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<ri:Resource created="2026-08-13T05:59:21Z" status="active" updated="2026-08-13T05:11:09Z" 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>Confirmed K2 exoplanet host stars opt. sp.</title><shortName>J/ApJS/281/61</shortName><identifier>ivo://CDS.VizieR/J/ApJS/281/61</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Loaiza-Tacuri V.</name></creator><creator><name>Souto D.</name></creator><creator><name>Quispe-Huaynasi F.</name></creator><creator><name>Cunha K.</name></creator><creator><name>Daflon S.,Costa-Almeida E.</name></creator><creator><name>Smith V.V.</name></creator><creator><name>Ghezzi L.</name></creator><date role="Updated">2026-08-13T05:11:09Z</date><date role="Created">2026-08-13T05:59:21Z</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>multiple-stars</subject><subject>exoplanets</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>chemical-abundances</subject><subject>stellar-masses</subject><subject>stellar-radii</subject><description>We present a homogeneous spectroscopic analysis of confirmed Kepler's extended mission (K2) exoplanet-hosting stars, comprising 301 targets with high-resolution optical spectra from HIRES and TRES taken from ExoFOP. We derived effective temperatures, surface gravities, and iron and magnesium abundances in local thermodynamic equilibrium by measuring the equivalent widths of Fe I, Fe II, and Mg I lines. Three estimates of stellar masses and radii were obtained via the Stefan-Boltzmann and isochrone methods using the codes PARAM and isochrones. These were used to derive exoplanetary radii reaching internal precisions of 2.5%, 2.6%, and 6.6%, respectively, and the radius gap was consistently detected near 1.9R_{Earth}_. We measured chromospheric activity from the CaII H and K and H{alpha} lines. Within the low-activity range (logR'_HK_{&lt;}-4.75), stellar activity appears to decrease with increasing planetary radius from super-Earths, sub-Neptunes, sub-Saturns, into the Jupiter regime. According to the [Mg/Fe] measurements, most of our K2 planet hosts belong to the Galactic thin disk, but our sample has a population from the thick disk (high-alpha sequence). Most stars show consistent chemodynamical behavior. We find that the [Mg/Fe] ratios are indistinguishable between systems containing large or small exoplanets, as well as single- or multi-exoplanetary systems. Both the [Fe/H] and [Mg/H] distributions reveal that stars hosting large planets are more iron and magnesium enhanced than those having only small planets, further confirming the link between stellar abundances and exoplanetary size, but no significant differences are found between the single-versus multi-exoplanetary systems.</description><source format="bibcode">2025ApJS..281...61L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/281/61</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/III/159">III/159 : Ca II H and K Measurements Made at MWO (Duncan+ 1991)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/335">II/335 : Catalog of GALEX UV sources (GUVcat_AIS GR6+7) (Bianchi+ 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IV/34">IV/34 : K2 Ecliptic Plane Input Catalog (EPIC) (Huber+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/350">I/350 : Gaia EDR3 (Gaia Collaboration, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/352">I/352 : Distances to 1.47 billion stars in Gaia EDR3 (Bailer-Jones+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/286">III/286 : APOGEE-2 DR17 final allStar catalog (Abdurro'uf+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/233">VII/233 : 2MASS All-Sky Extended Source Catalog (XSC) (IPAC/UMass, 2003-2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/111/439">J/AJ/111/439 : Chromospheric emission in late-type stars. 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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>EPIC</name><description>[201110617/251319382] EPIC identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">long</dataType></column><column><name>Host</name><description>Host name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>RAJ2000</name><description>[8.7/356.3] Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>[-28.8/27.3] Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Bmag</name><description>[8.77/18.43] Apparent B band magnitude (1)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Vmag</name><description>[8.24/17.24] Apparent V band magnitude (1)</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>Camp</name><description>K2 observing campaign number(s)</description><ucd>meta.id;obs</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>Inst</name><description>Spectrograph identifier (HIRES or TRES)</description><ucd>meta.id;instr</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>Nsp</name><description>[1/260] Number of spectra</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Np</name><description>Number of planets for this star (link to Table 5)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>All</name><description>Display all data in this catalog for this star (Tables 1, 3 and 4)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table><table><name>J/ApJS/281/61/table2</name><description>Line list</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>lambda</name><description>[4571/6862] Wavelength; Angstroms</description><unit>0.1nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ion</name><description>[12/26.1] Species identifier (1)</description><ucd>phys.atmol.ionStage</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>ExPot</name><description>[0/5.11] Excitation potential</description><unit>eV</unit><ucd>phys.atmol.excitation</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>log(gf)</name><description>[-5.63/-0.22] log oscillator strength</description><ucd>phys.atmol.oscStrength</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/ApJS/281/61/table3</name><description>Stellar parameters</description><column><name>Teff</name><description>[4474/6539]? Effective temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>All</name><description>Display all data in this catalog for this star (Tables 1, 3 and 4)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</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><flag>nullable</flag></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><flag>nullable</flag></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>ID</name><description>Identifier (Host name or EPIC)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>SHK</name><description>[0.097/3.8]? Mount