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<ri:Resource created="2010-04-04T14:29:15Z" 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>Galaxies with strong PAH emission</title><shortName>J/A+A/507/713</shortName><identifier>ivo://CDS.VizieR/J/A+A/507/713</identifier><altIdentifier>doi:10.26093/cds/vizier.35070713</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Haas M.</name></creator><creator><name>Leipski C.</name></creator><creator><name>Siebenmorgen R.</name></creator><creator><name>Meusinger H.</name></creator><creator><name>Drass H.</name></creator><creator><name>Chini R.</name></creator><date role="Updated">2017-10-09T13:33:40Z</date><date role="Created">2010-04-04T14:29:15Z</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>infrared-sources</subject><subject>infrared-photometry</subject><subject>interstellar-medium</subject><description>This is the fourth in a series of papers based on the ISOCAM Parallel Survey at 6.7um. While the first three papers have been devoted to active galactic nuclei (AGN), here we report on emission-line galaxies without AGN signatures in their optical spectra. Polycyclic aromatic hydrocarbon (PAH) emission has been found in both starbursts and modestly starforming galaxies, but the relation between starforming activity and PAH luminosity is still a matter of debate. The different correlation degrees could be caused by the variety of optical and far-infrared sample selection criteria. 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