The PASTEL catalogue of stellar parameters

By C. Soubiran, J. Campion, G. C. Strobel, A. Caillo. 2010

213 citations recorded by the source corpus.

Aims. The PASTEL catalogue is an update of the [Fe/H] catalogue, published in 1997 and 2001. It is a bibliographical compilation of stellar atmospheric parameters providing (Teff ,l ogg ,[ Fe/H]) determinations obtained from the analysis of high resolution, high signal-to-noise spectra, carried out with model atmospheres. PASTEL also provides determinations of the one parameter Teff based on various methods. It is aimed in the future to provide also homogenized atmospheric parameters and elemental abundances, radial and rotational velocities. A web interface has been created to query the catalogue on elaborated criteria. PASTEL is also distributed through the CDS database and VizieR. Methods. To make it as complete as possible, the main journals have been surveyed, as well as the CDS database, to find relevant publications. The catalogue is regularly updated with new determinations found in the literature. Results. As of Febuary 2010, PASTEL includes 30151 determinations of either Teff or (Teff ,l ogg ,[ Fe/H]) for 16 649 different stars corresponding to 865 bibliographical references. Nearly 6000 stars have a determination of the three parameters (Teff ,l ogg ,[ Fe/H]) with a high quality spectroscopic metallicity.

Subfields: Astronomy and Astrophysics, Computational Mechanics

View Paper: https://www.semanticscholar.org/paper/7e9bbc058f15e04ddc335ca303e8d330f0da9522

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Citations in the corpus

The Gaia-ESO Survey: the analysis of high-resolution UVES spectra of FGK-type stars (2014, methodology): “For the remaining few stars, either the recent values tabulated in the PASTEL catalog (Soubiran et al. 2010) or derived in the works of Rojas-Ayala et al. (2012) and Boyajian et al. (2012), for the M-type dwarfs, were used.”
THE RADIAL VELOCITY EXPERIMENT (RAVE): FIFTH DATA RELEASE (2013, methodology): “This corrected the metallicity offsets with the external datasets of Pasquini et al. (2004); Pancino et al. (2010); Cayrel et al. (2004); Ruchti et al. (2011) and the PASTEL database (Soubiran et al. 2010).”
SWEET-Cat: A catalogue of parameters for Stars With ExoplanETs - I. New atmospheric parameters and masses for 48 stars with planets (2013, methodology): “For the remaining stars, values were compiled from the literature, both from the discovery papers or from other compilations/catalogs (e.g. Luck & Heiter 2007; Soubiran et al. 2010).”
TESTING A PREDICTIVE THEORETICAL MODEL FOR THE MASS LOSS RATES OF COOL STARS (2011, methodology): “In cases whereTeff, logg, or [Fe/H] were estimated from the PASTEL database (Soubiran et al. 2010), we averaged together multiple measurements when more than one was given.”
FUNDAMENTAL PARAMETERS AND CHEMICAL COMPOSITION OF ARCTURUS (2011, methodology): “The PASTEL database of stellar parameters by Soubiran et al. (2010), for example, lists 28 entries for Arcturus, with 24 of them including [Fe/H] determinations from high resolution spectra.”
A CHARA ARRAY SURVEY OF CIRCUMSTELLAR DISKS AROUND NEARBY Be-TYPE STARS (2013, methodology): “The stellar effective temperature Teff and the gravity log g (generally from the compilation of Soubiran et al. 2010) are used to produce a model flux distribution that is based on Kurucz stellar atmosphere models.”
OXYGEN ABUNDANCES IN NEARBY FGK STARS AND THE GALACTIC CHEMICAL EVOLUTION OF THE LOCAL DISK AND HALO (2013, methodology): “For these stars (the “manual” sample), whenever possible, we constrained Teff and/or log g from excitation and ionization balance; otherwise we adopted the averages of values found in the literature, as compiled by Soubiran et al. (2010).”
The PASTEL catalogue: 2016 version (2016, background): “The initial version (Soubiran et al. 2010) included 30 151 records.”
Gaia FGK benchmark stars: Effective temperatures and surface gravities (2015, methodology): “We queried the PASTEL catalogue14 (Soubiran et al. 2010) for temperatures of Gaia FGK benchmark stars published between 2000 and 2012.”
INTRINSIC COLORS, TEMPERATURES, AND BOLOMETRIC CORRECTIONS OF PRE-MAIN-SEQUENCE STARS (2013, background): “…Valenti & Fischer (2005); Paunzen et al. (2006); Gerbaldi et al. (2007); Fitzpatrick & Massa (2007); Prugniel et al. (2007); Zorec et al. (2009); Soubiran et al. (2010); Casagrande et al. (2011), and the authors calculated photometric Teffs for OB dwarf standards using photometry from Hauck &…”
The Kepler characterization of the variability among A- and F-type stars I. General overview (2011, methodology): “Besides papers dedicated to specific targets of our sample, the on-line catalogues by Soubiran et al. (2010), Lafrasse et al. (2010), Kharchenko et al. (2009), Masana, Jordi, & Ribas (2006), Nordström et al. (2004), Glebocki & Stawikowski (2000), Allende Prieto & Lambert (1999), and Wright et al.…”
Gaia FGK benchmark stars: Metallicity (2013, methodology): “Based on the recently updated PASTEL catalogue (Soubiran et al. 2010), metallicity values have been reported in 259 different works until 2012, varying from 57 [Fe/H] measurements in the case of HD140283 to only one measurement forβ Ara (Luck 1979), and no measurement at all forψ Phe.”
XHIP: An extended hipparcos compilation (2011, background): “The PASTEL catalogue of stellar atmospheric parameters (“PASTEL,” Soubiran et al., 2010) is a compilation containing metallicities from over 450 separate sources.”