Stellar Radial Velocities, Atmospheric Parameters and Chemical Abundances
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https://doi.eso.org/10.18727/archive/18
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资源简介:
The MATISSE/OCA-ESO project AMBRE (Archéologie avec Matisse: aBondances dans les aRchives de l'ESO) has been designed to automatically analyse the spectral archives of the FEROS, UVES and HARPS instruments with the MATISSE algorithm (Recio-Blanco et al., 2006MNRAS.370..141R). Stellar radial velocity, atmospheric parameters (effective temperature, surface gravity, mean metallicity [M/H]) and enrichment in α-elements ([α/Fe]) are the main products of this analysis (see de Laverny et al., 2013Msngr.153...18D). The parameterisation relies on a specific grid of synthetic spectra (de Laverny et al., 2012A&A...544A.126D) and is detailed in Worley et al. (2016, A&A...591A..81W).
提供机构:
European Southern Observatory (ESO)
创建时间:
2022-04-01



