J/A+A/497/563ivo://CDS.VizieR/J/A+A/497/563doi:10.26093/cds/vizier.34970563CDSNeves V.Santos N.C.Sousa S.G.Correia A.C.M.Israelian G.2017-06-30T05:49:02Z2010-01-19T10:02:44ZCDS support team

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

cds-question@unistra.frsolar-system-planetschemically-peculiar-starsWe present a uniform study of the chemical abundances of 12 elements (Si, Ca, Sc, Ti, V, Cr, Mn, Co, Ni, Na, Mg, and Al) derived from the spectra of 451 stars observed as part of one of the HARPS GTO planet search programs. Sixty eight of these are planet-bearing stars. The main goals of our work are: i) the investigation of possible differences between the abundances of stars with and without planets; ii) the study of the possible differences in the abundances of stars in the thin and the thick disc. We confirm that there is a systematically higher metallicity in planet host stars, when compared to non planet-hosts, common to all studied species. We also found that there is no difference in the galactic chemical evolution trends of the stars with and without planets. Stars that harbour planetary companions simply appear to be in the high metallicity tail of the distribution. We also confirm that Neptunian and super-Earth class planets may be easier to find at lower metallicities. A statistically significative abundance difference between stars of the thin and the thick disc was found for [Fe/H]<0. However, the populations from the thick and the thin disc cannot be clearly separated.2009A&A...497..563Nhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/497/563CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/A+A/275/101 : Chemical evolution of Galactic disk I. (Edvardsson+ 1993)J/A+AS/102/603 : Chemical evolution of Galactic disk II. (Edvardsson+ 1993)J/A+A/392/491 : Galactic abundance gradient. III. (Andrievsky+, 2002)J/A+A/410/527 : Abundances in the Galactic disk (Bensby+, 2003)J/A+A/413/159 : Galactic abundance gradient. V. (Andrievsky+, 2004)J/A+A/418/551 : Galactic disk stars abund. & velocities (Mishenina+, 2004)J/AJ/128/1177 : Galactic stellar abundances (Venn+, 2004)J/MNRAS/367/1329 : Elemental abundances for 176 stars (Reddy+, 2006)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/497/563https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/497/563http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/497/563https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/497/563https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/497/563http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/497/563GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/497/563/stars (Parameters related to Galactic population of the studied stars, and their abundances)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/497/563/stars?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/497/563/stars?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/497/563/stars?GETtext/xml+votable180.050000true1.3236989-67.83258970.0055555555555555566/12644 16502 16518 16528 16543 16603 16639 16652 16883 16890 16986 17177 17218 17249 17266 17314 17341 17419 17425 17435 17453 17496 17529 17540 17641 17671 17714 17730 17768 17804 17944 17954 17993 18005 18466 18548 18614-18615 18637 18641 18711 18785 18792 18838 19003 19072 19108 20557 20593 20621 20640 20746 20766 20873 21066 21080 21117 21121 21211 21400 21412 21477 21484 21516 21691 21779 21906 21912 22036 22159 22590 22608 22613 22619 22708 22746 22813 23061 23096 23123 23177 23201 24729 24769 24816 24831 24924 25078 25102 25225 25512 25567 25584 25622 25862 25880 25889 25906 25939 26183 26242 26652 26768 26796 26828 26888 26901 26906 27018 27040 28719 28763 28874 28887 28894 28961 29289 29349 29513 29563 29675 29756 29833 29838 29842 29900 30310 30343 30789 30848 30862 30878 30943 30951 31011 31015 31029 31254 31393 32787 32848 32912 32930 32986 33063 33082 33091 33179 33210 33214 33219 33243 33357 33418 33430 33442 33456 33510 33552 33608 33630 33662 33705 33717 33813 33879 33945 34064 34172 34336 34408 34442 34446 34515-34516 34530 34577 34612 34673 34817 34864 34905 34947 34953 34983 35017 35121 35228 35230 35291 35362 35440 35468 35691 35733 35776 35781 35784 35786 35790 35831 35896 35928 35954 35968-35969 36008 36015 36019 36089 36115 36288 36418 36541 36590 36635 36693 36697 36723 36800 36813 37018 37074 37208 37357 37419 37422 37573 37595 37660 37807-37808 37831 37954-37955 38099 38219 38229 38238 38279 38311 38339 38414 38434 38443 38461 38521 38545 38562 38605 38698 38728 38738 38742 38788 38807 38836 38857 38870 38955 38975 38998 39034 39219 39257 39282-39283 39364 39377 39422 39461 39576 39767 39854 39915 40007 40078 40101 40105 40302 40317 40442 40453 40514 40686-40687 40692 40722 40802 40921 40932 40938 40970 40985 41058 41094 41143 41204 41463 41521 41590 41607 