J/AJ/153/21ivo://CDS.VizieR/J/AJ/153/21doi:10.26093/cds/vizier.51530021CDSLuck R.E.2020-09-18T08:20:28Z2017-07-04T06:03:03ZCDS support team

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

cds-question@unistra.frf-starsdwarf-starschemical-abundancesstellar-massesstellar-ageseffective-temperatureParameters and abundances have been derived for 1002 stars of spectral types F, G, and K, and luminosity classes IV and V. After culling the sample for rotational velocity and effective temperature, 867 stars remain for discussion. Twenty-eight elements are considered in the analysis. The {alpha}, iron-peak, and Period 5 transition metal abundances for these stars show a modest enhancement over solar averaging about 0.05dex. The lanthanides are more abundant, averaging about +0.2dex over solar. The question is: Are these stars enhanced, or is the Sun somewhat metal-poor relative to these stars? The consistency of the abundances derived here supports an argument for the latter view. Lithium, carbon, and oxygen abundances have been derived. The stars show the usual lithium astration as a function of mass/temperature. There are more than 100 planet-hosts in the sample, and there is no discernible difference in their lithium content, relative to the remaining stars. The carbon and oxygen abundances show the well-known trend of decreasing [x/Fe] ratio with increasing [Fe/H].2017AJ....153...21Lhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/153/21CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toI/274 : Catalog of Components of Double & Multiple stars (Dommanget+ 2002)I/239 : The Hipparcos and Tycho Catalogues (ESA 1997)J/AJ/150/88 : Abundances in local region. I. G and K giants (Luck, 2015)J/A+A/562/A71 : Abundances of solar neighbourhood dwarfs (Bensby+, 2014)J/AJ/147/137 : Atmospheric parameters in luminous stars (Luck, 2014)J/AJ/142/136 : Spectroscopy of Cepheids. l=30-250{deg} (Luck+, 2011)J/AJ/133/2464 : Parameters and abundances of nearby giants (Luck+, 2007)J/AJ/129/1063 : Abundances of stars within 15pc of the Sun (Luck+, 2005)J/MNRAS/349/757 : Masses, ages and metallicities of F-G dwarfs (Lambert+, 2004)J/A+AS/106/275 : Theoretical isochrones (Bertelli+ 1994)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/153/21https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/153/21http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/153/21https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/153/21https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/153/21http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/153/21GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/AJ/153/21/table3 (Parameter and iron data)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/153/21/table3?https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/153/21/table3?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/153/21/table3?GETtext/xml+votable180.050000true191.247521139.27891610.005555555555555556Cone search capability for table J/AJ/153/21/table4 (Z>10 abundances for mass-derived gravities)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/153/21/table4?https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/153/21/table4?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/153/21/table4?GETtext/xml+votable180.050000true191.247521139.27891610.005555555555555556Cone search capability for table J/AJ/153/21/table5 (Lithium, carbon, and oxygen data)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/153/21/table5?https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/153/21/table5?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/153/21/table5?GETtext/xml+votable180.050000true191.247521139.27891610.005555555555555556Cone search capability for table J/AJ/153/21/table7 ([x/H] detail for Z>10: physical parameters)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/153/21/table7?https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/153/21/table7?