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<ri:Resource created="2008-08-10T23:09:18Z" 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>Physical parameters of Wolf-Rayet galaxies</title><shortName>J/A+A/485/657</shortName><identifier>ivo://CDS.VizieR/J/A+A/485/657</identifier><altIdentifier>doi:10.26093/cds/vizier.34850657</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Brinchmann J.</name></creator><creator><name>Kunth D.</name></creator><creator><name>Durret F.</name></creator><date role="Updated">2017-07-04T07:08:54Z</date><date role="Created">2008-08-10T23:09:18Z</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>spectroscopy</subject><subject>chemical-abundances</subject><subject>line-intensities</subject><description>The availability of large spectroscopic datasets has opened up the possibility of constructing large samples of rare objects in a systematic manner. The goal of this study is to analyse the properties of galaxies showing Wolf-Rayet features in their optical spectrum using spectra from the Sloan Digital Sky Survey Release 6. With this unprecedentedly large sample we aim to constrain the properties of the Wolf-Rayet phase and its impact on the surrounding interstellar medium. We carried out very careful continuum subtraction on all galaxies with equivalent widths of H{beta}&gt;2{AA} in emission and identify Wolf-Rayet features using a mixture of automatic and visual classification. 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