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<ri:Resource created="2017-01-20T09:17:55Z" 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>Kohonen selected E+A galaxies from SDSS DR7</title><shortName>J/A+A/597/A134</shortName><identifier>ivo://CDS.VizieR/J/A+A/597/A134</identifier><altIdentifier>doi:10.26093/cds/vizier.35970134</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Meusinger H.</name></creator><creator><name>Bruenecke J.</name></creator><creator><name>Schalldach P.</name></creator><creator><name>in der Au A.</name></creator><date role="Updated">2020-02-14T15:17:17Z</date><date role="Created">2017-01-20T09:17:55Z</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>active-galactic-nuclei</subject><subject>spectroscopy</subject><subject>galaxy-classification-systems</subject><description>We created and analysed a large sample of local (z&lt;0.4) post-starburst (PSB) galaxies. In the colour-mass diagram, the PSB sample is clearly concentrated towards the region between the red and the blue cloud, in agreement with the idea that PSB galaxies represent the transitioning phase between actively and passively evolving galaxies. The relative frequency of distorted PSB galaxies is at least 57%, significantly higher than in a comparison sample. The search for active galactic nuclei (AGN) based on conventional selection criteria in the radio and MIR results in a low AGN fraction of 2-3%. We confirm an MIR excess in the mean SED of the PSB galaxy sample that may indicate hidden AGNs, though other sources are also possible.</description><source format="bibcode">2017A&amp;A...597A.134M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/597/A134</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/410/166">J/MNRAS/410/166 : Morphological types from Galaxy Zoo 1 (Lintott+, 2011)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface 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