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<ri:Resource created="2013-08-09T09:55:37Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>SWEETCat I. Stellar parameters for host stars</title><shortName>J/A+A/556/A150</shortName><identifier>ivo://CDS.VizieR/J/A+A/556/A150</identifier><altIdentifier>doi:10.26093/cds/vizier.35560150</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Santos N. C.</name></creator><creator><name>Sousa S. G.</name></creator><creator><name>Mortier A.</name></creator><creator><name>Neves V.</name></creator><creator><name>Adibekyan V.</name></creator><creator><name>Tsantaki M.,Delgado Mena E.</name></creator><creator><name>Bonfils X.</name></creator><creator><name>Israelian G.</name></creator><creator><name>Mayor M.</name></creator><creator><name>Udry</name></creator><creator><name>S.</name></creator><date role="Updated">2017-10-16T14:58:04Z</date><date role="Created">2013-08-09T09:55:37Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>multiple-stars</subject><subject>solar-system-planets</subject><subject>late-type-stars</subject><subject>effective-temperature</subject><subject>stellar-masses</subject><subject>metallicity</subject><description>In this paper we present new precise atmospheric parameters for stars with planets. We then take the opportunity to present a new catalogue of stellar parameters for FGK and M stars with planets detected by radial velocity, transit, and astrometry programs. Stellar atmospheric parameters and masses for the sample were derived assuming LTE and using high resolution and high signal-to-noise spectra. The methodology used is based on the measurement of equivalent widths for a list of iron lines and making use of iron ionization and excitation equilibrium principles. For the catalog, and whenever possible, we used parameters derived in previous works published by our team, using well defined methodologies for the derivation of stellar atmospheric parameters. This set of parameters amounts to over 65% of all planet host stars known, including more than 90% of all stars with planets discovered through radial velocity surveys. For the remaining targets, stellar parameters were collected from the literature.</description><source format="bibcode">2013A&amp;A...556A.150S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/556/A150</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/V/133">V/133 : Kepler Input Catalog (Kepler Mission Team, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/551/A112">J/A+A/551/A112 : Metallicity-giant planet correlation (Mortier+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/204/24">J/ApJS/204/24 : Kepler planetary candidates. 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