J/PASJ/57/65ivo://CDS.VizieR/J/PASJ/57/65CDSTakeda Y.Honda S.2017-11-29T11:48:23Z2005-05-27T21:05:02ZCDS support team

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

cds-question@unistra.frchemical-abundancesline-intensitiesWe determined the C, N, and O abundances of 160 nearby F, G, and K dwarfs and subgiants by using spectra obtained with the HIDES spectrograph at Okayama Astrophysical Observatory, with the purposes of (1) establishing the runs of [C/Fe], [N/Fe], and [O/Fe] for these galactic disk stars in the metallicity range of -1<~[Fe/H]~<+0.4, (2) searching for any difference in the CNO abundances of planet-host stars as compared to non-planet-host stars, and (3) examining the consistency of the abundances derived from different lines to check the validity of the analysis. The non-LTE effect on the abundance determination was taken into consideration based on our extensive statistical-equilibrium calculations.2005PASJ...57...65Thttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/PASJ/57/65CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/PASJ/57/27 : Atmospheric parameters of nearby F-K stars (Takeda+, 2005)J/PASJ/57/45 : Lithium abundances of F-K stars (Takeda+, 2005)J/PASJ/57/109 : Late-G giants abundances (Takeda+, 2005)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/PASJ/57/65https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/PASJ/57/65http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/PASJ/57/65https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/PASJ/57/65https://vizier.iucaa.in/viz-bin/votable?-source=J/PASJ/57/65http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/PASJ/57/65GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/PASJ/57/65/fitabund (Abundance results of spectral fitting analyses)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/PASJ/57/65/fitabund?https://vizier.iucaa.in/viz-bin/conesearch/J/PASJ/57/65/fitabund?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/PASJ/57/65/fitabund?GETtext/xml+votable180.050000true1.56589258.4367330.005555555555555556Cone search capability for table J/PASJ/57/65/ackerman (Reanalysis of the data of Ackerman et al. (2004A&A...414..931A))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/PASJ/57/65/ackerman?https://vizier.iucaa.in/viz-bin/conesearch/J/PASJ/57/65/ackerman?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/PASJ/57/65/ackerman?GETtext/xml+votable180.050000true176.711039-14.1120690.005555555555555556Cone search capability for table J/PASJ/57/65/tomkin92 (Reanalysis of the data of Tomkin et al. (1992AJ....104.1568T))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/PASJ/57/65/tomkin92?https://vizier.iucaa.in/viz-bin/conesearch/J/PASJ/57/65/tomkin92?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/PASJ/57/65/tomkin92?GETtext/xml+votable180.050000true18.530168-16.4263860.005555555555555556Cone search capability for table J/PASJ/57/65/tomkin95 (Reanalysis of the data of Tomkin et al. (1995AJ....109.2204T))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/PASJ/57/65/tomkin95?https://vizier.iucaa.in/viz-bin/conesearch/J/PASJ/57/65/tomkin95?