Catalogue of [Fe/H] determinations for FGK stars: 2001 edition

By G. C. Strobel, C. Soubiran, N. R. O. D. Paris-Meudon, O. Bordeaux. 2001

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The catalogue presented here is a compilation of published atmospheric parameters ($T_\mathrm{eff}$, $\log g$, [Fe/H]) obtained from high resolution, high signal-to-noise spectroscopic observations. This new edition has changed compared to the five previous versions. It is now restricted to intermediate and low mass stars (F, G and K stars). It contains 6354 determinations of ($T_\mathrm{eff}$, $\log g$, [Fe/H]) for 3356 stars, including 909 stars in 79 stellar systems. The literature is complete between January 1980 and December 2000 and includes 378 references. The catalogue is made up of two tables, one for field stars and one for stars in galactic associations, open and globular clusters and external galaxies. The catalogue is distributed through the CDS database. Access to the catalogue with cross-identification to other sets of data is also possible with VizieR (Ochsenbein et al. [CITE]).

Subfields: Astronomy and Astrophysics, Computational Mechanics

View Paper: https://www.semanticscholar.org/paper/b7567b36ace66417169a8a5ca33ee179c011651c

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Citations in the corpus

Evolutionary synthesis of galaxies at high spectral resolution with the code PEGASE-HR. Metallicity and age tracers (2004, methodology): “The atmospheric parameters of the stars (Teff , g, [Fe/H]) are taken from the literature in an up-to-date version of Cayrel de Strobel et al. (2001), when available.”
Post-T Tauri Stars in the Nearest OB Association (2002, result): “Although changing the classification of some standards may appear imprudent, the H-R diagram positions, Sr/Fe line ratio, and derived log g values (Cayrel de Strobel et al. 2001) are all consistent with our new adopted luminosity classes3.”
Coudé-feed stellar spectral library – atmospheric parameters (2010, background): “Cayrel de Strobel et al. (2001) present a compilation of published atmospheric parameters obtained from various sources and hence their data are inhomogeneous.”
ULySS: a full spectrum fitting package (2009, background): “The effective temperature,Teff, surface gravity, log(g), and metallicity, [Fe/H], are fundamental characteristics that can be derived from spectroscopic analysis (Cayrel de Strobel et al. 2001).”
Effective temperature scale and bolometric corrections from 2MASS photometry (2006, methodology): “The metallicity was extracted from the compilation of Cayrel de Strobel et al. (2001) or computed from uvby–β photometry – either measured from our own observations or obtained from the Hauck & Mermilliod (1998) catalogue –, using a slightly revised version of the Schuster & Nissen (1989)…”
STELIB: A library of stellar spectra at R 2000 ?;?? (2003, background): “Most of the atmospheric parameters (Teff, log(g), [Fe/H]) listed in Tables 5 to 10 come from the 2 latest editions of the Catalogue of [Fe/H] determinations (Cayrel de Strobel et al. 1997, 2001).”
SPECTRAL PROPERTIES OF COOL STARS: EXTENDED ABUNDANCE ANALYSIS OF 1,617 PLANET-SEARCH STARS (2016, background): “However, different data sets often had large differences in the derived Teff , log g and metallicity (Cayrel de Strobel et al. 2001) limiting their usefulness in detailed comparisons between them and precluded most comparisons of abundances altogether.”
Vertical distribution of Galactic disk stars - I. Kinematics and metallicity (2002, methodology): “The TGMET library was built from the ELODIE database described in Prugniel & Soubiran (2001), selecting high S/N spectra of reference stars having well known atmospheric parameters from published detailed analyses listed in the Catalogue of [Fe/H] determinations (Cayrel de Strobel et al. 2001).”
Vertical distribution of Galactic disk stars , IV. AMR and AVR from clump giants (2007, methodology): “…using the ELODIE spectrograph at OHP, we have also taken advantage of other available material like the Hipparcos and Tycho2 catalogues, the [Fe/H] catalogue (Cayrel de Strobel et al. 2001) updated with a number of new references and the PARAM code to derive ages (da Silva et al. 2006).”