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<ri:Resource created="2015-06-22T08:57:00Z" 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>The GUViCS FUV diffuse emission</title><shortName>J/A+A/579/A29</shortName><identifier>ivo://CDS.VizieR/J/A+A/579/A29</identifier><altIdentifier>doi:10.26093/cds/vizier.35790029</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Boissier S.</name></creator><creator><name>Boselli A.</name></creator><creator><name>Voyer E.</name></creator><creator><name>Bianchi S.</name></creator><creator><name>Pappalardo C.,Guhathakurta P.</name></creator><creator><name>Heinis S.</name></creator><creator><name>Cortese L.</name></creator><creator><name>Duc P.-A.</name></creator><creator><name>Cuillandre J.-C.,Davies J.I.</name></creator><creator><name>Smith M.W.L.</name></creator><date role="Updated">2018-09-29T16:36:48Z</date><date role="Created">2015-06-22T08:57:00Z</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>ultraviolet-astronomy</subject><subject>extinction</subject><description>The Virgo direction has been observed at many wavelengths in recent years, in particular in the ultraviolet with GALEX. The far ultraviolet (FUV) diffuse light detected by GALEX offers interesting information on the large scale distribution of Galactic dust, owing to the GALEX FUV band sensitivity and resolution. We aim to characterise the ultraviolet large scale distribution of diffuse emission in the Virgo direction. A map of this emission may become useful for various studies by identifying regions where dust affects observations by either scattering light or absorbing radiation.</description><source format="bibcode">2015A&amp;A...579A..29B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/579/A29</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/J/A+A/528/A107">J/A+A/528/A107 : GALEX Ultraviolet Virgo Cluster Survey, GUViCS (Boselli+ 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/569/A124">J/A+A/569/A124 : GUViCS. