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<ri:Resource created="2012-08-13T13:30:28Z" 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>The submillimeter spectrum of glycolaldehyde</title><shortName>J/ApJ/723/845</shortName><identifier>ivo://CDS.VizieR/J/ApJ/723/845</identifier><altIdentifier>doi:10.26093/cds/vizier.17230845</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Carroll P.B.</name></creator><creator><name>Drouin B.J.</name></creator><creator><name>Widicus Weaver S.L.</name></creator><date role="Updated">2012-08-31T10:17:50Z</date><date role="Created">2012-08-13T13:30:28Z</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>radio-spectroscopy</subject><subject>atomic-physics</subject><description>Glycolaldehyde (HOCH_2_CHO) is a sugar-related interstellar prebiotic molecule that has been detected in two star-forming regions, Sgr B2(N) and G31.41+0.31. Glycolaldehyde is suspected to form from photodissociation-driven ice chemistry, and therefore can be used to trace complex organic chemistry in interstellar environments. The relative abundance of glycolaldehyde to its structural isomers, methyl formate (HCOOCH_3_) and acetic acid (CH_3_COOH), can be used to constrain astrochemical models. Given its central role in the complex chemistry of the interstellar medium, glycolaldehyde has been suggested as a prime molecular target for upcoming high-frequency molecular line searches using new far-infrared observatories. In particular, glycolaldehyde is a target for the Herschel Space Observatory HEXOS Key Program, which is conducting spectral line surveys of the Sgr B2(N) and Orion KL star-forming regions across the entire HIFI band. Laboratory investigation of glycolaldehyde in the HIFI frequency range is required before its lines can be identified in these spectra. We have therefore acquired the laboratory spectrum of glycolaldehyde in selected frequency ranges across the submillimeter range. We present here the laboratory spectral analysis of the ground vibrational state of glycolaldehyde up to 1.2THz.</description><source format="bibcode">2010ApJ...723..845C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/723/845</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/540/A51">J/A+A/540/A51 : Submm spectrum of deuterated glycolaldehydes (Bouchez+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/158/188">J/ApJS/158/188 : Detection of glycolaldehyde toward Sgr B2 (Widicus+, 2005)</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/723/845</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/723/845</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/723/845</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/723/845</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/723/845</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/723/845</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/723/845/table2</name><description>Assigned transitions for the the ground vibrational state of glycolaldehyde (O=CH-CH_2_-OH)</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>J'</name><description>[1/63] Upper J level</description><ucd>instr.det.qe;phys.mol.rotation</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Ka'</name><description>[0/32] Upper K_a_ level</description><ucd>phys.atmol.qn;phys.mol.rotation</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Kc'</name><description>[0/60] Upper K_c_ level</description><ucd>phys.atmol.qn;phys.mol.rotation</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>J"</name><description>[0/62] Lower J level</description><ucd>instr.det.qe;phys.mol.rotation</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Ka"</name><description>[0/31] Lower K_a_ level</description><ucd>phys.atmol.qn;phys.mol.rotation</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Kc"</name><description>[0/59] Lower K_c_ level</description><ucd>phys.atmol.qn;phys.mol.rotation</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Freq</name><description>Frequency observed (mean error is +/-0.1MHz)</description><unit>MHz</unit><ucd>stat.error;em.freq</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>O-C</name><description>Observed - Calculated frequency</description><unit>MHz</unit><ucd>stat.fit.residual</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Int</name><description>? Intensity weighting for blended lines</description><ucd>stat.weight</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>