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<ri:Resource created="2024-02-19T09:09:59Z" 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>23 low mass stars photometry</title><shortName>J/MNRAS/528/5703</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/528/5703</identifier><altIdentifier>doi:10.26093/cds/vizier.75285703</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Swayne M.I.</name></creator><creator><name>Maxted P.F.L.</name></creator><creator><name>Triaud A.H.M.J.</name></creator><creator><name>Sousa S.G.</name></creator><creator><name>Deline A.,Ehrenreich D.</name></creator><creator><name>Hoyer S.</name></creator><creator><name>Olofsson G.</name></creator><creator><name>Boisse I.</name></creator><creator><name>Duck A.</name></creator><creator><name>Gill S.,Martin D.</name></creator><creator><name>McCormac J.</name></creator><creator><name>Persson C.M.</name></creator><creator><name>Santerne A.</name></creator><creator><name>Sebastian D.,Standing M.R.</name></creator><creator><name>Acuna L.</name></creator><creator><name>Alibert Y.</name></creator><creator><name>Alonso R.</name></creator><creator><name>Anglada G.</name></creator><creator><name>Barczy T.,Barrado Navascues D.</name></creator><creator><name>Barros S.C.C.</name></creator><creator><name>Baumjohann W.</name></creator><creator><name>Baycroft T.A.</name></creator><creator><name>Beck M.,Beck T.</name></creator><creator><name>Benz W.</name></creator><creator><name>Billot N.</name></creator><creator><name>Bonfils X.</name></creator><creator><name>Borsato L.</name></creator><creator><name>Bourrier V.,Brandeker A.</name></creator><creator><name>Broeg C.</name></creator><creator><name>Carmona A.</name></creator><creator><name>Charnoz S.</name></creator><creator><name>Collier Cameron A.,Cortes-Zuleta P.</name></creator><creator><name>Csizmadia Sz.</name></creator><creator><name>Cubillos P.E.</name></creator><creator><name>Davies M.B.</name></creator><creator><name>Deleuil M.,Delfosse X.</name></creator><creator><name>Delrez L.</name></creator><creator><name>Demangeon O.D.S.</name></creator><creator><name>Demory B.-O.</name></creator><creator><name>Dransfield G.,Erikson A.</name></creator><creator><name>Fortier A.</name></creator><creator><name>Forveille T.</name></creator><creator><name>Fossati L.</name></creator><creator><name>Fridlund M.</name></creator><creator><name>Gandolfi D.,Gillon M.</name></creator><creator><name>Guedel M.</name></creator><creator><name>Guenther M.N.</name></creator><creator><name>Hara N.</name></creator><creator><name>Hebrard G.</name></creator><creator><name>Heidari N.,Hellier C.</name></creator><creator><name>Helling C.</name></creator><creator><name>Isaak K.G.</name></creator><creator><name>Kerschbaum F.</name></creator><creator><name>Kiefer F.</name></creator><creator><name>Kiss L.L.,Kunovac V.</name></creator><creator><name>Lalitha S.</name></creator><creator><name>Lam K.W.F.</name></creator><creator><name>Laskar J.</name></creator><creator><name>Lecavelier des Etangs A.,Lendl M.</name></creator><creator><name>Magrin D.</name></creator><creator><name>Marafatto L.</name></creator><creator><name>Martioli E.</name></creator><creator><name>Miller N.J.</name></creator><creator><name>Mordasini C.,Moutou C.</name></creator><creator><name>Nascimbeni V.</name></creator><creator><name>Ottensamer R.</name></creator><creator><name>Pagano I.</name></creator><creator><name>Palle E.</name></creator><creator><name>Peter G.,Piazza D.</name></creator><creator><name>Piotto G.</name></creator><creator><name>Pollacco D.</name></creator><creator><name>Queloz D.</name></creator><creator><name>Ragazzoni R.</name></creator><creator><name>Rando N.,Rauer H.</name></creator><creator><name>Ribas I.</name></creator><creator><name>Santos N.C.</name></creator><creator><name>Scandariato G.</name></creator><creator><name>Segransan D.</name></creator><creator><name>Simon A.E.,Smith A.M.S.</name></creator><creator><name>Southworth R.</name></creator><creator><name>Stalport M.</name></creator><creator><name>Szabo Gy.M.</name></creator><creator><name>Thomas N.</name></creator><creator><name>Udry S.,Ulmer B.</name></creator><creator><name>Van Grootel V.</name></creator><creator><name>Venturini J.</name></creator><creator><name>Walton N.A.</name></creator><creator><name>Willett E.</name></creator><creator><name>Wilson T.G.</name></creator><date role="Updated">2024-11-06T20:35:14Z</date><date role="Created">2024-02-19T09:09:59Z</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>m-stars</subject><subject>photometry</subject><subject>visible-astronomy</subject><description>Observations of low-mass stars have frequently shown a disagreement between observed stellar radii and radii predicted by theoretical stellar structure models. This "`radius inflation" problem could have an impact on both stellar and exoplanetary science. We present the final results of our observation programme with the CHEOPS satellite to obtain high-precision light curves of eclipsing binaries with low mass stellar companions (EBLMs). Combined with the spectroscopic orbits of the solar-type companion, we can derive the masses, radii and effective temperatures of 23 M-dwarf stars. We use the PYCHEOPS data analysis software to analyse their primary and secondary occultations. For all but one target, we also perform analyses with TESS light curves for comparison. We have assessed the impact of starspot-induced variation on our derived parameters and account for this in our radius and effective temperature uncertainties using simulated light curves. We observe trends for inflation with both metallicity and orbital separation. We also observe a strong trend in the difference between theoretical and observational effective temperatures with metallicity. There is no such trend with orbital separation. These results are not consistent with the idea that observed inflation in stellar radius combines with lower effective temperature to preserve the luminosity predicted by low-mass stellar models. Our EBLM systems are high- quality and homogeneous measurements that can be used in further studies into radius inflation.</description><source format="bibcode">2024MNRAS.528.5703S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/528/5703</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><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/626/A119">J/A+A/626/A119 : EBLM J2349-32 photometry, RV and spectra (Gill+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/519/3546">J/MNRAS/519/3546 : The EBLM project - IX. 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