The planet-metallicity correlation.

DOI

We have recently carried out spectral synthesis modeling to determine T_eff_, log(g), vsin(i), and [Fe/H] for 1040 FGK-type stars on the Keck, Lick, and Anglo-Australian Telescope planet search programs. This is the first time that a single, uniform spectroscopic analysis has been made for every star on a large Doppler planet search survey. We identify a subset of 850 stars that have Doppler observations sufficient to detect uniformly all planets with radial velocity semiamplitudes K>30m/s and orbital periods shorter than 4yr.

Cone search capability for table J/ApJ/622/1102/table1 (Derived parameters for stars with planets)

Cone search capability for table J/ApJ/622/1102/table3 (Stars with uniform planet detectability)

Identifier
DOI http://doi.org/10.26093/cds/vizier.16221102
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/ApJ/622/1102
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/622/1102
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/622/1102
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/ApJ/622/1102
Provenance
Creator Fischer D.A.; Valenti J.
Publisher CDS
Publication Year 2006
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; Solar System Astronomy; Stellar Astronomy