J/A+A/630/A106ivo://CDS.VizieR/J/A+A/630/A106doi:10.26093/cds/vizier.36300106CDSGaulme P.Guzik J.A.2021-01-08T16:44:11Z2020-01-31T12:28:11ZCDS support team

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

cds-question@unistra.freclipsing-binary-starsasteroseismologyEclipsing binaries (EBs) are unique targets for measuring precise stellar properties and can be used to constrain stellar evolution models. In particular, it is possible to measure masses and radii of both components of a double-lined spectroscopic EB at the percent level. Since the advent of high-precision photometric space missions (MOST, CoRoT, Kepler, BRITE, TESS), the use of stellar pulsation properties to infer stellar interiors and dynamics constitutes a revolution for studies of low-mass stars. The Kepler mission has led to the discovery of thousands of classical pulsators such as {delta} Scuti and solar-like oscillators (main sequence and evolved), but also almost 3000 EBs with orbital periods shorter than 1100 days. We report the first systematic search for stellar pulsators in the entire Kepler EB catalog. The focus is mainly aimed at discovering {delta} Scuti, {gamma} Doradus, red giant, and tidally excited pulsators. We developed a data inspection tool (DIT) that automatically produces a series of plots from the Kepler light curves that allows us to visually identify whether stellar oscillations are present in a given time series. We applied the DIT to the whole Kepler EB database and identified 303 systems whose light curves display oscillations, including 163 new discoveries. A total of 149 stars are flagged as {delta} Scuti (100 from this paper), 115 as {gamma} Doradus (69 new), 85 as red giants (27 new), and 59 as tidally excited oscillators (29 new). There is some overlap among these groups, as some display several types of oscillations. Despite the likelihood that many of these systems are false positives, for example, when an EB light curve is blended with a pulsator, this catalog gathers a vast sample of systems that are valuable for a better understanding of stellar evolution.2019A&A...630A.106Ghttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/630/A106CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/630/A106https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/630/A106http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/630/A106https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/630/A106https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/630/A106http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/630/A106GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/630/A106/tablea1 (Properties of the systems where pulsations are detected)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/630/A106/tablea1?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/630/A106/tablea1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/630/A106/tablea1?GETtext/xml+votable180.050000true291.5834736.918320.0055555555555555565/3646 3683 3689 3693-3694 3704 3706 3780 3782 3792-3793 6/14575 14578-14579 14581-14583 14589 14591 14730-14731 14738 14744 14746 14749 14751-14754 14761-14763 14765 14767-14768 14770-14771 14781-14783 14794-14795 14830 14915 14918 14921 14923-14925 14927-14929 14931-14933 14935-14937 14939 14941-14942 14948 14950 14952 14956 14958-14960 14963-14964 14967 14969-14970 14975 15041 15044 15062 15106-15107 15109-15113 15116 15124 15126-15127 15134 15139 15141 15144 15146 15148 15150 15157 15200https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/630/A106?format=asciidefaultJ/A+A/630/A106/tablea1Properties of the systems where pulsations are detectedrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintKICKIC numbermeta.id;meta.mainintTeff? Effective temperatureKphys.temperature.effectiveintnullableKepmag? Kepler magnitudemagphot.mag;em.optfloatnullableTypeType of binary systems (1)src.classcharEclNumber of eclipses that are visible per orbital period (0 for ELL systems, 1 or 2 for the others)meta.numberintPorbOrbital period rounded at two digitsdtime.periodfloatDepth? Eclipse depth of the deepest eclipse (primary)%phys.absorption.opticalDepth;arith.ratiofloatnullableSep? Orbital phase separation in between the secondary and the primary eclipsepos.angDistancefloatnullableW2/W1? Eclipse duration ratio W2/W1time.duration;arith.ratiofloatnullableW1+W2/Porb? Sum of eclipse duration relative to orbital period, W1+w2/Porbstat.fit.paramfloatnullablePulstypePulsator type (2)meta.noteRefLiterature, in refs.dat filemeta.bibcharNewPB[Y] Target identified both as a pulsator and a binary for first timemeta.codecharNotesNotes (3)meta.notecharSimbadSimbad column added by the CDSmeta.ref.urlchar_RAPositions from KIC (right ascension part)degpos.eq.ra;meta.main_DEPositions from KIC (declination part)degpos.eq.dec;meta.mainJ/A+A/630/A106/refsReferencesAutAuthor's namemeta.bib.authorcharComCommentsmeta.notecharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRefReference codemeta.notecharBibCodeBibCodemeta.bib.bibcodechar