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<ri:Resource created="2021-07-05T08:34:27Z" 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>A 3mm molecular line survey of NGC1068</title><shortName>J/A+A/549/A39</shortName><identifier>ivo://CDS.VizieR/J/A+A/549/A39</identifier><altIdentifier>doi:10.26093/cds/vizier.35490039</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Aladro R.</name></creator><creator><name>Viti S.</name></creator><creator><name>Bayet E.</name></creator><creator><name>Riquelme D.</name></creator><creator><name>Martin S.</name></creator><creator><name>Mauersberger R.,Martin-Pintado J.</name></creator><creator><name>Requena-Torres M.A.</name></creator><creator><name>Kramer C.</name></creator><creator><name>Weiss A.</name></creator><date role="Updated">2021-07-05T07:46:44Z</date><date role="Created">2021-07-05T08:34:27Z</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-spectroscopy</subject><subject>active-galactic-nuclei</subject><description>We study the molecular composition of the interstellar medium (ISM) surrounding an active galactic nucleus (AGN), by making an inventory of molecular species and their abundances, to establish a chemical differentiation between starburst galaxies and AGN. We used the IRAM-30m telescope to observe the central 1.5-2kpc region of NGC 1068, covering the frequencies between 86.2GHz and 115.6GHz. Using Boltzmann diagrams, we calculated the column densities of the detected molecules. 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