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/153/21/table7?GETtext/xml+votable180.050000true191.247521139.27891610.005555555555555556Cone search capability for table J/AJ/153/21/table1 (Program stars)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/153/21/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/153/21/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/153/21/table1?GETtext/xml+votable180.050000true169.5451531.52911720.005555555555555556Cone search capability for table J/AJ/153/21/table2 (Temperature, luminosity, mass, age, and gravity)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/153/21/table2?https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/153/21/table2?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/153/21/table2?GETtext/xml+votable180.050000true191.247521139.27891610.0055555555555555566/49 60 100 137 215 309 311 322 333 336 373 377 400 418 475 483 497 634 679 684 706 725 734 742 748 770 798 815 819 849 871 917 934 944 953 987 993 1032 1033 1042 1075 1077 1247 1341 1433 1452 1530 1556 1597 1603 1642 1715 1728 1792 1827 1875 1904 1914 1938 2062 2094 2110 2111 2133 2167 2169 2254 2294 2305 2317 2366 2472 2476 2489 2491 2572 2579 2622 2650 2652 2717 2747 2923 2961 2984 3006 3020 3036 3085 3102 3118 3147 3258 3313 3360 3363 3372 3405 3511 3638 3639 3649 3683 3691 3697 3715 3780 3786 3809 3837 3865 3915 3932 3954 3979 4019 4079 4129 4136 4156 4184 4225 4227 4234 4241 4333 4376 4429 4438 4468 4528 4591 4665 4762 4808 4839 4854 4912 4920 5009 5041 5044 5053 5074 5108 5143 5154 5160 5207 5266 5304 5309 5343 5377 5413 5474 5488 5498 5522 5531 5587 5670 5718 5726 5836 5853 5899 5929 5930 6052 6066 6087 6130 6217 6226 6256 6273 6287 6308 6385 6409 6418 6457 6522 6523 6760 6766 6791 6831 6926 6941 6953 7052 7141 7204 7238 7240 7264 7299 7326 7354 7390 7443 7622 7665 7746 7763 7868 8094 8109 8224 8345 8357 8381 8429 8433 8466 8476 8602 8614 8663 8700 8716 8788 8790 8822 8843 8845 8887 8896 8923 8985 8995 9026 9056 9072 9125 9128 9179 9327 9339 9357 9375 9403 9442 9443 9459 9460 9492 9553 9570 9648 9660 9679 9753 9801 9807 9835 9843 9857 9873 10004 10062 10140 10225 10313 10325 10375 10400 10408 10439 10559 10598 10735 10812 10899 10914 11034 11087 11103 11126 11142 11150 11165 11197 11212 11225 11228 11290 11314 11403 11405 11412 11534 11633 11644 11691 11732 11735 11806 11807 11810 11834 11930 12108 12146 12228 12238 12289 12295 12337 12340 12388 12421 12424 12451 12464 12465 12494 12526 12592 12621 12634 12644 12654 12704 12788 12792 12795 12798 12825 12827 12850 12856 12890 12899 12944 12983 13025 13028 13101 13106 13110 13122 13142 13172 13219 13301 13440 13474 13487 13568 13725 13749 13763 13769 13778 13791 13808 13947 13966 13998 14015 14155 14172 14180 14221 14253 14278 14290 14329 14358 14385 14412 14416 14419 14432 14434 14438 14466 14502 14522 14525 14534 14539 14548 14573 14630 14650 14726 14831 14878 14931 15007 15030 15107 15118 15154 15174 15177 15221 15227 15249 15305 15356 15373 15505 15562 15583 15597 15607 15620 15727 15746 15755 15799 15812 15883 15962 16069 16105 16183 16213 16220 16252 16342 16564 16652 16678 16679 16680 16765 16792 16883 16931 16995 17017 17028 17035 17137 17171 17180 17218 17219 17266 17308 17341 17425 17455 17541 17576 17606 17721 17730 17752 17768 17812 17847 17860 17954 17965 18002 18042 18043 18067 18115 18123 18139 18157 18184 18299 18373 18496 18553 18614 18615 18693 18710 18711 18726 18747 18821 18881 18915 18932 18966 19027 19056 19102 19132 19138 19156 19181 19219 19237 19309 19312 19323 19327 19329 19417 19424 19491 19585 19592 19745 19831 19904 19905 19912 19923 20005 20015 20121 20127 20145 20278 20328 20402 20428 20438 20440 20446 20593 20605 20683 20701 20739 20753 20872 21060 21061 21080 21121 21177 