J/A+A/624/A19ivo://CDS.VizieR/J/A+A/624/A19doi:10.26093/cds/vizier.36240019CDSBuder S.Lind K.Ness M.K.Asplund M.Duong L.Lin J.Kos J.,Casagrande L.Casey A.R.Bland-Hawthorn J.De Silva G.M.D'Orazi V.,Freeman K.C.Martell S.L.Schlesinger K.J.Sharma S.Simpson J.D.,Zucker D.B.Zwitter T.Cotar K.Dotter A.Hayden M.R.Hyde E.A.,Kafle P.R.Lewis G.F.Nataf D.M.Nordlander T.Reid W.Rix H.-W.,Skuladottir A.Stello D.Ting Y.-S.Traven G.Wyse R.F.G.,GALAH collaboration2021-01-08T16:41:12Z2019-04-02T08:37:32ZCDS support team

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

cds-question@unistra.frsurveyschemical-abundancesphotometryThe overlap between the spectroscopic Galactic Archaeology with HERMES (GALAH) survey and Gaia provides a high-dimensional chemodynamical space of unprecedented size. We present a first analysis of a subset of this overlap, of 7066 turn-off, and sub-giant stars. These stars have spectra from the GALAH survey and high parallax precision from the Gaia DR1 Tycho-Gaia Astrometric Solution. We investigate correlations between chemical compositions, ages, and kinematics for this sample. Stellar parameters and elemental abundances are derived from the GALAH spectra with the spectral synthesis code Spectroscopy Made Easy. We determine kinematics and dynamics, including action angles, from the Gaia astrometry and GALAH radial velocities. Stellar masses and ages are determined with Bayesian isochrone matching, using our derived stellar parameters and absolute magnitudes. We report measurements of Li, C, O, Na, Mg, Al, Si, K, Ca, Sc, Ti, V, Cr, Mn, Co, Ni, Cu, Zn, Y, as well as Ba and we note that we have employed non-LTE calculations for Li, O, Al, and Fe. We show that the use of astrometric and photometric data improves the accuracy of the derived spectroscopic parameters, especially log g. Focusing our investigation on the correlations between stellar age, iron abundance [Fe/H], and mean alpha-enhancement [{alpha}/Fe] of the magnitude-selected sample, we recover the result that stars of the high-{alpha} sequence are typically older than stars in the low-{alpha} sequence, the latter spanning iron abundances of -0.7<[Fe/H]<+0.5. While these two sequences become indistinguishable in [{alpha}/Fe] vs. [Fe/H] at the metal-rich regime, we find that age can be used to separate stars from the extended high-alpha and the low-alpha sequence even in this regime. When dissecting the sample by stellar age, we find that the old stars (>8Gyr) have lower angular momenta L_z_ than the Sun, which implies that they are on eccentric orbits and originate from the inner disc. Contrary to some previous smaller scale studies we find a continuous evolution in the high-alpha-sequence up to super-solar [Fe/H] rather than a gap, which has been interpreted as a separate 'high-alpha metal-rich' population. Stars in our sample that are younger than 10Gyr, are mainly found on the low alpha-sequence and show a gradient in L_z_ from low [Fe/H] (L_z_>L_z,{sun}_) towards higher [Fe/H] (L_z_<L_z,{sun}_), which implies that the stars at the ends of this sequence are likely not originating from the close solar vicinity.2019A&A...624A..19Bhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/624/A19CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toI/337 : Gaia DR1 (Gaia Collaboration, 2016)II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)II/336 : AAVSO Photometric All Sky Survey (APASS) DR9 (Henden+, 2016)II/328 : AllWISE Data Release (Cutri+ 2013)J/ApJ/833/119 : Distances of Gaia DR1 TGAS sources (Astraatmadja+, 2016)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/624/A19https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/624/A19http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/624/A19https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/624/A19https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/624/A19http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/624/A19GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/624/A19/catalog (Chemo-dymamical catalog)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/624/A19/catalog?