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<ri:Resource created="2026-03-03T09:21:31Z" status="active" updated="2026-04-02T06:28:33Z" 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>MaNGA and ATLAS3D ETGs kinematic data</title><shortName>J/A+A/707/A137</shortName><identifier>ivo://CDS.VizieR/J/A+A/707/A137</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Zhong W.</name></creator><creator><name>Du M.</name></creator><creator><name>Lu S.</name></creator><creator><name>Jin Y.</name></creator><creator><name>Zhu K.</name></creator><date role="Updated">2026-04-02T06:28:33Z</date><date role="Created">2026-03-03T09:21:31Z</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>visible-astronomy</subject><description>This study aims to make a comparative analysis of galaxy kinematics using IllustrisTNG simulations and integral-field spectroscopy (IFS) observations. We identify 2342 early-type galaxies (ETGs) from the TNG100 simulation and 236 ETGs from the TNG50 simulation to compare with those from MaNGA and ATLAS^3D^ surveys. For these systems, we measure key kinematic parameters widely employed in both observational and simulation-based studies, including the intrinsic spin parameter {lambda}_R,intr_ (it indicates that the {lambda}_R_ parameter is measured when the galaxy is viewed edge-on), the cylindrical rotational energy fraction {kappa}_rot_, and structural mass ratios such as the spheroid mass fraction f_spheroid_ and the stellar halo mass fraction f_halo_. This study performs a comparative kinematic analysis of early-type galaxies using IllustrisTNG simulations and IFS data from MaNGA and ATLAS^3D^ . We demonstrate that standard classifiers --- the {lambda}_R_(Re)=0.31 SQRT(epsilon) relation and k_5_{bar} coefficient (the higher-order term of the Fourier decomposition of velocity fields) --- fail to align with kinematic bimodality. Revised thresholds are proposed: the spin {lambda}_R,intr_~0.4, the ratio of rotation energy {kappa}_rot_~0.5, and the mass fraction of a spheroid component f_spheroid_~0.6. It provides a universal threshold that classifies all kinds of galaxies into rotation-dominated (fast rotators) and random motion-dominated (slow rotators) cases. Scaling relations derived from TNG enable estimation of {kappa}_rot_ and f_spheroid_ from observations. TNG simulations exhibit a bimodality deficit, characterized by a lack of fast rotators and suppressed {lambda}_R,intr_, attributable to excess galaxies with intermediate rotation and high spheroid/stellar halo mass. A novel method for estimating stellar halo mass fractions from IFS kinematics is introduced, though significant uncertainties persist.</description><source format="bibcode">2026A&amp;A...707A.137Z</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/707/A137</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></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/A+A/707/A137</accessURL><mirrorURL title="VizieR at IUCAA: Pune, 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