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<ri:Resource created="2025-10-30T09:17:09Z" status="active" updated="2026-08-31T14:27:10Z" 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>TIC low mass stars radius</title><shortName>J/A+A/703/A8</shortName><identifier>ivo://CDS.VizieR/J/A+A/703/A8</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Mysore Parashivamurthy H.</name></creator><creator><name>Mulders G.D.</name></creator><date role="Updated">2026-08-31T14:27:10Z</date><date role="Created">2025-10-30T09:17:09Z</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>multiple-stars</subject><subject>exoplanets</subject><description>The Transiting Exoplanet Survey Satellite (TESS) has been highly successful in detecting planets in close orbits around low-mass stars, particularly M dwarfs. This presents a valuable opportunity to conduct detailed population studies to understand how these planets depend on the properties of their host stars. The previously observed radius valley in Sun-like stars has also been observed among M dwarfs; however, how its properties vary when compared with more massive stars remains uncertain. We select the volume limited Bioverse stellar catalog, with precise photometric stellar parameters, which was cross-matched with the planet catalog consisting of TESS objects of interests (TOI) candidates and confirmed planets. We detect the radius valley around M dwarfs at a location of 1.64+/-0.03 R_{Earth}_ and with a depth of approximately 45%. The radius valley among GKM stars scales with stellar mass as Rp{prop.to M*^0.15+/-0.04^. The slope is consistent, within 0.3{sigma}, with those around Sun-like stars. For M dwarfs, the discrepancy is 3.6{sigma} with the extrapolated slope from the Kepler FGK sample, marking the point where the deviation from previous results begins. Moreover, we do not see a clear shift in the radius valley between early and mid M dwarfs. The flatter scaling of the radius valley for lower-mass stars suggests that mechanisms other than atmospheric mass loss through photoevaporation may shape the radius distribution of planets around M dwarfs. A comparison of the slope with various planet formation and evolution models leads to a good match with pebble accretion models including water worlds, indicating a potentially different regime of planet formation that can be probed with exoplanets around the lowest-mass stars.</description><source format="bibcode">2025A&amp;A...703A...8M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/703/A8</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/IV/39">IV/39 : TESS Input Catalog version 8.2 (TIC v8.2) (Paegert+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/165/267">J/AJ/165/267 : O2 levels in Nearby Transiting Exoplanets</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/703/A8</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/703/A8</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/703/A8</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/703/A8</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/703/A8</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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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>Gaia-DR3</name><description>Display the Gaia DR3 data (Cat. I/355)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>TIC</name><description>TESS Input Catalog (TIC) identifier</description><ucd>meta.id;meta.main</ucd></column><column><name>Planet</name><description>Number of planet candidates in the system</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Teff</name><description>Stellar effective temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Radius</name><description>Stellar radius</description><unit>solRad</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Mass</name><description>Stellar mass</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Dist</name><description>Stellar distance</description><unit>pc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Per</name><description>? 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