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<ri:Resource created="2015-09-03T13:54:48Z" 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>Northern bright planet host stars parameters</title><shortName>J/A+A/576/A94</shortName><identifier>ivo://CDS.VizieR/J/A+A/576/A94</identifier><altIdentifier>doi:10.26093/cds/vizier.35760094</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Sousa S.G.</name></creator><creator><name>Santos N.C.</name></creator><creator><name>Mortier A.</name></creator><creator><name>Tsantaki M.</name></creator><creator><name>Adibekyan V.,Delgado Mena E.</name></creator><creator><name>Israelian G.</name></creator><creator><name>Rojas-Ayala B.</name></creator><creator><name>Neves V.</name></creator><date role="Updated">2018-01-05T08:56:25Z</date><date role="Created">2015-09-03T13:54:48Z</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>metallicity</subject><description>In this work we derive new precise and homogeneous parameters for 37 stars with planets. For this purpose, we analyze high resolution spectra obtained by the NARVAL spectrograph for a sample composed of bright planet host stars in the northern hemisphere. The new parameters are included in the SWEET-Cat online catalogue. To ensure that the catalogue is homogeneous, we use our standard spectroscopic analysis procedure, ARES + MOOG, to derive effective temperatures, surface gravities, and metallicities. 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