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<ri:Resource created="2023-10-27T07:18:03Z" 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>Properties of 363 M-dwarfs from TESS</title><shortName>J/AJ/165/265</shortName><identifier>ivo://CDS.VizieR/J/AJ/165/265</identifier><altIdentifier>doi:10.26093/cds/vizier.51650265</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ment K.</name></creator><creator><name>Charbonneau D.</name></creator><date role="Updated">2023-12-20T08:15:28Z</date><date role="Created">2023-10-27T07:18:03Z</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>m-stars</subject><subject>visible-astronomy</subject><subject>stellar-masses</subject><subject>stellar-radii</subject><description>We present an analysis of a volume-complete sample of 363 mid-to-late M-dwarfs within 15pc of the Sun with masses between 0.1 and 0.3M{sun} observed by TESS within sectors 1-42. The median stellar mass of the sample is 0.17M{sun}. We search the TESS light curves for transiting planets with orbital periods below 7 days and recover all six known planets within the sample, as well as a likely planet candidate orbiting LHS-475. Each of these planets is consistent with a terrestrial composition, with planet radii between 0.91 and 1.31R{Earth}. We characterize the transit detection sensitivity for each star as a function of planet radius, insolation, and orbital period. We obtain a cumulative occurrence rate of 0.61_-0.19_^+0.24^ terrestrial planets per star with radii above 0.5R{Earth} and orbital periods between 0.4 and 7days. We find that for comparable insolations, planets larger than 1.5R{Earth} (sub-Neptunes) are significantly less abundant around mid-to-late M dwarfs compared to earlier-type stars, while the occurrence rate of terrestrial planets is comparable to that of more massive M-dwarfs. We estimate that overall, terrestrials outnumber sub-Neptunes around mid-to-late M-dwarfs by 14 to 1, in contrast to GK dwarfs, where they are roughly equinumerous. We place a 1{sigma} upper limit of 0.07 planets larger than 1.5R{Earth} per star within the orbital period range of 0.5-7days. We find evidence for a downturn in occurrence rates for planet radii below 0.9R{Earth}, suggesting that Earth-sized and larger terrestrials may be more common around mid-to-late M-dwarfs.</description><source format="bibcode">2023AJ....165..265M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/165/265</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/ApJ/757/112">J/ApJ/757/112 : Stellar diameters. II. K and M-stars (Boyajian+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/549/A109">J/A+A/549/A109 : HARPS XXXI. 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