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<ri:Resource created="2020-01-22T09:09:11Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>GALAH Survey DR2</title><shortName>J/MNRAS/478/4513</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/478/4513</identifier><altIdentifier>doi:10.26093/cds/vizier.74784513</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Buder S.</name></creator><creator><name>Asplund M.</name></creator><creator><name>Duong L.</name></creator><creator><name>Kos J.</name></creator><creator><name>Lind K.</name></creator><creator><name>Ness M.K.</name></creator><creator><name>Sharma S.,Bland-hawthorn J.</name></creator><creator><name>Casey A.R.</name></creator><creator><name>De Silva G.M.</name></creator><creator><name>D'orazi V.</name></creator><creator><name>Freeman K.C.,Lewis G.F.</name></creator><creator><name>Lin J.</name></creator><creator><name>Martell S.L.</name></creator><creator><name>Schlesinger K.J.</name></creator><creator><name>Simpson J.D.,Zucker D.B.</name></creator><creator><name>Zwitter T.</name></creator><creator><name>Amarsi A.M.</name></creator><creator><name>Anguiano B.</name></creator><creator><name>Carollo D.,Casagrande L.</name></creator><creator><name>Cotar K.</name></creator><creator><name>Cottrell P.L.</name></creator><creator><name>Da Costa G.</name></creator><creator><name>Gao X.D.</name></creator><creator><name>Hayden M.R.,Horner J.</name></creator><creator><name>Ireland M.J.</name></creator><creator><name>Kafle P.R.</name></creator><creator><name>Munari U.</name></creator><creator><name>Nataf D.M.</name></creator><creator><name>Nordlander T.,Stello D.</name></creator><creator><name>Ting Y.-S.</name></creator><creator><name>Traven G.</name></creator><creator><name>Watson F.</name></creator><creator><name>Wittenmyer R.A.</name></creator><creator><name>Wyse R.F.G.,Yong D.</name></creator><creator><name>Zinn J.C.</name></creator><creator><name>Zerjal M.</name></creator><creator><name>(the Galah collaboration)</name></creator><date role="Updated">2024-08-18T20:20:13Z</date><date role="Created">2020-01-22T09:09:11Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>surveys</subject><subject>milky-way-galaxy</subject><subject>infrared-photometry</subject><subject>chemical-abundances</subject><description>The Galactic Archaeology with HERMES (GALAH) survey is a large-scale stellar spectroscopic survey of the Milky Way, designed to deliver complementary chemical information to a large number of stars covered by the Gaia mission. We present the GALAH second public data release (GALAH DR2) containing 342 682 stars. For these stars, the GALAH collaboration provides stellar parameters and abundances for up to 23 elements to the community. Here we present the target selection, observation, data reduction, and detailed explanation of how the spectra were analysed to estimate stellar parameters and element abundances. For the stellar analysis, we have used a multistep approach. We use the physics-driven spectrum synthesis of Spectroscopy Made Easy (SME) to derive stellar labels (Teff, logg, [Fe/H], [X/Fe], vmic, vsini, A_KS_) for a representative training set of stars. This information is then propagated to the whole sample with the data-driven method of The Cannon. Special care has been exercised in the spectral synthesis to only consider spectral lines that have reliable atomic input data and are little affected by blending lines. Departures from local thermodynamic equilibrium (LTE) are considered for several key elements, including Li, O, Na, Mg, Al, Si, and Fe, using 1D marcs stellar atmosphere models. Validation tests including repeat observations, Gaia benchmark stars, open and globular clusters, and K2 asteroseismic targets lend confidence to our methods and results. Combining the GALAH DR2 catalogue with the kinematic information from Gaia will enable a wide range of Galactic Archaeology studies, with unprecedented detail, dimensionality, and scope.</description><source format="bibcode">2018MNRAS.478.4513B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/478/4513</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource>https://galah-survey.org/ : GALAH Home Page</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL 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45617 45619-45620 45622 45624 45626 45635 45638 45641 45643-45644 45646 45655 45657 45659 45693 45695-45696 45698 45704 45706-45707 45709 45711 45724 45726 45732-45733 45738 45743-45745 45747-45748 45754-45756 45758 45767 45773 45781 45784-45785 45827 45830 45836 45838 45847 45853 45858-45859 45862 45868 45870 45896-45897 45899 45921 45924-45925 45936-45937 45948-45949 45956 45958 45960-45961 45963-45964 45967 45987 45990-45991 45993 45995 46000 46002 46006-46008 46023 46029-46031 46040-46042 46053 46055 46058-46059 46061-46063 46079 46081 46084-46085 46087 46093 46100 46102-46105 46108-46109 46152 46160 46239 46242 46248 46250 46262-46263 46284 46286 46304-46306 46312 46340-46341 46352 46592 46594 46604 46606 46632-46633 46635 46640 46642 46652 46654 46721 46724-46725 46729-46732 46734-46737 46739 46745-46747 46756 46758-46761 46764 46769 46771 46777 46780-46781 46786-46787 46790 46796 46825-46828 46830 46842-46843 46846 47018-47019 47022 47061 47063 47069 47104 47106-47107 47109-47114 47124 47126 47143 47149-47151 47154 47157 47159 47178-47179 47208 47215 47226 47232-47234 47238-47239 47248-47249 47251 47260-47261 47264-47265 47268-47269 