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/624/A19/catalog?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/624/A19/catalog?GETtext/xml+votable180.050000true0.03408306-77.298308890.0055555555555555565/70 88 94 101 1173 4503 4556 4583 4612 4624 4642 5187 5277 5472 5519 5604 5687 5723 5871 6394 6401 6428 6431 6436 6439 6725 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39690 39712 39714 39808 39819 39822 39841-39844 39846 39848-39850 39852 39959 39965 39967 39989 39991 39997 40002-40003 40008-40009 40012-40014 40020 40024 40027 40034 40037-40039 40045 40087 40093 40117 40119 40125 40128-40130 40136 40160 40162-40163 40168 40206 40251 40337-40338 40343 40349 40403 40709 40997-40998 41011 41021 41042-41043 41048-41049 41051 41053-41055 41063-41064 41069-41071 41074-41075 41080-41082 41111-41113 41127 41138 41142-41143 41157-41158 41163-41164 41166-41167 41181-41182 41193-41194 41226 41235 41257-41260 41262 41265-41268 41274-41275 41277-41278 41280-41281 41283 41286 41288-41289 41291-41293 41295 41303-41304 41306 41311 41320 41322-41323 41332 41342-41345 41348 41350-41352 41354-41355 41357 41359 41361-41363 41408-41410 41412 41479 41486-41487 41492 41984-41985 41988-41990 42002 42011 42033 42040 42054 42058 42060-42061 42074-42075 42085 42096-42097 42240 42248 42253 42264 42304 42306 42619 42642 42646 42656-42657 42659 42661 42663-42665 42669-42671 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43748 43765 43783 43785 43787-43789 43796-43797 43799-43800 43808 43817 43819 43824 43826-43827 43832 43840 43842 43849-43852 43916 43934 44023 44029 44036-44037 44171 44174 44242 44300 44305 44307-44308 44310-44311 44317 44319 44351 44353-44358 44360-44362 44365 44367 44373-44376 44378 44380 44383 44385 44387 44393-44394 44403 44412-44413 44480 44491 44494 44554-44555 44577 44624 44637-44639 44676 44678-44679 44688-44690 44718-44719 44722-44723 44750-44751 44770-44773 44776-44777 44779 44810 44865 45124-45125 45127 45136-45137 45140 45143-45145 45147-45148 45150 45157 45180-45181 45183 45202 45206 45209 45211 45213 45215 45256 45258 45312-45313 45324 45326-45327 45329-45331 45336-45337 45339 45346-45347 45349 45365-45367 45410-45411 45414 45420-45422 45432 45440-45441 45444-45445 45461 45469-45471 45477 45479 45488-45490 45492-45493 45506 45510 45512-45514 45539-45540 45542-45543 45545 45548 45550-45551 45559 45563-45565 45567 45615 45660-45662 45696 45698 45700 45707 45741 45746 45754-45755 45830 45833 45835-45836 45847 45858 45885 45900-45901 45920 45922 45928 45952-45953 45955-45956 45976-45977 45979 46023 46029 46031 46040 46042 46053 46055 46061 46064 46066 46242 46248 46250 46592 46594 46628 46630 46632-46633 46649-46651 46654 46736 46745 46747-46748 46750 46753-46755 46758 46760-46761 46764 46769 46786 47104 47116 47119-47120 47159 47174-47175 47181 47200-47202 47226 47239 47253 47255 47258-47259 47261 47268 47279-47281 47283-47284 47288-47290 47301 47309 47314 47325 47336 47338 47345 47347 47353-47356 47383 47389 47393 47395-47396 47398 47401 47406-47407 47417 47419 47426-47427 47430 47432-47433 47436 47443 47459-47460 47462 47478 47481-47484 47490 47492 47496-47497 47501 47503 47509-47512 47515 47517-47518 47537 47539 47554 47566 47568 47584-47585 47592-47594 47611-47612 47614-47615 47621-47622 47631-47632 47643 47653 47655-47656 47659 47665 47675 47682 47691 47694 47713-47716 47719-47721 47725 47736 47745 47762 47764 47774-47775 