J/ApJS/225/32ivo://CDS.VizieR/J/ApJS/225/32doi:10.26093/cds/vizier.22250032CDSBrewer J.M.Fischer D.A.Valenti J.A.Piskunov N.2021-08-20T08:02:55Z2016-11-21T15:19:04ZCDS support team

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

cds-question@unistra.frspectroscopychemical-abundancesstellar-massesWe present a catalog of uniformly determined stellar properties and abundances for 1615 F, G, and K stars using an automated spectral synthesis modeling procedure. All stars were observed using the HIRES spectrograph at Keck Observatory. Our procedure used a single line list to fit model spectra to observations of all stars to determine effective temperature, surface gravity, metallicity, projected rotational velocity, and the abundances of 15 elements (C, N, O, Na, Mg, Al, Si, Ca, Ti, V, Cr, Mn, Fe, Ni, and Y). Sixty percent of the sample had Hipparcos parallaxes and V-band photometry, which we combined with the spectroscopic results to obtain mass, radius, and luminosity. Additionally, we used the luminosity, effective temperature, metallicity and {alpha}-element enhancement to interpolate in the Yonsei-Yale isochrones to derive mass, radius, gravity, and age ranges for those stars. Finally, we determined new relations between effective temperature and macroturbulence for dwarfs and subgiants. Our analysis achieved precisions of 25K in T_eff_, 0.01dex in [M/H], 0.028dex for logg, and 0.5km/s in vsini based on multiple observations of the same stars. The abundance results were similarly precise, between ~0.01 and ~0.04dex, though trends with respect to T_eff_ remained for which we derived empirical corrections. The trends, though small, were much larger than our uncertainties and are shared with published abundances. We show that changing our model atmosphere grid accounts for most of the trend in [M/H] between 5000 and 5500K, indicating a possible problem with the atmosphere models or opacities.2016ApJS..225...32Bhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/225/32CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/ApJ/809/8 : Terrestrial planet occurrence rates for KOIs (Burke+, 2015)J/ApJ/800/22 : Radial velocities of long-period planets (Feng+, 2015)J/A+A/577/A9 : Sc, V, Mn, and Co in Milky Way stars (Battistini+, 2015)J/A+A/568/A25 : C and O abundances in stellar populations (Nissen+, 2014)J/A+A/562/A71 : Abundances of solar neighbourhood dwarfs (Bensby+, 2014)J/ApJ/771/40 : Main-sequence A, F, G, & K stars photometry (Boyajian+, 2013)J/A+A/555/A150 : Physical parameters of cool solar-type stars (Tsantaki+, 2013)J/ApJ/764/78 : Oxygen abundances in nearby FGK stars (Ramirez+, 2013)J/ApJ/757/161 : Spectroscopy of 56 exoplanet host stars (Torres+, 2012)J/A+A/545/A32 : Chemical abundances of 1111 FGK stars (Adibekyan+, 2012)J/ApJ/725/2349 : C/O vs Mg/Si of planetary systems (Delgado Mena+, 2010)J/ApJ/725/875 : Chromospheric activity for CPS stars (Isaacson+, 2010)J/other/Sci/330.653 : Detected planets in the Eta-Earth Survey (Howard+, 2010)J/ApJ/715/1050 : Predicted abundances for extrasolar planets. I. (Bond+, 2010)J/A+A/512/A54 : Teff and Fbol from Infrared Flux Method (Casagrande+, 2010)J/A+A/497/497 : Physical parameters from JHK flux (Gonzalez-Hernandez+, 2009)J/ApJS/159/141 : Spectroscopic properties of cool stars. I. (Valenti+, 2005)J/A+A/435/373 : Broadening of Fe II lines by H collisions (Barklem+, 2005)J/ApJ/622/1102 : The planet-metallicity correlation. (Fischer+, 2005)J/A+A/415/1153 : [Fe/H] for 98 extra-solar planet-host stars (Santos+, 2004)J/A+A/394/927 : Age-metallicity relation for nearby stars (Ibukiyama+, 2002)J/A+A/275/101 : Chemical evolution of the galactic disk I. (Edvardsson+ 