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<ri:Resource created="2020-07-28T13:07:40Z" 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>4 planet-hosting stars asteroseismic masses</title><shortName>J/MNRAS/496/5423</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/496/5423</identifier><altIdentifier>doi:10.26093/cds/vizier.74965423</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Malla S.P.</name></creator><creator><name>Stello D.</name></creator><creator><name>Huber D.</name></creator><creator><name>Montet B.T.</name></creator><creator><name>Bedding T.R.</name></creator><creator><name>Andersen M.F.,Grundahl F.</name></creator><creator><name>Jessen-Hansen J.</name></creator><creator><name>Hey D.R.</name></creator><creator><name>Palle P.L.</name></creator><creator><name>Deng L.</name></creator><creator><name>Zhang C.,Chen X.</name></creator><creator><name>Lloyd J.</name></creator><creator><name>Antoci V.</name></creator><date role="Updated">2024-08-21T20:15:31Z</date><date role="Created">2020-07-28T13:07:40Z</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>stellar-masses</subject><description>The study of planet occurrence as a function of stellar mass is important for a better understanding of planet formation. Estimating stellar mass, especially in the red giant regime, is difficult. In particular, stellar masses of a sample of evolved planet-hosting stars based on spectroscopy and grid-based modelling have been put to question over the past decade with claims they were overestimated. Although efforts have been made in the past to reconcile this dispute using asteroseismology, results were inconclusive. In an attempt to resolve this controversy, we study four more evolved planet-hosting stars in this paper using asteroseismology, and we revisit previous results to make an informed study of the whole ensemble in a self-consistent way. For the four new stars, we measure their masses by locating their characteristic oscillation frequency, numax, from their radial velocity time series observed by SONG. For two stars, we are also able to measure the large frequency separation, Delta nu, helped by extended SONG single-site and dual-site observations and new TESS observations. We establish the robustness of the numax-only-based results by determining the stellar mass from Delta nu, and from both Delta nu and numax. We then compare the seismic masses of the full ensemble of 16 stars with the spectroscopic masses from three different literature sources. We find an offset between the seismic and spectroscopic mass scales that is mass-dependent, suggesting that the previously claimed overestimation of spectroscopic masses only affects stars more massive than about 1.6M_{sun}_.</description><source format="bibcode">2020MNRAS.496.5423M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/496/5423</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/I/311">I/311 : Hipparcos, the New Reduction (van Leeuwen, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/475/1003">J/A+A/475/1003 : Stellar parameters of G and K giant stars (Hekker+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/487/373">J/A+A/487/373 : Spectroscopic parameters of 451 HARPS-GTO stars (Sousa+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/526/A71">J/A+A/526/A71 : C abundances in G and K nearby stars (da Silva+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/543/A160">J/A+A/543/A160 : Normalized spectra of 82 Kepler red giants (Thygesen+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/557/A70">J/A+A/557/A70 : Evolved planet hosts - 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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>Star</name><description>Name of the star</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>logg</name><description>Spectroscopic surface gravity (1)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_logg</name><description>Error in spectroscopic surface gravity</description><unit>log(cm.s**-2)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Teff</name><description>Spectroscopic effective temperature (1)</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_Teff</name><description>Error in spectroscopic effective temperature</description><unit>K</unit><ucd>stat.error;phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[Fe/H]</name><description>Metallicity (1)</description><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[Fe/H]</name><description>Error in metallicity</description><ucd>stat.error;phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>plx</name><description>Hipparcos Parallax (2)</description><unit>mas</unit><ucd>pos.parallax</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_plx</name><description>Error in Hipparcos Parallax</description><unit>mas</unit><ucd>stat.error;pos.parallax</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Mspec</name><description>Spectroscopic stellar mass</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Mspec</name><description>Error in spectroscopic stellar mass</description><unit>solMass</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>L</name><description>Derived Luminosity (3)</description><unit>solLum</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_L</name><description>Error in derived luminosity</description><unit>solLum</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>numax-pre</name><description>Predicted numax</description><unit>uHz</unit><ucd>em.freq</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_numax-pre</name><description>Error in predicted numax</description><unit>uHz</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>numax-obs</name><description>Observed numax</description><unit>uHz</unit><ucd>em.freq</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_numax-obs</name><description>Error in observed numax</description><unit>uHz</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Mseis</name><description>Numax only based asteroseismic mass</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Mseis</name><description>Error in numax only based asteroseismic mass</description><unit>solMass</unit><ucd>stat.error</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>_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/MNRAS/496/5423/table3</name><description>Updated Results from Stello et al. 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(2013, J/A+A/557/A70) (2)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_MHM07</name><description>? Error in MHM07</description><unit>solMass</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>MJofre</name><description>? Spectroscopic mass of the star from Jofre et al. (2015, J/A+A/574/A50) (3)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_MJofre</name><description>? Error in MJofre</description><unit>solMass</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>MStock</name><description>? Spectroscopic mass of the star from the Stock et al. (2018, J/A+A/616/A33) (4)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_MStock</name><description>? Positive error in MStock</description><unit>solMass</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_MStock</name><description>? Negative error in MStock</description><unit>solMass</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Mseis</name><description>Mass of the star from asteroseismology</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_Mseis</name><description>Positive error in Mseis</description><unit>solMass</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Mseis</name><description>Negative error in Mseis</description><unit>solMass</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ref</name><description>[efg] Reference for the asteroseismic mass (5)</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</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>_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>