Automated stellar spectra parameterisation for Gaia-RVS

Degeneracies in the stellar atmospheric parameters can pollute large spectroscopic surveys, introducing possible biases in the derived distances, kinematics and chemical abundances. We focus at the wavelength range shared by RAVE, the RVS of Gaia and the ESO-FLAMES/GIRAFFE spectrograph setups LR8 an...

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Main Authors: Wyse R.F.G., Gilmore G., Hill V., Bijaoui A., de Laverny P., Recio-Blanco A., Kordopatis G., Ordenovic C.
Format: Article
Language:English
Published: EDP Sciences 2012-02-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/20121909010
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author Wyse R.F.G.
Gilmore G.
Hill V.
Bijaoui A.
de Laverny P.
Recio-Blanco A.
Kordopatis G.
Ordenovic C.
author_facet Wyse R.F.G.
Gilmore G.
Hill V.
Bijaoui A.
de Laverny P.
Recio-Blanco A.
Kordopatis G.
Ordenovic C.
author_sort Wyse R.F.G.
collection DOAJ
description Degeneracies in the stellar atmospheric parameters can pollute large spectroscopic surveys, introducing possible biases in the derived distances, kinematics and chemical abundances. We focus at the wavelength range shared by RAVE, the RVS of Gaia and the ESO-FLAMES/GIRAFFE spectrograph setups LR8 and HR21. Based on the algorithms DEGAS and MATISSE, trained on a grid of synthetic spectra, we propose a pipeline in order to derive the atmospheric parameters.
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spelling doaj.art-d7bd596a422b4316a138ebb7e9d24f352022-12-21T19:30:56ZengEDP SciencesEPJ Web of Conferences2100-014X2012-02-01190901010.1051/epjconf/20121909010Automated stellar spectra parameterisation for Gaia-RVSWyse R.F.G.Gilmore G.Hill V.Bijaoui A.de Laverny P.Recio-Blanco A.Kordopatis G.Ordenovic C.Degeneracies in the stellar atmospheric parameters can pollute large spectroscopic surveys, introducing possible biases in the derived distances, kinematics and chemical abundances. We focus at the wavelength range shared by RAVE, the RVS of Gaia and the ESO-FLAMES/GIRAFFE spectrograph setups LR8 and HR21. Based on the algorithms DEGAS and MATISSE, trained on a grid of synthetic spectra, we propose a pipeline in order to derive the atmospheric parameters.http://dx.doi.org/10.1051/epjconf/20121909010
spellingShingle Wyse R.F.G.
Gilmore G.
Hill V.
Bijaoui A.
de Laverny P.
Recio-Blanco A.
Kordopatis G.
Ordenovic C.
Automated stellar spectra parameterisation for Gaia-RVS
EPJ Web of Conferences
title Automated stellar spectra parameterisation for Gaia-RVS
title_full Automated stellar spectra parameterisation for Gaia-RVS
title_fullStr Automated stellar spectra parameterisation for Gaia-RVS
title_full_unstemmed Automated stellar spectra parameterisation for Gaia-RVS
title_short Automated stellar spectra parameterisation for Gaia-RVS
title_sort automated stellar spectra parameterisation for gaia rvs
url http://dx.doi.org/10.1051/epjconf/20121909010
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