47777-47780 47784-47785 47793 47796-47797 47841 47870-47871 47956 48028-48029 48031-48032 48058-48059 48065 48067-48068 48070-48071 48078-48079 48086 48089-48094 48100-48101 48103 48108-48109 48112 48127 48153-48155 48163 48166-48169 48171-48173 48176-48178 48184 48266-48267 48289 48306 48310-48312 48440 48500-48501 48503 48511 48605 48676 48678 48810 488958.157980699529898e-21 4.920466254354166e-19https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/624/A19?format=asciidefaultJ/A+A/624/A19/catalogChemo-dymamical catalogrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSourceIdGaia DR1 identifier (source_id) (1)meta.id2MASS2MASS identifier (tmass_id) (2)meta.idcharGALAHGALAH spectrum identifier (sobject_id)meta.id;meta.mainRAICRSRight Ascension (ICRS,Epoch=J2000) (ra)degpos.eq.ra;meta.mainDEICRSDeclination (ICRS,Epoch=J2000) (dec)degpos.eq.dec;meta.mainsnrc1S/N per pixel for ccd-1 (blue channel) (snr_c1)stat.snrdoublesnrc2S/N per pixel for ccd-2 (green channel) (snr_c2)stat.snrdoublesnrc3S/N per pixel for ccd-3 (red channel) (snr_c3)stat.snrdoublesnrc4S/N per pixel for ccd-4 (IR channel) (snr_c4)stat.snrdoubleBmag? APASS B magnitude (Bmag) (3)magphot.mag;em.opt.Bfloatnullablee_Bmag? Uncertainty in APASS Bmag (e_Bmag) (3)magstat.error;phot.magdoublenullableVmag? APASS V magnitude (Vmag) (3)magphot.mag;em.opt.Vfloatnullablee_Vmag? Uncertainty in APASS Vmag (e_Vmag) (3)magstat.error;phot.magdoublenullableJmag2MASS J magnitude (Jmag) (2)magphot.mag;em.IR.Jfloate_Jmag? Uncertainty in 2MASS Jmag (e_Jmag) (2)magstat.error;phot.magfloatnullableHmag2MASS H magnitude (Hmag) (2)magphot.mag;em.IR.Hfloate_HmagUncertainty in 2MASS Hmag (e_Hmag) (2)magstat.error;phot.magfloatKmag2MASS Ks magnitude (Kmag) (2)magphot.mag;em.IR.Kfloate_KmagUncertainty in 2MASS Kmag (e_Kmag) (2)magstat.error;phot.magfloatQflQuality flag 2MASS (Qfl) (2)meta.code.qualcharW1mag? WISE W1 magnitude (W1mag) (4)magphot.mag;em.IR.3-4umfloatnullablee_W1mag? Uncertainty in WISE W1 mag (e_W1mag) (4)magstat.error;phot.magfloatnullableW2mag? WISE W2 magnitude (W2mag) (4)magphot.mag;em.IR.4-8umfloatnullablee_W2mag? Uncertainty in WISE W2 mag (e_W2mag) (4)magstat.error;phot.magfloatnullableW3mag? WISE W3 magnitude (W3mag) (4)magphot.flux.density;em.IR.8-15umfloatnullablee_W3mag? Uncertainty in WISE W3 mag (e_W3mag) (4)magstat.error;phot.magfloatnullableW4mag? WISE W4 magnitude (W4mag) (4)magphot.flux.density;em.IR.15-30umfloatnullablee_W4mag? Uncertainty in WISE W4 mag (e_W4mag) (4)magstat.error;phot.magfloatnullableE(B-V)Reddening E(B-V) (ebv) (5)magphot.color.excessdoubleAKAttenuation in Ks (A_K)magphot.mag;em.IR.Kdoublee_AKUncertainty in attenuation in Ks (e_A_K)magstat.errordoubleBCKBolometric corrections for Ks (BC_K)magphot.mag.bcdoubleplxParallax (parallax) (1)maspos.parallax.trigfloate_plxParallax error (parallax_error) (1)masstat.error;pos.parallaxfloatpmRAProper motion in Right Ascension (pmra) (1)mas/yrpos.pm;pos.eq.radoublee_pmRA? Proper motion error in RA (pmra_error) (1)mas/yrstat.error;pos.pm;pos.eq.rafloatnullablepmDEProper motion in Declination (pmdec) (1)mas/yrpos.pm;pos.eq.decdoublee_pmDE? Proper motion error in Dec (pmdec_error) (1)mas/yrstat.error;pos.pm;pos.eq.decfloatnullablerMo3Mode distance of the posterior, using Milky Way Prior (rMo_3) (6)pcpos.distancedoubler53? 5th percentile of the posterior, using Milky Way Prior (r5_3) (6)pcstat.errordoublenullabler50350th percentile of the posterior, using Milky Way Prior (r50_3) (6)pcstat.errordoubler953? 