J/ApJ/835/172ivo://CDS.VizieR/J/ApJ/835/172doi:10.26093/cds/vizier.18350172CDSLund M.N.Silva Aguirre V.Davies G.R.Chaplin W.J.,Christensen-Dalsgaard J.Houdek G.White T.R.Bedding T.R.Ball W.H.,Huber D.Antia H.M.Lebreton Y.Latham D.W.Handberg R.Verma K.,Basu S.Casagrande L.Justesen A.B.Kjeldsen H.Mosumgaard J.R.2017-11-27T07:53:30Z2017-09-15T15:04:53ZCDS support team

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

cds-question@unistra.frdwarf-starsThe advent of space-based missions like Kepler has revolutionized the study of solar-type stars, particularly through the measurement and modeling of their resonant modes of oscillation. Here we analyze a sample of 66 Kepler main-sequence stars showing solar-like oscillations as part of the Kepler seismic LEGACY project. We use Kepler short-cadence data, of which each star has at least 12 months, to create frequency-power spectra optimized for asteroseismology. For each star, we identify its modes of oscillation and extract parameters such as frequency, amplitude, and line width using a Bayesian Markov chain Monte Carlo "peak-bagging" approach. We report the extracted mode parameters for all 66 stars, as well as derived quantities such as frequency difference ratios, the large and small separations {Delta}{nu} and {delta}{nu}_02_; the behavior of line widths with frequency and line widths at {nu}_max_ with T_eff_, for which we derive parametrizations; and behavior of mode visibilities. These average properties can be applied in future peak-bagging exercises to better constrain the parameters of the stellar oscillation spectra. The frequencies and frequency ratios can tightly constrain the fundamental parameters of these solar-type stars, and mode line widths and amplitudes can test models of mode damping and excitation.2017ApJ...835..172Lhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/835/172CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toV/133 : Kepler Input Catalog (Kepler Mission Team, 2009)J/A+A/508/L17 : Abundances in solar analogs (Ramirez+, 2009)J/A+A/510/A21 : Stellar Limb-Darkening Coefficients (Sing, 2010)J/A+A/531/A124 : Visibilities of stellar oscillation modes (Ballot+, 2011)J/A+A/529/A75 : Limb-darkening coefficients (Claret+, 2011)J/other/Nat/486.375 : Stellar parameters of KOI stars (Buchhave+, 2012)J/ApJS/199/30 : Effective temperatures for KIC stars (Pinsonneault+, 2012)J/ApJ/757/161 : Spectroscopy of 56 exoplanet host stars (Torres+, 2012)J/ApJ/767/127 : Asteroseismic solutions for 77 Kepler stars (Huber+, 2013)J/ApJ/787/110 : SAGA: Stromgren survey of seismic stars (Casagrande+, 2014)J/ApJS/210/1 : Asteroseismic study of solar-type stars (Chaplin+, 2014)J/A+A/569/A21 : Age and mass of CoRoT exoplanet host HD 52265 (Lebreton, 2014)J/ApJS/215/19 : APOKASC catalog of Kepler red giants (Pinsonneault+, 2014)J/MNRAS/452/2127 : Fundamental param. of Kepler stars (Silva Aguirre+, 2015)J/A+A/588/A87 : Seismic global parameters of 6111 KIC (Vrard+, 2016)J/ApJ/835/173 : Kepler asteroseismic LEGACY sample. II. (Silva Aguirre+, 2017)http://www.mso.anu.edu.au/saga/saga_home.html : SAGA home pagehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/835/172https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/835/172http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/835/172https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/835/172https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/835/172http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/835/172GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/835/172/table1 (Parameters for the targets in the studied sample)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/835/172/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/835/172/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/835/172/table1?GETtext/xml+votable180.050000true292.08265537.05981530.0055555555555555566/14578 14581 14751 14757 14759 14763 14765 14767 14770 14771 14776 14778 14779 14780 14781 14782 14819 14918 14921 14930 14931 14932 14935 14937 14938 14939 14948 14959 14960 14962 14963 14966 14967 14969 15044 15057 15061 15062 15106 15109 15112 15118 15121 15123 15129 15131 15145 15146 15156 15168 15171 15172 15173 15174 