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<ri:Resource created="2024-11-15T12:00:01Z" 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>Solar-type stars Halpha line</title><shortName>J/MNRAS/532/563</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/532/563</identifier><altIdentifier>doi:10.26093/cds/vizier.75320563</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Souza dos Santos P.V.</name></creator><creator><name>Porto de Mello G.F.</name></creator><creator><name>Costa-Bhering E.,Lorenzo-Oliveira D.</name></creator><creator><name>Almeida-Fernandes F.</name></creator><creator><name>Dutra-Ferreira L.</name></creator><creator><name>Ribas I.</name></creator><date role="Updated">2025-02-13T20:15:41Z</date><date role="Created">2024-11-15T12:00:01Z</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>f-stars</subject><subject>stellar-ages</subject><subject>spectroscopy</subject><subject>visible-astronomy</subject><subject>h-alpha-photometry</subject><description>Excess chromospheric emissions within deep photospheric lines are effective proxies of stellar magnetism for FGK stars. This emission decays with stellar age and is a potential determinant of this important stellar quantity. We report absolutely calibrated H{alpha} chromospheric fluxes for 511 solar-type stars in a wide interval of precisely determined masses, [Fe/H], ages, and evolution states from high S/N, moderately high-resolution spectra. The comparison of H{alpha} and H+K chromospheric fluxes reveals a metallicity bias (absent from H{alpha}) affecting Ca II H+K fluxes thereby metal-rich stars with deep line profiles mimic low chromospheric flux levels, and vice versa for metal-poor stars. This bias blurs the age-activity relation, precluding age determinations for old, inactive stars unless mass and [Fe/H] are calibrated into the relation. The H+K lines being the most widely studied tool to quantify magnetic activity in FGK stars, care should be exercised in its use whenever wide ranges of mass and [Fe/H] are involved. The H{alpha} age-activity-mass-metallicity calibration appears to be in line with the theoretical expectation that (other parameters being equal) more massive stars possess narrower convective zones and are less active than less massive stars, while more metal-rich stars have deeper convective zones and appear more active than metal-poorer stars. If regarded statistically in tandem with other age diagnostics, H{alpha} chromospheric fluxes may be suitable to constrain ages for FGK stars with acceptable precision.</description><source format="bibcode">2024MNRAS.532..563S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/532/563</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/839/94">J/ApJ/839/94 : Abundances of solar twins from Keck/HIRES (Bedell+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/619/A73">J/A+A/619/A73 : Solar twins age-chromospheric activity</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/529/2946">J/MNRAS/529/2946 : Abundance catalogue of solar twins in GALAH (Walsen+, 2024)</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/MNRAS/532/563</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/532/563</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/532/563</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/532/563</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/532/563</mirrorURL><mirrorURL 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arraysize="9*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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Surface gravity compiled from the literature</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_Tefflit</name><description>Reference of the atmospheric parameters compiled, in refs.dat file</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>Teff</name><description>Effective temperature adopted in this work</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_Teff</name><description>? 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>BibCode</name><description>BibCode</description><ucd>meta.bib.bibcode</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>Aut</name><description>Author's name</description><ucd>meta.bib.author</ucd><dataType xsi:type="vs:VOTableType" arraysize="22*">char</dataType></column><column><name>Com</name><description>Comments</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="130*">char</dataType></column><column><name>Ref</name><description>Reference code</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column></table><table><name>J/MNRAS/532/563/table4</name><description>Bolometric correction and magnitude, luminosity, radius, mass and age for the stars</description><column><name>Name</name><description>Star name (including Sun)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>BC</name><description>Bolometric correction</description><unit>mag</unit><ucd>phot.mag.bc</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>Mbol</name><description>Bolometric magnitude</description><unit>mag</unit><ucd>phys.magAbs.bol</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Mbol</name><description>Bolometric magnitude error</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Lum</name><description>Luminosity</description><unit>solLum</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Lum</name><description>Luminosity error</description><unit>solLum</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Rad</name><description>Radius</description><unit>solRad</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Rad</name><description>Radius error</description><unit>solRad</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Mass</name><description>Mass</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Mass</name><description>Mass error</description><unit>solMass</unit><ucd>stat.error;phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Age</name><description>? Age</description><unit>Gyr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Age</name><description>? Age error (inferior)</description><unit>Gyr</unit><ucd>stat.error;time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_Age</name><description>? Age error (superior)</description><unit>Gyr</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Note</name><description>[*A] Note (1)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table><table><name>J/MNRAS/532/563/table5</name><description>Final total and purely chromospheric fluxes for the stars</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>Star name (including Sun)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>Ftotal</name><description>H{alpha} total absolute flux (M.erg/cm^2^/s)</description><unit>1000W.m**-2</unit><ucd>phot.flux;em.line.Halpha</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Fchrom</name><description>H{alpha} chromospheric absolute flux</description><unit>1000W.m**-2</unit><ucd>phot.flux;em.line.Halpha</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Fchrom</name><description>H{alpha} chromospheric absolute flux error</description><unit>1000W.m**-2</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/MNRAS/532/563/table10</name><description>Chromospheric ages for the stars</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>Star name (including Sun)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>AgeHa</name><description>H{alpha} chromospheric age</description><unit>Gyr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_AgeHa</name><description>H{alpha} chromospheric age upper error</description><unit>Gyr</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_AgeHa</name><description>H{alpha} chromospheric age lower error</description><unit>Gyr</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>AgeHK</name><description>HK chromospheric age</description><unit>Gyr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_AgeHK</name><description>H{alpha} chromospheric age upper error</description><unit>Gyr</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_AgeHK</name><description>H{alpha} chromospheric age lower error</description><unit>Gyr</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>