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<ri:Resource created="2020-11-24T08:51:23Z" 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>rotational transitions of cyanoacetamide</title><shortName>J/A+A/644/A3</shortName><identifier>ivo://CDS.VizieR/J/A+A/644/A3</identifier><altIdentifier>doi:10.26093/cds/vizier.36440003</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Sanz-Novo M.</name></creator><creator><name>Leon I.</name></creator><creator><name>Alonso J.L.</name></creator><creator><name>Largo A.</name></creator><creator><name>Barrientos C.</name></creator><date role="Updated">2021-02-15T10:53:30Z</date><date role="Created">2020-11-24T08:51:23Z</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>spectroscopy</subject><subject>atomic-physics</subject><description>Cyanoacetamide is a branched chain -CN bearing molecule which is also an amide derivative target molecule in the interstellar medium. The aim of our investigation is to analyze the feasibility of a plausible formation process of protonated cyanoacetamide under interstellar conditions and to provide direct experimental frequencies of the ground vibrational state of the neutral form in the microwave region in order to enable its eventual identification in the interstellar medium. We used high-level theoretical computations to study the formation process of protonated cyanoacetamide. Furthermore, we employed a high resolution laser ablation molecular beam Fourier transform (LA-MB-FTMW) spectroscopic technique to measure the frequencies of the neutral form. We report the first rotational characterization of cyanoacetamide and a precise set of the relevant rotational spectroscopic constants have been determined as a first step to identify the molecule in the interstellar medium. We performed full exploration of the Potential Energy Surface (PES) to study a gas-phase reaction on the formation process of protonated cyanoacetamide. We found an exothermic process with no net activation barrier initiated by the high-energy isomer of protonated hydroxylamine, which leads to protonated cyanoacetamide.</description><source format="bibcode">2020A&amp;A...644A...3S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/644/A3</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/644/A3</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/644/A3</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/644/A3</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/644/A3</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/644/A3</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/644/A3</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/644/A3/catalog</name><description>Calculated rotational transitions of cyanoacetamide in the ground state</description><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>Freq</name><description>Frequency of the line</description><unit>MHz</unit><ucd>em.freq</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Freq</name><description>Estimated or experimental error</description><unit>MHz</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logInt</name><description>Base 10 logarithm of the integrated intensity</description><unit>log(nm**2.MHz)</unit><ucd>meta.code;spect.line.intensity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>DOF</name><description>Degrees of freedom in the partition function</description><ucd>stat.fit.dof</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Elow</name><description>Lower state in wavenumbers</description><ucd>phys.energy;phys.atmol.level</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>gup</name><description>Upper state degeneracy</description><ucd>phys.electron.degen</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Tag</name><description>Species tag or molecular identifier</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>QNFMT</name><description>Identifies the format of the quantum numbers given in the field QN</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>QN</name><description>Quantum numbers coded according to QNFMT</description><ucd>phys.mol.qn</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column></table></schema></tableset></ri:Resource>