Nicholas Wright n.j.wright@keele.ac.uk
The Gaia-ESO Public Spectroscopic Survey: Implementation, data products, open cluster survey, science, and legacy
Wright; Jeffries; Abbas, U; Borsen-Koch, VA; Villanova, S; Wright, NJ; Spina, L; Tabernero, HM; Soubiran, C; Valentini, M; Van der Swaelmen, M; Alves, J; Balaguer-Nunez, L; Gonzalez, HJI; Barklem, PS; Traven, G; Herrero, A; Lobel, A; Maiz Apellaniz, J; Montes, D; Morel, T; Guiglion, G; Gebran, M; Feuillet, DK; Daflon, S; Bonito, R; Caffau, E; Kordopatis, G; Kos, J; Adibekyan, V; Lagarde, N; Mahy, L; Mapelli, M; Marfil, E; Martell, SL; Messina, S; Franchini, M; Fremat, Y; Friel, ED; Fu, X; Geisler, D; Gerhard, O; Solares, EAG; Grebel, EK; Gutierrez Albarran, ML; Hatzidimitriou, D; Held, EV; Jimenez-Esteban, F; Jonsson, H; Jordi, C; Khachaturyants, T; Drazdauskas, A; Evans, NW; Feltzing, S; Binney, J; Famaey, B; Randich, S; Gilmore, G; Magrini, L; Sacco, GG; Jackson, RJ; Jeffries, RD; Drew, J; Ferguson, AMN; Micela, G; Negueruela, I; Prusti, T; Rix, H-W; Vallenari, A; Bonifacio, P; Zwitter, T; Asplund, M; Bayo, A; Bergemann, M; Biazzo, K; Carraro, G; Casey, AR; Damiani, F; Koposov, SE; K...
Authors
Robin Jeffries r.d.jeffries@keele.ac.uk
U Abbas
VA Borsen-Koch
S Villanova
NJ Wright
L Spina
HM Tabernero
C Soubiran
M Valentini
M Van der Swaelmen
J Alves
L Balaguer-Nunez
HJI Gonzalez
PS Barklem
G Traven
A Herrero
A Lobel
J Maiz Apellaniz
D Montes
T Morel
G Guiglion
M Gebran
DK Feuillet
S Daflon
R Bonito
E Caffau
G Kordopatis
J Kos
V Adibekyan
N Lagarde
L Mahy
M Mapelli
E Marfil
SL Martell
S Messina
M Franchini
Y Fremat
ED Friel
X Fu
D Geisler
O Gerhard
EAG Solares
EK Grebel
ML Gutierrez Albarran
D Hatzidimitriou
EV Held
F Jimenez-Esteban
H Jonsson
C Jordi
T Khachaturyants
A Drazdauskas
NW Evans
S Feltzing
J Binney
B Famaey
S Randich
G Gilmore
L Magrini
GG Sacco
RJ Jackson
RD Jeffries
J Drew
AMN Ferguson
G Micela
I Negueruela
T Prusti
H-W Rix
A Vallenari
P Bonifacio
T Zwitter
M Asplund
A Bayo
M Bergemann
K Biazzo
G Carraro
AR Casey
F Damiani
SE Koposov
AJ Korn
AC Lanzafame
E Pancino
A Recio-Blanco
R Smiljanic
S Van Eck
NA Walton
E Flaccomio
P Francois
MJ Irwin
L Casagrande
L Casamiquela
RS Collins
V D'Orazi
MLL Dantas
VP Debattista
E Delgado-Mena
P Di Marcantonio
A Miglio
I Minchev
A Moitinho
J Montalban
MJPFG Monteiro
C Morossi
N Mowlavi
A Mucciarelli
DNA Murphy
N Nardetto
S Ortolani
F Paletou
J Palous
E Paunzen
JC Pickering
A Quirrenbach
PR Fiorentin
JI Read
D Romano
N Ryde
N Sanna
W Santos
GM Seabroke
A Spagna
M Steinmetz
E Stonkute
E Sutorius
F Thevenin
M Tosi
D Barrado
SR Berlanas
AS Binks
A Bressan
R Capuzzo-Dolcetta
M Tsantaki
S Vink
N Wright
RFG Wyse
M Zoccali
J Zorec
DB Zucker
A Frasca
U Heiter
V Hill
P Jofre
P de Laverny
K Lind
G Marconi
C Martayan
T Masseron
L Monaco
L Morbidelli
L Prisinzano
L Sbordone
SG Sousa
S Zaggia
CC Worley
A Hourihane
A Gonneau
CV Vazquez
E Franciosini
JR Lewis
EJ Alfaro
C Allende Prieto
T Bensby
R Blomme
A Bragaglia
Abstract
Context. 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 astrometry. Among those surveys, the Gaia-ESO Public Spectroscopic Survey, the only one performed on a 8m class telescope, was designed to target 100 000 stars using FLAMES on the ESO VLT (both Giraffe and UVES spectrographs), covering all the Milky Way populations, with a special focus on open star clusters. Aims. This article provides an overview of the survey implementation (observations, data quality, analysis and its success, data products, and releases), of the open cluster survey, of the science results and potential, and of the survey legacy. A companion article reviews the overall survey motivation, strategy, Giraffe pipeline data reduction, organisation, and workflow. Methods. We made use of the information recorded and archived in the observing blocks; during the observing runs; in a number of relevant documents; in the spectra and master catalogue of spectra; in the parameters delivered by the analysis nodes and the working groups; in the final catalogue; and in the science papers. Based on these sources, we critically analyse and discuss the output and products of the Survey, including science highlights. We also determined the average metallicities of the open clusters observed as science targets and of a sample of clusters whose spectra were retrieved from the ESO archive. Results. The Gaia-ESO Survey has determined homogeneous good-quality radial velocities and stellar parameters for a large fraction of its more than 110 000 unique target stars. Elemental abundances were derived for up to 31 elements for targets observed with UVES. Lithium abundances are delivered for about 1/3 of the sample. The analysis and homogenisation strategies have proven to be successful; several science topics have been addressed by the Gaia-ESO consortium and the community, with many highlight results achieved. Conclusions. The final catalogue will be released through the ESO archive in the first half of 2022, including the complete set of advanced data products. In addition to these results, the Gaia-ESO Survey will leave a very important legacy, for several aspects and for many years to come.
Citation
Wright, Jeffries, Abbas, U., Borsen-Koch, V., Villanova, S., Wright, N., …Bragaglia, A. (2022). The Gaia-ESO Public Spectroscopic Survey: Implementation, data products, open cluster survey, science, and legacy. Astronomy & Astrophysics, https://doi.org/10.1051/0004-6361/202243141
Acceptance Date | Mar 8, 2022 |
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Publication Date | Oct 18, 2022 |
Journal | Astronomy and Astrophysics: a European journal |
Print ISSN | 0004-6361 |
Publisher | EDP Sciences |
DOI | https://doi.org/10.1051/0004-6361/202243141 |
Public URL | https://keele-repository.worktribe.com/output/425003 |
Publisher URL | https://www.aanda.org/articles/aa/full_html/2022/10/aa43141-22/aa43141-22.html |
Related Public URLs | https://arxiv.org/abs/2206.02901 |
Files
aa43141-22.pdf
(26.3 Mb)
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Publisher Licence URL
https://creativecommons.org/licenses/by-nc/4.0/
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