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<ri:Resource created="2019-07-17T06:55:53Z" 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>CARMENES stars multi wavelength measurements</title><shortName>J/A+A/627/A161</shortName><identifier>ivo://CDS.VizieR/J/A+A/627/A161</identifier><altIdentifier>doi:10.26093/cds/vizier.36270161</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Passegger V.M.</name></creator><creator><name>Schweitzer A.</name></creator><creator><name>Shulyak D.</name></creator><creator><name>Nagel E.</name></creator><creator><name>Hauschildt P.H.,Reiners A.</name></creator><creator><name>Amado P.J.</name></creator><creator><name>Caballero J.A.</name></creator><creator><name>Cortes-Contreras M.,Dominguez-Fernandez A.J.</name></creator><creator><name>Quirrenbach A.</name></creator><creator><name>Ribas I.</name></creator><creator><name>Azarro M.,Anglada-Escude G.</name></creator><creator><name>Bauer F.F.</name></creator><creator><name>Bejar V.J.S.</name></creator><creator><name>Dreizler S.</name></creator><creator><name>Guenther E.W.,Henning T.</name></creator><creator><name>Jeffers S.V.</name></creator><creator><name>Kaminski A.</name></creator><creator><name>Kuerster M.</name></creator><creator><name>Lafarga M.</name></creator><creator><name>Martin E.L.,Montes D.</name></creator><creator><name>Morales J.C.</name></creator><creator><name>Schmidt J.H.M.M.</name></creator><creator><name>Zechmeister M.</name></creator><date role="Updated">2020-01-10T09:51:04Z</date><date role="Created">2019-07-17T06:55:53Z</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>m-stars</subject><subject>metallicity</subject><subject>effective-temperature</subject><subject>spectroscopy</subject><description>We present precise photospheric parameters of 282 M dwarfs determined from fitting the most recent version of PHOENIX models to high-resolution CARMENES spectra in the visible (0.52-0.96um) and near-infrared wavelength range (0.96-1.71um). With its aim to search for habitable planets around M dwarfs, several planets of different masses have been detected. The characterization of the target sample is important for the ability to derive and constrain the physical properties of any planetary systems that are detected. As a continuation of previous work in this context, we derived the fundamental stellar parameters effective temperature, surface gravity, and metallicity of the CARMENES M-dwarf targets from PHOENIX model fits using a {chi}^2^ method. We calculated updated PHOENIX stellar atmosphere models that include a new equation of state to especially account for spectral features of low-temperature stellar atmospheres as well as new atomic and molecular line lists. We show the importance of selecting magnetically insensitive lines for fitting to avoid effects of stellar activity in the line profiles. For the first time, we directly compare stellar parameters derived from multi wavelength range spectra, simultaneously observed for the same star. In comparison with literature values we show that fundamental parameters derived from visible spectra and visible and near-infrared spectra combined are in better agreement than those derived from the same spectra in the near-infrared alone.</description><source format="bibcode">2019A&amp;A...627A.161P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/627/A161</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/J/A+A/612/A49">J/A+A/612/A49 : 324 CARMENES M dwarfs velocities (Reiners+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/623/A44">J/A+A/623/A44 : CARMENES M-dwarfs activity indicators (Schoefer+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/615/A6">J/A+A/615/A6 : Photospheric parameters of CARMENES stars (Passegger+, 2018)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/627/A161</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/627/A161</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/627/A161</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/627/A161</accessURL><mirrorURL title="VizieR at IUCAA: Pune, 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(computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services)</description><ucd>pos.eq.ra</ucd><flag>nullable</flag><flag>indexed</flag></column><column><name>_DE.icrs</name><description>Declination (ICRS) at Epoch=J2016. (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services)</description><ucd>pos.eq.dec</ucd><flag>nullable</flag><flag>indexed</flag></column></table><table><name>J/A+A/627/A161/tableb2</name><description>Basic astrophysical parameters of investigated M dwarfs in multiple wavelength ranges (corrected version)</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Karmn</name><description>Carmencita identifier (JHHMMm+DDMMA)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>TeffVN</name><description>? Effective temperature in VIS+NIR</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>e_TeffVN</name><description>? Error in effective temperature in VIS+NIR</description><unit>K</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>loggVN</name><description>? 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