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<ri:Resource created="2005-04-19T20:53:13Z" 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>Rest frequencies of methanol maser lines</title><shortName>J/A+A/428/1019</shortName><identifier>ivo://CDS.VizieR/J/A+A/428/1019</identifier><altIdentifier>doi:10.26093/cds/vizier.34281019</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Mueller H.S.P.</name></creator><creator><name>Menten K.M.</name></creator><creator><name>Maeder H.</name></creator><date role="Updated">2005-04-19T20:53:22Z</date><date role="Created">2005-04-19T20:53:13Z</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>astrophysical-masers</subject><subject>radio-astronomy</subject><subject>molecular-clouds</subject><description>We report accurate laboratory measurements of selected methanol transition frequencies between 0.834 and 230GHz in order to facilitate astronomical velocity analyses. New data have been obtained between 10 and 27GHz and between 60 and 119GHz. Emphasis has been put on known or potential interstellar maser lines as well as on transitions suitable for the investigation of cold dark clouds. Because of the narrow line widths (&lt;0.5km/s) of maser lines and lines detected in dark molecular clouds, accurate frequencies are needed for comparison of the velocities of different methanol lines with each other as well as with lines from other species. In particular, frequencies for a comprehensive set of transitions are given which, because of their low energy levels (&lt;20cm^-1^ or 30K), are potentially detectable in cold clouds. Global Hamiltonian fits generally do not yet yield the required accuracy. Additionally, we report transition frequencies for other lines that may be used to test and to improve existing Hamiltonian models.</description><source format="bibcode">2004A&amp;A...428.1019M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/428/1019</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/413/233">J/A+A/413/233 : 12.2 GHz methanol survey (Blaszkiewicz+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/432/737">J/A+A/432/737 : General Catalogue of 6.7GHz Methanol Masers (Pestalozzi+ 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/134/115">J/A+AS/134/115 : Medicina 6.7GHz methanol masers survey (Slysh+ 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/143/269">J/A+AS/143/269 : 6.7GHz methanol maser emission survey (Szymczak+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AZh/72/22">J/AZh/72/22 : A 95 GHz Survey of Methanol Masers (Valtts+, 1995)</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/428/1019</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/428/1019</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/428/1019</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/428/1019</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/428/1019</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/428/1019</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/A+A/428/1019/table1</name><description>Methanol maser transitions</description><column><name>Class</name><description>Maser type (1)</description><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><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Note</name><description>[g] g: lines discussed in Sect. 4.3 of the paper</description><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Trans</name><description>Transition, J_k_ (2)</description></column><column><name>n_Trans</name><description>[*] Note on Trans (7)</description><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Freq</name><description>Frequency</description><unit>MHz</unit><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Freq</name><description>Measurement uncertainty</description><unit>MHz</unit><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>n_Freq</name><description>[h] Note on Freq (3)</description><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Elow</name><description>Lower state energy (4)</description><unit>cm**-1</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Smu2</name><description>Line strength, S{mu}^2^ (D^2^)</description><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ref(1)</name><description>Laboratory reference</description><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>Ref(2)</name><description>Astronomical (table1) or dark cloud (table2) reference (5)</description><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>n_Ref(2)</name><description>[* ND NO I] Note on Ref(2) (6)</description><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column></table><table><name>J/A+A/428/1019/table2</name><description>Accurately known methanol transitions detected or potentially detectable in dark clouds</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Class</name><description>Maser type (1)</description><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>Note</name><description>[g] g: lines discussed in Sect. 4.3 of the paper</description><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Trans</name><description>Transition, J_k_ (2)</description></column><column><name>n_Trans</name><description>[*] Note on Trans (7)</description><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Freq</name><description>Frequency</description><unit>MHz</unit><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Freq</name><description>Measurement uncertainty</description><unit>MHz</unit><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>n_Freq</name><description>[h] Note on Freq (3)</description><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Elow</name><description>Lower state energy (4)</description><unit>cm**-1</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Smu2</name><description>Line strength, S{mu}^2^ (D^2^)</description><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ref(1)</name><description>Laboratory reference</description><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>Ref(2)</name><description>Astronomical (table1) or dark cloud (table2) reference (5)</description><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>n_Ref(2)</name><description>[* ND NO I] Note on Ref(2) (6)</description><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column></table><table><name>J/A+A/428/1019/refs</name><description>References</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Ref</name><description>Reference code</description><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>BibCode</name><description>BibCode</description><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>Aut</name><description>Author's name</description><dataType xsi:type="vs:VOTableType" arraysize="24*">char</dataType></column><column><name>Com</name><description>Comments</description><dataType xsi:type="vs:VOTableType" arraysize="117*">char</dataType></column></table><table><name>J/A+A/428/1019/table3</name><description>Other methanol transitions measured in the course of the present investigation</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Vt</name><description>[0/1] Torsional state</description><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Trans</name><description>Transition</description></column><column><name>Freq</name><description>Frequency</description><unit>MHz</unit><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Freq</name><description>rms uncertainty on Freq</description><unit>MHz</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>n_Freq</name><description>[xT] Note on Freq (1)</description><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Note</name><description>[ND NO U] Note (2)</description><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column></table></schema></tableset></ri:Resource>