15178https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/835/172?format=asciidefaultJ/ApJ/835/172/table1Parameters for the targets in the studied sampleBkQBraketing quarters (2)time.epochcharMgQMissing quarters (2)time.epochcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintKICKIC numbermeta.id;meta.maincharprimaryN2Number of calculated second differences (table 8)meta.numberintnullableNfNumber of calculated mode frequency difference ratios (table 7)meta.numberintnullableNamePopular namemeta.idcharKpmag[5.8/11] Kepler magnitudemagphot.mag;em.optfloatnumax[885/4197] Frequency of maximum amplitude ({nu}_max_) (1)uHzem.freq;src.varintDnu[48.4/173.5] Large frequency separation ({Delta}{nu}) (1)uHzem.freq;src.varfloatN[22/59] Number of peak-bagged modesmeta.numberintCatCategory according to Appourchaux+ (2012A&A...543A..54A); "F-like" or "Simple" (44 occurrences)src.classcharTeff[5180/6642] Effective temperature (3)Kphys.temperature.effectiveinte_Teff[50/180] Teff uncertainty (4)Kstat.error;phys.temperature.effectiveintr_Teff[1/6]? Reference for Teff (5)meta.ref;pos.frameintnullable[Fe/H][-1/0.4] Metallicity (3)phys.abund.Zfloate_[Fe/H][0.02/0.2] [Fe/H] uncertainty (4)stat.error;phys.abund.Fefloatr_[Fe/H][1/6]? Reference for [Fe/H] (5)meta.refintnullablelogg[3.9/4.6] Log surface gravity from Paper II (Silva Aguirre+, 2017, J/ApJ/835/173)log(cm.s**-2)phys.gravityfloate_logg[0.002/0.02] Negative uncertainty on logglog(cm.s**-2)stat.errorfloatE_logg[0.002/0.02] Positive uncertainty on logglog(cm.s**-2)stat.error;stat.maxfloatVlos[-116/32]? Line-of-sight velocity (3)km/sphys.velocfloatnullablee_Vlos[0.1]? Vlos uncertaintykm/sstat.errorfloatnullablevsini[0/24.1]? Rotational velocity (3)km/sphys.veloc.rotatfloatnullablee_vsini[0.5]? vsini uncertaintykm/sstat.error;phys.veloc.rotatfloatnullablePapIIDisplay data from Paper II (Silva Aguirre+, 2017, J/ApJ/835/173)meta.ref.urlcharSimbadSimbad column added by the CDSmeta.ref.urlchar_RARight Ascension (J2000) from SIMBAD (not part of the original data)degpos.eq.ra;meta.main_DEDeclination (J2000) from SIMBAD (not part of the original data)degpos.eq.dec;meta.mainJ/ApJ/835/172/table8*Calculated second differences {Delta}_2_{nu}(n,l) (Equation 20) for all sources and the SunrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintKICKepler Input Catalog Identifier or "Sun"meta.id;meta.maincharn[9/30] Radial orderstat.fit.paramintl[0/3] Angular degreestat.fit.paramintDel2nu[-11.4/12.1] Calculated 2nd difference {Delta}_2_{nu} (1)uHzem.freq;src.vardoublee_Del2nu[0.05/15.5] Lower error in Del2nuuHzstat.errordoubleE_Del2nu[0.06/12.1] Upper error in Del2nuuHzstat.error;stat.maxdoubleJ/ApJ/835/172/table6*Extracted mode parameters and quality control (Equations in section 3.2.3) for all sources including the Sunn[8/31] Radial orderstat.fit.paramintrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintKICKepler Input Catalog Identifier or "Sun"meta.id;meta.maincharl[0/3] Angular degreestat.fit.paramintFreq[527.6/5729.7] FrequencyuHzem.freq;src.vardoublee_Freq[0.03/6] Lower error on FrequHzstat.errordoubleE_Freq[0.03/6] Upper error on FrequHzstat.error;stat.maxdoubleAmp[0.05/6.5]? Amplitude(10-6)src.var.amplitudedoublenullablee_Amp[0.02/0.8]? Lower error on Amp(10-6)stat.errordoublenullableE_Amp[0.03/0.7]? Upper error on Amp(10-6)stat.error;stat.maxdoublenullableWidth[0.2/14.9]? Line widthuHzspect.line.widthdoublenullablee_Width[0.04/4.3]? Lower error on WidthuHzstat.error;spect.line.widthdoublenullableE_Width[0.04/7.5]? Upper error on WidthuHzstat.error;stat.maxdoublenullablel_lnKLimit flag on lnKmeta.code.errorcharlnK[-1.4/6] Natural log of Bayes factorstat.fit.paramfloatJ/ApJ/835/172/table7*The calculated mode frequency difference ratios r_01,10,02(n)_ (Equation 16) for all sources including the SunrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintKICKepler Input Catalog Identifier or "Sun"meta.id;meta.maincharTypeRatio type (r_01_, r_02_ or r_10_) (1)meta.coden[10/30] Radial orderstat.fit.paramintRatio[-0.02/0.15] Mode frequency difference ratiostat.fit.omcdoublee_Ratio[0.0003/0.07] Lower error on Ratiostat.error;arith.ratiodoubleE_Ratio[0.0003/0.06] Upper error on Ratiostat.error;stat.maxdouble