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<ri:Resource created="2015-11-26T13:27:18Z" 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>Galactic cold cores. VI. List of Herschel fields</title><shortName>J/A+A/584/A94</shortName><identifier>ivo://CDS.VizieR/J/A+A/584/A94</identifier><altIdentifier>doi:10.26093/cds/vizier.35840094</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Juvela M.</name></creator><creator><name>Demyk K.</name></creator><creator><name>Doi Y.</name></creator><creator><name>Hughes A.</name></creator><creator><name>Lefevre C.</name></creator><creator><name>Marshall D.J.</name></creator><creator><name>Meny C.,Montillaud J.</name></creator><creator><name>Pagani L.</name></creator><creator><name>Paradis D.</name></creator><creator><name>Ristorcelli I.</name></creator><creator><name>Malinen J.,Montier L.A.</name></creator><creator><name>Paladini R.</name></creator><creator><name>Pelkonen V.-M.</name></creator><creator><name>Rivera-Ingraham A.</name></creator><date role="Updated">2017-12-22T05:33:11Z</date><date role="Created">2015-11-26T13:27:18Z</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><description>The Galactic Cold Cores project has carried out Herschel photometric observations of 116 fields where the Planck survey has found signs of cold dust emission. The fields contain sources in different environments and different phases of star formation. Previous studies have revealed variations in their dust submillimetre opacity. The aim is to measure the value of dust opacity spectral index and to understand its variations spatially and with respect to other parameters, such as temperature, column density, and Galactic location. The dust opacity spectral index {beta} and the dust colour temperature T are derived using Herschel and Planck data. The relation between {beta} and T is examined for the whole sample and inside individual fields.</description><source format="bibcode">2015A&amp;A...584A..94J</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/584/A94</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>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/VI/139">VI/139 : Herschel Observation Log (Herschel Science Centre, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/584/A92">J/A+A/584/A92 : Galactic cold cores. IV. Cold submm sources (Montillaud+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/584/A93">J/A+A/584/A93 : Galactic cold cores. V. 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