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<ri:Resource created="2026-07-08T12:19:57Z" status="active" updated="2026-10-10T20:30:32Z" 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>APOGEE: M dwarfs metallicity &amp; planet parameters</title><shortName>J/AJ/170/177</shortName><identifier>ivo://CDS.VizieR/J/AJ/170/177</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Wanderley F.</name></creator><creator><name>Cunha K.</name></creator><creator><name>Souto D.</name></creator><creator><name>Smith V.V.</name></creator><creator><name>Daflon S.</name></creator><date role="Updated">2026-10-10T20:30:32Z</date><date role="Created">2026-07-08T12:19:57Z</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>exoplanets</subject><subject>dwarf-stars</subject><subject>m-stars</subject><subject>stellar-radii</subject><subject>infrared-astronomy</subject><subject>spectroscopy</subject><subject>photometry</subject><subject>visible-astronomy</subject><subject>chemical-abundances</subject><description>One important property in studying the exoplanet population is the host star metallicity ([M/H]). In this study, we derived stellar metallicities and oxygen abundances for 48 M dwarf stars using the near-infrared high-resolution spectra from the SDSS APOGEE survey and synthetic spectra computed in LTE. We also investigated the exoplanetary radii distribution for a larger sample of 246 exoplanets orbiting 188 M dwarf stars. The [M/H] versus [O/M] distribution obtained indicates that our sample is composed mainly of thin disk stars, which follow the behavior of the low-alpha sequence in the Milky Way thin disk. Small planets with radii smaller than 3R_{Earth}_ were found around stars with a range of metallicities (-0.6&lt;[M/H]&lt;+0.3), while larger planets of the sample orbit only stars with [M/H]&gt;=0.0. These results indicate that while small planets can form in different environments, larger planets preferentially form in metal-rich protoplanetary disks. Exoplanets with P_orb_&lt;4.3days orbit on average more metal-rich stars than planets with longer periods. This threshold is smaller than that found for FGK stars (8-10days) and might be related to M dwarfs having a smaller dust sublimation radius. The distribution of exoplanets with R_p_&gt;4R_{Earth}_ shows a concentration at orbital periods between 2 and 5days, which may result from inward orbital migration. There is also a different behavior between single-detected exoplanets and planets from multiplanetary systems, with the latter being found on average around more metal-poor stars, and with planetary radii roughly up to 3R_{Earth}_.</description><source format="bibcode">2025AJ....170..177W</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/170/177</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/IV/34">IV/34 : K2 Ecliptic Plane Input Catalog (EPIC) (Huber+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/352">I/352 : Distances to 1.47 billion stars in Gaia EDR3 (Bailer-Jones+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/306">II/306 : The SDSS Photometric Catalog, Release 8 (Adelman-McCarthy+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/284">III/284 : APOGEE-2 data from DR16 (Johnsson+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/133">V/133 : Kepler Input Catalog (Kepler Mission Team, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/349/757">J/MNRAS/349/757 : Masses, ages &amp; metallicities of F-G dwarfs (Lambert+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/622/1102">J/ApJ/622/1102 : The planet-metallicity correlation. 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