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<ri:Resource created="2016-08-02T15:55:08Z" 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>CH_3_CH_2_SH detection in Orion KL</title><shortName>J/ApJ/784/L7</shortName><identifier>ivo://CDS.VizieR/J/ApJ/784/L7</identifier><altIdentifier>doi:10.26093/cds/vizier.17849007</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kolesnikova L.</name></creator><creator><name>Tercero B.</name></creator><creator><name>Cernicharo J.</name></creator><creator><name>Alonso J.L.</name></creator><creator><name>Daly A.M.,Gordon B.P.</name></creator><creator><name>Shipman S.T.</name></creator><date role="Updated">2017-01-23T22:00:00Z</date><date role="Created">2016-08-02T15:55:08Z</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>spectroscopy</subject><subject>radio-spectroscopy</subject><subject>radio-astronomy</subject><description>New laboratory data of ethyl mercaptan, CH_3_CH_2_SH, in the millimeter- and submillimeter-wave domains (up to 880GHz) provided very precise values of the spectroscopic constants that allowed the detection of gauche-CH_3_CH_2_ SH toward Orion KL. This identification is supported by 77 unblended or slightly blended lines plus no missing transitions in the range 80-280GHz. A detection of methyl mercaptan, CH_3_SH, in the spectral survey of Orion KL is reported as well. Our column density results indicate that methyl mercaptan is {=~}5 times more abundant than ethyl mercaptan in the hot core of Orion KL.</description><source format="bibcode">2014ApJ...784L...7K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/784/L7</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/572/A44">J/A+A/572/A44 : Vibrationally excited vinyl cyanide in Orion-KL (Lopez+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/779/119">J/ApJ/779/119 : HCOOCH_2_D detection in Orion KL (Coudert+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/770/L13">J/ApJ/770/L13 : Detection of CH_3_COOCH_3_ in Orion (Tercero+, 2013)</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/559/A47">J/A+A/559/A47 : Sgr B2(N) and Sgr B2(M) IRAM 30m line survey (Belloche+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/532/A32">J/A+A/532/A32 : HCOOCH3 map of Orion-KL (Favre+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/714/1120">J/ApJ/714/1120 : Rotational spectrum and DCOOCH3 in Orion (Margules+, 2010)</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/784/L7</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/784/L7</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/784/L7</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/784/L7</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/784/L7</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/784/L7</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/ApJ/784/L7/table2</name><description>*Laboratory measurements and astronomically detected lines of ethyl mercaptan</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>[1/89] Upper J quantum number (J')</description><ucd>phys.atmol.qn</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Ka1</name><description>[0/25] Upper K_a_ quantum number (K'_a_)</description><ucd>phys.mol.qn</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Kc1</name><description>[0/89] Upper K_c_ quantum number (K'_c_)</description><ucd>phys.mol.qn</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>v1</name><description>[0/1]? 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