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<ri:Resource created="2019-04-08T13:33:22Z" status="active" updated="2025-06-13T15:25:00Z" 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>Stellar properties for M dwarfs in MEarth-South</title><shortName>J/AJ/156/217</shortName><identifier>ivo://CDS.VizieR/J/AJ/156/217</identifier><altIdentifier>doi:10.26093/cds/vizier.51560217</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Newton E.R.</name></creator><creator><name>Mondrik N.</name></creator><creator><name>Irwin J.</name></creator><creator><name>Winters J.G.</name></creator><creator><name>Charbonneau D.</name></creator><date role="Updated">2019-12-16T06:47:20Z</date><date role="Created">2019-04-08T13:33:22Z</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>dwarf-stars</subject><subject>m-stars</subject><subject>proper-motions</subject><subject>visible-astronomy</subject><subject>trigonometric-parallax</subject><subject>stellar-distance</subject><subject>radial-velocity</subject><subject>stellar-radii</subject><subject>stellar-masses</subject><description>Stellar rotation periods are valuable both for constraining models of angular momentum loss and for understanding how magnetic features impact inferences of exoplanet parameters. Building on our previous work in the northern hemisphere, we have used long-term, ground-based photometric monitoring from the MEarth Observatory to measure 234 rotation periods for nearby, southern hemisphere M dwarfs. Notable examples include the exoplanet hosts GJ 1132, LHS 1140, and Proxima Centauri. We find excellent agreement between our data and K2 photometry for the overlapping subset. Among the sample of stars with the highest quality data sets, we recover periods in 66%; as the length of the data set increases, our recovery rate approaches 100%. The longest rotation periods we detect are around 140 days, which we suggest represent the periods that are reached when M dwarfs are as old as the local thick disk (about 9 Gyr).</description><source format="bibcode">2018AJ....156..217N</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/156/217</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/812/3">J/ApJ/812/3 : MEarth mid-to-late M dwarfs rotation + kinematics (West+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/818/153">J/ApJ/818/153 : MEarth photometry: nearby M-dwarf magnitudes (Dittmann+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/156/140">J/AJ/156/140 : Four new eclipsing mid M-dwarf systems from MEarth</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/AJ/156/217</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/156/217</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/156/217</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/156/217</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/156/217</mirrorURL><mirrorURL title="VizieR 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Parallax</description><unit>arcsec</unit><ucd>pos.parallax.trig</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_plx</name><description>[0.0003/0.03]? Uncertainty in plx</description><unit>arcsec</unit><ucd>stat.error;pos.parallax</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>RV</name><description>[-141.9/77.6]? Radial velocity</description><unit>km/s</unit><ucd>phys.veloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_RV</name><description>[0.1/40]? Uncertainty in RV</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_RV</name><description>ADS bibliography code reference for RV</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>Per</name><description>[0.129/225.16]? Photometric rotation period</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Amp</name><description>[0.0009/0.5567]? Semi-amplitude of variability</description><unit>mag</unit><ucd>src.var.amplitude</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Amp</name><description>[0/1.6207]? 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