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<ri:Resource created="2011-12-14T16:55:14Z" status="active" updated="2026-03-17T20:05:12Z" 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 parameters and abundances of 99 giants</title><shortName>J/PASJ/63/1035</shortName><identifier>ivo://CDS.VizieR/J/PASJ/63/1035</identifier><altIdentifier>doi:10.26093/cds/vizier/bj-1z-10b</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Wang L.</name></creator><creator><name>Liu Y.</name></creator><creator><name>Zhao G.</name></creator><creator><name>Sato B.</name></creator><date role="Updated">2026-03-17T20:05:12Z</date><date role="Created">2011-12-14T16:55:14Z</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>giant-stars</subject><subject>g-stars</subject><subject>chemical-abundances</subject><description>We present basic stellar parameters of 99 late-type G giants based on high-resolution spectra obtained by the High Dispersion Spectrograph attached to Subaru Telescope. These stars are targets of a Doppler survey program searching for extra-solar planets among evolved stars, with a metallicity of -0.8&lt;[Fe/H]&lt;+0.2. We also derived their abundances of 15 chemical elements, including four {alpha}-elements (Mg, Si, Ca, Ti), three odd-Z light elements (Al, K, Sc), four iron peak elements (V, Cr, Fe, Ni), and four neutron-capture elements (Y, Ba, La, Eu). 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Bolometric correction</description><unit>mag</unit><ucd>phot.mag.bc</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Mass</name><description>? Mass of star</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logAge</name><description>? Logarithm of stellar age</description><unit>log(yr)</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logL</name><description>? Logarithm of luminosity</description><unit>log(solLum)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Teff2</name><description>Effective temperature (3)</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[Fe/H]2</name><description>Metallicity, [Fe/H]</description><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logg2</name><description>Logarithm of stellar surface gravity (4)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Vt2</name><description>Microturbulent velocity</description><unit>km/s</unit><ucd>phys.veloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>HRV</name><description>Heliocentric radial velocity</description><unit>km/s</unit><ucd>spect.dopplerVeloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_HRV</name><description>Error of heliocentric radial velocity</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ulsr</name><description>Galactic velocity component U relative to LSR</description><unit>km/s</unit><ucd>phys.veloc;pos.cartesian.x</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Ulsr</name><description>Error of Ulsr</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Vlsr</name><description>Galactic velocity component V relative to LSR</description><unit>km/s</unit><ucd>phys.veloc;pos.cartesian.y;pos.lsr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Vlsr</name><description>Error of Vlsr</description><unit>km/s</unit><ucd>stat.error;phys.veloc;pos.lsr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Wlsr</name><description>Galactic velocity component W relative to LSR</description><unit>km/s</unit><ucd>phys.veloc;pos.cartesian.z</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Wlsr</name><description>Error of Wlsr</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>TD/D</name><description>Relative probability of thick-disk/thin-disk (5)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Note</name><description>[TD] TD for star likely to be a thick-disk star rather than a thin-disk star</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>[Fe1/H]</name><description>Abundance of [FeI/H]</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Fe2/H]</name><description>Abundance of [FeII/H]</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Al/Fe]</name><description>? 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