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Sökning: L773:0004 6361 OR L773:1432 0746 > The Gaia-ESO Survey :

The Gaia-ESO Survey : Target selection of open cluster stars & x22c6

Bragaglia, A. (författare)
INAF Osservatorio Astrofis & Sci Spazio Bologna, Via P Gobetti 93-3, I-40129 Bologna, Italy.,INAF Osservatorio Astronomico di Bologna
Alfaro, E. J. (författare)
Inst Astrofis Andalucia CSIC, Apdo 3004, Granada 18080, Spain.,CSIC Instituto de Astrofísica de Andalucía (IAA)
Flaccomio, E. (författare)
INAF Osservatorio Astron Palermo, Piazza Parlamento 1, I-90134 Palermo, Italy.,INAF Palermo Astronomical Observatory,CSIC Centro de Astrobiologia (INTA),Ctr Astrobiol CSIC INTA, Dept Astrofis, ESAC Campus,Camino Bajo Castillo S-N, Madrid 28692, Spain.
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Blomme, R. (författare)
Royal Observ Belgium, Ringlaan 3, B-1180 Brussels, Belgium.,Royal Observatory of Belgium
Donati, P. (författare)
INAF Osservatorio Astrofis & Sci Spazio Bologna, Via P Gobetti 93-3, I-40129 Bologna, Italy.,INAF Osservatorio Astronomico di Bologna
Costado, M. (författare)
Univ Cadiz, Cadiz, Spain.,University of Cádiz
Damiani, F. (författare)
INAF Osservatorio Astron Palermo, Piazza Parlamento 1, I-90134 Palermo, Italy.,INAF Palermo Astronomical Observatory,Indiana University,Indiana Univ, Dept Astron, Bloomington, IN 47405 USA.
Franciosini, E. (författare)
INAF Osservatorio Astrofis Arcetri, Largo E Fermi 5, I-50125 Florence, Italy.,INAF - Osservatorio Astrofisico di Arcetri
Prisinzano, L. (författare)
INAF Osservatorio Astron Palermo, Piazza Parlamento 1, I-90134 Palermo, Italy.,INAF Palermo Astronomical Observatory
Randich, S. (författare)
INAF Osservatorio Astrofis Arcetri, Largo E Fermi 5, I-50125 Florence, Italy.,INAF - Osservatorio Astrofisico di Arcetri,Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences,Polish Acad Sci, Nicolaus Copernicus Astron Ctr, Ul Bartycka 18, PL-00716 Warsaw, Poland.
Friel, E. D. (författare)
Indiana Univ, Dept Astron, Bloomington, IN 47405 USA.
Hatztidimitriou, D. (författare)
Natl & Kapodistrian Univ Athens, Dept Phys, Sect Astrophys Astron & Mech, Athens 15784, Greece.,National and Kapodistrian University of Athens
Vallenari, A. (författare)
INAF Osservatorio Astron Padova, Vicolo Osservatorio 5, I-35122 Padua, Italy.,INAF - Osservatorio Astronomico di Padova
Spagna, A. (författare)
INAF Osservatorio Astrofis Torino, Via Osservatorio 20, I-10025 Turin, Italy.,INAF - Osservatorio Astrofisico di Torino
Balaguer-Nunez, L. (författare)
Univ Barcelona IEEC ICCUB, Inst Ciencies Cosmos, Marti & Franques 1, Barcelona 08028, Spain.,University of Barcelona
Bonito, R. (författare)
INAF Osservatorio Astron Palermo, Piazza Parlamento 1, I-90134 Palermo, Italy.,INAF Palermo Astronomical Observatory
Gaudin, T. Cantat (författare)
Univ Barcelona IEEC ICCUB, Inst Ciencies Cosmos, Marti & Franques 1, Barcelona 08028, Spain.,University of Barcelona
Casamiquela, L. (författare)
Univ Bordeaux, Lab Astrophys Bordeaux, CNRS, B18N,Allee Geoffroy St Hilaire, F-33615 Pessac, France.,University of Bordeaux
Jeffries, R. D. (författare)
Keele Univ, Res Inst Environm Phys Sci & Appl Math, Astrophys Grp, Keele ST5 5BG, Staffs, England.,Keele University
Jordi, C. (författare)
Univ Barcelona IEEC UB, Inst Ciencies Cosmos ICCUB, Dept Fis Quant & Astrofis, Marti Franques 1, Barcelona 08028, Spain.,University of Barcelona
Magrini, L. (författare)
INAF Osservatorio Astrofis Arcetri, Largo E Fermi 5, I-50125 Florence, Italy.,INAF - Osservatorio Astrofisico di Arcetri
Drew, J. E. (författare)
Univ Hertfordshire, Ctr Astrophys Res, STRI, Coll Lane Campus, Hatfield AL10 9AB, Herts, England.,University of Hertfordshire
Jackson, R. J. (författare)
Keele Univ, Res Inst Environm Phys Sci & Appl Math, Astrophys Grp, Keele ST5 5BG, Staffs, England.,Keele University
Abbas, U. (författare)
INAF Osservatorio Astron Padova, Vicolo Osservatorio 5, I-35122 Padua, Italy.,University of Padova
Caramazza, M. (författare)
Inst Astron & Astrophys Tubingen IAAT, Sand 1, D-72076 Tubingen, Germany.,University of Tübingen
Hayes, C. (författare)
Univ Washington, Dept Astron, Box 351580, Seattle, WA 98195 USA.,University of Washington
Jimenez-Esteban, F. M. (författare)
Ctr Astrobiol CSIC INTA, Dept Astrofis, ESAC Campus,Camino Bajo Castillo S-N, Madrid 28692, Spain.
Fiorentin, P. Re (författare)
INAF Osservatorio Astron Padova, Vicolo Osservatorio 5, I-35122 Padua, Italy.,INAF - Osservatorio Astronomico di Padova
Wright, N. (författare)
Keele Univ, Res Inst Environm Phys Sci & Appl Math, Astrophys Grp, Keele ST5 5BG, Staffs, England.,Keele University
Bayo, A. (författare)
Univ Valparaiso, Inst Fis & Astron, Fac Ciencias, Av Gran Bretana 1111, Valparaiso 5030, Chile.,University of Valparaíso
Bensby, T. (författare)
Lund University,Lunds universitet,Astronomi - Genomgår omorganisation,Institutionen för astronomi och teoretisk fysik - Genomgår omorganisation,Naturvetenskapliga fakulteten,Lund Observatory - Undergoing reorganization,Department of Astronomy and Theoretical Physics - Undergoing reorganization,Faculty of Science,Lund Observ, Dept Astron & Theoret Phys, Box 43, S-22100 Lund, Sweden.
