J/MNRAS/434/1422ivo://CDS.VizieR/J/MNRAS/434/1422doi:10.26093/cds/vizier.74341422CDSMolenda-Zakowicz J.Sousa S.G.Frasca A.Uytterhoeven K.Briquet M.,Van Winckel H.Drobek D.Niemczura E.Lampens P.Lykke J.Bloemen S.,Gameiro J.F.Jean C.Volpi D.Gorlova N.Mortier A.Tsantaki M.,Raskin G.2026-01-13T20:16:46Z2014-09-24T12:45:39ZCDS support team

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

cds-question@unistra.fropen-star-clustersf-starsmetallicityeffective-temperatureThe asteroseismic and planetary studies, like all research related to stars, need precise and accurate stellar atmospheric parameters as input. We aim at deriving the effective temperature (Teff), the surface gravity (logg), the metallicity ([Fe/H]), the projected rotational velocity (vsini) and the MK type for 169 F-, G-, K- and M-type Kepler targets which were observed spectroscopically from the ground with five different instruments. We use two different spectroscopic methods to analyse 189 high-resolution, high-signal-to-noise spectra acquired for the 169 stars. For 67 stars, the spectroscopic atmospheric parameters are derived for the first time. KIC 9693187 and 11179629 are discovered to be double-lined spectroscopic binary systems. The results obtained for those stars for which independent determinations of the atmospheric parameters are available in the literature are used for a comparative analysis. As a result, we show that for solar-type stars the accuracy of present determinations of atmospheric parameters is +/-150K in Teff, +/-0.15dex in [Fe/H] and +/-0.3dex in logg. Finally, we confirm that the curve-of-growth analysis and the method of spectral synthesis yield systematically different atmospheric parameters when they are applied to stars hotter than 6000K.2013MNRAS.434.1422Mhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/434/1422CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toB/pastel : The PASTEL catalogue (Soubiran+, 2010-)V/133 : Kepler Input Catalog (Kepler Mission Team, 2009)Table 1: A summary of instruments and observations.Note: n is the number of acquired spectra and R is the resolving power of thehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/434/1422https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/434/1422http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/434/1422https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/434/1422https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/434/1422http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/434/1422GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/434/1422/table2 (*The MK type, effective temperature, surface gravity, and metallicity of 221 reference stars used by the ROTFIT.)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/434/1422/table2?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/434/1422/table2?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/434/1422/table2?GETtext/xml+votable180.050000true264.93997862.41655750.005555555555555556Cone search capability for table J/MNRAS/434/1422/table3 (*The atmospheric parameters, the MK type and the type of variability of our programme stars)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/434/1422/table3?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/434/1422/table3?