21179 21185 21240 21484 21535 21696 21699 21726 21748 21790 21809 21838 21858 21864 21868 21869 21901 21953 21961 21989 22036 22040 22103 22111 22122 22125 22157 22180 22202 22205 22238 22240 22243 22250 22252 22263 22289 22291 22300 22330 22332 22336 22340 22354 22355 22419 22427 22590 22616 22654 22707 22708 22761 22771 22773 22813 22818 22823 22841 22878 22990 23013 23057 23076 23096 23140 23150 23161 23190 23191 23201 23230 23323 23342 23344 23369 23382 23454 23479 23503 23515 23535 23537 23545 23548 23561 23575 23583 23600 23624 23634 23636 23661 23681 23731 23774 23780 23818 23880 23893 23921 23960 23974 24003 24016 24019 24028 24029 24036 24058 24102 24110 24117 24151 24160 24178 24207 24212 24239 24373 24536 24558 24731 24743 24777 24793 24839 24920 24924 25070 25071 25113 25192 25233 25277 25407 25444 25567 25766 25846 25862 25869 25870 25902 25906 25919 25930 25939 25966 25989 26050 26174 26183 26379 26402 26440 26462 26468 26521 26575 26706 26975 27006 27018 27040 27088 27109 27124 27143 27179 27199 27255 27268 27374 27462 27712 27750 27907 27925 27954 27973 27975 27980 28122 28130 28153 28173 28180 28341 28400 28439 28489 28490 28494 28605 28628 28664 28763 28792 28987 29084 29190 29196 29291 29327 29374 29513 29541 29591 29657 29675 29756 29765 29784 29900 29926 29950 29996 30015 30049 30059 30078 30100 30109 30120 30123 30127 30154 30166 30175 30176 30190 30206 30230 30246 30257 30289 30318 30319 30330 30339 30365 30374 30375 30378 30380 30407 30410 30412 30419 30437 30450 30458 30459 30471 30481 30490 30508 30518 30526 30529 30535 30540 30543 30561 30576 30579 30595 30601 30604 30658 30665 30707 30848 30878 30965 30989 31011 31015 31029 31073 31087 31101 31130 31132 31172 31204 31369 31374 31393 31399 31416 31428 31433 31478 31494 31619 31751 31768 31781 31796 31812 31813 31821 31832 31848 31874 31912 31984 32000 32001 32017 32067 32086 32158 32192 32205 32224 32296 32297 32318 32429 32511 32516 32520 32549 32552 32575 32612 32617 32619 32620 32645 32757 34717 34730 34743 35739 35948 36035 36069 36248 36288 36298 36365 36379 36446 36483 36489 36572 36628 36638 36664 36693 36697 36723 36735 36762 39854 39893 39915 40149 40197 40242 40283 40404 40442 40453 40515 40590 40692 40716 40823 40892 40932 42903 42983 43888 43963 43989 44243 44284 44398 44411 44542 44626 44638 44681 44931 45029 46939 46956 46967 47045 47997 48045 48105 48119 48254 48335 48350 48355 48545 48589 48613 48652 48705 48749 48768 48913 48955 49026 49060 49106 49114 491213.322582951404819e-19 3.852589004194616e-19https://cdsarc.cds.unistra.fr/viz-bin/moc/J/AJ/153/21?format=asciidefaultJ/AJ/153/21/table3Parameter and iron dataSimbadNameSimbad column added by the CDSmeta.idcharVt2[0.1/5.65] Microturbulent velocity (2)km/sphys.veloc.microTurbfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameName of the primary starmeta.id;meta.maincharAllDisplay the data from all the tables (tables 1-5 and 7)meta.ref.urlcharSce[EHS] Source for spectroscopic material (E=ELODIE, H=HET, or S=Sandiford) (G1)meta.codecharTeff1[3644/7671] Effective temperature (1)Kphys.temperature.effectiveintlogg1[3.08/5] Log surface acceleration (gravity), computed from average mass, temperature, and luminosity (1)cm.s**-2phys.gravityfloatVt1[0.15/5.7] Microturbulent velocity (V_t_) (1)km/sphys.veloc.microTurbfloatFeI1[5.15/8.5] Total iron abundance, computed from neutral iron lines (the solar iron abundance is 7.47) (1)phys.abund.Fefloate_FeI1[0.04/0.6] Standard deviation of the neutral iron line abundances ({sigma}) (1)stat.errorfloato_FeI1[3/639] Number of neutral iron lines used (1)meta.numberintFeII1[5.2/11.4] Total iron abundance, computed from first ionization stage iron lines (the solar iron abundance is 7.47) (1)phys.abund.Fefloate_FeII1[0/1.63] Standard deviation of the first ionization stage iron line abundances (1)stat.errorfloato_FeII1[1/90] Number