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xmlns:vodm="http://www.ivoa.net/xml/DataModel/v1" xmlns:voe="http://www.ivoa.net/xml/VOEventRegExt/v2" xmlns:vosi10="http://www.ivoa.net/xml/VOSITables/v1.0" xmlns:vot="http://www.ivoa.net/xml/VOTable/v1.2" xmlns:vot0="http://www.ivoa.net/xml/VOTable/v1.3" xmlns:vot1="http://www.ivoa.net/xml/VOTable/v1.1" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vr0="https://www.ivoa.net/xml/VOResource/v1.0" xmlns:vr1="http://www.ivoa.net/xml/VOResource/v1.1" xmlns:vr2="http://Www.ivoa.net/xml/VOResource/v1.0" xmlns:vr3="http://www.ivoa.net/xml/VOResource/v1%20.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:vs0="http://www.ivoa.net/xml/VODataService/v1.0" xmlns:vs1="https://www.ivoa.net/xml/VODataService/v1.0" xmlns:vstd="http://www.ivoa.net/xml/StandardsRegExt/v1.0" xmlns:xdtn="http://www.w3.org/2004/07/xpath-datatypes" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:xlink0="https://www.w3.org/1999/xlink" xmlns:xsd="http://www.w3.org/2001/XMLSchema" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:xsi0="https://www.w3.org/2001/XMLSchema-instance" xmlns:xu="http://www.xmldb.org/xupdate"><oai:identifier>ivo://CDS.VizieR/J/ApJ/993/233</oai:identifier><oai:datestamp>2026-04-07T10:34:12Z</oai:datestamp><oai:setSpec>J.ApJ</oai:setSpec></oai:header><oai:metadata><eudc:resource xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:eudc="http://schema.eudat.eu/schema/kernel-1" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:oai="http://www.openarchives.org/OAI/2.0/" xmlns:dachs="urn:dachs" xsi:schemaLocation="http://schema.eudat.eu/schema/kernel-1           http://docs.g-vo.org/schemata/eudat-core.xsd"><eudc:community>IVOA</eudc:community><eudc:titles><eudc:title>Stellar and planetary param. of M-dwarf systems</eudc:title></eudc:titles><eudc:descriptions><eudc:description>Planetary radii are derived for 218 exoplanets orbiting 161 M dwarf stars. Stellar radii are based on an analysis of APOGEE high-resolution near-IR spectra for a subsample of the M dwarfs; these results are used to define a stellar radius-M_Ks_ calibration that is applied to the sample of M-dwarf planet hosts. The planetary radius distribution displays a gap over Rp~1.6-2.0R_{Earth}_, bordered by two peaks at Rp~1.2-1.6R_{Earth}_ (super-Earths) and 2.0-2.4R_{Earth}_ (sub-Neptunes). The radius gap is nearly constant with exoplanetary orbital period (a power-law slope of m=+0.01_-0.04_^+0.03^), which is different (2{sigma}-3{sigma}) from m~-0.10 found previously for FGK dwarfs. This flat slope agrees with pebble accretion models, which include photoevaporation and inward orbital migration. The radius gap as a function of insolation is approximately constant over the range of Sp~20-250S_{Earth}_. The Rp-Porb plane exhibits a sub-Neptune desert for Porb&lt;2-days, which appears at Sp&gt;120S_{Earth}_, being significantly smaller than Sp&gt;650S_{Earth}_ found in the FGK planet-hosts, indicating that the appearance of the sub-Neptune desert is a function of host- star mass. Published masses for 51 exoplanets are combined with our radii to determine densities, which exhibit a gap at {rho}_p_~0.9{rho}_{Earth}_, separating rocky exoplanets from sub-Neptunes. The density distribution within the sub-Neptune family itself reveals two peaks, at {rho}_p_~0.4{rho}_{Earth}_ and ~0.7{rho}_{Earth}_. Comparisons to planetary models find that the low-density group are gas-rich sub-Neptunes, while the group at &lt;{rho}_p_&gt;~0.7{rho}_{Earth}_ likely consists of volatile-rich water worlds.</eudc:description></eudc:descriptions><eudc:keywords><eudc:keyword>multiple-stars</eudc:keyword><eudc:keyword>m-stars</eudc:keyword><eudc:keyword>exoplanets</eudc:keyword><eudc:keyword>orbits</eudc:keyword><eudc:keyword>stellar-radii</eudc:keyword><eudc:keyword>stellar-masses</eudc:keyword><eudc:keyword>astrophysical-processes</eudc:keyword><eudc:keyword>exoplanet-astronomy</eudc:keyword><eudc:keyword>stellar-astronomy</eudc:keyword></eudc:keywords><eudc:identifiers><eudc:identifier identifierType="URL">https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/ApJ/993/233</eudc:identifier></eudc:identifiers><eudc:relatedIdentifiers><eudc:relatedIdentifier relatedIdentifierType="URL">https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/993/233</eudc:relatedIdentifier><eudc:relatedIdentifier relatedIdentifierType="bibcode">2025ApJ...993..233W</eudc:relatedIdentifier><eudc:relatedIdentifier relatedIdentifierType="URL">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/993/233</eudc:relatedIdentifier><eudc:description>Cone search capability for table J/ApJ/993/233/table1 (Stellar and Planetary Data)</eudc:description></eudc:relatedIdentifiers><eudc:creators><eudc:creator><eudc:creatorName>Wanderley F.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Cunha K.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Smith V.V.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Souto D.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Pascucci I.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Behmard A.,Allende Prieto C.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Beaton R.L.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Bizyaev D.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Daflon S.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Hasselquist S.,Howell S.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Majewski S.R.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Pinsonneault M.</eudc:creatorName></eudc:creator></eudc:creators><eudc:publishers><eudc:publisher>CDS</eudc:publisher></eudc:publishers><eudc:instruments/><eudc:publicationYear>2026</eudc:publicationYear><eudc:rightsList><eudc:rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</eudc:rights></eudc:rightsList><eudc:fundingReferences/><eudc:contacts><eudc:contact>CDS support team &lt;cds-question@unistra.fr&gt;</eudc:contact></eudc:contacts><eudc:resourceTypes><eudc:resourceType>Dataset</eudc:resourceType><eudc:resourceType>AstroObjects</eudc:resourceType></eudc:resourceTypes><eudc:disciplines><eudc:discipline>astronomy</eudc:discipline></eudc:disciplines></eudc:resource></oai:metadata></oai:record></oai:GetRecord></oai:OAI-PMH>