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/434/1422/table3?GETtext/xml+votable180.050000true290.8884337.0893590.0055555555555555565/3688 3694 3776 6/684 798 815 1015 1033 1341 1408 1556 1642 2133 2194 2282 2317 2650 2678 2837 2921 2923 2997 3044 3064 3077 3085 3258 3390 3494 3618 3623 3662 3712 3970 4079 4129 4376 4574 4905 5009 5154 5304 5420 5534 5587 5853 6058 6256 7101 7264 7354 7763 8767 8843 8887 9125 9327 9753 9843 9873 10055 10375 11177 11394 11412 12332 12424 12451 12464 12526 12544 12604 12621 12704 12890 12962 13025 13028 13075 13158 13301 13332 13392 13633 13777 13882 14151 14180 14278 14358 14385 14416 14573 14575 14578 14581 14583 14585-14587 14590-14591 14630 14690 14726 14734-14735 14744 14750-14751 14757 14762-14763 14765 14767 14770-14771 14774-14775 14781-14782 14794 14816 14818-14819 14824-14825 14827 14878 14918 14921-14923 14926 14930-14933 14935 14938-14939 14941 14945 14947-14948 14952 14958-14962 14965-14970 14972 14974-14975 15041 15044 15057 15061-15062 15108-15110 15112-15113 15118 15121 15123-15124 15126-15128 15131-15132 15136-15137 15139-15141 15143-15146 15148 15150 15152-15154 15156-15158 15160 15168 15170 15172 15174 15178 15249 15364 15481 15597 15715 15730 16069 16115 16213 17171 17245 17425 17606 17847 17860 18002 18067 18139 18204 18425 18553 18821 18911 18978 18990 19045 19179 19237 19312 19912 19923 19941 20110 20145 20278 20308 20313 20390 20440 20446 21177 21269 21307 21484 21696 22120 22134 22171 22180 22199 22205 22220 22252 22257 22300 22330 22355 22654 22709 22807 22818 22823 23161 23190 23201 23339 23540 23621 23623 23695 23822 24016 24029 24570 25567 25846 25869 25930 25966 26552 26575 26583 27075 27088 27374 28336 28494 28646 29548 29765 30176 30274 30331 30339 30375 30407 30440 30529 30576 30665 30709 30825 30878 30965 31087 31094 31751 31757 31789 31821 31874 32185 32192 32468 32554 32645 32757 40932 44284 44542 44771 49114https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/434/1422?format=asciidefaultJ/MNRAS/434/1422/table2*The MK type, effective temperature, surface gravity, and metallicity of 221 reference stars used by the ROTFIT.SimbadNameSimbad column added by the CDSmeta.idnullableSeqSequential numbermeta.recordintprimaryNameStar namemeta.id;meta.maincharSpTypeMK spectral typesrc.spTypecharTeffEffective temperatureKphys.temperature.effectiveintloggSurface gravitylog(cm.s**-2)phys.gravityfloat[Fe/H]Metallicitylog(Sun)phys.abund.ZfloatAutReference author's name for adopted valuesmeta.bib.authorcharBibCodeReference Bibcode for adopted valuesmeta.bib.bibcodecharComReference comments for adopted valuesmeta.notechar_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/MNRAS/434/1422/table3*The atmospheric parameters, the MK type and the type of variability of our programme starsKICKIC number (Cat. V/133)meta.id;meta.mainintprimaryInstInstrumentmeta.id;instrcharn_KIC[*] New atmopsheric parameters (1)meta.notecharTeff1? ROTFIF Effective temperatureKphys.temperature.effectiveintnullablee_Teff1? rms uncertainty on Teff1Kstat.errorintnullablelogg1? ROTFIF Surface gravitylog(cm.s**-2)phys.gravityfloatnullablee_logg1? rms uncertainty on logg1log(cm.s**-2)stat.errorfloatnullable[Fe/H]1? ROTFIF Metallicitylog(Sun)phys.abund.Zfloatnullablee_[Fe/H]1? rms uncertainty on [Fe/H]1log(Sun)stat.error;phys.abund.Fefloatnullablevsini? ROTFIF Rotational velocitykm/sphys.veloc.rotatfloatnullablee_vsini? rms uncertainty on vsinikm/sstat.error;phys.veloc.rotatfloatnullableSpTypeMK spectral typesrc.spTypecharTeff2? ARES+MOOG Effective temperatureKphys.temperature.effectiveintnullablee_Teff2? rms uncertainty on Teff2Kstat.errorintnullablelogg2? ARES+MOOG Surface gravitylog(cm.s**-2)phys.gravityfloatnullablee_logg2? rms uncertainty on logg2log(cm.s**-2)stat.errorfloatnullable[Fe/H]2? ARES+MOOG Metallicitylog(Sun)phys.abund.Zfloatnullablee_[Fe/H]2? rms uncertainty on [Fe/H]2log(Sun)stat.error;phys.abund.Fefloatnullablevturb? ARES+MOOG Microturbulent velocity {xi}km/sphys.velocfloatnullablee_vturb? rms uncertainty on vturbkm/sstat.errorfloatnullableVarType of variability (2)meta.notecharr_VarReferences for Var (3)meta.ref;pos.framechar_RAPosition form KIC (2009, Cat. V/133) catalog (right ascension part)degpos.eq.ra;meta.main_DEPosition form KIC (2009, Cat. V/133) catalog (declination part)degpos.eq.dec;meta.main