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<ri:Resource created="2026-07-28T11:23:09Z" status="active" updated="2026-07-28T10:27:13Z" 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>MgII line profiles &amp; refined param. of FGKM stars</title><shortName>J/ApJ/964/80</shortName><identifier>ivo://CDS.VizieR/J/ApJ/964/80</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Taylor A.</name></creator><creator><name>Dunn A.</name></creator><creator><name>Peacock S.</name></creator><creator><name>Youngblood A.</name></creator><creator><name>Redfield S.</name></creator><date role="Updated">2026-07-28T10:27:13Z</date><date role="Created">2026-07-28T11:23:09Z</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>spectroscopy</subject><subject>ultraviolet-astronomy</subject><subject>metallicity</subject><subject>stellar-ages</subject><subject>stellar-masses</subject><subject>stellar-radii</subject><subject>astronomical-reference-materials</subject><description>The MgII h&amp;k emission lines (2803, 2796{AA}) are a useful tool for understanding stellar chromospheres and transition regions due to their intrinsic brightness, relatively low interstellar medium (ISM) absorption interference, and abundance of archival spectra available. Similar to other optically thick chromospheric emission lines such as HI Ly{alpha}, MgII emissions commonly present with a self-reversed line core, the depth and shape of which vary from star to star. We explore the relationship between self-reversal and the stellar atmosphere by investigating the extent to which fundamental stellar parameters affect self-reversal. We present a search for correlations between photospheric parameters such as effective temperature, surface gravity, and metallicity with the MgII k self-reversal depth for a group of 135 FGKM main-sequence stars with high-resolution near-ultraviolet spectra from the Hubble Space Telescope. We modeled the observed MgII k line profiles to correct for ISM attenuation and recover the depth of the emission line's self-reversal in relation to the intensity of the line. We used the PHOENIX atmosphere code to homogeneously determine the stellar parameters by computing a suite of stellar atmosphere models that include a chromosphere and transition region, and using archival photometry to guide the models of each star. We quantify the sensitivity of the visible and near-infrared photometry to chromospheric and photospheric parameters. We find weak trends between MgII k self-reversal depth and age, rotation period, MgII luminosity, temperature, and mass. All stars in our sample older than ~2Gyr or rotating slower than ~10days exhibit self-reversal.</description><source format="bibcode">2024ApJ...964...80T</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/964/80</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/B/hst">B/hst : HST Archived Exposures Catalog (STScI, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/B/gcvs">B/gcvs : General Catalogue of Variable Stars (Samus+, 2007-2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/135">III/135 : Henry Draper Catalogue and Extension (Cannon+ 1918-1924; ADC 1989)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/101">V/101 : Nearest stars until 10pc (Zakhozhaj, 1979-1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/200">III/200 : Catalogue of [Fe/H] (Cayrel de Strobel+, 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/224">II/224 : Catalogue of Stellar Diameters (CADARS) (Pasinetti-Fracassini+ 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/117">V/117 : Geneva-Copenhagen Survey of Solar neighbourhood (Holmberg+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/130">V/130 : Geneva-Copenhagen Survey of Solar neighbourhood III (Holmberg+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/355">I/355 : Gaia DR3 Part 1. 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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>RP</name><description>Refined parameters in Table 3</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Name</name><description>Star name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType><flag>primary</flag></column><column><name>Tmin</name><description>[2665/6825]? Minimum effective temperature</description><unit>K</unit><ucd>phys.temperature.effective;stat.min</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType><flag>nullable</flag></column><column><name>r_Tmin</name><description>Reference bibcode for Tmin (see refs.dat file)</description><ucd>meta.ref;phys.temperature.effective;stat.min</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>Tmax</name><description>[2810/7229]? Maximum effective temperature</description><unit>K</unit><ucd>phys.temperature.effective;stat.max</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>r_Tmax</name><description>Reference bibcode for Tmax (see refs.dat file)</description><ucd>meta.ref;phys.temperature.effective;stat.max</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>log(g)min</name><description>[2.3/5.17]? Minimum log surface gravity</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_log(g)min</name><description>Reference bibcode for log(g)min (see refs.dat file)</description><ucd>meta.ref;phys.gravity;stat.min</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>log(g)max</name><description>[3.22/5.5]? Maximum log surface gravity</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_log(g)max</name><description>Reference bibcode for log(g)max (see refs.dat file)</description><ucd>meta.ref;phys.gravity;stat.max</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>[Fe/H]min</name><description>[-3.06/0.24]? Minimum metallicity</description><unit>log(Sun)</unit><ucd>phys.abund.Fe;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_[Fe/H]min</name><description>Reference bibcode for [Fe/H]min (see refs.dat file)</description><ucd>meta.ref;phys.abund.Fe;stat.min</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>[Fe/H]max</name><description>[-1.25/1.05]? Maximum metallicity</description><unit>log(Sun)</unit><ucd>phys.abund.Fe;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_[Fe/H]max</name><description>Reference bibcode for [Fe/H]max (see refs.dat file)</description><ucd>meta.ref;phys.abund.Fe;stat.max</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>Age</name><description>[0.01/12.0]? Stellar age</description><unit>Gyr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_Age</name><description>[28/287]? Reference bibcode for Age (see refs.dat file)</description><ucd>meta.ref;time.age</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Mass</name><description>[0.08/1.9]? Stellar mass</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_Mass</name><description>[0.003/0.25]? Upper uncertainty in Mass</description><unit>solMass</unit><ucd>stat.error;stat.max;phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Mass</name><description>[0.003/0.25]? Lower uncertainty in Mass</description><unit>solMass</unit><ucd>stat.error;stat.min;phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_Mass</name><description>[10/289]? Reference bibcode for Mass (see refs.dat file)</description><ucd>meta.ref;phys.mass</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Rad</name><description>[0.11/7.87]? Stellar radius</description><unit>solRad</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_Rad</name><description>[0.0036/0.1]? Upper uncertainty in Rad</description><unit>solRad</unit><ucd>stat.error;stat.max;phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Rad</name><description>[0.0036/0.1]? Lower uncertainty in Rad</description><unit>solRad</unit><ucd>stat.error;stat.min;phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_Rad</name><description>[21/288]? Reference bibcode for Rad (see refs.dat file)</description><ucd>meta.ref;phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Dist</name><description>[1.35/81.66]? 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Reference bibcode for Per (see refs.dat file)</description><ucd>meta.ref;time.period</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>_RA</name><description>Right Ascension (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Declination (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table><table><name>J/ApJ/964/80/table3</name><description>Refined stellar parameters</description><column><name>Name</name><description>Star name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>[Fe/H]</name><description>[-2.1/0.4] Metallicity</description><unit>log(Sun)</unit><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>b_[Fe/H]</name><description>[-2.1/0.4] Upper boundary value in [Fe/H]</description><unit>log(Sun)</unit><ucd>phys.abund.Fe;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>B_[Fe/H]</name><description>[-1.5/0.6] Lower boundary value in [Fe/H]</description><unit>log(Sun)</unit><ucd>phys.abund.Fe;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</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><column><name>Teff</name><description>[2732/7150] Effective temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>b_Teff</name><description>[2700/7100] Upper boundary value in Teff</description><unit>K</unit><ucd>phys.temperature.effective;stat.min</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>B_Teff</name><description>[2830/7200] Lower boundary value in Teff</description><unit>K</unit><ucd>phys.temperature.effective;stat.max</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>log(g)</name><description>[3.3/5.4] Log surface gravity</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>b_log(g)</name><description>[3.2/5.2] Upper boundary value in log(g)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>B_log(g)</name><description>[3.5/5.5] Lower boundary value in log(g)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Age</name><description>[0.01/9] Stellar age</description><unit>Gyr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>b_Age</name><description>[0.01/8.1] Upper boundary value in Age</description><unit>Gyr</unit><ucd>time.age;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>B_Age</name><description>[0.05/10] Lower boundary value in Age</description><unit>Gyr</unit><ucd>time.age;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Mass</name><description>[0.03/2.4] Stellar mass</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>b_Mass</name><description>[0.01/1.4] Upper boundary value in Mass</description><unit>solMass</unit><ucd>phys.mass;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>B_Mass</name><description>[0.09/4.2] Lower boundary value in Mass</description><unit>solMass</unit><ucd>phys.mass;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Rad</name><description>[0.08/5] Stellar radius</description><unit>solRad</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>b_Rad</name><description>[0.08/4] Upper boundary value in Rad</description><unit>solRad</unit><ucd>phys.size.radius;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>B_Rad</name><description>[0.09/6] Lower boundary value in Rad</description><unit>solRad</unit><ucd>phys.size.radius;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SRPar</name><description>[0/3.43] Self-Reversal parameter</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_SRPar</name><description>[0/2.5] Uncertainty in SRPar</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SRVel</name><description>[-3.42/5] Self-Reversal velocity</description><unit>km/s</unit><ucd>phys.veloc;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_SRVel</name><description>[0.03/41]? 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