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/PASJ/57/65/tomkin95?GETtext/xml+votable180.050000true2.17057636.6271250.0055555555555555566/373 679 684 706 798 819 934 1341 1531 1556 1808 2472 2476 2650 2923 3006 3020 3036 3085 3118 3494 3639 3970 4376 4468 4808 4839 4854 5009 5053 5154 5195 5266 5304 5339 5522 5531 5622 5670 5718 5836 5932 6056 6058 6130 6153 6256 6308 6539 6792 6926 7238 7334 7390 8476 8602 8716 8788 8790 8843 8845 9004 9072 9125 9403 9476 9835 9843 10359 10375 10598 10812 10899 11150 11290 11620 11644 11691 11773 12146 12332 12337 12451 12464 12621 12890 12899 12944 13020 13028 13354 13474 13620 14146 14180 14385 14459 14534 14539 14573 14901 15030 15118 15174 15356 15620 15962 16069 16759 16883 17171 17425 17576 17588 17606 17730 17860 18002 18139 18614 18821 18887 19217 19312 19323 19347 19585 19745 20145 20278 20402 20440 20446 21696 21809 21864 21989 22036 22120 22180 22300 22355 22594 22654 22823 22841 22878 23011 23013 23161 23190 23201 23230 23938 23974 24019 24029 24151 24160 24212 24536 24775 24827 24920 24924 24951 25198 25385 25407 25444 25554 25862 25869 25891 25948 26025 26284 26289 26462 26521 26575 26676 26963 26975 27088 27394 27857 28122 28336 28494 28605 28664 28763 29541 30179 30296 30576 30577 30665 30798 30825 30848 30965 30989 31094 31346 31478 31503 31650 31751 31768 32067 32192 32343 32357 32619 32645 36564 36664 36697 36723 36745 36762 40442 40567 40692 40716 40722 40823 40932 41260 42331 43310 43575 44243 44542 44653 44879 46302 46828 47347 47512 47530 48105 48281 48367 48719 48736 49106 49114https://cdsarc.cds.unistra.fr/viz-bin/moc/J/PASJ/57/65?format=asciiOpticaldefaultJ/PASJ/57/65/fitabundAbundance results of spectral fitting analysesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintHDHD number of the star (999999 for the Sun)intprimaryTeffAdopted effective temperatureKintloggAdopted logarithmic surface gravitycm.s**-2floatvtAdopted microturbulencekm/sfloat[Fe/H]Adopted metallicity (Fe abundance relative to Sun)floatA(Si)1Si abundance (6080-6089 fitting) (1)floatA(Ti)1? Ti abundance (6080-6089 fitting) (1)floatnullableA(V)1V abundance (6080-6089 fitting) (1)floatA(Fe)1Fe abundance (6080-6089 fitting) (1)floatA(Co)1Co abundance (6080-6089 fitting) (1)floatA(Ni)1Ni abundance (6080-6089 fitting) (1)floatn_A(O)2[*] "*" --> O solution may be of low accuracy (e.g.,too weak line)charA(O)2? O abundance (6156.4-6158.6 fitting) (1)floatnullableA(Ti)2? Ti abundance (6156.4-6158.6 fitting) (1)floatnullableA(Fe)2Fe abundance (6156.4-6158.6 fitting) (1)floatn_A(C)3[*] "*" --> C solution may be of low accuracy (e.g.,too weak line)charA(C)3? C abundance (8726-8730 fitting) (1)floatnullableA(Si)3Si abundance (8726-8730 fitting) (1)floatA(Fe)3Fe abundance (8726-8730 fitting) (1)floatSimbadSimbad column added by the CDSchar_RARight Ascension (J2000) from SIMBAD (not part of the original data)degpos.eq.ra;meta.mainnullable_DEDeclination (J2000) from SIMBAD (not part of the original data)degpos.eq.dec;meta.mainnullableJ/PASJ/57/65/cabundResults of the analyses of carbon linesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintHDHD number of the star (999999 for the Sun)intTeffAdopted effective temperatureKintloggAdopted logarithmic surface gravitycm.s**-2floatvtAdopted microturbulencekm/sfloat[Fe/H]Adopted metallicity (Fe abundance relative to Sun)floatEW(C5052)Measured equivalent width of C I 5052.170.1nmfloatEW(C5380)? Measured equivalent width of C I 5380.340.1nmfloatnullableEW(C8727)Equivalent width of [C I] 8727.13 (evaluated from the fitting solution)0.1nmfloatEW(Fe8727)? Equivalent width of Fe I 8727.13 (evaluated from the fitting solution)0.1nmfloatnullable[C/H]8727Abundance [C/H] from [C I] 8727.13float[C/H]5052? Abundance [C/H] from C I 5052.17floatnullableDel(5052)? Non-LTE correction for C I 5052.17floatnullable[C/H]5380? Abundance [C/H] from C I 5380.34floatnullableDel(5380)? Non-LTE