The PASTEL catalogue: 2016 version
By C. Soubiran, J. Campion, N. Brouillet, L. Chemin. 2016
166 citations recorded by the source corpus.
The bibliographical compilation of stellar atmospheric parameters (Teff, logg, [Fe/H]) relying on high-resolution, high signal-to-noise spectroscopy started in the eighties with the so-called [Fe/H] catalogue, and was continued in 2010 with the PASTEL catalogue, which also includes determinations of Teff alone, based on various methods. Here we present an update of the PASTEL catalogue. The main journals and the CDS database have been surveyed to find relevant publications presenting new determinations of atmospheric parameters. As of February 2016, PASTEL includes 64082 determinations of either Teff or (Teff, logg, [Fe/H]) for 31401 stars, corresponding to 1142 bibliographical references. Some 11197 stars have a determination of the three parameters (Teff, logg, [Fe/H]) with a high-quality spectroscopic metallicity.
Subfields: Astronomy and Astrophysics, Instrumentation
View Paper: https://www.semanticscholar.org/paper/e2f77290735b895a4410020419fd42e5f42b3d50
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Citations in the corpus
- Accurate Empirical Radii and Masses of Planets and Their Host Stars with Gaia Parallaxes (2016, methodology): “However, where possible, we opted to instead use Teff , glog , and [Fe/H] from the recently updated PASTEL catalog (Soubiran et al. 2016), which compiles stellar properties determined from high-quality8 spectroscopic analyses in the literature.”
- The Revised TESS Input Catalog and Candidate Target List (2019, background): “…Catalogs in the TIC Name Data Release Approximate No. of Stars Priority References SPOCS L 1.6 k 1 Brewer et al. (2016) PASTEL L 93 k 2 Soubiran et al. (2016) Gaia-ESO DR3 29 k 3 Gilmore et al. (2012) TESS-HERMES DR1 25 k 4 Sharma et al. (2018) GALAH DR2 340 k 5 Buder et al. (2018)…”
- Fundamental Parameters of 87 Stars from the Navy Precision Optical Interferometer (2017, background): “…on the star’s SIMBAD spectral type; (5) Le Borgne et al. (2003), (6) Houdashelt et al. (2000), (7) Katz et al. (2011), (8) Valdes et al. (2004), (9) Soubiran et al. (2016), (10)Milone et al. (2011), (11) Prugniel et al. (2011), (12) Bordé et al. (2002), (13) Hekker & Meléndez (2007), and (14)…”