J/A+A/540/A82ivo://CDS.VizieR/J/A+A/540/A82doi:10.26093/cds/vizier.35400082CDSKrejcova T.Budaj J.2017-09-29T09:03:17Z2012-08-22T12:11:21ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frmultiple-starssolar-system-planetsline-intensitiesThe planet-star interaction is manifested in many ways. It has been found that a close-in exoplanet causes small but measurable variability in the cores of a few lines in the spectra of several stars, which corresponds to the orbital period of the exoplanet. Stars with and without exoplanets may have different properties. The main goal of our study is to search for the influence that exoplanets might have on atmospheres of their host stars. Unlike the previous studies, we do not study changes in the spectrum of a host star or differences between stars with and without exoplanets. We aim to study a large number of stars with exoplanets and the current level of their chromospheric activity and to look for a possible correlation with the exoplanetary properties.2012A&A...540A..82Khttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/540/A82CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/MNRAS/414/108 : Calibrator of exoplanet-host stars (Beust+, 2011)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/540/A82https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/540/A82http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/540/A82https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/540/A82https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/540/A82http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/540/A82GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/A+A/540/A82/table1Parameters of exoplanetary systemsSimbadNameSimbad column added by the CDSmeta.idcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintObjectPlanet namemeta.id;meta.maincharONameOther planet namemeta.idcharMpsiniPlanet mass (Mp*sini)(1.898187x10+27kg)phys.massfloatPorbOrbital perioddtime.perioddoubleaPlanet distance to the starAUphys.angSize.smajAxis;src.orbitaldoubleTeffEffective temperature of starKphys.temperature.effectiveintEWCaIIK? CaII K equivalent width0.1nmspect.line.eqWidth;em.IR.KfloatnullablelogR'HK? Activity indexphot.flux;arith.ratiofloatnullableDet[T RV] Detection method: transit (T) or radial velocity (RV)meta.code;obschar