95th percentile of the posterior, using Milky Way Prior (r95_3) (6)pcstat.errordoublenullablesigmaR3? Distance standard error, using Milky Way Prior (sigmaR_3) (6)pcstat.errordoublenullablecombsp[1/3] Spectra used for the combination of stellar parameters (Nsp)meta.numberintTeffEffective temperature T_eff (teff_sme)Kphys.temperature.effectivedoublee_TeffUncertainty in teff_sme (e_teff_sme)Kstat.error;phys.temperature.effectivefloatloggSurface gravity logg (logg_sme)log(cm.s**-1)phys.gravitydoublee_loggUncertainty in surface gravity logg (e_logg_sme)log(cm.s**-1)stat.errordouble[Fe/H]SME pseudo iron abundance [Fe/H] (feh_sme)phys.abund.Fedoublee_[Fe/H]Uncertainty in feh_sme (e_feh_sme)stat.error;phys.abund.FedoublevmicMicroturbulence velocity xi (vmic_sme)km/sphys.veloc.microTurbdoublee_vmic? Uncertainty of vmic_sme (e_vmic_sme)km/sstat.errordoublenullablevsiniRotational and macroturbulence velocity v_{mac+rot} (vsini_sme)km/sphys.veloc.rotatdoublee_vsini? Uncertainty of v_{mac+rot} (e_vsini_sme)km/sstat.error;phys.veloc.rotatdoublenullableRVRadial velocity (rv_sme)km/sphys.veloc;pos.heliocentricdoublee_RVUncertainty of radial velocity (e_rv_sme)km/sstat.errordoubleChi? chi^2^ of the spectroscopic stellar parameter fit (chisme)stat.fit.chi2;stat.fit.param;meta.modelleddoublenullableFlag? Spectroscopic quality flag (f_sme)meta.code.errordoublenullable[alpha/Fe]? Combined [alpha/Fe] (alpha_fe_sme)phys.abunddoublenullablee_[alpha/Fe]? Uncertainty of [alpha/Fe] (e_alpha_fe_sme)stat.error;phys.abunddoublenullableLiAbund? Abundance [X/Fe] of element X (li_abund_sme)phys.abunddoublenullablee_LiAbund? Uncertainty of x_abund_sme (e_li_abund_sme)stat.errordoublenullablechiLiAbund? chi^2^ of abundance fit for element X (chi_li_abund_sme)stat.fit.chi2;stat.fit.param;meta.modelleddoublenullablef_LiAbund? Spectroscopic quality flag for abundance of X (flag_li_abund_sme)meta.codedoublenullableo_LiAbund[0/3] Number of spectra used to estimate x_abund_sme (comb_li_abund_sme)meta.numberdoubleCAbund? Abundance [X/Fe] of element X (c_abund_sme)phys.abunddoublenullablee_CAbund? Uncertainty of x_abund_sme (e_c_abund_sme)stat.errordoublenullablechiCAbund? chi^2^ of abundance fit for element X (chi_c_abund_sme)stat.fit.chi2;stat.fit.param;meta.modelleddoublenullablef_CAbund? Spectroscopic quality flag for abundance of X (flag_c_abund_sme)meta.codedoublenullableo_CAbund[0/3] Number of spectra used to estimate x_abund_sme (comb_c_abund_sme)meta.numberdoubleOAbund? Abundance [X/Fe] of element X (o_abund_sme)phys.abunddoublenullableOAbundLTE? LTE ? Abundance [X/Fe] of element X (o_abund_sme_lte)phys.abunddoublenullablee_OAbund? Uncertainty of x_abund_sme (e_o_abund_sme)stat.errordoublenullablechiOAbund? chi^2^ of abundance fit for element X (chi_o_abund_sme)stat.fit.chi2;stat.fit.param;meta.modelleddoublenullablef_OAbund? Spectroscopic quality flag for abundance of X (flag_o_abund_sme)meta.codedoublenullableo_OAbund[0/3] Number of spectra used to estimate x_abund_sme (comb_o_abund_sme)meta.numberdoubleNaAbund? Abundance [X/Fe] of element X (na_abund_sme)phys.abunddoublenullablee_NaAbund? Uncertainty of x_abund_sme (e_na_abund_sme)stat.errordoublenullablechiNaAbund? chi^2^ of abundance fit for element X (chi_na_abund_sme)stat.fit.chi2;stat.fit.param;meta.modelleddoublenullablef_NaAbund? Spectroscopic quality flag for abundance of X (flag_na_abund_sme)meta.codedoublenullableo_NaAbund[0/3] Number of spectra used to estimate x_abund_sme (comb_na_abund_sme)meta.numberdoubleMgAbund? Abundance [X/Fe] of element X (mg_abund_sme)phys.abunddoublenullablee_MgAbund? Uncertainty of x_abund_sme (e_mg_abund_sme)stat.errordoublenullablechiMgAbund? chi^2^ of abundance fit for element X (chi_mg_abund_sme)stat.fit.chi2;stat.fit.param;meta.modelleddoublenullablef_MgAbund? Spectroscopic quality flag for abundance of X (flag_mg_abund_sme)meta.codedoublenullableo_MgAbund[0/3] Number of spectra used to estimate x_abund_sme (comb_mg_abund_sme)meta.numberdoubleAlAbund? Abundance [X/Fe] of element X (al_abund_sme)phys.abunddoublenullablee_AlAbund? Uncertainty of x_abund_sme (e_al_abund_sme)stat.errordoublenullablechiAlAbund? chi^2^ of abundance fit for element X (chi_al_abund_sme)stat.fit.chi2;stat.fit.param;meta.modelleddoublenullablef_AlAbund? Spectroscopic quality flag for abundance of X (flag_al_abund_sme)meta.codedoublenullableo_AlAbund[0/3] Number of spectra used to estimate x_abund_sme (comb_al_abund_sme)meta.numberdoubleSiAbund? Abundance [X/Fe] of element X (si_abund_sme)phys.abunddoublenullablee_SiAbund? Uncertainty of x_abund_sme (e_si_abund_sme)stat.errordoublenullablechiSiAbund? chi^2^ of abundance fit for element X (chi_si_abund_sme)stat.fit.chi2;stat.fit.param;meta.modelleddoublenullablef_SiAbund? Spectroscopic quality flag for abundance of X (flag_si_abund_sme)meta.codedoublenullableo_SiAbund[0/3] Number of spectra used to estimate x_abund_sme (comb_si_abund_sme)meta.numberdoubleKAbund? Abundance [X/Fe] of element X (k_abund_sme)phys.abunddoublenullablee_KAbund? Uncertainty of x_abund_sme (e_k_abund_sme)stat.errordoublenullablechiKAbund? chi^2^ of abundance fit for element X (chi_k_abund_sme)stat.fit.chi2;stat.fit.param;meta.modelleddoublenullablef_KAbund? Spectroscopic quality flag for abundance of X (flag_k_abund_sme)meta.codedoublenullableo_KAbund[0/3] Number of spectra used to estimate x_abund_sme (comb_k_abund_sme)meta.numberdoubleCaAbund? Abundance [X/Fe] of element X (ca_abund_sme)phys.abunddoublenullablee_CaAbund? Uncertainty of x_abund_sme (e_ca_abund_sme)stat.errordoublenullablechiCaAbund? chi^2^ of abundance fit for element X (chi_ca_abund_sme)stat.fit.chi2;stat.fit.param;meta.modelleddoublenullablef_CaAbund? Spectroscopic quality flag for abundance of X (flag_ca_abund_sme)meta.codedoublenullableo_CaAbund[0/3] Number of spectra used to estimate x_abund_sme (comb_ca_abund_sme)meta.numberdoubleScAbund? Abundance [X/Fe] of element X (sc_abund_sme)phys.abunddoublenullablee_ScAbund? Uncertainty of x_abund_sme (e_sc_abund_sme)stat.errordoublenullablechiScAbund? chi^2^ of abundance fit for element X (chi_sc_abund_sme)stat.fit.chi2;stat.fit.param;meta.modelleddoublenullablef_ScAbund? Spectroscopic quality flag for abundance of X (flag_sc_abund_sme)meta.codedoublenullableo_ScAbund[0/3] Number of spectra used to estimate x_abund_sme (comb_sc_abund_sme)meta.numberdoubleTiAbund? Abundance [X/Fe] of element X (ti_abund_sme)phys.abunddoublenullablee_TiAbund? Uncertainty of x_abund_sme (e_ti_abund_sme)stat.errordoublenullablechiTiAbund? chi^2^ of abundance fit for element X (chi_ti_abund_sme)stat.fit.chi2;stat.fit.param;meta.modelleddoublenullablef_TiAbund? Spectroscopic quality flag for abundance of X (flag_ti_abund_sme)meta.codedoublenullableo_TiAbund[0/3] Number of spectra used to estimate x_abund_sme (comb_ti_abund_sme)meta.numberdoubleVAbund? Abundance [X/Fe] of element X (v_abund_sme)phys.abunddoublenullablee_VAbund? Uncertainty of x_abund_sme (e_v_abund_sme)stat.errordoublenullablechiVAbund? chi^2^ of abundance fit for element X (chi_v_abund_sme)stat.fit.chi2;stat.fit.param;meta.modelleddoublenullablef_VAbund? Spectroscopic quality flag for abundance of X (flag_v_abund_sme)meta.codedoublenullableo_VAbund[0/3] Number of spectra used to estimate x_abund_sme (comb_v_abund_sme)meta.numberdoubleCrAbund? Abundance [X/Fe] of element X (cr_abund_sme)phys.abunddoublenullablee_CrAbund? Uncertainty of x_abund_sme (e_cr_abund_sme)stat.errordoublenullablechiCrAbund? chi^2^ of abundance fit for element X (chi_cr_abund_sme)stat.fit.chi2;stat.fit.param;meta.modelleddoublenullablef_CrAbund? Spectroscopic quality flag for abundance of X (flag_cr_abund_sme)meta.codedoublenullableo_CrAbund[0/3] Number of spectra used to estimate x_abund_sme (comb_cr_abund_sme)meta.numberdoubleMnAbund? Abundance [X/Fe] of