The AMBRE project: Results from the MATISSE analysis of the ESO-FEROS archived spectra

The AMBRE project: Results from the MATISSE analysis of the ESO-FEROS archived spectra

The goal of AMBRE, a joint project between ESO and the Observatoire de la Cote d’Azur, is to provide a homogeneous determination of the stellar parameters (including mean metallicity and some chemical abundances) for the archived spectra of the FEROS, HARPS, UVES and Flames/GIRAFFE spectrographs. We...

Full description

Bibliographic Details
Main Authors: Hill V., Recio-Blanco A., de Laverny P., Worley C.C., Kordopatis G.
Format: Article
Language:English
Published: EDP Sciences 2012-02-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/20121909008
id doaj-f01fb02623714032851269bf74cfb996
record_format Article
spelling doaj-f01fb02623714032851269bf74cfb9962021-08-02T05:21:46ZengEDP SciencesEPJ Web of Conferences2100-014X2012-02-01190900810.1051/epjconf/20121909008The AMBRE project: Results from the MATISSE analysis of the ESO-FEROS archived spectraHill V.Recio-Blanco A.de Laverny P.Worley C.C.Kordopatis G.The goal of AMBRE, a joint project between ESO and the Observatoire de la Cote d’Azur, is to provide a homogeneous determination of the stellar parameters (including mean metallicity and some chemical abundances) for the archived spectra of the FEROS, HARPS, UVES and Flames/GIRAFFE spectrographs. We present here a preliminary analysis of the FEROS stellar sample. The stellar parameters, derived using the stellar classification algorithm MATISSE, have been combined with distances and radial velocities in order to explore current theories regarding galactic stellar populations. We have reviewed the sample for potential disk stars with which we can explore kinematic and chemical signatures of the thin and thick disk. We present here a comparison of the potential disk stellar sample to the analysis of 66 disk stars that was carried out in. http://dx.doi.org/10.1051/epjconf/20121909008
collection DOAJ
language English
format Article
sources DOAJ
author Hill V.
Recio-Blanco A.
de Laverny P.
Worley C.C.
Kordopatis G.
spellingShingle Hill V.
Recio-Blanco A.
de Laverny P.
Worley C.C.
Kordopatis G.
The AMBRE project: Results from the MATISSE analysis of the ESO-FEROS archived spectra
EPJ Web of Conferences
author_facet Hill V.
Recio-Blanco A.
de Laverny P.
Worley C.C.
Kordopatis G.
author_sort Hill V.
title The AMBRE project: Results from the MATISSE analysis of the ESO-FEROS archived spectra
title_short The AMBRE project: Results from the MATISSE analysis of the ESO-FEROS archived spectra
title_full The AMBRE project: Results from the MATISSE analysis of the ESO-FEROS archived spectra
title_fullStr The AMBRE project: Results from the MATISSE analysis of the ESO-FEROS archived spectra
title_full_unstemmed The AMBRE project: Results from the MATISSE analysis of the ESO-FEROS archived spectra
title_sort ambre project: results from the matisse analysis of the eso-feros archived spectra
publisher EDP Sciences
series EPJ Web of Conferences
issn 2100-014X
publishDate 2012-02-01
description The goal of AMBRE, a joint project between ESO and the Observatoire de la Cote d’Azur, is to provide a homogeneous determination of the stellar parameters (including mean metallicity and some chemical abundances) for the archived spectra of the FEROS, HARPS, UVES and Flames/GIRAFFE spectrographs. We present here a preliminary analysis of the FEROS stellar sample. The stellar parameters, derived using the stellar classification algorithm MATISSE, have been combined with distances and radial velocities in order to explore current theories regarding galactic stellar populations. We have reviewed the sample for potential disk stars with which we can explore kinematic and chemical signatures of the thin and thick disk. We present here a comparison of the potential disk stellar sample to the analysis of 66 disk stars that was carried out in.
url http://dx.doi.org/10.1051/epjconf/20121909008
work_keys_str_mv AT hillv theambreprojectresultsfromthematisseanalysisoftheesoferosarchivedspectra
AT recioblancoa theambreprojectresultsfromthematisseanalysisoftheesoferosarchivedspectra
AT delavernyp theambreprojectresultsfromthematisseanalysisoftheesoferosarchivedspectra
AT worleycc theambreprojectresultsfromthematisseanalysisoftheesoferosarchivedspectra
AT kordopatisg theambreprojectresultsfromthematisseanalysisoftheesoferosarchivedspectra
AT hillv ambreprojectresultsfromthematisseanalysisoftheesoferosarchivedspectra
AT recioblancoa ambreprojectresultsfromthematisseanalysisoftheesoferosarchivedspectra
AT delavernyp ambreprojectresultsfromthematisseanalysisoftheesoferosarchivedspectra
AT worleycc ambreprojectresultsfromthematisseanalysisoftheesoferosarchivedspectra
AT kordopatisg ambreprojectresultsfromthematisseanalysisoftheesoferosarchivedspectra
_version_ 1721241427940212736

Similar Items