47271 47277-47279 47284 47286 47292 47296 47298 47301 47303 47309 47312 47314 47319 47322 47325 47327 47331 47340-47342 47348 47350 47356 47358 47364 47374-47375 47381-47383 47386-47387 47393-47395 47401 47404 47406-47407 47420 47422-47423 47428 47430 47432-47433 47436 47442-47443 47448-47450 47452 47457-47460 47462 47465-47467 47476 47478 47481-47486 47489-47494 47496-47497 47501-47503 47509-47512 47514-47517 47540 47542 47547 47549-47554 47557 47559 47562-47563 47565-47567 47588 47590 47596 47600-47601 47609 47611 47628-47629 47631-47632 47634-47635 47648 47656 47658-47659 47661 47668-47670 47675 47688 47690-47692 47694 47696-47697 47699-47700 47716 47729 47731-47732 47734 47737 47740-47741 47743 47764-47766 47774-47775 47780 47782 47784-47786 47792-47793 47796-47798 47809 47811 47817-47822 47825 47827 47836 47844 47846-47847 47858 47863-47864 47866-47867 47869-47871 47888-47889 47892 47919 47930-47931 47953 47956 47959 47965 48000 48005 48007 48016-48018 48034 48040-48042 48156 48158 48162-48163 48166-48169 48171 48184-48186 48192-48193 48196 48212 48214 48223 48226-48227 48230 48236 48249 48252-48253 48255 48260 48262 48265-48268 48270 48286-48289 48292 48294-48295 48300-48301 48306 48312 48388 48390 48394-48395 48433 48435 48444-48445 48581 48583 48589 48592 48594-48595 48600-48601 48642 48648 48684 48696-48697 48927 48949 48962-48963 48966-48967 48978 48984 48992-48993 49043 49046 49048-49049 49051-49052 49054</spatial><spectral>1.1166583743361574e-19 3.852589004194616e-19</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/478/4513?format=ascii</footprint><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/MNRAS/478/4513/catalog</name><description>GALAH DR2 catalog</description><column><name>SNRC1</name><description>Signal to noise per pixel in the HERMES blue channel (snr_c1)</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>SNRC2</name><description>Signal to noise per pixel in the HERMES green channel (snr_c2)</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>SNRC3</name><description>Signal to noise per pixel in the HERMES red channel (snr_c3)</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>SNRC4</name><description>Signal to noise per pixel in the HERMES IR channel (snr_c4)</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RVsynt</name><description>Barycentric radial velocity from cross-correlation against synthetic spectra (rv_synt)</description><unit>km/s</unit><ucd>phys.veloc</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_RVsynt</name><description>Uncertainty in rv_synt (e_rv_synt)</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RVobst</name><description>? Radial velocity from internal cross-correlation against data (rv_obst)</description><unit>km/s</unit><ucd>phys.veloc</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_RVobst</name><description>? Uncertainty in rv_obst (e_rv_obst)</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>RVnogrobst</name><description>? Radial velocity from internal cross-correlation against data, uncorrected for gravitational redshift (rv_nogr_obst)</description><unit>km/s</unit><ucd>phys.veloc</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_RVnogrobst</name><description>? Uncertainty in rv_nogr_obst (e_rv_nogr_obst)</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>chi2cannon</name><description>Summed chi-squared over all spectral pixels (chi2_cannon)</description><ucd>stat.fit.chi2</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>splabeldist</name><description>Label distance similar to Ho et al. (2017, Cat. J/ApJ/836/5) (sp_label_distance)</description><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>flagcannon</name><description>Flags for spectrum information in a bitmask format 0=No flag recommended (flag_cannon) (1)</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Teff</name><description>Effective temperature (teff)</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Teff</name><description>Uncertainty of Teff (e_teff)</description><unit>K</unit><ucd>stat.error;phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logg</name><description>Surface gravity (logg)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_logg</name><description>Uncertainty of logg (e_logg)</description><unit>log(cm.s**-2)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>[Fe/H]</name><description>Iron abundance (not overall metallicity [M/H]) (fe_h)</description><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_[Fe/H]</name><description>Uncertainty in [Fe/H] (e_fe_h)</description><ucd>stat.error;phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>vmic</name><description>Microturbulence velocity (vmic)</description><unit>km/s</unit><ucd>phys.veloc.microTurb</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_vmic</name><description>Uncertainty in vmic (e_vmic)</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>vsini</name><description>Line of sight rotational velocity (vsini)</description><unit>km/s</unit><ucd>phys.veloc.rotat;spect.line</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_vsini</name><description>Uncertainty in vsini (e_vsini)</description><unit>km/s</unit><ucd>stat.error;phys.veloc.rotat</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[alpha/Fe]</name><description>? {alpha} enhancement, determined as an error-weighted combination of Mg, Si, Ca, Ti abundances (alpha_fe)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>[Li/Fe]</name><description>Abundance [Li/Fe] for element Li (li_fe)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_[Li/Fe]</name><description>Uncertainty in Li/Fe] (e_lix_fe)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>f_[Li/Fe]</name><description>indicating difficulty in abundance determination in a bitmask format (flag_li_fe) (2)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[C/Fe]</name><description>Abundance [X/Fe] for element C (c_fe)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_[C/Fe]</name><description>Uncertainty in [C/Fe] (e_c_fe)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>f_[C/Fe]</name><description>indicating difficulty in abundance determination in a bitmask format (flag_c_fe) (2)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[O/Fe]</name><description>Abundance [O/Fe] for element O (o_fe)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_[O/Fe]</name><description>Uncertainty in [O/Fe] (e_o_fe)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>f_[O/Fe]</name><description>indicating difficulty in abundance determination in a bitmask format (flag_o_fe) (2)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[Na/Fe]</name><description>Abundance [Na/Fe] for element Na (na_fe)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_[Na/Fe]</name><description>Uncertainty in [Na/Fe] (e_na_fe)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>f_[Na/Fe]</name><description>indicating difficulty in abundance determination in a bitmask format (flag_na_fe) (2)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[Mg/Fe]</name><description>? Abundance [Mg/Fe] for element Mg (mg_fe)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_[Mg/Fe]</name><description>? Uncertainty in [Mg/Fe] (e_mg_fe)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>f_[Mg/Fe]</name><description>indicating difficulty in abundance determination in a bitmask format (flag_mg_fe) (2)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[Al/Fe]</name><description>? Abundance [Al/Fe] for element Al (x_fe)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_[Al/Fe]</name><description>? Uncertainty in x_fe (e_x_fe)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>f_[Al/Fe]</name><description>indicating difficulty in abundance determination in a bitmask format (flag_x_fe) (2)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[Si/Fe]</name><description>? Abundance [Si/Fe] for element Si (si_fe)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_[Si/Fe]</name><description>? Uncertainty in [Si/Fe] (e_si_fe)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>f_[Si/Fe]</name><description>indicating difficulty in abundance determination in a bitmask format (flag_si_fe) (2)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[K/Fe]</name><description>? Abundance [K/Fe] for element K (k_fe)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_[K/Fe]</name><description>? Uncertainty in [K/Fe] (e_k_fe)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>f_[K/Fe]</name><description>indicating difficulty in abundance determination in a bitmask format (flag_k_fe) (2)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[Ca/Fe]</name><description>Abundance [Ca/Fe] for element Ca (ca_fe)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_[Ca/Fe]</name><description>Uncertainty in [Ca/Fe] (e_ca_fe)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>f_[Ca/Fe]</name><description>indicating difficulty in abundance determination in a bitmask format (flag_ca_fe) (2)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[Sc/Fe]</name><description>? Abundance [Sc/Fe] for element Sc (sc_fe)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_[Sc/Fe]</name><description>? Uncertainty in [Sc/Fe] (e_sc_fe)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_[Zn/Fe]</name><description>? Uncertainty in [Zn/Fe] (e_zn_fe)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>f_[Zn/Fe]</name><description>indicating difficulty in abundance determination in a bitmask format (flag_zn_fe) (2)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[Y/Fe]</name><description>Abundance [Y/Fe] for element Y (y_fe)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_[Y/Fe]</name><description>Uncertainty in [Y/Fe] (e_y_fe)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>f_[Y/Fe]</name><description>indicating difficulty in abundance determination in a bitmask format (flag_y_fe) (2)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[Ba/Fe]</name><description>? Abundance [Ba/Fe] for element Ba (ba_fe)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_[Ba/Fe]</name><description>? Uncertainty in [Ba/Fe] (e_ba_fe)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>f_[Ba/Fe]</name><description>indicating difficulty in abundance determination in a bitmask format (flag_ba_fe) (2)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[La/Fe]</name><description>Abundance [La/Fe] for element La (la_fe)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_[La/Fe]</name><description>Uncertainty in [La/Fe] (e_la_fe)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>f_[La/Fe]</name><description>indicating difficulty in abundance determination in a bitmask format (flag_la_fe) (2)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[Eu/Fe]</name><description>? Abundance [Eu/Fe] for element Eu (eu_fe)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_[Eu/Fe]</name><description>? Uncertainty in [Eu/Fe] (e_eu_fe)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>f_[Eu/Fe]</name><description>indicating difficulty in abundance determination in a bitmask format (flag_eu_fe) (2)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>StarId</name><description>2MASS ID number by default (HHMMSSss+DDMMSSs, UCAC4 ID number if 2MASS unavailable (begins with UCAC4-) (star_id)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>sobjectId</name><description>Unique per-observation star ID (sobject_id)</description><ucd>meta.id</ucd><flag>indexed</flag></column><column><name>e_[alpha/Fe]</name><description>? Uncertainty in alpha_fe (e_alpha_fe)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>GaiaId</name><description>? Gaia DR2 identifier (gaia_id)</description><ucd>meta.id</ucd><flag>nullable</flag></column><column><name>ndfclass</name><description>Observation type (MFOBJECT (regular observation) or MFFLX (benchmark observation)) (ndfclass)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>FieldId</name><description>GALAH field identification number (field_id)</description><ucd>meta.id;obs.field</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RAJ2000</name><description>Right ascension from 2MASS (J2000) (raj2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><flag>indexed</flag></column><column><name>DEJ2000</name><description>Declination from 2MASS (J2000) (dej2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><flag>indexed</flag></column><column><name>Jmag</name><description>J magnitude from 2MASS (jmag)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Hmag</name><description>H magnitude from 2MASS (hmag)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Kmag</name><description>K magnitude from 2MASS (kmag)</description><unit>mag</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>VmagJK</name><description>Synthetic V magnitude calculated from JHK, used for target selection (vmag_jk)</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Jmag</name><description>Uncertainty in J magnitude, from 2MASS (e_jmag)</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Hmag</name><description>Uncertainty in H magnitude, from 2MASS (e_hmag)</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Mn/Fe]</name><description>Abundance [Mn/Fe] for element Mn (mn_fe)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_[Mn/Fe]</name><description>Uncertainty in [Mn/Fe] (e_mn_fe)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>f_[Mn/Fe]</name><description>indicating difficulty in abundance determination in a bitmask format (flag_mn_fe) (2)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_Kmag</name><description>Uncertainty in K magnitude, from 2MASS (e_kmag)</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>f_[Sc/Fe]</name><description>indicating difficulty in abundance determination in a bitmask format (flag_sc_fe) (2)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[Ti/Fe]</name><description>Abundance [Ti/Fe] for element Ti (ti_fe)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_[Ti/Fe]</name><description>Uncertainty in [Ti/Fe] (e_ti_fe)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>f_[Ti/Fe]</name><description>indicating difficulty in abundance determination in a bitmask format (flag_ti_fe) (2)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[V/Fe]</name><description>? Abundance [V/Fe] for element V (v_fe)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_[V/Fe]</name><description>? Uncertainty in [V/Fe] (e_v_fe)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>f_[V/Fe]</name><description>indicating difficulty in abundance determination in a bitmask format (flag_v_fe) (2)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[Cr/Fe]</name><description>? Abundance [Cr/Fe] for element Cr (cr_fe)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_[Cr/Fe]</name><description>? Uncertainty in [Cr/Fe] (e_cr_fe)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>f_[Cr/Fe]</name><description>indicating difficulty in abundance determination in a bitmask format (flag_cr_fe) (2)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[Co/Fe]</name><description>Abundance [Co/Fe] for element Co (co_fe)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_[Co/Fe]</name><description>Uncertainty in [Co/Fe] (e_co_fe)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>f_[Co/Fe]</name><description>indicating difficulty in abundance determination in a bitmask format (flag_co_fe) (2)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[Ni/Fe]</name><description>? Abundance [Ni/Fe] for element Ni (ni_fe)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_[Ni/Fe]</name><description>? Uncertainty in [Ni/Fe] (e_ni_fe)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>f_[Ni/Fe]</name><description>indicating difficulty in abundance determination in a bitmask format (flag_ni_fe) (2)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[Cu/Fe]</name><description>Abundance [Cu/Fe] for element Cu (cu_fe)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_[Cu/Fe]</name><description>Uncertainty in [Cu/Fe] (e_cu_fe)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>f_[Cu/Fe]</name><description>indicating difficulty in abundance determination in a bitmask format (flag_cu_fe) (2)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[Zn/Fe]</name><description>? Abundance [Zn/Fe] for element Zn (zn_fe)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>