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<ri:Resource created="2015-07-07T08:54:17Z" 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>3mm molecular line survey of 8 AGN</title><shortName>J/A+A/579/A101</shortName><identifier>ivo://CDS.VizieR/J/A+A/579/A101</identifier><altIdentifier>doi:10.26093/cds/vizier.35790101</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Aladro R.</name></creator><creator><name>Martin S.</name></creator><creator><name>Riquelme D.</name></creator><creator><name>Henkel C.</name></creator><creator><name>Mauersberger R.,Martin-Pintado J.</name></creator><creator><name>Weiss A.</name></creator><creator><name>Lefevre C.</name></creator><creator><name>Kramer C.</name></creator><creator><name>Requena-Torres M.A.,Armijos-Abendano R.J.</name></creator><date role="Updated">2017-12-15T10:55:20Z</date><date role="Created">2015-07-07T08:54:17Z</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>radio-galaxies</subject><subject>active-galactic-nuclei</subject><subject>molecular-clouds</subject><subject>galaxies</subject><subject>spectroscopy</subject><description>We aim for a better understanding of the imprints that the nuclear activity in galaxies leaves in the molecular gas. We used the IRAM 30m telescope to observe the frequency range ~[86-116]GHz towards the central regions of the star- burst galaxies M83, M82, and NGC253, the galaxies hosting an active galactic nucleus (AGN) M51, NGC1068, and NGC7469, and the ultra-luminous infrared galaxies (ULIRGs) Arp220 and Mrk231. 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