of first ionization stage iron lines used (1)meta.numberintTeff2[3644/7671] Effective temperature (2)Kphys.temperature.effectiveintlogg2[3/5] Log surface acceleration (gravity), computed from ionization balance (2)cm.s**-2phys.gravityfloatFeI2[5.15/8.3] Total iron abundance, computed from neutral iron lines (the solar iron abundance is 7.47) (2)phys.abund.Fefloate_FeI2[0.04/0.6] Standard deviation of the neutral iron line abundances (2)stat.errorfloato_FeI2[3/639] Number of neutral iron lines used (2)meta.numberintFeII2[5.15/11.4] Total iron abundance, computed from first ionization stage iron lines (the solar iron abundance is 7.47) (2)phys.abund.Fefloate_FeII2[0/1.63] Standard deviation of the first ionization stage iron line abundances (2)stat.errorfloato_FeII2[1/90] Number of first ionization stage iron lines used (2)meta.numberint_RAPosition from SIMBAD database (right ascension part)degpos.eq.ra;meta.main_DEPosition from SIMBAD database (declination part)degpos.eq.dec;meta.mainJ/AJ/153/21/table4Z>10 abundances for mass-derived gravitiesSimbadNameSimbad column added by the CDSmeta.idcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameName of the primary starphys.abundcharAllDisplay the data from all the tables (tables 1-5 and 7)phys.abundcharSce[EHS] Source for spectroscopic material (E=ELODIE, H=HET, or S=Sandiford) (G1)phys.abundcharTeff[3644/7671] Effective temperatureKphys.temperature.effectiveintlogg[3.08/5] Log of the surface acceleration due to gravitylog(cm.s**-2)phys.gravityfloatVt[0.15/5.68] Microturbulent velocity (V_t_)km/sphys.abundfloat[Na/H][-2.5/1.9]? Log abundance of sodiumlog(Sun)phys.abundfloatnullable[Mg/H][-2.1/2.1]? Log abundance of magnesiumlog(Sun)phys.abundfloatnullable[Al/H][-1.2/1.3]? Log abundance of aluminumlog(Sun)phys.abundfloatnullable[Si/H][-1.7/3.2]? Log abundance of siliconlog(Sun)phys.abundfloatnullable[S/H][-0.6/4.7]? Log abundance of sulfurlog(Sun)phys.abundfloatnullable[Ca/H][-2.3/2.1]? Log abundance of calciumlog(Sun)phys.abundfloatnullable[Sc/H][-1.8/2.4]? Log abundance of scandiumlog(Sun)phys.abundfloatnullable[Ti/H][-2.2/1.9]? Log abundance of titaniumlog(Sun)phys.abundfloatnullable[V/H][-2.8/2.1]? Log abundance of vanadiumlog(Sun)phys.abundfloatnullable[Cr/H][-2.5/1.8]? Log abundance of chromiumlog(Sun)phys.abundfloatnullable[Mn/H][-2.7/1.9]? Log abundance of manganeselog(Sun)phys.abundfloatnullable[Fe/H][-2.3/1.1]? Log abundance of ironlog(Sun)phys.abundfloatnullable[Co/H][-1.9/2.1]? Log abundance of cobaltlog(Sun)phys.abundfloatnullable[Ni/H][-2.2/1.8]? Log abundance of nickellog(Sun)phys.abundfloatnullable[Cu/H][-2.1/1.7]? Log abundance of copperlog(Sun)phys.abundfloatnullable[Zn/H][-2.3/4]? Log abundance of zinclog(Sun)phys.abundfloatnullable[Sr/H][-1.7/2.7]? Log abundance of strontiumlog(Sun)phys.abundfloatnullable[Y/H][-1.9/2.4]? Log abundance of yttriumlog(Sun)phys.abundfloatnullable[Zr/H][-1.1/4.6]? Log abundance of zirconiumlog(Sun)phys.abundfloatnullable[Ba/H][-3.2/1.2]? Log abundance of bariumlog(Sun)phys.abundfloatnullable[La/H][-1.2/2.6]? Log abundance of lanthanumlog(Sun)phys.abundfloatnullable[Ce/H][-1.1/3.1]? Log abundance of ceriumlog(Sun)phys.abundfloatnullable[Nd/H][-1/3.6]? Log abundance of neodymiumlog(Sun)phys.abundfloatnullable[Sm/H][-0.9/3.4]? Log abundance of samariumlog(Sun)phys.abundfloatnullable[Eu/H][-2.3/3.3]? Log abundance of europiumlog(Sun)phys.abundfloatnullable_RAPosition from SIMBAD database (right ascension part)degpos.eq.ra;meta.main_DEPosition from SIMBAD database (declination part)degpos.eq.dec;meta.mainJ/AJ/153/21/table5Lithium, carbon, and oxygen dataSimbadNameSimbad column added by the CDSmeta.idcharLi[-1.1/3.8]? Lithium abundance (2)phys.abundfloatnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameName of the primary starmeta.id;meta.maincharAllDisplay the data from all