element X (mn_abund_sme)phys.abunddoublenullablee_MnAbund? Uncertainty of x_abund_sme (e_mn_abund_sme)stat.errordoublenullablechiMnAbund? chi^2^ of abundance fit for element X (chi_mn_abund_sme)stat.fit.chi2;stat.fit.param;meta.modelleddoublenullablef_MnAbund? Spectroscopic quality flag for abundance of X (flag_mn_abund_sme)meta.codedoublenullableo_MnAbund[0/3] Number of spectra used to estimate x_abund_sme (comb_mn_abund_sme)meta.numberdoubleFeAbund? Abundance [X/Fe] of element X (fe_abund_sme)phys.abunddoublenullablee_FeAbund? Uncertainty of x_abund_sme (e_fe_abund_sme)stat.errordoublenullablechiFeAbund? chi^2^ of abundance fit for element X (chi_fe_abund_sme)stat.fit.chi2;stat.fit.param;meta.modelleddoublenullablef_FeAbund? Spectroscopic quality flag for abundance of X (flag_fe_abund_sme)meta.codedoublenullableo_FeAbund[0/1] Number of spectra used to estimate x_abund_sme (comb_fe_abund_sme)meta.numberdoubleCoAbund? Abundance [X/Fe] of element X (co_abund_sme)phys.abunddoublenullablee_CoAbund? Uncertainty of x_abund_sme (e_co_abund_sme)stat.errordoublenullablechiCoAbund? chi^2^ of abundance fit for element X (chi_co_abund_sme)stat.fit.chi2;stat.fit.param;meta.modelleddoublenullablef_CoAbund? Spectroscopic quality flag for abundance of X (flag_co_abund_sme)meta.codedoublenullableo_CoAbund[0/2] Number of spectra used to estimate x_abund_sme (comb_co_abund_sme)meta.numberdoubleNiAbund? Abundance [X/Fe] of element X (ni_abund_sme)phys.abunddoublenullablee_NiAbund? Uncertainty of x_abund_sme (e_ni_abund_sme)stat.errordoublenullablechiNiAbund? chi^2^ of abundance fit for element X (chi_ni_abund_sme)stat.fit.chi2;stat.fit.param;meta.modelleddoublenullablef_NiAbund? Spectroscopic quality flag for abundance of X (flag_ni_abund_sme)meta.codedoublenullableo_NiAbund[0/3] Number of spectra used to estimate x_abund_sme (comb_ni_abund_sme)meta.numberdoubleCuAbund? Abundance [X/Fe] of element X (cu_abund_sme)phys.abunddoublenullablee_CuAbund? Uncertainty of x_abund_sme (e_cu_abund_sme)stat.errordoublenullablechiCuAbund? chi^2^ of abundance fit for element X (chi_cu_abund_sme)stat.fit.chi2;stat.fit.param;meta.modelleddoublenullablef_CuAbund? Spectroscopic quality flag for abundance of X (flag_cu_abund_sme)meta.codedoublenullableo_CuAbund[0/3] Number of spectra used to estimate x_abund_sme (comb_cu_abund_sme)meta.numberdoubleZnAbund? Abundance [X/Fe] of element X (zn_abund_sme)phys.abunddoublenullablee_ZnAbund? Uncertainty of x_abund_sme (e_zn_abund_sme)stat.errordoublenullablechiZnAbund? chi^2^ of abundance fit for element X (chi_zn_abund_sme)stat.fit.chi2;stat.fit.param;meta.modelleddoublenullablef_ZnAbund? Spectroscopic quality flag for abundance of X (flag_zn_abund_sme)meta.codedoublenullableo_ZnAbund[0/3] Number of spectra used to estimate x_abund_sme (comb_zn_abund_sme)meta.numberdoubleRbAbund? Abundance [X/Fe] of element X (rb_abund_sme)phys.abunddoublenullablee_RbAbund? Uncertainty of x_abund_sme (e_rb_abund_sme)stat.errordoublenullablechiRbAbund? chi^2^ of abundance fit for element X (chi_rb_abund_sme)stat.fit.chi2;stat.fit.param;meta.modelleddoublenullablef_RbAbund? Spectroscopic quality flag for abundance of X (flag_rb_abund_sme)meta.codedoublenullableo_RbAbund[0/3] Number of spectra used to estimate x_abund_sme (comb_rb_abund_sme)meta.numberdoubleSrAbund? Abundance [X/Fe] of element X (sr_abund_sme)phys.abunddoublenullablee_SrAbund? Uncertainty of x_abund_sme (e_sr_abund_sme)stat.errordoublenullablechiSrAbund? chi^2^ of abundance fit for element X (chi_sr_abund_sme)stat.fit.chi2;stat.fit.param;meta.modelleddoublenullablef_SrAbund? Spectroscopic quality flag for abundance of X (flag_sr_abund_sme)meta.codedoublenullableo_SrAbund[0/1] Number of spectra used to estimate x_abund_sme (comb_sr_abund_sme)meta.numberdoubleYAbund? Abundance [X/Fe] of element X (y_abund_sme)phys.abunddoublenullablee_YAbund? Uncertainty of x_abund_sme (e_y_abund_sme)stat.errordoublenullablechiYAbund? chi^2^ of abundance fit for element X (chi_y_abund_sme)stat.fit.chi2;stat.fit.param;meta.modelleddoublenullablef_YAbund? Spectroscopic quality flag for abundance of X (flag_y_abund_sme)meta.codedoublenullableo_YAbund[0/3] Number of spectra used to estimate x_abund_sme (comb_y_abund_sme)meta.numberdoubleZrAbund? Abundance [X/Fe] of element X (zr_abund_sme)phys.abunddoublenullablee_ZrAbund? Uncertainty of x_abund_sme (e_zr_abund_sme)stat.errordoublenullablechiZrAbund? chi^2^ of abundance fit for element X (chi_zr_abund_sme)stat.fit.chi2;stat.fit.param;meta.modelleddoublenullablef_ZrAbund? Spectroscopic quality flag for abundance of X (flag_zr_abund_sme)meta.codedoublenullableo_ZrAbund[0/1] Number of spectra used to estimate x_abund_sme (comb_zr_abund_sme)meta.numberdoubleRkpcGalactocentric radius (R_kpc)kpcpos.distance;pos.galactocentricdoubleMoAbund? Abundance [X/Fe] of element X (mo_abund_sme)phys.abunddoublenullablee_MoAbund? Uncertainty of x_abund_sme (e_mo_abund_sme)stat.errordoublenullablechiMoAbund? chi^2^ of abundance fit for element X (chi_mo_abund_sme)stat.fit.chi2;stat.fit.param;meta.modelleddoublenullablef_MoAbund? Spectroscopic quality flag for abundance of X (flag_mo_abund_sme)meta.codedoublenullableo_MoAbund[0/1] Number of spectra used to estimate x_abund_sme (comb_mo_abund_sme)meta.numberdoubleRuAbund? Abundance [X/Fe] of element X (ru_abund_sme)phys.abunddoublenullablee_RuAbund? Uncertainty of x_abund_sme (e_ru_abund_sme)stat.errordoublenullablechiRuAbund? chi^2^ of abundance fit for element X (chi_ru_abund_sme)stat.fit.chi2;stat.fit.param;meta.modelleddoublenullablef_RuAbund? Spectroscopic quality flag for abundance of X (flag_ru_abund_sme)meta.codedoublenullableo_RuAbund[0/1] Number of spectra used to estimate x_abund_sme (comb_ru_abund_sme)meta.numberdoubleBaAbund? Abundance [X/Fe] of element X (ba_abund_sme)phys.abunddoublenullablee_BaAbund? Uncertainty of x_abund_sme (e_ba_abund_sme)stat.errordoublenullablechiBaAbund? chi^2^ of abundance fit for element X (chi_ba_abund_sme)stat.fit.chi2;stat.fit.param;meta.modelleddoublenullablef_BaAbund? Spectroscopic quality flag for abundance of X (flag_ba_abund_sme)meta.codedoublenullableo_BaAbund[0/3] Number of spectra used to estimate x_abund_sme (comb_ba_abund_sme)meta.numberdoubleLaAbund? Abundance [X/Fe] of element X (la_abund_sme)phys.abunddoublenullablee_LaAbund? Uncertainty of x_abund_sme (e_la_abund_sme)stat.errordoublenullablechiLaAbund? chi^2^ of abundance fit for element X (chi_la_abund_sme)stat.fit.chi2;stat.fit.param;meta.modelleddoublenullablef_LaAbund? Spectroscopic quality flag for abundance of X (flag_la_abund_sme)meta.codedoublenullableo_LaAbund[0/1] Number of spectra used to estimate x_abund_sme (comb_la_abund_sme)meta.numberdoubleCeAbund? Abundance [X/Fe] of element X (ce_abund_sme)phys.abunddoublenullablee_CeAbund? Uncertainty of x_abund_sme (e_ce_abund_sme)stat.errordoublenullablechiCeAbund? chi^2^ of abundance fit for element X (chi_ce_abund_sme)stat.fit.chi2;stat.fit.param;meta.modelleddoublenullablef_CeAbund? Spectroscopic quality flag for abundance of X (flag_ce_abund_sme)meta.codedoublenullableo_CeAbund[0/3] Number of spectra used to estimate x_abund_sme (comb_ce_abund_sme)meta.numberdoubleNdAbund? Abundance [X/Fe] of element X (nd_abund_sme)phys.abunddoublenullablee_NdAbund? Uncertainty of x_abund_sme (e_nd_abund_sme)stat.errordoublenullablechiNdAbund? chi^2^ of abundance fit for element X (chi_nd_abund_sme)stat.fit.chi2;stat.fit.param;meta.modelleddoublenullablef_NdAbund? Spectroscopic quality flag for abundance of X (flag_nd_abund_sme)meta.codedoublenullableo_NdAbund[0/3] Number of spectra used to estimate x_abund_sme (comb_nd_abund_sme)meta.numberdoubleSmAbund? Abundance [X/Fe] of element X (sm_abund_sme)phys.abunddoublenullablee_SmAbund? Uncertainty of x_abund_sme (e_sm_abund_sme)stat.errordoublenullablechiSmAbund? chi^2^ of abundance fit for element X (chi_sm_abund_sme)stat.fit.chi2;stat.fit.param;meta.modelleddoublenullablef_SmAbund? Spectroscopic quality flag for abundance of X (flag_sm_abund_sme)meta.codedoublenullableo_SmAbund[0/1] Number of spectra used to estimate x_abund_sme (comb_sm_abund_sme)meta.numberdoubleEuAbund? Abundance [X/Fe] of element X (eu_abund_sme)phys.abunddoublenullablee_EuAbund? Uncertainty of x_abund_sme (e_eu_abund_sme)stat.errordoublenullablechiEuAbund? chi^2^ of abundance fit for element X (chi_eu_abund_sme)stat.fit.chi2;stat.fit.param;meta.modelleddoublenullablef_EuAbund? Spectroscopic quality flag for abundance of X (flag_eu_abund_sme)meta.codedoublenullableo_EuAbund[0/1] Number of spectra used to estimate x_abund_sme (comb_eu_abund_sme)meta.numberdoubleAge55th percentile of age PDF (age_5)Gyrstat.errordoubleAge1616th percentile of age PDF (age_16)Gyrstat.errordoubleAge5050th percentile of age PDF (age_50)Gyrstat.errordoubleAge8484th percentile of age PDF (age_84)Gyrstat.errordoubleAge9595th percentile of age PDF (age_95)Gyrstat.errordoubleAgemeanMean age (age_mean)Gyrtime.age;stat.meandoubleAgestdUncertainty of age (age_std)Gyrstat.errordoubleMass55th percentile of actual mass PDF (mass_5)Sunstat.errordoubleMass1616th percentile of actual mass PDF (mass_16)Sunstat.errordoubleMass5050th percentile of actual mass PDF (mass_50)Sunstat.errordoubleMass8484th percentile of actual mass PDF (mass_84)Sunstat.errordoubleMass9595th percentile of actual mass PDF (mass_95)Sunstat.errordoubleMassmeanActual mass m_act (incl. mass loss) (mass_mean)Sunphys.massdoubleMassstdStandard deviation of actual mass m_act (mass_std)Sunstat.errordoublePhiGalactocentric azimuth angle (Phi)kpcpos.posAng;pos.galactocentricdoubleZkpcHeight above Galactocentric plane (z_kpc)kpcpos.cartesian.z;pos.galactocentricdoubleVRkmsGalactocentric radial velocity (vR_kms)km/sspect.dopplerVeloc;pos.galactocentricdoubleVTkmsGalactocentric transversal velocity (vT_kms)km/sphys.veloc;pos.galactocentricdoubleVZkmsGalactocentric vertical velocity (vz_kms)km/sphys.veloc;pos.galactocentricdoubleXposGalactocentric cartesian coordinate X (x_xyz_kpc)kpcpos.cartesian.x;pos.galactocentricdoubleYposGalactocentric cartesian coordinate Y (y_xyz_kpc)kpcpos.cartesian.y;pos.galactocentricdoubleZposGalactocentric cartesian coordinate Z (z_xyz_kpc)kpcpos.cartesian.z;pos.galactocentricdoubleULSRGalactocentric cartesian velocity U (U_LSR)km/sphys.veloc;pos.cartesian.xdoubleVLSRGalactocentric cartesian velocity V (V_LSR)km/sphys.veloc;pos.cartesian.ydoubleWLSRGalactocentric cartesian velocity W (W_LSR)km/sphys.veloc;pos.cartesian.zdoublejRmean? Radial action (jR_kpckms_mean)kpc.km/sarith.grad;phys.velocdoublenullablejRstd? Uncertainty of radial action (jR_kpckms_std)kpc.km/sstat.errordoublenullableLzmean? Angular momentum / azimuthal action (Lz_kpckms_mean)kpc.km/sphys.angSizedoublenullableLzstd? Uncertainty of angular momentum (Lz_kpckms_std)kpc.km/sstat.error;phys.angMomentumdoublenullablejzmean? Vertical action (jz_kpckms_mean)kpc.km/sarith.grad;phys.velocdoublenullablejzstd? Uncertainty of vertical action (jz_kpckms_std)kpc.km/sstat.errordoublenullableTDDRel. kinematic probabilities of the thick disc-to-thin disc (TD_D)stat.fit.goodnessdoubleTDHRel. kinematic probabilities of the thick disc-to-halo (TD_H)stat.fit.goodnessdoubleDHRel. kinematic probabilities of the thin disc-to-halo (D_H)stat.fit.goodnessdoubleSimbadSimbad column added by the CDSmeta.ref.urlchar