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<ri:Resource created="2021-07-16T10:21:54Z" 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 project. VIII.43 M-dwarf light curve</title><shortName>J/MNRAS/506/306</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/506/306</identifier><altIdentifier>doi:10.26093/cds/vizier.75060306</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>Broeg C.,Floren H.-G.</name></creator><creator><name>Guterman P.</name></creator><creator><name>Simon A.E.</name></creator><creator><name>Boisse I.</name></creator><creator><name>Bonfanti A.</name></creator><creator><name>Martin D.,Santerne A.</name></creator><creator><name>Salmon S.</name></creator><creator><name>Standing M.R.</name></creator><creator><name>Van Grootel V.</name></creator><creator><name>Wilson T.G.,Alibert Y.</name></creator><creator><name>Alonso R.</name></creator><creator><name>Anglada Escude G.</name></creator><creator><name>Asquier J.</name></creator><creator><name>Barczy T.</name></creator><creator><name>Barrado D.,Barros S.C.C.</name></creator><creator><name>Battley M.</name></creator><creator><name>Baumjohann W.</name></creator><creator><name>Beck M.</name></creator><creator><name>Beck T.</name></creator><creator><name>Bekkelien A.,Benz W.</name></creator><creator><name>Billot N.</name></creator><creator><name>Bonfils X.</name></creator><creator><name>Brandeker A.</name></creator><creator><name>Busch M.-D.</name></creator><creator><name>Cabrera J.,Charnoz S.</name></creator><creator><name>Collier Cameron A.</name></creator><creator><name>Csizmadia Sz.</name></creator><creator><name>Davies M.B.</name></creator><creator><name>Deleuil M.,Deline A.</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.,Ehrenreich D.</name></creator><creator><name>Erikson A.</name></creator><creator><name>Fortier A.</name></creator><creator><name>Fossati L.</name></creator><creator><name>Fridlund M.</name></creator><creator><name>Futyan D.,Gandolfi D.</name></creator><creator><name>Gillon M.</name></creator><creator><name>Guedel M.</name></creator><creator><name>Hebrard G.</name></creator><creator><name>Heidari N.</name></creator><creator><name>Hellier C.,Heng K.</name></creator><creator><name>Hobson M.</name></creator><creator><name>Hoyer S.</name></creator><creator><name>Isaak K.G.</name></creator><creator><name>Kiss L.</name></creator><creator><name>Kunovac Hodzic V.,Lalitha S.</name></creator><creator><name>Laskar J.</name></creator><creator><name>Lecavelier des Etangs A.</name></creator><creator><name>Lendl M.</name></creator><creator><name>Lovis C.,Magrin D.</name></creator><creator><name>Marafatto L.</name></creator><creator><name>McCormac J.</name></creator><creator><name>Miller N.</name></creator><creator><name>Nascimbeni V.</name></creator><creator><name>Olofsson G.,Ottensamer R.</name></creator><creator><name>Pagano I.</name></creator><creator><name>Palle E.</name></creator><creator><name>Peter G.</name></creator><creator><name>Piotto G.</name></creator><creator><name>Pollacco D.,Queloz D.</name></creator><creator><name>Ragazzoni R.</name></creator><creator><name>Rando N.</name></creator><creator><name>Rauer H.</name></creator><creator><name>Ribas I.</name></creator><creator><name>Santos N.C.,Scandariato G.</name></creator><creator><name>Segransan D.</name></creator><creator><name>Smith A.M.S.</name></creator><creator><name>Steinberger M.</name></creator><creator><name>Steller M.,Szabo G.M.</name></creator><creator><name>Thomas N.</name></creator><creator><name>Udry S.</name></creator><creator><name>Walter I.</name></creator><creator><name>Walton N.A.</name></creator><creator><name>Willett E.</name></creator><date role="Updated">2024-08-21T20:18:15Z</date><date role="Created">2021-07-16T10:21:54Z</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><description>The accuracy of theoretical mass, radius and effective temperature values for M-dwarf stars is an active topic of debate. Differences between observed and theoretical values have raised the possibility that current theoretical stellar structure and evolution models are inaccurate towards the low-mass end of the main sequence. To explore this issue we use the CHEOPS satellite to obtain high-precision light curves of eclipsing binaries with low mass stellar companions. We use these light curves combined with the spectroscopic orbit for the solar-type companion to measure the mass, radius and effective temperature of the M-dwarf star. Here we present the analysis of three eclipsing binaries. We use the pycheops data analysis software to fit the observed transit and eclipse events of each system. Two of our systems were also observed by the TESS satellite - we similarly analyse these light curves for comparison. We find consistent results between CHEOPS and TESS, presenting three stellar radii and two stellar effective temperature values of low-mass stellar objects. These initial results from our on-going observing programme with CHEOPS show that we can expect to have ~24 new mass, radius and effective temperature measurements for very low mass stars within the next few years.</description><source format="bibcode">2021MNRAS.506..306S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/506/306</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></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/MNRAS/506/306</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/506/306</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/506/306</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/506/306</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/506/306</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/506/306</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/MNRAS/506/306/list (List of fits files)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/506/306/list?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/506/306/list?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/506/306/list?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>265.338625</ra><dec>31.4153611</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/12334 32689 47528</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/506/306?format=ascii</footprint></coverage><tableset><schema><name>default</name><table><name>J/MNRAS/506/306/j1741</name><description>Detrended CHEOPS light curve containing the transit and eclipse of EBLM J1741+31</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>Time</name><description>Time of observation (JD-2450000)</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Flux</name><description>Detrended flux</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Flux</name><description>Error on flux</description><ucd>stat.error;phot.flux</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table><table><name>J/MNRAS/506/306/j1934</name><description>Detrended CHEOPS light curve containing the transit and eclipse of EBLM J1934-42</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>Time</name><description>Time of observation (JD-2450000)</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Flux</name><description>Detrended flux</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Flux</name><description>Error on flux</description><ucd>stat.error;phot.flux</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table><table><name>J/MNRAS/506/306/j2046</name><description>Detrended CHEOPS light curve containing the transit and eclipse of EBLM J2046+06</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>Time</name><description>Time of observation (JD-2450000)</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Flux</name><description>Detrended flux</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Flux</name><description>Error on flux</description><ucd>stat.error;phot.flux</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table><table><name>J/MNRAS/506/306/list</name><description>List of fits files</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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