the tables (tables 1-5 and 7)meta.ref.urlcharSce[EHS] Source for spectroscopic material (E=ELODIE, H=HET, or S=Sandiford) (G1)meta.codecharTeff[3644/7671] Effective temperatureKphys.temperature.effectiveintlogg[3/5] Log surface gravitylog(cm.s**-2)phys.gravityfloatVt[0.15/5.7] Microturbulent velocity (V_t_)km/sphys.velocfloatvsini[0/97.2] Rotational velocity (V_r_)km/sphys.veloc.rotatfloatFe[5.15/8.5] Iron abundance (1)log(Sun)phys.abund.Fefloatl_Li[L] L=Upper limit flag on lithium abundancemeta.code.errorcharNLTE[-0.1/0.2]? Correction for Non Local Thermodynamic Equilibriumarith.factorfloatnullable505.2[6.4/8.9]? Carbon abundance from C I 505.2nm line (3)phys.abundfloatnullable538.0[6.9/9.1]? Carbon abundance from C I 538.0nm line (3)phys.abundfloatnullableC2[6.4/9.3]? Carbon abundance from C2 Swan lines (primary indicator at 513.5nm) (3)phys.abundfloatnullable615.5[6.5/9.4]? Oxygen abundance from [OI] 630.0nm line (4)phys.abundfloatnullable630.0[6.5/9.5]? Oxygen abundance from O I 615.5 triplet (4)phys.abundfloatnullable<C>[6.6/9.3]? Mean carbon abundance (weights discussed in Section 3.3) (3)phys.abundfloatnullable<O>[6.5/9.5]? Mean oxygen abundance (weights discussed in Section 3.3) (4)phys.abundfloatnullable_RAPosition from SIMBAD database (right ascension part)degpos.eq.ra;meta.main_DEPosition from SIMBAD database (declination part)degpos.eq.dec;meta.mainJ/AJ/153/21/table7[x/H] detail for Z>10: physical parametersSimbadNameSimbad column added by the CDSmeta.idcharNameName of the primary starmeta.id;meta.maincharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintAllDisplay the data from all the tables (tables 1-5 and 7)meta.ref.urlcharTagID tag for the starmeta.idcharSce[EHS] Source for spectroscopic material (E=ELODIE, H=HET, or S=Sandiford) (G1)meta.codecharTeff[3644/7671] Effective temperatureKphys.temperature.effectiveintlogg[3/5] Log surface gravitylog(cm.s**-2)phys.gravityfloatVt[0.15/5.7] Microturbulent velocity (V_t_)km/sphys.velocfloat<[NaI/H]>[-2.5/1.9]? Mean abundance of element [NaI/H] relative to solarlog(Sun)phys.abundfloatnullablee_<[NaI/H]>[0.02/1.2]? Standard Deviation of <[NaI/H]>log(Sun)stat.error;phys.abundfloatnullableo_<[NaI/H]>[1/8]? Number of lines used in <[NaI/H]>meta.numberintnullable<[MgI/H]>[-2.1/2.1]? Mean abundance of element [MgI/H] relative to solarlog(Sun)phys.abundfloatnullablee_<[MgI/H]>[0/1.4]? Standard Deviation of <[MgI/H]>log(Sun)stat.error;phys.abundfloatnullableo_<[MgI/H]>[1/8]? Number of lines used in <[MgI/H]>meta.numberintnullable<[AlI/H]>[-1.2/1.3]? Mean abundance of element [AlI/H] relative to solarlog(Sun)phys.abundfloatnullablee_<[AlI/H]>[0/0.95]? Standard Deviation of <[AlI/H]>log(Sun)stat.error;phys.abundfloatnullableo_<[AlI/H]>[1/8]? Number of lines used in <[AlI/H]>meta.numberintnullable<[SiI/H]>[-1.7/2.5]? Mean abundance of element [SiI/H] relative to solarlog(Sun)phys.abundfloatnullablee_<[SiI/H]>[0.04/1]? Standard Deviation of <[SiI/H]>log(Sun)stat.error;phys.abundfloatnullableo_<[SiI/H]>[1/70]? Number of lines used in <[SiI/H]>meta.numberintnullable<[SiII/H]>[-1.7/6.8]? Mean abundance of element [SiII/H] relative to solarlog(Sun)phys.abundfloatnullablee_<[SiII/H]>[0/1.1]? Standard Deviation of <[SiII/H]>log(Sun)stat.error;phys.abundfloatnullableo_<[SiII/H]>[1/2]? Number of lines used in <[SiII/H]>meta.numberintnullable<[SI/H]>[-0.6/4.7]? Mean abundance of element [SI/H] relative to solarlog(Sun)phys.abundfloatnullablee_<[SI/H]>[0/1.4]? Standard Deviation of <[SI/H]>log(Sun)stat.error;phys.abundfloatnullableo_<[SI/H]>[1/11]? Number of lines used in <[SI/H]>meta.numberintnullable<[CaI/H]>[-2.3/1.1]? Mean abundance of element [CaI/H] relative to solarlog(Sun)phys.abundfloatnullablee_<[CaI/H]>[0.02/1.7]? Standard Deviation of <[CaI/H]>log(Sun)stat.error;phys.abundfloatnullableo_<[CaI/H]>[1/36]? Number of lines used in <[CaI/H]>meta.numberintnullable<[CaII/H]>[-0.7/4.9]? Mean abundance of element [CaII/H] relative to solarlog(Sun)phys.abundfloatnullablee_<[CaII/H]>[0/1.1]? Standard Deviation of <[CaII/H]>log(Sun)stat.error;phys.abundfloatnullableo_<[CaII/H]>[1/4]? Number of lines used in <[CaII/H]>meta.numberintnullable<[ScI/H]>[-1.5/3.2]? Mean abundance of element [ScI/H] relative to solarlog(Sun)phys.abundfloatnullablee_<[ScI/H]>[0.01/1.2]? Standard Deviation of <[ScI/H]>log(Sun)stat.error;phys.abundfloatnullableo_<[ScI/H]>[1/13]? Number of lines used in <[ScI/H]>meta.numberintnullable<[ScII/H]>[-1.9/2.2]? Mean abundance of element [ScII/H] relative to solarlog(Sun)phys.abundfloatnullablee_<[ScII/H]>[0/1.4]? Standard Deviation of <[ScII/H]>log(Sun)stat.error;phys.abundfloatnullableo_<[ScII/H]>[1/18]? Number of lines used in <[ScII/H]>meta.numberintnullable<[TiI/H]>[-2.1/1.9]? Mean abundance of element [TiI/H] relative to solarlog(Sun)phys.abundfloatnullablee_<[TiI/H]>[0.07/1.5]? Standard Deviation of <[TiI/H]>log(Sun)stat.error;phys.abundfloatnullableo_<[TiI/H]>[3/152]? Number of lines used in <[TiI/H]>meta.numberintnullable<[TiII/H]>[-2.3/2.4]? Mean abundance of element [TiII/H] relative to solarlog(Sun)phys.abundfloatnullablee_<[TiII/H]>[0.03/1.1]? Standard Deviation of <[TiII/H]>log(Sun)stat.error;phys.abundfloatnullableo_<[TiII/H]>[1/48]? Number of lines used in <[TiII/H]>meta.numberintnullable<[VI/H]>[-2.8/2.7]? Mean abundance of element [VI/H] relative to solarlog(Sun)phys.abundfloatnullablee_<[VI/H]>[0.01/1.3]? Standard Deviation of <[VI/H]>log(Sun)stat.error;phys.abundfloatnullableo_<[VI/H]>[1/69]? Number of lines used in <[VI/H]>meta.numberintnullable<[VII/H]>[-1.6/4]? Mean abundance of element [VII/H] relative to solarlog(Sun)phys.abundfloatnullablee_<[VII/H]>[0/2.1]? Standard Deviation of <[VII/H]>log(Sun)stat.error;phys.abundfloatnullableo_<[VII/H]>[1/11]? Number of lines used in <[VII/H]>meta.numberintnullable<[CrI/H]>[-2.6/1.8]? Mean abundance of element [CrI/H] relative to solarlog(Sun)phys.abundfloatnullablee_<[CrI/H]>[0.06/2]? Standard Deviation of <[CrI/H]>log(Sun)stat.error;phys.abundfloatnullableo_<[CrI/H]>[1/142]? Number of lines used in <[CrI/H]>meta.numberintnullable<[CrII/H]>[-2.32/3.68]? Mean abundance of element [CrII/H] relative to solarlog(Sun)phys.abundfloatnullablee_<[CrII/H]>[0.03/1.2]? Standard Deviation of <[CrII/H]>log(Sun)stat.error;phys.abundfloatnullableo_<[CrII/H]>[1/21]? Number of lines used in <[CrII/H]>meta.numberintnullable<[MnI/H]>[-2.7/1.9]? Mean abundance of element [MnI/H] relative to solarlog(Sun)phys.abundfloatnullablee_<[MnI/H]>[0.02/1.5]? Standard Deviation of <[MnI/H]>log(Sun)stat.error;phys.abundfloatnullableo_<[MnI/H]>[1/38]? Number of lines used in <[MnI/H]>meta.numberintnullable<[FeI/H]>[-2.4/1.1]? Mean abundance of element [FeI/H] relative to solarlog(Sun)phys.abundfloatnullablee_<[FeI/H]>[0.04/0.6]? Standard Deviation of <[FeI/H]>log(Sun)stat.error;phys.abundfloatnullableo_<[FeI/H]>[3/639]? Number of lines used in <[FeI/H]>meta.numberintnullable<[FeII/H]>[-2.3/4]? Mean abundance of element [FeII/H] relative to solarlog(Sun)phys.abundfloatnullablee_<[FeII/H]>[0.01/1.7]? Standard Deviation of <[FeII/H]>log(Sun)stat.error;phys.abundfloatnullableo_<[FeII/H]>[1/90]? Number of lines used in <[FeII/H]>meta.numberintnullable<[CoI/H]>[-1.9/2.1]? Mean abundance of element [CoI/H] relative to solarlog(Sun)phys.abundfloatnullablee_<[CoI/H]>[0.05/1.1]? Standard Deviation of <[CoI/H]>log(Sun)stat.error;phys.abundfloatnullableo_<[CoI/H]>[1/96]? Number of lines used in <[CoI/H]>meta.numberintnullable<[NiI/H]>[-2.2/1.8]? Mean abundance of element [NiI/H] relative to solarlog(Sun)phys.abundfloatnullablee_<[NiI/H]>[0.05/1]? Standard Deviation of <[NiI/H]>log(Sun)stat.error;phys.abundfloatnullableo_<[NiI/H]>[1/201]? Number of lines used in <[NiI/H]>meta.numberintnullable<[CuI/H]>[-2.1/1.7]? Mean