 2 contains the 1st release of radial velocities complementing the kinematic data of a sample of about 7 million relatively bright, late-type stars. Aims: This paper provides a detailed description of the Gaia…

The Gaia-ESO Survey (GES) is a large public spectroscopic survey which acquired spectra for more than 100000 stars across all major components of the Milky Way. In addition to atmospheric parameters and stellar abundances that have been…

The extensive stellar spectroscopic datasets that are available for studies in Galactic Archeaology thanks to, for example, the Gaia-ESO Survey, now benefit from having a significant number of targets that overlap with asteroseismology…

With the large amounts of spectroscopic data available today and the very large surveys to come (e.g. Gaia), the need for automatic data analysis software is unquestionable. We thus developed an automatic spectra analysis program for the…

High resolution observations of the asteroids Iris and Juno have been performed by means of the UVES spectrograph at the ESO VLT to obtain the effective accurac y of the spectrograph's radial velocity. The knowledge of this quantity has…

天体物理学 · 物理学 2009-11-13 P. Molaro , S. A. Levshakov , S. Monai , M. Centurion , P. Bonifacio , S. D'Odorico , L. Monaco
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