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<ri:Resource created="2023-07-10T08:13:09Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>Low-mass eclipsing binaries</title><shortName>J/MNRAS/521/3405</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/521/3405</identifier><altIdentifier>doi:10.26093/cds/vizier.75213405</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Jennings Z.</name></creator><creator><name>Southworth J.</name></creator><creator><name>Maxted P.F.L.</name></creator><creator><name>Mancini L.</name></creator><date role="Updated">2024-08-22T20:17:08Z</date><date role="Created">2023-07-10T08:13:09Z</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>photometry</subject><subject>visible-astronomy</subject><description>Precise measurements of stellar parameters are required in order to develop our theoretical understanding of stellar structure. These measurements enable errors and uncertainties to be quantified in theoretical models and constrain the physical interpretation of observed phenomena, such as the inflated radii of low-mass stars. We use newly-available TESS (Transiting Exoplanet Survey Satellite) light curves combined with published radial velocity measurements to improve the characterization of 12 low mass eclipsing binaries composed of an M dwarf accompanied by a brighter F/G star. We present and analyse ground-based simultaneous four-colour photometry for two targets. Our results include the first measurements of the fundamental properties of two of the systems. Light curve and radial velocity information were converted into the physical parameters of each component of the systems using an isochrone fitting method. We also derive the effective temperatures of the M dwarfs, almost tripling the number of such measurements. The results are discussed in the context of radius inflation. We find that exquisite precision in the age estimation of young objects is required to determine their inflation status. Ho wever, all but three of the objects are securely located among the main sequence, demonstrating radius inflation and the necessity to develop our understanding of the complex physical processes governing the evolution of low-mass stars. We investigated the hypothesis that luminosity is unaffected by the inflation problem but the findings were not conclusive.</description><source format="bibcode">2023MNRAS.521.3405J</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/521/3405</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>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/396/1023">J/MNRAS/396/1023 : Transiting planetary system WASP-5 (Southworth+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/399/287">J/MNRAS/399/287 : Transiting planetary system WASP-4 (Southworth+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/707/167">J/ApJ/707/167 : Transiting planetary system WASP-18 (Southworth+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/408/1680">J/MNRAS/408/1680 : Transiting planetary system WASP-2 (Southworth+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/527/A8">J/A+A/527/A8 : Transiting planetary system WASP-7 (Southworth+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/420/2580">J/MNRAS/420/2580 : Four transits of HAT-P-13 (Southworth+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/422/3099">J/MNRAS/422/3099 : Transits of HAT-P-5 (Southworth+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/426/1338">J/MNRAS/426/1338 : Transiting planetary system WASP-17 (Southworth+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/434/1300">J/MNRAS/434/1300 : Planetary systems WASP-15, WASP-16 (Southworth+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/444/776">J/MNRAS/444/776 : WASP-24, WASP-25 and WASP-26 (Southworth+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/447/711">J/MNRAS/447/711 : Transiting planetary system WASP-103 (Southworth+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/454/3094">J/MNRAS/454/3094 : Transiting planetary system WASP-57 (Southworth+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/457/4205">J/MNRAS/457/4205 : WASP-22, WASP-41, WASP-42 and WASP-55 (Southworth+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/153/191">J/AJ/153/191 : Transiting planetary system GJ 1132 (Southworth+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/490/4230">J/MNRAS/490/4230 : Transiting planet WASP-4b (Southworth+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/635/A73">J/A+A/635/A73 : Multiplicity study of transiting exoplanet hosts. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Filter</name><description>Filter used for the observation</description><ucd>instr.setup;instr.filter</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>BJD</name><description>Barycentric Julian Date for the midpoint of observation (TDB)</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>mag</name><description>Differential magnitude magnitude</description><unit>mag</unit><ucd>phot.mag;arith.diff</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_mag</name><description>Measurement error of the differential magnitude</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table><table><name>J/MNRAS/521/3405/tyc3121</name><description>Differential photometry of TYC 3121-1659-1</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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