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<ri:Resource created="2022-02-10T08:32:38Z" 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>Spectroscopy of CD_3_OH</title><shortName>J/A+A/658/A127</shortName><identifier>ivo://CDS.VizieR/J/A+A/658/A127</identifier><altIdentifier>doi:10.26093/cds/vizier.36580127</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ilyushin V.V.</name></creator><creator><name>Muller H.S.P.</name></creator><creator><name>Jorgensen J.K.</name></creator><creator><name>Bauerecker S.</name></creator><creator><name>Maul C.,Bakhmat Y.</name></creator><creator><name>Alekseev E.A.</name></creator><creator><name>Dorovskaya O.</name></creator><creator><name>Vlasenko S.</name></creator><creator><name>Lewen F.,Schlemmer S.</name></creator><creator><name>Berezkin K.</name></creator><creator><name>Lees R.M.</name></creator><date role="Updated">2022-08-25T12:50:11Z</date><date role="Created">2022-02-10T08:32:38Z</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>interstellar-medium</subject><subject>radio-spectroscopy</subject><subject>spectroscopy</subject><description>Solar-type protostars have been shown to harbor highly deuterated complex organics as for example witnessed by the high relative abundances of doubly and triply deuterated isotopologs. While this degree of deuteration may provide important clues to the formation of these species, spectroscopic information on multiply deuterated isotopologs is often insufficient. In particular, searches for triply deuterated methanol, CD_3_OH, are hampered to a large extent by the lack of intensity information from a spectroscopic model. The aim of the present study is to develop a spectroscopic model of CD_3_OH in low-lying torsional states sufficiently accurate to facilitate further searches for CD_3_OH in space. We have performed a new measurement campaign for CD_3_OH involving three spectroscopic laboratories which covers the 34GHz-1.1THz and the 20-900cm^-1^ ranges. The analysis was perfomed using the rho-axis-method torsion- rotation Hamiltonian model. We determined a model that describes the ground and first excited torsional states of CD_3_OH up to quantum numbers J&lt;=55 and K&lt;=23, and derived a line list for radio-astronomical observations. The resulting line list is accurate up to at least 1.1THz and should be sufficient for all types of radio-astronomical searches for this methanol isotopolog. This line list was used to search for CD_3_OH in data from the Protostellar Interferometric Line Survey of IRAS 16293-2422 using the Atacama Large Millimeter/submillimeter Array. CD_3_OH is securely detected in the data with a large number of clearly separated and well-reproduced lines. We detected not only lines belonging to the ground torsional state, but also several belonging to the first excited torsional state. The derived column density of CD_3_OH and abundance relative to non-deuterated isotopolog confirm the significant enhancement of this multiply deuterated variant. This is in line with other observations of multiply deuterated complex organic molecules and may serve as an important constraint on models for their formation.</description><source format="bibcode">2022A&amp;A...658A.127I</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/658/A127</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/658/A127</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/658/A127</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/658/A127</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/658/A127</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/658/A127</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/658/A127</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"/><waveband>Millimeter</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/658/A127/tablea1</name><description>Assigned microwave transitions of the CD_3_OH spectrum used in the analysis</description><column><name>Sym'</name><description>Upper level symmetry in the G6 group</description><ucd>phys.atmol</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>m'</name><description>Upper free rotor torsional quantum number</description><ucd>phys.atmol.qn;stat.max</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>J'</name><description>Upper J quantum number</description><ucd>instr.det.qe;stat.max</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Ka'</name><description>Upper Ka quantum number</description><ucd>phys.atmol.qn;stat.max</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Kc'</name><description>Upper Kc quantum number</description><ucd>phys.atmol.qn;stat.max</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Sym"</name><description>Lower level symmetry in the G6 group</description><ucd>phys.atmol</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>m"</name><description>Lower free rotor torsional quantum number</description><ucd>phys.atmol.qn;stat.min</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>J"</name><description>Lower J quantum number</description><ucd>instr.det.qe;stat.min</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Ka"</name><description>Lower Ka quantum number</description><ucd>phys.atmol.qn;stat.min</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Kc"</name><description>Lower Kc quantum number</description><ucd>phys.atmol.qn;stat.min</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Freq</name><description>Observed transition frequency</description><unit>MHz</unit><ucd>em.freq</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>unc</name><description>Uncertainty of measurement</description><unit>MHz</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>O-C</name><description>Residuals from the fit</description><unit>MHz</unit><ucd>stat.fit.residual</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Cmnt</name><description>Source of data</description><ucd>meta.bib</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column></table><table><name>J/A+A/658/A127/tablea2</name><description>Assigned FIR transitions of the CD_3_OH spectrum used in the analysis</description><column><name>Kc'</name><description>Upper Kc quantum number</description><ucd>phys.atmol.qn;stat.max</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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