Wilson CaII H &amp; K S-index</description><ucd>spect.index</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_SHK</name><description>[0.001/0.3]? Uncertainty in SHK</description><ucd>stat.error;spect.index</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logRHK</name><description>[-6.25/-3.89]? log R'_HK_ activity index</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_logRHK</name><description>[0.006/0.3]? Uncertainty in logR'HK</description><ucd>stat.error;phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Ha</name><description>[0.026/0.17]? The H{alpha} index</description><ucd>spect.index;em.line.Halpha</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Ha</name><description>[0/0.003]? Uncertainty in Ha</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logIHa</name><description>[-1.62/-0.77]? The log I_H{alpha}_ index</description><ucd>spect.index;em.line.Halpha</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_logIHa</name><description>[0/0.03]? Uncertainty in logIHa</description><ucd>stat.error;spect.index;em.line.Halpha</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Teff</name><description>[4/190]? Uncertainty in Teff</description><unit>K</unit><ucd>stat.error;phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>log(g)</name><description>[2.54/4.94]? log surface gravity</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_log(g)</name><description>[0.01/0.6]? Uncertainty in log(g)</description><unit>log(cm.s**-2)</unit><ucd>stat.error;phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>A(Fe)</name><description>[6.5/8.11]? log final iron abundance</description><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_A(Fe)</name><description>[0.004/0.2]? Uncertainty in A(Fe)</description><ucd>stat.error;phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>VTurb</name><description>[0.15/16.5]? Microtrubulent velocity</description><unit>km/s</unit><ucd>phys.veloc.microTurb</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_VTurb</name><description>[0.02/35]? Uncertainty in VTurb</description><unit>km/s</unit><ucd>stat.error;phys.veloc.microTurb</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>A(Mg)</name><description>[6.57/8.3]? log final magnesium abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_A(Mg)</name><description>[0/0.14]? Uncertainty in A(Mg)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/ApJS/281/61/table4</name><description>Stellar masses and radii</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>ID</name><description>Identifier (Host name or EPIC)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>RsSB</name><description>[0.5/8.4] Stefan-Boltzmann law derived stellar radius</description><unit>solRad</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_RsSB</name><description>[0.005/1.7] Uncertainty in RsSB</description><unit>solRad</unit><ucd>stat.error;phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RsPARAM</name><description>[0.39/3.7]? PARAM code derived 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_RsPARAM</name><description>[0/0.3]? Uncertainty in RsPARAM</description><unit>solRad</unit><ucd>stat.error;phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>MsPARAM</name><description>[0.45/1.5]? PARAM code derived stellar mass</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_MsPARAM</name><description>[0/0.06]? Uncertainty in MsPARAM</description><unit>solMass</unit><ucd>stat.error;phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</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="13*">char</dataType><flag>nullable</flag></column><column><name>Rsiso</name><description>[0.53/10.5] Isochrones code derived stellar radius</description><unit>solRad</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_Rsiso</name><description>[0.007/3.5] Upper uncertainty in Rsiso</description><unit>solRad</unit><ucd>stat.error;stat.max;phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Rsiso</name><description>[0.007/4.7] Lower uncertainty in Rsiso</description><unit>solRad</unit><ucd>stat.error;stat.min;phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Msiso</name><description>[0.56/3.1] Isochrones code derived stellar mass</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_Msiso</name><description>[0.004/0.7] Upper uncertainty in Msiso</description><unit>solMass</unit><ucd>stat.error;stat.max;phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Msiso</name><description>[0.006/0.9] Lower uncertainty in Msiso</description><unit>solMass</unit><ucd>stat.error;stat.min;phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>All</name><description>Display all data in this catalog for this star (Tables 1, 3 and 4)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></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/ApJS/281/61/table5</name><description>Planetary radii</description><column><name>Planet</name><description>Planet identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></column><column><name>e_RpPARAM</name><description>[0.001/2.4]? Uncertainty in PARAM-Rp</description><unit>(6.3781x10+6m)</unit><ucd>stat.error;phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">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><column><name>DeltaF</name><description>[73/28460] Transit depth in parts per million</description><unit>(10-6)</unit><ucd>phot.flux.density;arith.diff</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RpSB</name><description>[0.7/79] Stefan-Boltzmann law derived planetary radius</description><unit>(6.3781x10+6m)</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_RpSB</name><description>[0.009/16]? Uncertainty in SB-Rp</description><unit>(6.3781x10+6m)</unit><ucd>stat.error;phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>RpPARAM</name><description>[0.7/23]? PARAM code derived planetary radius</description><unit>(6.3781x10+6m)</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Rpiso</name><description>[0.7/99]? Isochrones code derived planetary radius</description><unit>(6.3781x10+6m)</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_Rpiso</name><description>[0.015/33]? Upper uncertainty in iso-Rp</description><unit>(6.3781x10+6m)</unit><ucd>stat.error;stat.max;phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Rpiso</name><description>[0.014/44]? Lower uncertainty in iso-Rp</description><unit>(6.3781x10+6m)</unit><ucd>stat.error;stat.min;phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</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></schema></tableset></ri:Resource>