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<ri:Resource created="2019-05-13T14:37:58Z" status="active" updated="2025-06-13T15:25:00Z" 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>Fundamental stellar &amp; halo data for local galaxies</title><shortName>J/ApJ/859/2</shortName><identifier>ivo://CDS.VizieR/J/ApJ/859/2</identifier><altIdentifier>doi:10.26093/cds/vizier.18590002</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Lapi A.</name></creator><creator><name>Salucci P.</name></creator><creator><name>Danese L.</name></creator><date role="Updated">2019-05-13T13:56:04Z</date><date role="Created">2019-05-13T14:37:58Z</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>absolute-magnitude</subject><subject>visible-astronomy</subject><description>We build templates of rotation curves as a function of the I-band luminosity via the mass modeling (by the sum of a thin exponential disk and a cored halo profile) of suitably normalized, stacked data from wide samples of local spiral galaxies. We then exploit such templates to determine fundamental stellar and halo properties for a sample of about 550 local disk-dominated galaxies with high-quality measurements of the optical radius R_opt_ and of the corresponding rotation velocity V_opt_. Specifically, we determine the stellar M_*_ and halo M_H_ masses, the halo size R_H_ and velocity scale V_H_, and the specific angular momenta of the stellar j_*_ and dark matter j_H_ components. We derive global scaling relationships involving such stellar and halo properties both for the individual galaxies in our sample and for their mean within bins; the latter are found to be in pleasing agreement with previous determinations by independent methods (e.g., abundance matching techniques, weak-lensing observations, and individual rotation curve modeling). Remarkably, the size of our sample and the robustness of our statistical approach allow us to attain an unprecedented level of precision over an extended range of mass and velocity scales, with 1{sigma} dispersion around the mean relationships of less than 0.1dex. We thus set new standard local relationships that must be reproduced by detailed physical models, which offer a basis for improving the subgrid recipes in numerical simulations, that provide a benchmark to gauge independent observations and check for systematics, and that constitute a basic step toward the future exploitation of the spiral galaxy population as a cosmological probe.</description><source format="bibcode">2018ApJ...859....2L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/859/2</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/VII/34">VII/34 : ESO/Uppsala Survey of the ESO(B) Atlas (Lauberts 1982)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VI/30">VI/30 : Plates of the ESO / SERC Sky Survey (Holmberg+ 1974-)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/612/L6">J/A+A/612/L6 : j-M law from dwarf to massive spirals (Posti+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/152/157">J/AJ/152/157 : Mass models for 175 disk galaxies with SPARC (Lelli+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/425/2741">J/MNRAS/425/2741 : Parameters of Spiral galaxies from SDSS 7 (Hall+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/417/2347">J/MNRAS/417/2347 : Tully-Fisher relation for SDSS galaxies (Reyes+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/99/501">J/ApJS/99/501 : Spiral galaxies rotation curves (Persic+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/81/413">J/ApJS/81/413 : Southern sky survey of 1355 spiral gal. 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