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<ri:Resource created="2019-07-22T13:13:07Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>NGC 3115 Stellar Populations and Kinematics</title><shortName>J/MNRAS/487/3776</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/487/3776</identifier><altIdentifier>doi:10.26093/cds/vizier.74873776</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Poci A.</name></creator><creator><name>McDermid R. M.</name></creator><creator><name>Zhu L.</name></creator><creator><name>van de Ven G.</name></creator><date role="Updated">2024-08-19T20:19:03Z</date><date role="Created">2019-07-22T13:13:07Z</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>galaxies</subject><subject>galaxy-classification-systems</subject><subject>radial-velocity</subject><subject>galaxy-kinematics</subject><description>We present a combination of the Schwarzschild orbit-superposition dynamical modelling technique with the spatially-resolved mean stellar age and metallicity maps to uncover the formation history of galaxies. We apply this new approach to a remarkable 5-pointing mosaic of VLT/MUSE observations obtained by Guerou et al. (2016A&amp;A...591A.143G, Cat. J/A+A/591/A143) extending to a maximum galactocentric distance of ~120'' (5.6kpc) along the major axis, corresponding to ~2.5R_e. Our method first identifies 'families' of orbits from the dynamical model that represent dynamically distinct structures of the galaxy. Individual ages and metallicities of these components are then fit for using the stellar-population information. Our results highlight components of the galaxy that are distinct in the combined stellar dynamics/populations space, which implies distinct formation paths. We find evidence for a dynamically-cold, metal-rich disk, consistent with a gradual in-situ formation. This disk is embedded in a generally-old population of stars, with kinematics ranging from dispersion-dominated in the centre to an old, diffuse, metal-poor stellar halo at the extremities. We find also a direct correlation between the dominant dynamical support of these components, and their associated age, akin to the relation observed in the Milky Way. This approach not only provides a powerful model for inferring the formation history of external galaxies, but also paves the way to a complete population-dynamical model.</description><source format="bibcode">2019MNRAS.487.3776P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/487/3776</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>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/564/L3">J/A+A/564/L3 : NGC 3115 globular clusters JHK photometry (Cantiello+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/148/32">J/AJ/148/32 : Globular cluster candidates in NGC 3115 (Jennings+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/808/19">J/ApJ/808/19 : Megasecond Chandra XVP obs. of NGC3115. II. (Lin+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/591/A143">J/A+A/591/A143 : NGC 3115 MUSE images (Guerou+, 2016)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/487/3776</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/487/3776</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/487/3776</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/487/3776</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/487/3776</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/487/3776</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/MNRAS/487/3776/popul</name><description>NGC 3115 populations</description><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>N</name><description>Voronoi bin number</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>xbin</name><description>Voronoi bin x centroid</description><unit>arcsec</unit><ucd>pos.cartesian.x</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>ybin</name><description>Voronoi bin y centroid</description><unit>arcsec</unit><ucd>pos.cartesian.y</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>ageLW</name><description>luminosity-weighted mean stellar age</description><unit>Gyr</unit><ucd>time.age;stat.mean</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_ageLW</name><description>luminosity-weighted mean stellar age error</description><unit>Gyr</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>metalLW</name><description>luminosity-weighted mean stellar metallicity</description><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_metalLW</name><description>luminosity-weighted mean stellar metallicity error</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>(M/LV)KB</name><description>V-band M/L assuming Kroupa (2002Sci...295...82K) IMF</description><unit>solMass/solLum</unit><ucd>phys.composition.massLightRatio</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table><table><name>J/MNRAS/487/3776/mge</name><description>*NGC 3115 mass surface density MGE (table A1)</description><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>SDens</name><description>Projected surface mass density</description><unit>solMass.pc**-2</unit><ucd>phot.flux.density.sb</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Disp</name><description>Projected dispersion</description><unit>arcsec</unit><ucd>instr.dispersion</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>AxisRatio</name><description>Projected axis ratio</description><ucd>phys.size.axisRatio</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table><table><name>J/MNRAS/487/3776/kinemat</name><description>NGC 3115 kinematics</description><column><name>h3</name><description>h3 coefficient</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_s</name><description>Velocity dispersion error</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</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>N</name><description>Voronoi bin number</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>xbin</name><description>Voronoi bin x centroid</description><unit>arcsec</unit><ucd>pos.cartesian.x</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>ybin</name><description>Voronoi bin y centroid</description><unit>arcsec</unit><ucd>pos.cartesian.y</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>V</name><description>Mean velocity</description><unit>km/s</unit><ucd>phys.veloc;stat.mean</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_V</name><description>Mean velocity error</description><unit>km/s</unit><ucd>stat.error;pos.cartesian.y</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>s</name><description>Velocity dispersion</description><unit>km/s</unit><ucd>phys.veloc.dispersion</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_h3</name><description>h3 coefficient error</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>h4</name><description>h4 coefficient</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_h4</name><description>h4 coefficient error</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>h5</name><description>h5 coefficient</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_h5</name><description>h5 coefficient error</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>h6</name><description>h6 coefficient</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_h6</name><description>h6 coefficient error</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table></schema></tableset></ri:Resource>