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<ri:Resource created="2023-08-23T08:20:53Z" 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>Stars from GAIA and APOGEE data</title><shortName>J/A+A/676/A140</shortName><identifier>ivo://CDS.VizieR/J/A+A/676/A140</identifier><altIdentifier>doi:10.26093/cds/vizier.36760140</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ortigoza-Urdaneta M.</name></creator><creator><name>Vieira K.</name></creator><creator><name>Fernandez-Trincado J.G.</name></creator><creator><name>Queiroz A..B.A.,Barbuy B.</name></creator><creator><name>Beers T.C.</name></creator><creator><name>Chiappini C.</name></creator><creator><name>Anders F.</name></creator><creator><name>Minniti D.</name></creator><creator><name>Tang B.</name></creator><date role="Updated">2025-02-27T20:01:38Z</date><date role="Created">2023-08-23T08:20:53Z</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>giant-stars</subject><subject>chemical-abundances</subject><subject>visible-astronomy</subject><subject>infrared-astronomy</subject><description>Based on high-quality APOGEE DR17 and Gaia DR3 data for 1742 red giants stars within 5 kpc of the Sun and not rotating with the Galactic disc (V_phi_&lt;100km/s), we use the nonlinear technique of unsupervised analysis t-SNE to detect coherent structures in the space of ten chemical-abundance ratios: [Fe/H], [O/Fe], [Mg/Fe], [Si/Fe], [Ca/Fe], [C/Fe], [N/Fe], [Al/Fe], [Mn/Fe], and [Ni/Fe]. Additionally, we obtain orbital parameters for each star using the non-axisymmetric gravitational potential GravPot16. Seven structures are detected, including the Splash, Gaia-Sausage-Enceladus (GSE), the high-alpha heated-disc population, N-C-O peculiar stars, and inner disk-like stars, plus two other groups that did not match anything previously reported in the literature, here named Galileo 5 and Galileo 6 (G5 and G6). These two groups overlap with Splash in [Fe/H], G5 being lower metallicity than G6, both between GSE and Splash in the [Mg/Mn] versus [Al/Fe] plane, G5 in the alpha -rich in-situ locus, and G6 on the border of the alpha-poor in-situ one; nonetheless their low [Ni/Fe] hints to a possible ex-situ origin. Their orbital energy distributions are between the Splash and GSE, with G5 being slightly more energetic than G6. We verified the robustness of all the obtained groups by exploring a large range of t-SNE parameters, applying it to various subsets of data, and also measuring the effect of abundance errors through Monte Carlo tests.</description><source format="bibcode">2023A&amp;A...676A.140O</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/676/A140</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 ivo-id="ivo://CDS.VizieR/I/355">I/355 : Gaia DR3 Part 1. Main source (Gaia Collaboration, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/284">III/284 : APOGEE-2 data from DR16 (Johnsson+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/673/A155">J/A+A/673/A155 : StarHorse data for 8 spectroscopic surveys (Queiroz+, 2023)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/663/A126">J/A+A/663/A126 : GALILEO. I. 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xsi:type="vs:VOTableType">double</dataType></column><column><name>Vphi</name><description>Galactocentric azimuthal velocity</description><unit>km/s</unit><ucd>phys.veloc;pos.galactocentric</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Rperi</name><description>Perigalactocentric distance</description><unit>kpc</unit><ucd>pos.distance;src.orbital</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Rperi</name><description>Uncertainty in PERIGALACTICON</description><unit>kpc</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Rapo</name><description>Apogalactocentric distance</description><unit>kpc</unit><ucd>pos.distance;src.orbital</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Rapo</name><description>Uncertainty in APOGALACTICON</description><unit>kpc</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ecc</name><description>Orbital eccentricity</description><ucd>src.orbital.eccentricity</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Ecc</name><description>Uncertainty in eccentricity</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Zmax</name><description>Maximum vertical excursion from the Galactic plane</description><unit>kpc</unit><ucd>src.orbital</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Zmax</name><description>Uncertainty in Zmax</description><unit>kpc</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ej</name><description>Jacobi energy</description><unit>100km**2.s**-2</unit><ucd>src.orbital</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Ej</name><description>Uncertainty in Jacobi energy</description><unit>100km**2.s**-2</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Echar</name><description>Characteristic orbital energy</description><unit>100km**2.s**-2</unit><ucd>src.orbital</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Echar</name><description>Uncertainty in Characteristic orbital energy</description><unit>100km**2.s**-2</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Lmin</name><description>Minimum z-component of angular momentum</description><unit>100km**2.s**-2</unit><ucd>phys.angMomentum</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Lmin</name><description>Uncertainty in minimum z-component of angular momentum</description><unit>100km**2.s**-2</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Lmax</name><description>Maximum z-component of angular momentum</description><unit>100km**2.s**-2</unit><ucd>phys.angMomentum</ucd><dataType xsi:type="vs:VOTableType">float</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>GaiaDR3</name><description>GAIA DR3 source id</description><ucd>meta.id</ucd></column><column><name>Group</name><description>[1/7] Group as determined by t-SNE</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></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>APOGEE</name><description>APOGEE id (2MHHMMSSss+DDMMSSs)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="18*">char</dataType></column><column><name>e_Lmax</name><description>Uncertainty in maximum z-component of angular momentum</description><unit>100km**2.s**-2</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RUWE</name><description>Gaia DR3 renormalized unit weight error</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Dist</name><description>Bayesian StarHorse distance, 50th percentile</description><unit>kpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Dist</name><description>Uncertainty in Dist, error=(84th-16th)/2 percentile</description><unit>kpc</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>pmRA</name><description>Proper motion along RA, pmRAcos(DE), from Gaia DR3</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_pmRA</name><description>Uncertainty in pmRAcos(DE) from Gaia DR3</description><unit>mas/yr</unit><ucd>stat.error;pos.pm;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>pmDE</name><description>Proper motion along DE from Gaia DR3</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.dec</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_pmDE</name><description>Uncertainty in pmDE from Gaia DR3</description><unit>mas/yr</unit><ucd>stat.error;pos.pm;pos.eq.dec</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>