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<ri:Resource created="2021-09-09T07:00:05Z" 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>Sample of 45 H{alpha}EW outliers</title><shortName>J/AJ/161/277</shortName><identifier>ivo://CDS.VizieR/J/AJ/161/277</identifier><altIdentifier>doi:10.26093/cds/vizier.51610277</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kiman R.</name></creator><creator><name>Faherty J.K.</name></creator><creator><name>Cruz K.L.</name></creator><creator><name>Gagne J.</name></creator><creator><name>Angus R.</name></creator><creator><name>Schmidt S.J.,Mann A.W.</name></creator><creator><name>Bardalez Gagliuffi D.C.</name></creator><creator><name>Rice E.</name></creator><date role="Updated">2021-12-07T21:30:14Z</date><date role="Created">2021-09-09T07:00:05Z</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>m-stars</subject><subject>dwarf-stars</subject><subject>visible-astronomy</subject><subject>h-alpha-photometry</subject><subject>stellar-spectral-types</subject><description>In this work, we calibrate the relationship between H{alpha} emission and M-dwarf ages. We compile a sample of 892 M-dwarfs with H{alpha} equivalent width (H{alpha}EW) measurements from the literature that are either comoving with a white dwarf of known age (21 stars) or in a known young association (871 stars). In this sample we identify 7 M-dwarfs that are new candidate members of known associations. By dividing the stars into active and inactive categories according to their H{alpha}EW and spectral type (SpT), we find that the fraction of active dwarfs decreases with increasing age, and the form of the decline depends on SpT. Using the compiled sample of age calibrators, we find that H{alpha} EW and fractional H{alpha} luminosity (L_H{alpha}_/L_bol_) decrease with increasing age. H{alpha}EW for SpT&lt;~M7 decreases gradually up until ~1Gyr. For older ages, we found only two early M dwarfs that are both inactive and seem to continue the gradual decrease. We also found 14 mid-type M-dwarfs, out of which 11 are inactive and present a significant decrease in H{alpha}EW, suggesting that the magnetic activity decreases rapidly after ~1Gyr. We fit L_H{alpha}_/L_bol_ versus age with a broken power law and find an index of -0.11_-0.01_^+0.02^ for ages &lt;~776Myr. The index becomes much steeper at older ages, but a lack of field age-calibrators (&gt;&gt;1Gyr) leaves this part of the relation far less constrained. Finally, from repeated independent measurements for the same stars, we find that 94% of them have a level of H{alpha}EW variability &lt;~5{AA} at young ages (&lt;1Gyr).</description><source format="bibcode">2021AJ....161..277K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/161/277</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/MNRAS/447/1126">J/MNRAS/447/1126 : Halpha measurements in Abell 2465 (Wegner+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/466/163">J/MNRAS/466/163 : Candidate Halpha sources in GBS (Wevers+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/624/A10">J/A+A/624/A10 : Normalized Halpha line profiles of FGK stars (Giribaldi+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/630/A90">J/A+A/630/A90 : Halpha emission-line stars in Canis Major (Pettersson+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/253/19">J/ApJS/253/19 : Halpha and other EWs of LAMOST M-type stars (Zhang+, 2021)</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/161/277</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/161/277</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/161/277</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/161/277</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/161/277</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/161/277</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/AJ/161/277/table3 (*H{alpha}EW outliers)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/161/277/table3?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/161/277/table3?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/161/277/table3?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>165.4662725</ra><dec>-34.7047311</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/1052 1074 5282 9949 22884-22885 23509 23717 24629 24763 26416 28132 33737 34885 37013 38191 38347 38359 38382 39792 41130 41472 42959 42981 42985-42986 42988 43002 43670 44317 44358 44363 44366-44367 44378-44379 44389 44401 46087</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/AJ/161/277?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/AJ/161/277/table3</name><description>*H{alpha}EW outliers</description><column><name>2MASS</name><description>2MASS identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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