41611-41612 41687 41723-41724 41752 41861 41912 41941 41954 41969 42022 42146 42171 42248 42318 42326 42333 42448 42460 42510 42595 42700 42760 42814 42845 42918 43012 43228 43258 43290 43345 43544 43577 43639 43649 43676 43724 43813 43818 43911 43928 43977 44005 44115 44131 44150-44151 44243 44262 44355 44359 44398 44792 44879 45121 45143 45168 45182 45228 45237 45245 45265 45299 45309 45334 45337 45386 45412 45502 45511 45564 45589 45627 45641 45668-45669 45717 45823 45853 45865 45892 45902 46019 46076 46080 46111-46112 46135 46172 46193 46234 46247 46271 46287 46297 46306 46355 46640 46664 46681 46768 46800 46874 46944 46967 46983 46997 47020 47022 47045 47077 47198 47253 47364 47390 47567 47575 47590 47629 47740 47780 47858 47898 47903 48105 48172 48362 48519 48530 48545 48583 48607 48652 48664 48705 48792 48821 48846 48943 49060 49064 49114 49128https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/497/563?format=asciidefaultJ/A+A/497/563/starsParameters related to Galactic population of the studied stars, and their abundancesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintStarHD or HIP name of the starmeta.id;meta.mainchar[Si/H]Abundance [Si/H] (Z=14)log(Sun)phys.abundfloate_[Si/H]rms uncertainty of [Si/H]log(Sun)stat.error;phys.abundfloato_[Si/H]Number of SiI lines usedmeta.numberint[Ca/H]Abundance [Ca/H] (Z=20)log(Sun)phys.abundfloate_[Ca/H]rms uncertainty of [Ca/H]log(Sun)stat.error;phys.abundfloato_[Ca/H]Number of CaI lines usedmeta.numberint[ScI/H]Abundance [ScI/H] (Z=21.0)log(Sun)phys.abundfloate_[ScI/H]rms uncertainty of [ScI/H]log(Sun)stat.error;phys.abundfloato_[ScI/H]Number of ScI lines usedmeta.numberint[ScII/H]Abundance [ScII/H] (Z=21.1)log(Sun)phys.abundfloate_[ScII/H]rms uncertainty of [ScII/H]log(Sun)stat.error;phys.abundfloato_[ScII/H]Number of ScII lines usedmeta.numberint[TiI/H]Abundance [TiI/H] (Z=22.0)log(Sun)phys.abundfloate_[TiI/H]rms uncertainty of [TiI/H]log(Sun)stat.error;phys.abundfloato_[TiI/H]Number of TiI lines usedmeta.numberint[TiII/H]Abundance [TiII/H] (Z=22.1)log(Sun)phys.abundfloate_[TiII/H]rms uncertainty of [TiII/H]log(Sun)stat.error;phys.abundfloato_[TiII/H]Number of TiII lines usedmeta.numberint[V/H]Abundance [V/H] (Z=23)log(Sun)phys.abundfloate_[V/H]rms uncertainty of [V/H]log(Sun)stat.error;phys.abundfloato_[V/H]Number of VI lines usedmeta.numberint[CrI/H]Abundance [CrI/H] (Z=24.0)log(Sun)phys.abundfloate_[CrI/H]rms uncertainty of [CrI/H]log(Sun)stat.error;phys.abundfloato_[CrI/H]Number of CrI lines usedmeta.numberint[CrII/H]Abundance [CrII/H] (Z=24.1)log(Sun)phys.abundfloate_[CrII/H]rms uncertainty of [CrII/H]log(Sun)stat.error;phys.abundfloato_[CrII/H]Number of CrII lines usedmeta.numberint[Mn/H]Abundance [Mn/H] (Z=25)log(Sun)phys.abundfloate_[Mn/H]rms uncertainty of [Mn/H]log(Sun)stat.error;phys.abundfloato_[Mn/H]Number of MnI lines usedmeta.numberint[Co/H]Abundance [Co/H] (Z=27)log(Sun)phys.abundfloate_[Co/H]rms uncertainty of [Co/H]log(Sun)stat.error;phys.abundfloato_[Co/H]Number of CoI lines usedmeta.numberint[Ni/H]Abundance [Ni/H] (Z=28)log(Sun)phys.abundfloate_[Ni/H]rms uncertainty of [Ni/H]log(Sun)stat.error;phys.abundfloato_[Ni/H]Number of NiI lines usedmeta.numberint[Na/H]Abundance [Na/H] (Z=11)log(Sun)phys.abundfloate_[Na/H]rms uncertainty of [Na/H]log(Sun)stat.error;phys.abundfloato_[Na/H]Number of Na lines usedmeta.numberint[Mg/H]Abundance [Mg/H] (Z=12)log(Sun)phys.abundfloate_[Mg/H]rms uncertainty of [Mg/H]log(Sun)stat.error;phys.abundfloato_[Mg/H]Number of MgI lines usedmeta.numberint[Al/H]Abundance [Al/H] (Z=13)log(Sun)phys.abundfloate_[Al/H]rms uncertainty of [Al/H]log(Sun)stat.error;phys.abundfloato_[Al/H]Number of AlI lines usedmeta.numberintUlsrU velocity of the star relative to the LSR (1)km/sphys.veloc;pos.cartesian.xdoubleVlsrV velocity of the star relative to the LSR (1)km/sphys.veloc;pos.cartesian.ydoubleWlsrW velocity of the star relative to the LSR (1)km/sphys.veloc;pos.cartesian.zdoublefDDistribution of the thin disc population (2)stat.paramdoublefTDDistribution of the thick disc population (2)stat.paramdoublefHDistribution of the halo population (2)stat.paramdoubleTDDProbability of a star belonging to the thick disc relative to the thin diskstat.probabilitydoubleTDHProbability of a star belonging to the thick disc relative to the halostat.probabilitydoublepopprobable population where the star belongsmeta.idcharSimbadSimbad column added by the CDSchar_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/497/563/table2Atomic parameters for lines selected in the paperrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintElElement (1)phys.atmol.elementcharlambdaCentral wavelength0.1nmem.wl.centralfloatEPExcitation potentialphys.atmol.excitationfloatloggfOscilator strengthphys.atmol.collStrengthfloatEWsunSolar equivalent width0.1pmspect.line.eqWidthfloat