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<ri:Resource created="1999-10-28T22:40:39Z" 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>X-ray selected ROSAT AGN spectra</title><shortName>J/A+A/350/805</shortName><identifier>ivo://CDS.VizieR/J/A+A/350/805</identifier><altIdentifier>doi:10.26093/cds/vizier.33500805</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Grupe D.</name></creator><creator><name>Beuermann K.</name></creator><creator><name>Mannheim K.</name></creator><creator><name>Thomas H.-C.</name></creator><date role="Updated">1999-10-28T22:41:20Z</date><date role="Created">1999-10-28T22:40:39Z</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>active-galactic-nuclei</subject><subject>quasars</subject><subject>spectroscopy</subject><description>We present the emission line properties of a sample of 76 bright soft X-ray selected ROSAT Active Galactic Nuclei. All optical counterparts are Seyfert 1 galaxies with rather narrow permitted lines, strong optical FeII line blends, and weak forbidden lines. By selection, they also have steep soft X-ray spectra when compared with typical Seyfert 1 galaxies. We discuss possible origins of these peculiar trends employing detailed correlation analyses, including a Principal Component Analysis. The optical spectra are presented in the Appendix.</description><source format="bibcode">1999A&amp;A...350..805G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/350/805</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/A+AS/109/147">J/A+AS/109/147 : ROSAT AGN content (Brinkmann+, 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/110/469">J/A+AS/110/469 : AGN from the RASS (Bade+, 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/323/739">J/A+A/323/739 : ROSAT detected quasars. II. 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