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<ri:Resource created="2018-06-28T14:27:36Z" 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>High-resolution FIR spectrum of anti-vinyl alcohol</title><shortName>J/ApJ/847/67</shortName><identifier>ivo://CDS.VizieR/J/ApJ/847/67</identifier><altIdentifier>doi:10.26093/cds/vizier.18470067</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Bunn H.</name></creator><creator><name>Soliday R.M.</name></creator><creator><name>Sumner I.</name></creator><creator><name>Raston P.L.</name></creator><date role="Updated">2018-08-22T08:21:39Z</date><date role="Created">2018-06-28T14:27:36Z</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><subject>molecular-physics</subject><subject>infrared-astronomy</subject><subject>spectroscopy</subject><description>We report a detailed analysis of the high-resolution far-infrared spectrum of anti-vinyl alcohol, which has been previously identified toward Sagittarius B2(N). The {nu}_15_ OH torsional fundamental investigated here is more than 200cm^-1^ removed from the next nearest vibration, making it practically unperturbed and ideal to help refine the ground state rotational constants that were previously determined from 25 microwave lines. We assigned 1335 lines within the {nu}_15_ fundamental centered at 261.5512cm^-1^, with J and K_a_ ranges of 1-59 and 0-16, respectively. The microwave and far-infrared line positions were fit with Watson-type A- and S-reduced Hamiltonians, with the inclusion of quartic and select sextic distortion terms. This resulted in a significant refinement of the ground state constants, in addition to the determination of the {nu}_15_=1 state constants for the first time. The spectroscopic parameters are in good agreement with the results from anharmonic coupled-cluster calculations, and should be useful in searches for rotationally and/or vibrationally warm anti-vinyl alcohol in interstellar molecular clouds.</description><source format="bibcode">2017ApJ...847...67B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/847/67</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/753/18">J/ApJ/753/18 : FIR spectrum of ethylene oxide (CH_2_-O-CH_2_) (Medcraft+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/768/81">J/ApJ/768/81 : Ethyl cyanide, CH_3_CH_2_CN, vibrational states (Daly+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/572/A44">J/A+A/572/A44 : Vibrationally excited vinyl cyanide in Orion-KL (Lopez+, 2014)</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/ApJ/847/67</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/847/67</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/847/67</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/847/67</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/847/67</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/847/67</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>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/847/67/table3</name><description>Linelist for the {nu}_15_ fundamental of anti-VA; the residuals were determined using the A-reduced constants</description><column><name>v1</name><description>[0/1] Upper v state</description><ucd>phys.mol.qn</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>J0</name><description>[1/59] Lower J state</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Ka0</name><description>[0/15] Lower Ka state</description><ucd>phys.mol.qn</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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Observed energy in MHz (microwave (MW) lines, Rodler 1985JMoSp.114...23R ; v1=v0=0)</description><unit>MHz</unit><ucd>phys.energy;phys.atmol.level</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>O-CMW</name><description>[-0.06/0.05]? Observed - Calculated energy in MHz</description><unit>MHz</unit><ucd>stat.fit.residual</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_EobsMW</name><description>[0.020]? Uncertainty in observed energy in MHz</description><unit>MHz</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Eobs</name><description>[198/323]? Observed energy in cm^-1^ (IR lines; v1=1, v0=0)</description><unit>cm**-1</unit><ucd>phys.energy;phys.atmol.level</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>O-C</name><description>[-0.0007/0.0007]? Observed - Calculated energy</description><unit>cm**-1</unit><ucd>stat.fit.residual</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_Eobs</name><description>[0.0002/0.0003]? Uncertainty in observed energy</description><unit>cm**-1</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Wght</name><description>[0.25/0.5]? Weight for blended lines</description><ucd>stat.weight;phys.atmol</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/ApJ/847/67/table4</name><description>Linelist for the {nu}_15_ fundamental of anti-VA; the residuals were determined using the S-reduced constants</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>J1</name><description>[1/59] Upper J state</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Ka1</name><description>[0/16] Upper Ka state</description><ucd>phys.mol.qn</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Kc1</name><description>[0/59] Upper Kc state</description><ucd>phys.mol.qn</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>v1</name><description>[0/1] Upper v state</description><ucd>phys.mol.qn</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>J0</name><description>[1/59] Lower J state</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Ka0</name><description>[0/15] Lower Ka state</description><ucd>phys.mol.qn</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Kc0</name><description>[0/59] Lower Kc state</description><ucd>phys.mol.qn</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>v0</name><description>[0] Lower v state</description><ucd>phys.mol.qn</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>EobsMW</name><description>[27681.7/55999]? 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