J/A+A/687/A208ivo://CDS.VizieR/J/A+A/687/A208doi:10.26093/cds/vizier.36870208CDSPaunzen E.Binder F.Cyniburk A.Duffek M.N.Haberhauer F.,Heinreichsberger C.Kohlhofer H.Kuess L.Maitzen H.M.Saalmann T.,Schanz A.M.Schauer S.Schmidt K.Tokareva A.Wizani I.2024-11-21T20:02:06Z2024-07-12T08:40:32ZCDS support team

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

cds-question@unistra.frvariable-starseffective-temperaturevisible-astronomyThe analysis of non-variable stars is generally neglected in the literature. However, such objects are needed for many calibration processes and for testing pulsational models. The photometric time series of the Kepler satellite mission still stand as the most accurate data available today and are excellently suited to the search for non-variable stars. We analysed all long-cadence light curves for stars not reported as a variable so far from the Kepler satellite mission. Using the known characteristics and flaws of these data sets, we defined three different frequency ranges where we searched for non-variability. The found non-variable objects are mostly cooler than the 7000K populating the whole main sequence (MS) to the red giant branch (RGB).2024A&A...687A.208Phttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/687/A208CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toV/133 : Kepler Input Catalog (Kepler Mission Team, 2009)J/AJ/159/280 : Gaia-Kepler stellar properties catalog. I. KIC starshttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/687/A208https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/687/A208http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/687/A208https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/687/A208https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/687/A208http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/687/A208GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/687/A208/table1 (The data for the apparent non-variable stars)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/687/A208/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/687/A208/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/687/A208/table1?GETtext/xml+votable180.050000true286.2796938937.580638890.0055555555555555564/922-923 933-935 944-946 5/3645-3647 3683 3704 3706 3729-3731 3760 3788-3789 3792-3793 6/14559 14567 14573 14575 14577-14579 14730-14731 14738 14744 14746-14747 14749-14751 14792 14794-14795 14822 14828 14830 14914-14915 15044-15045 15057 15059-15062 15160-15161 15164 15176-15178 15200 15202 15232-15233https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/687/A208?format=asciiOpticaldefaultJ/A+A/687/A208/table1The data for the apparent non-variable starsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintKICKIC identifiermeta.id;meta.mainintRAJ2000Right ascension (J2000)degpos.eq.ra;meta.mainindexedDEJ2000Declination (J2000)degpos.eq.dec;meta.mainindexedTeffEffective temperature from Berger et al., 2020AJ....159..280B, Cat. J/AJ/159/280Kphys.temperature.effectiveintloggSurface gravity from Berger et al., 2020AJ....159..280B, Cat. J/AJ/159/280log(cm.s**-2)phys.gravityfloatZPZero point of the light curve (HJD)darith.zpdoublesigmaStandard deviation of the mean of the light curvemagstat.stdev;phot.magdoublelogFAP1Logarithmic False-Alarm probability for the frequency range below 0.1 c/dstat.fit.goodnessintlogFAP2Logarithmic False-Alarm probability for the frequency range 0.1 to 2.0 c/dstat.fit.goodnessintlogFAP3Logarithmic False-Alarm probability for the frequency range 2.0 to 25.0 c/dstat.fit.goodnessint