Bergemann, M. (författare)
Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany.,Max Planck Institute for Astronomy
Gilmore, G. (författare)
Univ Cambridge, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England.,University of Cambridge,INAF - Osservatorio Astrofisico di Arcetri,INAF Osservatorio Astrofis Arcetri, Largo E Fermi 5, I-50125 Florence, Italy.
Gonneau, A. (författare)
Univ Cambridge, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England.,University of Cambridge
Heiter, Ulrike (författare)
Uppsala University,Uppsala universitet,Observationell astrofysik
Hourihane, A. (författare)
Univ Cambridge, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England.,University of Cambridge
Pancino, E. (författare)
INAF Osservatorio Astrofis Arcetri, Largo E Fermi 5, I-50125 Florence, Italy.;Agenzia Spaziale Italiana, Space Sci Data Ctr, Via Politecn Snc, I-00133 Rome, Italy.,INAF - Osservatorio Astrofisico di Arcetri,Italian Space Agency
Sacco, G. (författare)
INAF Osservatorio Astrofis Arcetri, Largo E Fermi 5, I-50125 Florence, Italy.
Smiljanic, R. (författare)
Polish Acad Sci, Nicolaus Copernicus Astron Ctr, Ul Bartycka 18, PL-00716 Warsaw, Poland.
Zaggia, S. (författare)
INAF Osservatorio Astron Padova, Vicolo Osservatorio 5, I-35122 Padua, Italy.,INAF - Osservatorio Astronomico di Padova
Vink, J. S. (författare)
Armagh Observ & Planetarium, Coll Hill, Armagh BT61 9DG, North Ireland.,Armagh Observatory
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INAF Osservatorio Astrofis & Sci Spazio Bologna, Via P Gobetti 93-3, I-40129 Bologna, Italy INAF Osservatorio Astronomico di Bologna (creator_code:org_t)
2022-03-29
2022
Engelska.
Ingår i: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 659
  • Tidskriftsartikel (refereegranskat)
Abstract Ämnesord
Stäng  
  • Context. The Gaia-ESO Survey (GES) is a public, high-resolution spectroscopic survey, conducted with the multi-object spectrograph Fibre Large Array Multi Element Spectrograph (FLAMES) on the Very Large Telescope (European Southern Observatory, ESO, Cerro Paranal, Chile) from December 2011 to January 2018. Gaia-ESO has targeted all the main stellar components of the Milky Way, including thin and thick disc, bulge, and halo. In particular, a large sample of open clusters has been observed, from very young ones, just out of the embedded phase, to very old ones. Aims. The different kinds of clusters and stars targeted in them are useful to reach the main science goals of the open cluster part of GES, which are the study of the open cluster structure and dynamics, the use of open clusters to constrain and improve stellar evolution models, and the definition of Galactic disc properties (e.g., metallicity distribution). Methods. The Gaia-ESO Survey is organised in 19 working groups (WGs), each one being responsible for a task. We describe here the work of three of them, one in charge of the selection of the targets within each cluster or association (WG4), one responsible for defining the most probable candidate member stars (WG1), and another one in charge of the preparation of the observations (WG6). As the entire GES has been conducted before the second Gaia data release, we could not make use of the Gaia astrometry to define cluster member candidates. We made use of public and private photometry to select the stars to be observed with FLAMES, once brought on a common astrometric system (the one defined by 2MASS). Candidate target selection was based on ground-based proper motions, radial velocities, and X-ray properties when appropriate, for example, and it was mostly used to define the position of the clusters' evolutionary sequences in the colour-magnitude diagrams. Targets for GIRAFFE were then selected near the sequences in an unbiased way. We used known information on membership, when available, only for the few stars to be observed with UVES. Results. We collected spectra for 62 confirmed clusters in the main observing campaign (and a few more clusters were taken from the ESO archive). Among them are very young clusters, where the main targets are pre-main sequence stars, clusters with very hot and massive stars currently on the main sequence, intermediate-age and old clusters where evolved stars are the main targets. Our strategy of making the selection of targets as inclusive and unbiased as possible and of observing a significant and representative fraction of all possible targets permitted us to collect the largest, most accurate, and most homogeneous spectroscopic data set on open star clusters ever achieved.

Ämnesord

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Nyckelord

surveys
stars
abundances
kinematics and dynamics
open clusters and associations
general
techniques
radial velocities
spectroscopic

Publikations- och innehållstyp

ref (ämneskategori)
art (ämneskategori)

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