Catalog Service: Metallicity of M dwarfs. III.
Description
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.
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Publisher: CDSivo://CDS[Pub. ID]
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This resource was registered on: 2013 Aug 23 08:48:24ZThis resource description was last updated on: 2021 Oct 21 00:00:00Z
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This section describes the data's coverage over the sky, frequency, and time.
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This is service that does not comply with any IVOA standard but instead provides access to special capabilities specific to this resource.
This is a standard IVOA service that takes as input an ADQL or PQL query and returns tabular data.
This is a standard IVOA service that takes as input a position in the sky and a radius and returns catalog records with positions within that radius.
Cone search capability for table J/A+A/551/A36/table2 (HARPS M dwarf sample, sorted by right ascension)
VERB=1
VERB=3
Cone search capability for table J/A+A/551/A36/table8 (California Planet Survey (CPS) sample, sorted by right ascension)
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