Metallicity of M dwarfs. III.

DOI

The aim of this work is the study of the planet-metallicity and the planet-stellar mass correlations for M dwarfs from the HARPS GTO M dwarf subsample. We use a new method that takes advantage of the HARPS high-resolution spectra to increase the precision of metallicity, using previous photometric calibrations of [Fe/H] and effective temperature as starting values.

Cone search capability for table J/A+A/551/A36/table2 (HARPS M dwarf sample, sorted by right ascension)

Cone search capability for table J/A+A/551/A36/table8 (California Planet Survey (CPS) sample, sorted by right ascension)

Identifier
DOI http://doi.org/10.26093/cds/vizier.35510036
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/551/A36
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/551/A36
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/551/A36
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/551/A36
Provenance
Creator Neves V.; Bonfils X.; Santos N.C.; Delfosse X.; Forveille T.; Allard F.,Udry S.
Publisher CDS
Publication Year 2013
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Interdisciplinary Astronomy; Natural Sciences; Physics; Stellar Astronomy