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<ri:Resource created="2010-11-08T09:21:50Z" 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 spectrum of H^13^COOCH_3_</title><shortName>J/ApJS/190/315</shortName><identifier>ivo://CDS.VizieR/J/ApJS/190/315</identifier><altIdentifier>doi:10.26093/cds/vizier.21900315</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Carvajal M.</name></creator><creator><name>Kleiner I.</name></creator><creator><name>Demaison J.</name></creator><date role="Updated">2010-11-30T21:13:40Z</date><date role="Created">2010-11-08T09:21:50Z</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>atomic-physics</subject><subject>radio-spectroscopy</subject><description>A compilation of the available spectroscopic millimeter- and submillimeter-wave data of the ground and first excited states of ^13^C_1_-methyl formate (H^13^COOCH_3_) has been carried out. The exhaustive analysis of the available transition lines of H^13^COOCH_3_ has led to the assignment of 7457 spectral lines by means of a global fit of 45 parameters, using the Rho-Axis Method (RAM) and the BELGI-Cs code, with a resulting unitless standard deviation of 0.57. Over 1600 lines are included for the first time in the fit. In addition, the line strengths of spectral lines are also calculated using the most recent experimental measurement of the electric dipole moment. In conclusion, the present study represents a notable improvement with respect to previous H^13^COOCH_3_ spectral analyses. Therefore, the better accuracy of the present analysis may help the future identification of new H^13^COOCH_3_ lines in the interstellar and circumstellar media, and may contribute to decrease some of the spectral confusion due to these species in astronomical surveys.</description><source format="bibcode">2010ApJS..190..315C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/190/315</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/A+A/500/1109">J/A+A/500/1109 : Rotational spectrum of HCOO^13^CH_3_ (Carvajal+, 2009)</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/ApJS/190/315</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/190/315</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/190/315</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/190/315</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/190/315</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/190/315</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>Radio</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJS/190/315/table3</name><description>Assignments, observed frequencies, calculated frequencies, residuals from the RAM fit, line strengths, and lower energy levels for ^13^C_1_-methyl formate (H^13^COOCH_3_) microwave transitions from v_t_=0 and v_t_=1 torsional states included in the fit wi</description><column><name>LNum</name><description>Line number (1)</description><ucd>meta.id;spect.line</ucd><dataType xsi:type="vs:VOTableType">int</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>Upper</name><description>Upper state information (2)</description><ucd>meta.note;phys.atmol.configuration</ucd><dataType xsi:type="vs:VOTableType" arraysize="21*">char</dataType></column><column><name>Lower</name><description>Lower state information (2)</description><ucd>meta.note;phys.atmol.configuration</ucd><dataType xsi:type="vs:VOTableType" arraysize="21*">char</dataType></column><column><name>OFreq</name><description>Observed frequency</description><unit>MHz</unit><ucd>em.freq</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_OFreq</name><description>Uncertainty in OFreq</description><unit>MHz</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>CFreq</name><description>Calculated frequency</description><unit>MHz</unit><ucd>em.freq</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_CFreq</name><description>Uncertainty in CFreq</description><unit>MHz</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>LStr</name><description>Line strength; see text for details</description><unit>D**2</unit><ucd>spect.line.intensity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E</name><description>Lower state energy (3)</description><unit>cm**-1</unit><ucd>phys.energy;phys.atmol.level</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ref</name><description>Reference(s) (4)</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>f_LNum</name><description>[BC] Flag on line (5)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column></table><table><name>J/ApJS/190/315/table2</name><description>Torsion-Rotation parameters needed for the global fit of transitions involving v_t_=0 and v_t_=1 torsional energy levels of H^13^COOCH_3_</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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