abundance of element [CuI/H] relative to solarlog(Sun)phys.abundfloatnullablee_<[CuI/H]>[0/1]? Standard Deviation of <[CuI/H]>log(Sun)stat.error;phys.abundfloatnullableo_<[CuI/H]>[1/4]? Number of lines used in <[CuI/H]>meta.numberintnullable<[ZnI/H]>[-2.3/4]? Mean abundance of element [ZnI/H] relative to solarlog(Sun)phys.abundfloatnullablee_<[ZnI/H]>[0/1]? Standard Deviation of <[ZnI/H]>log(Sun)stat.error;phys.abundfloatnullableo_<[ZnI/H]>[1/4]? Number of lines used in <[ZnI/H]>meta.numberintnullable<[SrI/H]>[-1.7/2.7]? Mean abundance of element [SrI/H] relative to solarlog(Sun)phys.abundfloatnullablee_<[SrI/H]>[0/0.9]? Standard Deviation of <[SrI/H]>log(Sun)stat.error;phys.abundfloatnullableo_<[SrI/H]>[1/4]? Number of lines used in <[SrI/H]>meta.numberintnullable<[YI/H]>[-1.6/2.8]? Mean abundance of element [YI/H] relative to solarlog(Sun)phys.abundfloatnullablee_<[YI/H]>[0/2.1]? Standard Deviation of <[YI/H]>log(Sun)stat.error;phys.abundfloatnullableo_<[YI/H]>[1/13]? Number of lines used in <[YI/H]>meta.numberintnullable<[YII/H]>[-1.9/2.9]? Mean abundance of element [YII/H] relative to solarlog(Sun)phys.abundfloatnullablee_<[YII/H]>[0.03/1.4]? Standard Deviation of <[YII/H]>log(Sun)stat.error;phys.abundfloatnullableo_<[YII/H]>[1/18]? Number of lines used in <[YII/H]>meta.numberintnullable<[ZrI/H]>[-1.1/4.6]? Mean abundance of element [ZrI/H] relative to solarlog(Sun)phys.abundfloatnullablee_<[ZrI/H]>[0/1.4]? Standard Deviation of <[ZrI/H]>log(Sun)stat.error;phys.abundfloatnullableo_<[ZrI/H]>[1/20]? Number of lines used in <[ZrI/H]>meta.numberintnullable<[ZrII/H]>[-1.5/4]? Mean abundance of element [ZrII/H] relative to solarlog(Sun)phys.abundfloatnullablee_<[ZrII/H]>[0/1.6]? Standard deviation of <[ZrII/H]>log(Sun)stat.error;phys.abundfloatnullableo_<[ZrII/H]>[1/10]? Number of lines used in <[ZrII/H]>meta.numberintnullable<[BaII/H]>[-3.2/1.2]? Mean abundance of element [BaII/H] relative to solarlog(Sun)phys.abundfloatnullablee_<[BaII/H]>[0/0.8]? Standard Deviation of <[BaII/H]>log(Sun)stat.error;phys.abundfloatnullableo_<[BaII/H]>[1/4]? Number of lines used in <[BaII/H]>meta.numberintnullable<[LaII/H]>[-1.2/2.6]? Mean abundance of element [LaII/H] relative to solarlog(Sun)phys.abundfloatnullablee_<[LaII/H]>[0/1.4]? Standard Deviation of <[LaII/H]>log(Sun)stat.error;phys.abundfloatnullableo_<[LaII/H]>[1/12]? Number of lines used in <[LaII/H]>meta.numberintnullable<[CeII/H]>[-1.1/3.1]? Mean abundance of element [CeII/H] relative to solarlog(Sun)phys.abundfloatnullablee_<[CeII/H]>[0.01/2]? Standard Deviation of <[CeII/H]>log(Sun)stat.error;phys.abundfloatnullableo_<[CeII/H]>[1/38]? Number of lines used in <[CeII/H]>meta.numberintnullable<[PrII/H]>[-0.8/3.1]? Mean abundance of element [PrII/H] relative to solarlog(Sun)phys.abundfloatnullablee_<[PrII/H]>[0/1.5]? Standard Deviation of <[PrII/H]>log(Sun)stat.error;phys.abundfloatnullableo_<[PrII/H]>[1/8]? Number of lines used in <[PrII/H]>meta.numberintnullable<[NdII/H]>[-1/3.6]? Mean abundance of element [NdII/H] relative to solarlog(Sun)phys.abundfloatnullablee_<[NdII/H]>[0/2.9]? Standard Deviation of <[NdII/H]>log(Sun)stat.error;phys.abundfloatnullableo_<[NdII/H]>[1/53]? Number of lines used in <[NdII/H]>meta.numberintnullable<[SmII/H]>[-0.9/3.4]? Mean abundance of element [SmII/H] relative to solarlog(Sun)phys.abundfloatnullablee_<[SmII/H]>[0.01/1.7]? Standard Deviation of <[SmII/H]>log(Sun)stat.error;phys.abundfloatnullableo_<[SmII/H]>[1/35]? Number of lines used in <[SmII/H]>meta.numberintnullable<[EuI/H]>[-2.3/2.1]? Mean abundance of element [EuI/H] relative to solarlog(Sun)phys.abundfloatnullablee_<[EuI/H]>? Standard Deviation of <[EuI/H]>log(Sun)stat.error;phys.abundfloatnullableo_<[EuI/H]>[1/1]? Number of lines used in <[EuI/H]>meta.numberintnullable<[EuII/H]>[-1.6/3.22]? Mean abundance of element [EuII/H] relative to