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<ri:Resource created="2013-10-21T13:49:17Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" 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/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd 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>Far-IR study of G29.96-0.02</title><shortName>J/A+A/552/A123</shortName><identifier>ivo://CDS.VizieR/J/A+A/552/A123</identifier><altIdentifier>doi:10.26093/cds/vizier.35520123</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Beltran M.T.</name></creator><creator><name>Olmi L.</name></creator><creator><name>Cesaroni R.</name></creator><creator><name>Schisano E.</name></creator><creator><name>Elia D.</name></creator><creator><name>Molinari S.,Di Giorgio A.M.</name></creator><creator><name>Kirk J.M.</name></creator><creator><name>Mottram J.C.</name></creator><creator><name>Pestalozzi M.</name></creator><creator><name>Testi L.,Thompson M.A.</name></creator><date role="Updated">2017-10-13T15:42:11Z</date><date role="Created">2013-10-21T13:49:17Z</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>h-ii-regions</subject><subject>millimeter-astronomy</subject><subject>photometry</subject><subject>submillimeter-astronomy</subject><description>G29.96-0.02 is a high-mass star-forming cloud observed at 70, 160, 250, 350, and 500{mu}m as part of the Herschel survey of the Galactic plane (Hi-GAL) during the science demonstration phase. We wish to conduct a far-infrared study of the sources associated with this star-forming region by estimating their physical properties and evolutionary stage, and investigating the clump mass function, the star formation efficiency and rate in the cloud. 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ivo-id="ivo://CDS.VizieR/J/MNRAS/422/1071">J/MNRAS/422/1071 : Cores in IR Dark Clouds for 300&lt;=l&lt;=330 (Wilcock+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/537/A1">J/A+A/537/A1 : Infrared fluxes of HII regions and PNe (Anderson+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/549/A130">J/A+A/549/A130 : YSOs in Herschel-Hi-GAL survey (Veneziani+, 2013)</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/552/A123</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/552/A123</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/552/A123</mirrorURL></interface></capability><capability><interface 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