1993)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/225/32https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/225/32http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/225/32https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/225/32https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/225/32http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/225/32GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJS/225/32/stars (Spectroscopically determined stellar properties (table 8) , abundances (table 9) and derived parameters (table 11) for the 1615 F, G, and K stars)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJS/225/32/stars?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJS/225/32/stars?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJS/225/32/stars?GETtext/xml+votable180.050000true1.46875-41.7530560.0055555555555555565/3689 3691 3695 3706 3732 3733 3741 3742 3779 3780 3782 3783 3785 3792 6/0 49 60 75 100 174 181 188 220 257 276 292 309 311 377 400 414 418 423 431 460 462 463 475 548 558 576 649 679 684 701 712 713 742 748 753 758 766 790 814 815 819 824 841 871 876 913 934 935 944 957 960 987 1032 1058 1184 1186 1201 1237 1258 1268 1275 1288 1339 1341 1415 1433 1508 1530 1576 1577 1597 1603 1642 1669 1808 1817 1827 1875 1895 1907 1927 1940 1971 1975 1997 2072 2110 2152 2153 2167 2205 2250 2273 2274 2279 2299 2308 2315 2374 2416 2433 2436 2456 2459 2463 2476 2490 2497 2512 2551 2577 2584 2596 2645 2651 2691 2711 2756 2765 2790 2810 2816 2822 2838 2870 2923 2964 2972 3020 3041 3095 3102 3118 3121 3166 3199 3296 3344 3372 3383 3572 3622 3639 3645 3683 3691 3697 3780 3831 3837 3876 3925 3979 3981 4006 4106 4136 4156 4225 4280 4285 4286 4321 4328 4332 4345 4377 4422 4429 4591 4599 4634 4661 4665 4766 4776 4795 4839 4854 4881 4990 4993 4997 5009 5067 5074 5095 5170 5208 5244 5304 5308 5309 5343 5401 5413 5434 5447 5451 5475 5522 5524 5544 5553 5556 5572 5670 5726 5734 5833 5836 5843 5872 5895 5929 5973 5985 6006 6007 6017 6142 6226 6265 6269 6287 6293 6308 6349 6381 6385 6409 6485 6489 6522 6539 6568 6584 6585 6638 6662 6687 6737 6738 6739 6749 6760 6766 6791 6821 6831 6926 6932 6971 7036 7136 7208 7229 7238 7240 7241 7245 7250 7299 7345 7352 7373 7434 7546 7721 7746 7763 7803 7866 7868 7978 8094 8109 8197 8224 8237 8268 8319 8328 8357 8380 8466 8534 8614 8617 8618 8663 8700 8723 8738 8785 8788 8790 8792 8825 8881 8918 8993 8995 9026 9102 9173 9225 9355 9365 9391 9403 9435 9442 9459 9476 9482 9492 9524 9533 9591 9594 9654 9656 9662 9677 9679 9753 9801 9810 9843 9859 9873 9883 9885 9928 9934 9940 10004 10031 10079 10140 10207 10238 10263 10301 10407 10448 10476 10518 10537 10548 10550 10553 10567 10598 10629 10649 10659 10701 10730 10740 10766 10772 10787 10812 10854 10894 10899 10914 11014 11059 11091 11126 11142 11146 11165 11194 11197 11314 11348 11363 11412 11461 11510 11589 11633 11713 11732 11734 11856 11946 12146 12203 12228 12232 12296 12306 12312 12341 12347 12352 12388 12418 12424 12461 12465 12467 12477 12556 12612 12640 12644 12654 12658 12662 12676 12792 12798 12807 12813 12846 12853 12856 12857 12890 12899 12922 12944 12983 13002 13025 13062 13093 13117 13122 13134 13143 13230 13414 13415 13423 13425 13440 13487 13541 13568 13610 13625 13632 13650 13676 13684 13698 13702 13717 13734 13749 13922 13941 13946 13990 14007 14066 14089 14129 14131 14140 14155 14175 14180 14207 14248 14290 14305 14347 14412 14416 14419 14434 14459 14502 14525 14539 14548 14568 14573 14578 14579 14580 14581 14583 14584 14585 14586 14588 14589 14591 14624 14657 14730 14731 14733 14734 14735 14744 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17623 17637 17671 17714 17723 17730 17731 17812 17847 17860 17881 17888 17944 17999 18005 18028 18059 18139 18155 18171 18172 18192 18315 18340 18343 18366 18371 18373 18379 