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<ri:Resource created="2022-01-18T14:37:07Z" 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>Stellar mass dist. of local star-forming gal.</title><shortName>J/MNRAS/504/3831</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/504/3831</identifier><altIdentifier>doi:10.26093/cds/vizier.75043831</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Bonfini P.</name></creator><creator><name>Zezas A.</name></creator><creator><name>Ashby M.L.N.</name></creator><creator><name>Willner S.P.</name></creator><creator><name>Maragkoudakis A.,Kouroumpatzakis K.</name></creator><creator><name>Sell P.H.</name></creator><creator><name>Kovlakas K.</name></creator><date role="Updated">2024-08-21T20:17:48Z</date><date role="Created">2022-01-18T14:37:07Z</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>photometry</subject><description>We constrain the mass distribution in nearby, star-forming galaxies with the Star Formation Reference Survey (SFRS), a galaxy sample constructed to be representative of all known combinations of star formation rate, dust temperature, and specific star formation rate (sSFR) that exist in the Local Universe. An innovative 2D bulge/disc decomposition of the 2MASS/Ks-band images of the SFRS galaxies yields global luminosity and stellar mass functions (MFs), along with separate MFs for their bulges and discs. These accurate MFs cover the full range from dwarf galaxies to large spirals, and are representative of star-forming galaxies selected based on their infrared luminosity, unbiased by active galactic nucleus content and environment. We measure an integrated luminosity density j=1.72+/-0.93x10^9^L_{sun}/h/Mpc^3^ and a total stellar mass density {rho}_M_=4.61+/-2.40x10^8^M_{sun}_/h/Mpc^3^. While the stellar mass of the average star-forming galaxy is equally distributed between its sub-components, discs globally dominate the mass density budget by a ratio 4:1 with respect to bulges. In particular, our functions suggest that recent star formation happened primarily in massive systems, where they have yielded a disc stellar mass density larger than that of bulges by more than 1 dex. Our results constitute a reference benchmark for models addressing the assembly of stellar mass on the bulges and discs of local (z=0) star-forming galaxies.</description><source format="bibcode">2021MNRAS.504.3831B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/504/3831</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/J/PASP/123/1011">J/PASP/123/1011 : Star Formation Reference Survey (SFRS) (Ashby+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/482/560">J/MNRAS/482/560 : Star formation in nearby galaxies (Mahajan+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/506/3079">J/MNRAS/506/3079 : Halpha and other SFR indicators (Kouroumpatzakis+, 2021)</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/504/3831</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/504/3831</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/504/3831</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/504/3831</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/504/3831</mirrorURL><mirrorURL 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Component color form our decomposition (the global galaxy color is reported in Table D1)</description><unit>mag</unit><ucd>phot.color;em.opt.U;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>M/L</name><description>? Component mass-to-light ratio</description><unit>solLum/solMass</unit><ucd>phys.composition.massLightRatio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>M/Lgal</name><description>Galaxy mass-to-light ratio</description><unit>solLum/solMass</unit><ucd>phys.composition.massLightRatio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>M</name><description>? 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