correction for C I 5380.34floatnullable[C/H]50+53? Mean of [C/H]5052 and [C/H]5380 (finally adopted [C/H]) (1)floatnullableDel(50+53)? Mean of Del(5052) and Del(5380)floatnullableJ/PASJ/57/65/nabundResults of the analyses of nitrogen linesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintHDHD number of the star (999999 for the Sun)intTeffAdopted effective temperatureKintloggAdopted logarithmic surface gravitycm.s**-2floatvtAdopted microturbulencekm/sfloat[Fe/H]Adopted metallicity (Fe abundance relative to Sun)floatEWNIMeasured equivalent width of N I 8683.400.1pmfloat[N/H]Abundance [N/H] from N I 8683.40 (finally adopted [N/H])floatDelNon-LTE correction for N I 8683.40floatJ/PASJ/57/65/oabundResults of the analyses of oxygen linesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintHDHD number of the star (999999 for the Sun)intTeffAdopted effective temperatureKintloggAdopted logarithmic surface gravitycm.s**-2floatvtAdopted microturbulencekm/sfloat[Fe/H]Adopted metallicity (Fe abundance relative to Sun)floatEW(O6300)Measured/decomposed equivalent width of [O I] 6300.300.1pmfloatEW(Ni6300)Measured/decomposed equivalent width of Ni I 6300.350.1pmfloatEW(O6158)Equivalent width of O I 6158.2 (evaluated from the fitting solution)0.1pmfloatEW(O7771)Measured equivalent width of O I 7771.940.1pmfloatEW(O7774)Measured equivalent width of O I 7774.150.1pmfloatEW(O7775)Measured equivalent width of O I 7775.390.1pmfloat[O/H]6300Abundance [O/H] from [O I] 6300.30float[O/H]6158Abundance [O/H] from O I 6158.2floatDel(6158)Non-LTE correction for O I 6158.2float[O/H]7771Abundance [O/H] from O I 7771.94floatDel(7771)Non-LTE correction for O I 7771.94float[O/H]7774Abundance [O/H] from O I 7774.15floatDel(7774)Non-LTE correction for O I 7774.15float[O/H]7775Abundance [O/H] from O I 7775.39floatDel(7775)Non-LTE correction for O I 7775.39float[O/H]7773Mean [O/H] for the 7771-5 triplet (finally adopted [O/H])floatDel(7771-5)Mean non-LTE correction for the 7771-5 tripletfloatJ/PASJ/57/65/ackermanReanalysis of the data of Ackerman et al. (2004A&A...414..931A)NameName of the starcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTeffAdopted effective temperatureKintloggAdopted logarithmic surface gravitycm.s**-2floatvtAdopted microturbulence velocitykm/sfloat[Fe/H]Adopted metallicity (Fe abundance relative to Sun)floatEW(1)Adopted equivalent width of line 1 (1)0.1pmfloatANLTE(1)Resulting NLTE abundance for line 1 (1)floatDel(1)Non-LTE correction for line 1 (1)floatEW(2)Adopted equivalent width of line 2 (2)0.1pmfloatANLTE(2)Resulting NLTE abundance for line 2 (2)floatDel(2)Non-LTE correction for line 2 (2)floatEW(3)Adopted equivalent width of line 3 (3)0.1pmfloatANLTE(3)Resulting NLTE abundance for line 3 (3)floatDel(3)Non-LTE correction for line 3 (3)floatEW(4)Adopted equivalent width of line 4 (4)0.1pmfloatANLTE(4)Resulting NLTE abundance for line 4 (4)floatDel(4)Non-LTE correction for line 4 (4)floatEW(5)Adopted equivalent width of line 5 (5)0.1pmfloatANLTE(5)Resulting NLTE abundance for line 5 (5)floatDel(5)Non-LTE correction for line 5 (5)float<ANLTE>Mean NLTE abundancedouble<Del>Mean Non-LTE correctionfloat[C/H]Mean result of [C/H] (= <A_NLTE> - 8.56)float[C/Fe]Mean result of [C/Fe] (= [C/H] - [Fe/H])floatSimbadSimbad column added by the CDSchar_RARight Ascension (J2000) from SIMBAD (not part of the original data)degpos.eq.ra;meta.mainnullable_DEDeclination (J2000) from SIMBAD (not part of the original data)degpos.eq.dec;meta.mainnullableJ/PASJ/57/65/tomkin92Reanalysis