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<ri:Resource created="2019-07-05T13:10:02Z" 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>EBLM J2349-32 photometry, RV and spectra</title><shortName>J/A+A/626/A119</shortName><identifier>ivo://CDS.VizieR/J/A+A/626/A119</identifier><altIdentifier>doi:10.26093/cds/vizier.36260119</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Gill S.</name></creator><creator><name>Maxted P.F.L.</name></creator><creator><name>Evans J.A.</name></creator><creator><name>Evans D.F.</name></creator><creator><name>Southworth J.</name></creator><creator><name>Smalley B.,Gary B.L.</name></creator><creator><name>Anderson D.R.</name></creator><creator><name>Bouchy F.</name></creator><creator><name>Cameron A.C.</name></creator><creator><name>Dominik M.</name></creator><creator><name>Faedi F.,Gillon M.</name></creator><creator><name>Gomez Maqueo Chew L.Hebb Y.</name></creator><creator><name>Hellier C.</name></creator><creator><name>Jorgensen U.G.,Longa-Pena P.</name></creator><creator><name>Martin D.V.</name></creator><creator><name>McCormac J.</name></creator><creator><name>Pepe F.V.</name></creator><creator><name>Pollaco D.</name></creator><creator><name>Queloz D.,Segransan D.</name></creator><creator><name>Snodgrass C.</name></creator><creator><name>Turner O.D.</name></creator><creator><name>Triaud A.H.M.</name></creator><creator><name>Udry S.</name></creator><creator><name>West R.G.</name></creator><date role="Updated">2019-07-26T14:08:11Z</date><date role="Created">2019-07-05T13:10:02Z</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>eclipsing-binary-stars</subject><subject>radial-velocity</subject><subject>photometry</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><description>Some M-dwarfs around F-/G-type stars have been measured to be hotter and larger than predicted by stellar evolution models. Inconsistencies between observations and models need to be addressed with more mass, radius, and luminosity measurements of low-mass stars to test and refine evolutionary models. Our aim is to measure the masses, radii and ages of the stars in five low-mass eclipsing binary systems discovered by the WASP survey. We used WASP photometry to establish eclipse-time ephemerides and to obtain initial estimates for the transit depth and width. Radial velocity measurements were simultaneously fitted with follow-up photometry to find the best-fitting orbital solution. This solution was combined with measurements of atmospheric parameters to interpolate evolutionary models and estimate the mass of the primary star, and the mass and radius of the M-dwarf companion. We assess how the best fitting orbital solution changes if an alternative limb-darkening law is used and quantify the systematic effects of unresolved companions. We also gauge how the best-fitting evolutionary model changes if different values are used for the mixing length parameter and helium enhancement. We report the mass and radius of five M-dwarfs and find little evidence of inflation with respect to evolutionary models. The primary stars in two systems are near the "blue hook" stage of their post sequence evolution, resulting in two possible solutions for mass and age. We find that choices in helium enhancement and mixing-length parameter can introduce an additional 3-5% uncertainty in measured M-dwarf mass. Unresolved companions can introduce an additional 3-8% uncertainty in the radius of an M-dwarf, while the choice of limb-darkening law can introduce up to an additional 2% uncertainty. The choices in orbital fitting and evolutionary models can introduce significant uncertainties in measurements of physical properties of such systems.</description><source format="bibcode">2019A&amp;A...626A.119G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/626/A119</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/549/A18">J/A+A/549/A18 : WASP-30 and J1219-39 light + velocity curves (Triaud+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/572/A50">J/A+A/572/A50 : J0113+31 light + velocity curves (Gomez Maqueo Chew+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/604/L6">J/A+A/604/L6 : EBLM J0555-57 photometry and RV (von Boetticher+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/625/A150">J/A+A/625/A150 : 10 very-low-mass stars photometry (von Boetticher+, 2019)</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/626/A119</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/626/A119</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/626/A119</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/626/A119</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/626/A119</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/626/A119</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/A+A/626/A119/table1 (List of studied stars)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/626/A119/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/626/A119/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/626/A119/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>357.3134583</ra><dec>-32.7715278</dec><sr>0.005555555555555556</sr></testQuery></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/A+A/626/A119/list (List of fits spectra)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/626/A119/list?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/626/A119/list?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/626/A119/list?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>357.3135</ra><dec>-32.77153</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/14909 16442 35325 44928 46468</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/626/A119?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/626/A119/table1</name><description>List of studied stars</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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