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<ri:Resource created="2025-02-24T11:33:45Z" status="active" updated="2025-12-12T20:07:05Z" 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>GAMA DR4 spectrum catalog</title><shortName>J/MNRAS/513/439</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/513/439</identifier><altIdentifier>doi:10.26093/cds/vizier.75130439</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Driver S.P.</name></creator><creator><name>Bellstedt S.</name></creator><creator><name>Robotham A.S.G.</name></creator><creator><name>Baldry I.K.</name></creator><creator><name>Davies L.J.,Liske J.</name></creator><creator><name>Obreschkow D.</name></creator><creator><name>Taylor E.N.</name></creator><creator><name>Wright A.H.</name></creator><creator><name>Alpaslan M.,Bamford S.P.</name></creator><creator><name>Bauer A.E.</name></creator><creator><name>Bland-Hawthorn J.</name></creator><creator><name>Bilicki M.</name></creator><creator><name>Bravo M.,Brough S.</name></creator><creator><name>Casura S.</name></creator><creator><name>Cluver M.E.</name></creator><creator><name>Colless M.</name></creator><creator><name>Conselice C.J.</name></creator><creator><name>Croom S.M.,De Jong J.</name></creator><creator><name>D'Eugenio F.</name></creator><creator><name>De Propris R.</name></creator><creator><name>Dogruel B.</name></creator><creator><name>Drinkwater M.J.,Dvornik A.</name></creator><creator><name>Farrow D.J.</name></creator><creator><name>Frenk C.S.</name></creator><creator><name>Giblin B.</name></creator><creator><name>Graham A.W.</name></creator><creator><name>Grootes M.W.,Gunawardhana M.L.P.</name></creator><creator><name>Hashemizadeh A.</name></creator><creator><name>Haussler B.</name></creator><creator><name>Heymans C.,Hildebrandt H.</name></creator><creator><name>Holwerda B.W.</name></creator><creator><name>Hopkins A.M.</name></creator><creator><name>Jarrett T.H.</name></creator><creator><name>Heath Jones D.,Kelvin L.S.</name></creator><creator><name>Koushan S.</name></creator><creator><name>Kuijken K.</name></creator><creator><name>Lara-Lopez M.A.</name></creator><creator><name>Lange R.,Lopez-Sanchez A.R.</name></creator><creator><name>Loveday J.</name></creator><creator><name>Mahajan S.</name></creator><creator><name>Meyer M.</name></creator><creator><name>Moffett A.J.,Napolitano N.R.</name></creator><creator><name>Norberg P.</name></creator><creator><name>Owers M.S.</name></creator><creator><name>Radovich M.</name></creator><creator><name>Raouf M.,Peacock J.A.</name></creator><creator><name>Phillipps S.</name></creator><creator><name>Pimbblet K.A.</name></creator><creator><name>Popescu C.</name></creator><creator><name>Said K.,Sansom A.E.</name></creator><creator><name>Seibert M.</name></creator><creator><name>Sutherland W.J.</name></creator><creator><name>Thorne J.E.</name></creator><creator><name>Tuffs R.J.,Turner R.</name></creator><creator><name>van der Wel A.</name></creator><creator><name>van Kampen E.</name></creator><creator><name>Wilkins S.M.</name></creator><date role="Updated">2025-12-12T20:07:05Z</date><date role="Created">2025-02-24T11:33:45Z</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>surveys</subject><subject>galaxies</subject><subject>catalogs</subject><subject>redshifted</subject><subject>visible-astronomy</subject><subject>sloan-photometry</subject><subject>infrared-photometry</subject><subject>ultraviolet-astronomy</subject><subject>astrometry</subject><subject>spectroscopy</subject><description>In Galaxy And Mass Assembly Data Release 4 (GAMA DR4), we make available our full spectroscopic redshift sample. This includes 248682 galaxy spectra, and, in combination with earlier surveys, results in 330542 redshifts across five sky regions covering ~250 deg^2^. The redshift density, is the highest available over such a sustained area, has exceptionally high completeness (95 per cent to rKiDS = 19.65 mag), and is well-suited for the study of galaxy mergers, galaxy groups, and the low redshift (z &lt; 0.25) galaxy population. DR4 includes 32 value-added tables or Data Management Units (DMUs) that provide a number of measured and derived data products including GALEX, ESO KiDS, ESO VIKING, WISE, and HerschelSpace Observatory imaging. Within this release, we provide visual morphologies for 15330 galaxies to z &lt; 0.08, photometric redshift estimates for all 18 million objects to r_KiDS_ ~25 mag, and stellar velocity dispersions for 111830 galaxies. We conclude by deriving the total galaxy stellar mass function (GSMF) and its sub-division by morphological class (elliptical, compact-bulge and disc, diffuse-bulge and disc, and disc only). This extends our previous measurement of the total GSMF down to 10^6.75^ M_{sun}_ h_70_^-2^ and we find a total stellar mass density of {rho}* = (2.97 +/- 0.04) * 10^8^ M_{sun} h_70_ Mpc^-3^ or Omega_*_ = (2.17 +/- 0.03) * 10^-3^ h_70_^-1^. We conclude that at z &lt; 0.1, the Universe has converted 4.9 +/- 0.1 per cent of the baryonic mass implied by big bang Nucleosynthesis into stars that are gravitationally bound within the galaxy population.</description><source format="bibcode">2022MNRAS.513..439D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/513/439</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/MNRAS/474/3875">J/MNRAS/474/3875 : Galaxy And Mass Assembly (GAMA): DR3 (Baldry+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/413/971">J/MNRAS/413/971 : 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2016)</relatedResource><relatedResource>https://www.gama-survey.org/dr4/ : GAMA-DR4 Home Page</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/513/439</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/513/439</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/513/439</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/513/439</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/513/439</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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