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<ri:Resource created="2000-04-10T21:10:08Z" 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>Morphological classifications of APM galaxies</title><shortName>J/MNRAS/274/1107</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/274/1107</identifier><altIdentifier>doi:10.26093/cds/vizier.72741107</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Naim A.</name></creator><creator><name>Lahav O.</name></creator><creator><name>Buta R.J.</name></creator><creator><name>Corwin H.G.Jr.</name></creator><creator><name>De Vaucouleurs G.,Dressler A.</name></creator><creator><name>Huchra J.P.</name></creator><creator><name>Van Den Bergh S.</name></creator><creator><name>Raychaudhury S.</name></creator><creator><name>Sodre L.Jr,Storrie-Lombardi M.C.</name></creator><date role="Updated">2024-06-24T20:14:30Z</date><date role="Created">2000-04-10T21:10:08Z</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>catalogs</subject><subject>galaxy-classification-systems</subject><description>We investigate the consistency of visual morphological classifications of galaxies by comparing classifications for 831 galaxies from six independent observers. The galaxies were classified on laser print copy images or on computer screen using scans made with the Automated Plate Measuring (APM) machine. Classifications are compared using the Revised Hubble numerical type index T. We find that individual observers agree with one another with rms combined dispersions of between 1.3 and 2.3 type units, typically about 1.8 units. The dispersions tend to decrease slightly with increasing angular diameter and, in some cases, with increasing axial ratio (b/a). The agreement between independent observers is reasonably good but the scatter is non-negligible. In spite of the scatter, the Revised Hubble T system can be used to train an automated galaxy classifier, e.g. an artificial neural network, to handle the large number of galaxy images that are being compiled in the APM and other surveys.</description><source format="bibcode">1995MNRAS.274.1107N</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/274/1107</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/155">VII/155 : Third Reference Cat. of Bright Galaxies (RC3) (de Vaucouleurs+ 1991)</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/274/1107</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/274/1107</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/274/1107</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/274/1107</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/274/1107</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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Should Not be used for identification.</description><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RA1950</name><description>Right ascension (1950)</description></column><column><name>DE1950</name><description>Declination (1950)</description></column><column><name>Diam</name><description>Diameter</description><unit>arcmin</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RC3</name><description>? RC3 (Cat. &lt;VII/155&gt;) T-type classification (1)</description><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>RB</name><description>? R. Buta classification (1)</description><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>HC</name><description>? H. Corwin classification (1)</description><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>GV</name><description>? 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