solarlog(Sun)phys.abundfloatnullablee_<[EuII/H]>[0/1.11]? Standard Deviation of <[EuII/H]>log(Sun)stat.error;phys.abundfloatnullableo_<[EuII/H]>[1/4]? Number of lines used in <[EuII/H]>meta.numberintnullable_RAPosition from SIMBAD database (right ascension part)degpos.eq.ra;meta.main_DEPosition from SIMBAD database (declination part)degpos.eq.dec;meta.mainJ/AJ/153/21/table1Program starsSimbadNameSimbad column added by the CDSmeta.idchare_plx[0.1/21.6]? Uncertainty in plx (1)masstat.error;pos.parallaxfloatnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameName of the primary starmeta.id;meta.maincharAllDisplay the data from all the tables (tables 1-5 and 7)meta.ref.urlcharHDH. Draper identifier (1)meta.idcharHIP? Hipparcos catalogue identifier (Cat. I/239) (1)meta.idintnullableHR? The Bright Star Catalogue identifier (1)meta.idintnullableCCDMIdentifier in the Catalog of Double and Multiple Stars (Dommanget et al. 2002, Cat. I/274) (1)meta.idcharm_CCDMCCDM component (either A, AB, AD, B, C, or CD)meta.code.multipcharSpTSpectral Type (1)src.spTypecharplx[4.2/311]? Parallax (1)maspos.parallaxfloatnullableVmag[0.3/10.9]? Johnson V band apparent magnitude (1)magphot.mag;em.opt.VfloatnullableDist[3.2/234.2]? Distancepcpos.distance;pos.heliocentricfloatnullableE(B-V)[0/0.03]? B-V color excess (2)magphot.color.excessfloatnullableVMag[0.75/11.9]? Johnson V band absolute magnitudemagphys.magAbsfloatnullableHost[H] Planet host status (H=known host) (3)meta.codechar_RAPosition from SIMBAD database (right ascension part)degpos.eq.ra;meta.main_DEPosition from SIMBAD database (declination part)degpos.eq.dec;meta.mainJ/AJ/153/21/table2Temperature, luminosity, mass, age, and gravitySimbadNameSimbad column added by the CDSmeta.idcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameName of the primary starmeta.id;meta.maincharAllDisplay the data from all the tables (tables 1-5 and 7)meta.ref.urlcharSce[EHS] Source for spectroscopic material (E=ELODIE, H=HET, or S=Sandiford) (G1)meta.codecharTeff[3644/7671]? Effective TemperatureKphys.temperature.effectiveintnullablee_Teff[2/333]? Standard deviation of the effective temperatureKstat.error;phys.temperature.effectiveintnullableo_Teff[1/12]? Number of colors used in the effective temperature determinationmeta.numberintnullablelogL[-2.42/1.61] Luminosity (logL/L_{Sun}_)log(solLum)phys.luminosityfloatB1Mass[0.6/2.05]? Mass, determined from the Bertelli et al. 1994 (Cat. J/A+AS/106/275) isochronessolMassphys.massfloatnullableB1Age[0.63/12.02]? Age, determined from the Bertelli et al. 1994 (Cat. J/A+AS/106/275) isochronesGyrtime.agefloatnullableDMass[0.48/2.08]? Mass, determined from the Dotter et al. 2008ApJS..178...89D isochronessolMassphys.massfloatnullableDAge[0.55/12.5]? Age, determined from the Dotter et al. 2008ApJS..178...89D isochronesGyrtime.agefloatnullableYMass[0.39/2.16]? Mass, determined from the Demarque et al. 2004ApJS..155..667D isochronessolMassphys.massfloatnullableYAge[0.6/12]? Age, determined from the Demarque et al. 2004ApJS..155..667D isochronesGyrtime.agefloatnullableB2Mass[0.5/2.2]? Mass, determined from the BaSTI Team (2016, BaSTI Ver. 5.0.1: http://basti.oa-teramo.inaf.it/) isochrones (1)solMassphys.massfloatnullableB2Age[0.6/12.5]? Age, determined from the BaSTI Team (2016, BaSTI Ver. 5.0.1: http://basti.oa-teramo.inaf.it/) isochrones (1)Gyrtime.agefloatnullable<Mass>[0.39/2.1]? Average masssolMassphys.massfloatnullableMRange[0/0.75]? Range in mass determinationsolMassphys.massfloatnullable<Age>[0.58/12.5]? Average ageGyrtime.age;stat.meanfloatnullableARange[0/11.45]? Range in age determinationGyrtime.agefloatnullablelogg[3.08/6.88] Log surface gravity (2)log(cm.s**-2)phys.gravityfloat_RAPosition from SIMBAD database (right ascension part)degpos.eq.ra;meta.main_DEPosition from SIMBAD database (declination part)degpos.eq.dec;meta.main