18398 18417 18441 18453 18459 18462 18473 18510 18512 18521 18536 18539 18542 18544 18551 18560 18565 18588 18614 18628 18637 18638 18640 18650 18658 18711 18722 18764 18779 18784 18809 18821 18947 18953 18976 19002 19081 19139 19153 19196 19291 19327 19350 19488 19495 19509 19541 19555 19649 19669 19746 19786 19796 19830 19899 19904 19945 19974 20072 20081 20145 20166 20177 20217 20233 20269 20276 20328 20332 20339 20376 20402 20593 20605 20621 20633 20641 20665 20701 20716 20732 20739 20746 20792 20872 21003 21117 21119 21153 21177 21185 21223 21233 21406 21477 21484 21550 21673 21703 21726 21772 21779 21838 21906 21936 21956 21989 22001 22036 22065 22078 22087 22111 22120 22125 22157 22159 22252 22397 22408 22465 22505 22519 22539 22571 22590 22646 22708 22764 22800 22808 22878 22981 22982 23013 23018 23030 23130 23140 23177 23187 23201 23301 23322 23328 23367 23369 23382 23414 23441 23497 23506 23513 23544 23545 23583 23591 23636 23646 23661 23665 23681 23710 23723 23737 23739 23758 23780 23862 23871 23893 23932 23936 23938 23940 23941 23943 23948 23961 23997 24005 24016 24019 24028 24030 24043 24102 24105 24119 24151 24163 24178 24212 24255 24312 24327 24337 24344 24391 24409 24564 24568 24702 24713 24729 24731 24827 24924 24964 24991 25078 25102 25114 25127 25132 25192 25194 25225 25407 25446 25452 25521 25538 25571 25584 25595 25692 25707 25729 25766 25875 25880 25906 25930 25939 25966 26062 26160 26183 26242 26266 26268 26298 26335 26379 26417 26462 26473 26496 26551 26575 26652 26706 26707 26719 26727 26745 26761 26779 26828 26906 26938 26953 26959 26961 26976 26978 26986 26990 26991 26992 26997 26999 27001 27018 27019 27025 27060 27079 27085 27088 27164 27179 27195 27314 27395 27475 27518 27608 27642 27661 27684 27758 27777 27788 27793 27943 27973 28009 28041 28076 28085 28122 28130 28141 28180 28245 28258 28311 28392 28395 28400 28433 28473 28500 28518 28605 28609 28668 28763 28767 28792 28987 29047 29084 29291 29349 29413 29513 29541 29640 29683 29728 29852 30015 30066 30109 30170 30278 30344 30378 30419 30435 30466 30526 30529 30530 30540 30579 30665 30707 30837 30848 30878 30905 30919 30958 30968 31029 31068 31085 31104 31130 31145 31197 31399 31416 31425 31433 31449 31478 31494 31571 31606 31641 31667 31689 31720 31737 31739 31751 31768 31796 31821 31860 32029 32083 32192 32211 32217 32282 32318 32345 32372 32485 32499 32520 32561 32564 32575 32633 32645 32665 32693 32712 32717 32727 32749 32757 34282 34290 34673 34717 34739 34773 35166 35210 35497 35740 35753 35776 35789 35799 35802 35811 35822 35848 35865 35949 35958 36019 36029 36069 36070 36092 36115 36158 36162 36171 36292 36295 36323 36347 36365 36390 36482 36487 36506 36562 36565 36635 36661 36693 36697 36713 36723 36746 36759 36766 36813 36863 38238 38260 38452 38545 38742 38765 38807 38836 38880 39422 39543 39562 39646 39735 39767 39854 40078 40101 40105 40242 40270 40442 40590 40692 40722 41941 42318 42460 42879 42936 42941 42984 42986 42989 43577 43639 43677 43813 43847 44226 44228 44243 44260 44262 44317 44370 44398 44650 44685 44727 44740 44774 44792 44891 44959 45012 45034 45927 46437 46959 46982 46987 47935 48049 48082 48105 48108 48109 48230 48334 48394 48402 48454 48460 48501 48597 48652 48658 48705 48835 48955 49060 49114 49130 49142https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJS/225/32?format=asciidefaultJ/ApJS/225/32/table7Atomic and molecular line parametersrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintElElementphys.atmol.elementcharIon[1/5]? Ion identificationphys.atmol.ionStageintnullablelambda[5164/7799] Wavelength, Angstroms0.1nmem.wldoubleExPot[0/72] Excitation potentialeVphys.atmol.excitationfloatlog(gf)[-20.1/2] Log of the oscillator