J/A+A/526/A71ivo://CDS.VizieR/J/A+A/526/A71doi:10.26093/cds/vizier.35260071CDSda Silva R.Milone A.Reddy B.E.2017-12-06T07:38:53Z2010-12-23T08:57:16ZCDS support team

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

cds-question@unistra.frstellar-atmosphereschemical-abundancesatomic-physicsWe present a determination of photospheric parameters and carbon abundances for a sample of 172 G and K dwarf, subgiant, and giant stars with and without detected planets in the solar neighbourhood. The analysis was based on high signal-to-noise ratio and high resolution spectra observed with the ELODIE spectrograph (Haute Provence Observatory, France) and for which the observational data were publicly available. We intend to contribute precise and homogeneous C abundances in studies that compare the behaviour of light elements in stars with and without planets. This will bring new arguments to the discussion of possible anomalies that have been suggested and will contribute to a better understanding of different planetary formation process.2011A&A...526A..71Dhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/526/A71CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/526/A71https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/526/A71http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/526/A71https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/526/A71https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/526/A71http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/526/A71GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/526/A71/cfe_3reg ([C/Fe] abundances and errors for the three C abundance indicators: 5128, 5165, and 5380 {AA} (table 7 of the paper))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/526/A71/cfe_3reg?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/526/A71/cfe_3reg?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/526/A71/cfe_3reg?GETtext/xml+votable180.050000true175.196113921.35272920.0055555555555555566/210 309 322 327 341 377 428 587 684 737 742 915 944 1249 1452 1819 1960 2014 2167 2324 2433 2440 2472 2476 2541 3020 3026 3094 3313 3335 3619 3639 3755 3979 4051 4227 4969 5059 5522 5726 5815 6203 6219 6361 6385 6827 6933 7113 7177 7320 7763 8080 8626 8845 9061 9213 9219 9337 9403 9610 9753 9835 10256 10354 10632 10817 10899 11473 11659 11734-11735 12337 12592 12644 12792 12890 13158 13282 13333 13487 13643 13749 13778 13791 14005 14220 14290 14329 14534 14604 14630 14650 14693 14767 15174 15363 15597 15715 15727 16023 16031 16035 16056 16069 16213 17171 17219 17606 17731 17764 17847 17852 17860 18915 19237 19868 19912 20145 20308 20402 20893 20973 21423 21484 21612 21940 22157 22199 22330 22360 22878 22932 23190 23230 23533 23538 23547-23548 23575 23661 23695 23843 24151 24262 24558 25571 25608 26562 26575 26704 27386 27752 28104 28276 28436 29712 30339 30576 30665 30878 31204 31399 31416 31433 32067 32328 32348 32575 32645 40644 40932 49114https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/526/A71?format=asciidefaultJ/A+A/526/A71/cfe_3reg[C/Fe] abundances and errors for the three C abundance indicators: 5128, 5165, and 5380 {AA} (table 7 of the paper)HDHD stellar numbermeta.id;meta.mainintrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintm_HD[A] Multiplicity index on HDmeta.code.multipcharCFe5128? Abundance ratio [C/Fe] from the 5128 regionphys.abund;arith.ratiofloatnullablee_CFe5128? Error in [C/Fe] from the 5128 regionstat.errorfloatnullableCFe5165? Abundance ratio [C/Fe] from the 5165 regionphys.abund;arith.ratiofloatnullablee_CFe5165? Error in [C/Fe] from the 5165 regionstat.errorfloatnullableCFe5380? Abundance ratio [C/Fe] from the 5380 linephys.abund;arith.ratiofloatnullablee_CFe5380? Error in [C/Fe] from the 5380 linestat.errorfloatnullableSimbadSimbad 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/A+A/526/A71/atm_molAtomic and molecular line parameters (table 2 of the paper)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlambdaSpectral line wavelength0.1nmem.wl;spect.linedoubleIonAtomic and molecular line identification (606 stands for C_2_, 112 for MgH)phys.atmol.ionStagefloatchiExcitation potentialeVphys.atmol.excitationfloatgfOscillator strengthphys.atmol.oscStrengthdoubleD0? Dissociation energy for molecular featureseVphys.energy;phys.mol.dissociationfloatnullableJ/A+A/526/A71/atm_strgStrong atomic lines (table 3 of the paper)gfOscillator strengthphys.atmol.oscStrengthdoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlambdaSpectral line wavelength0.1nmem.wl;spect.linedoubleIonAtomic and molecular line identificationphys.atmol.ionStagefloatchiExcitation potentialeVphys.atmol.excitationfloat