of the data of Tomkin et al. (1992AJ....104.1568T)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameName of the starcharTeffAdopted effective temperatureKintloggAdopted logarithmic surface gravitycm.s**-2floatvtAdopted microturbulence velocitykm/sfloat[Fe/H]Adopted metallicity (Fe abundance relative to Sun)floatEW(1)Adopted equivalent width of line 1 (1)0.1pmfloatANLTE(1)Resulting NLTE abundance for line 1 (1)floatDel(1)Non-LTE correction for line 1 (1)floatEW(2)Adopted equivalent width of line 2 (2)0.1pmfloatANLTE(2)Resulting NLTE abundance for line 2 (2)floatDel(2)Non-LTE correction for line 2 (2)floatEW(3)Adopted equivalent width of line 3 (3)0.1pmfloatANLTE(3)Resulting NLTE abundance for line 3 (3)floatDel(3)Non-LTE correction for line 3 (3)floatEW(4)Adopted equivalent width of line 4 (4)0.1pmfloatANLTE(4)Resulting NLTE abundance for line 4 (4)floatDel(4)Non-LTE correction for line 4 (4)floatEW(5)Adopted equivalent width of line 5 (5)0.1pmfloatANLTE(5)Resulting NLTE abundance for line 5 (5)floatDel(5)Non-LTE correction for line 5 (5)float<ANLTE>Mean NLTE abundancedouble<Del>Mean Non-LTE correctionfloat[C/H]Mean result of [C/H] (= <A_NLTE> - 8.56)float[C/Fe]Mean result of [C/Fe] (= [C/H] - [Fe/H])floatSimbadSimbad column added by the CDSchar_RARight Ascension (J2000) from SIMBAD (not part of the original data)degpos.eq.ra;meta.mainnullable_DEDeclination (J2000) from SIMBAD (not part of the original data)degpos.eq.dec;meta.mainnullableJ/PASJ/57/65/tomkin95Reanalysis of the data of Tomkin et al. (1995AJ....109.2204T)NameName of the starcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTeffAdopted effective temperatureKintloggAdopted logarithmic surface gravitycm.s**-2floatvtAdopted microturbulence velocitykm/sfloat[Fe/H]Adopted metallicity (Fe abundance relative to Sun)floatEW(1)Adopted equivalent width of line 1 (1)0.1pmfloatANLTE(1)Resulting NLTE abundance for line 1 (1)floatDel(1)Non-LTE correction for line 1 (1)floatEW(2)Adopted equivalent width of line 2 (2)0.1pmfloatANLTE(2)Resulting NLTE abundance for line 2 (2)floatDel(2)Non-LTE correction for line 2 (2)floatEW(3)Adopted equivalent width of line 3 (3)0.1pmfloatANLTE(3)Resulting NLTE abundance for line 3 (3)floatDel(3)Non-LTE correction for line 3 (3)floatEW(4)Adopted equivalent width of line 4 (4)0.1pmfloatANLTE(4)Resulting NLTE abundance for line 4 (4)floatDel(4)Non-LTE correction for line 4 (4)floatEW(5)Adopted equivalent width of line 5 (5)0.1pmfloatANLTE(5)Resulting NLTE abundance for line 5 (5)floatDel(5)Non-LTE correction for line 5 (5)float<ANLTE>Mean NLTE abundancedouble<Del>Mean Non-LTE correctionfloat[C/H]Mean result of [C/H] (= <A_NLTE> - 8.56)float[C/Fe]Mean result of [C/Fe] (= [C/H] - [Fe/H])floatSimbadSimbad column added by the CDSchar_RARight Ascension (J2000) from SIMBAD (not part of the original data)degpos.eq.ra;meta.mainnullable_DEDeclination (J2000) from SIMBAD (not part of the original data)degpos.eq.dec;meta.mainnullableJ/PASJ/57/65/CIlinesEquivalent Widths and NLTE corrections of C I lines (9061.44, 9078.29, 9088.51, 9094.83, 9111.81 {AA})A(LTE)LTE abundancefloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintCodeModel code (1)charlambdaWavelength of the line0.1nmdoublevtMicroturbulence velocitykm/sfloat[C/Fe]aSodium-to-iron logarithmic abundance ratiofloatAinputAssigned sodium abundancefloatW(LTE)LTE equivalent width0.1pmdoubleW(NLTE)NLTE equivalent width0.1pmdoubleA(NLTE)NLTE abundancefloatDeltaNon-LTE abundance correctionfloat