strengthphys.atmol.oscStrengthdoubleGamma6[-10/1953]? Coefficient for broadening (1)stat.fit.paramdoublenullableM[x] x = Line masked from fittingmeta.codecharJ/ApJS/225/32/starsSpectroscopically determined stellar properties (table 8) , abundances (table 9) and derived parameters (table 11) for the 1615 F, G, and K starsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSPOCS[2/3247] SPOCS ID (G1)meta.id;meta.mainintNameStar namemeta.idcharTeff[4702/6773] Stellar effective temperatureKphys.temperature.effectiveintlogg[2.6/5] Stellar surface gravitylog(cm.s**-2)phys.gravityfloat[M/H][-1.2/0.6] Stellar metallicitylog(Sun)phys.abund.ZfloatS[-1.9/540] Mount Wilson Ca HK activity indexmeta.code;spect.indexfloatlogRhk[-6.3/-1.7]? log(R'HK) activity indexphot.flux;arith.ratiofloatnullableVbr[0.6/25] Derived velocity broadeningkm/sspect.line.broadfloatVsini[0/20.1] Derived projected rotational velocitykm/sphys.veloc.rotatfloatVmac[1.6/23.3] Derived macroturbulent velocitykm/sphys.velocfloatVrad[-137/164] Barycentric radial velocity at time of observationkm/sphys.veloc;pos.barycenterfloatSNR[14/492] Signal to Noise ratio at 6000 Angstromsstat.snrintCrms[0.01/0.3] RMS scatter in continuumstat.errorfloatLrms[0.01/0.1] RMS scatter in linestat.errorfloatN[1/23] Number of spectra fit for that starmeta.numberint[C/H][-0.9/0.7]? Derived [C/H] abundancephys.abundfloatnullable[N/H][-1.7/0.9]? Derived [N/H] abundancephys.abundfloatnullable[O/H][-0.5/0.8]? Derived [O/H] abundancephys.abundfloatnullable[Na/H][-21.5/0.8]? Derived [Na/H] abundancephys.abundfloatnullable[Mg/H][-1.2/0.6]? Derived [Mg/H] abundancephys.abundfloatnullable[Al/H][-1.5/1.1]? Derived [Al/H] abundancephys.abundfloatnullable[Si/H][-1.4/0.6]? Derived [Si/H] abundancephys.abundfloatnullable[Ca/H][-1.5/0.6]? Derived [Ca/H] abundancephys.abundfloatnullable[Ti/H][-0.9/0.6]? Derived [Ti/H] abundancephys.abundfloatnullable[V/H][-0.9/0.6]? Derived [V/H] abundancephys.abundfloatnullable[Cr/H][-1.2/0.6]? Derived [Cr/H] abundancephys.abundfloatnullable[Mn/H][-2.2/0.8]? Derived [Mn/H] abundancephys.abundfloatnullable[Fe/H][-1.2/0.6]? Derived [Fe/H] abundancephys.abund.Fefloatnullable[Ni/H][-1.5/0.7]? Derived [Ni/H] abundancephys.abundfloatnullable[Y/H][-1.6/2]? Derived [Y/H] abundancephys.abundfloatnullableRAJ2000SIMBAD Hour of Right Ascension (J2000)pos.eq.ra;meta.mainDEJ2000SIMBAD Degree of Declination (J2000)pos.eq.dec;meta.mainVmag[1.7/10.1]? V magnitude from SIMBADmagphot.mag;em.opt.VfloatnullableDist[3.6/353]? Distance from SIMBADpcpos.distance;pos.heliocentricfloatnullablelogL[-0.8/1.8]? Derived Stellar Luminosity (1)log(solLum)phys.luminosityfloatnullablee_logL[0.01/1.1]? Uncertainty in logL (1)log(solLum)stat.errorfloatnullableRstar[0.6/10]? Derived Stellar Radius (1)solRadphys.size.radiusfloatnullablee_Rstar[0.02/4]? Uncertainty in Rstar (1)solRadstat.errorfloatnullableMstar[0.2/7]? Derived Stellar Mass (1)solMassphys.massfloatnullablee_Mstar[0.03/14]? Uncertainty in Mstar (1)solMassstat.errorfloatnullableMiso[0.6/3]? Isochrone derived stellar mass (2)solMassphys.massfloatnullableb_Miso[0.6/2.2]? Lower bound on derived Miso (2)solMassphys.mass;stat.minfloatnullableB_Miso[0.6/3]? Upper bound on derived Miso (2)solMassphys.mass;stat.maxfloatnullablelogg2[1.6/5]? Isochrone derived surface gravity (2)log(cm.s**-2)phys.gravityfloatnullablee_logg2[0.01/0.3]? Uncertainty in logg-iso (2)log(cm.s**-2)stat.errorfloatnullableAge[0.6/15]? Isochrone derived age (2)Gyrtime.agefloatnullableb_Age[0.2/14]? Lower bound on derived Age (2)Gyrtime.age;stat.minfloatnullableB_Age[1/15]? Upper bound on derived Age (2)Gyrtime.age;stat.maxfloatnullableCCatDisplay data from Isaacson+, 2010, J/ApJ/725/875, within 1"meta.ref.urlintnullableSimbadSimbad column added by the CDSmeta.ref.urlchar