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<ri:Resource created="2021-07-28T07:17:18Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>CH_3_OCHD_2_ experimental frequencies</title><shortName>J/A+A/651/A120</shortName><identifier>ivo://CDS.VizieR/J/A+A/651/A120</identifier><altIdentifier>doi:10.26093/cds/vizier.36510120</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Richard C.</name></creator><creator><name>Jorgensen J.K.</name></creator><creator><name>Margules L.</name></creator><creator><name>Motiyenko R.A.</name></creator><creator><name>Guillemin J.C.,Groner P.</name></creator><date role="Updated">2022-01-17T11:29:32Z</date><date role="Created">2021-07-28T07:17:18Z</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>atomic-physics</subject><description>In 2013, we have published the first rotational analysis and detection of mono-deuterated dimethyl ether in the solar-type protostar IRAS 16293-2422 with the IRAM 30m telescope. Dimethyl ether is one of the most abundant complex organic molecules (COMs) in star-forming regions and their D-to-H (D/H) ratios is important to understand its chemistry and trace the source history. We present the first analysis of doubly-deuterated dimethyl ether (methoxy-d2-methane, 1,1-dideuteromethylether) in its ground- vibrational state, based on an effective Hamiltonian for an asymmetric rotor molecules with internal rotors. The analysis covers the frequency range 0.15-1.5THz. The laboratory rotational spectrum of this species was measured between 150 and 1500GHz with the Lille's submillimeter spectrometer. For the astronomical detection, we used the Atacama Large Millimeter/submillimeter Array (ALMA) observations from the Protostellar Interferometric Line Survey, PILS. New sets of spectroscopic parameters have been determined by a least squares fit with the ERHAM code for both symmetric and asymmetric conformers. As for the mono-deuterated species, these parameters have permitted the first identification in space of both conformers of a doubly-deuterated dimethyl ether via detection near the B component of the Class 0 protostar IRAS 16293-2422.</description><source format="bibcode">2021A&amp;A...651A.120R</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/651/A120</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/651/A120</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/651/A120</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/651/A120</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/651/A120</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/651/A120</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/651/A120</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/></coverage><tableset><schema><name>default</name><table><name>J/A+A/651/A120/tablea1</name><description>Experimental frequencies measured in laboratory up to 1.5THz for the symmetric conformer</description><column><name>Ka1</name><description>Ka value of the upper state</description><ucd>phys.mol.qn</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>J1</name><description>J value of the upper state</description><ucd>stat.value;phys.atmol.configuration</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Kc1</name><description>Kc value of the upper state</description><ucd>phys.mol.qn</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Freq</name><description>Measured frequency</description><ucd>em.freq</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Acc</name><description>Accuracy of the measure</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>O-C</name><description>Observed-calculated frequency</description><ucd>stat.fit.residual</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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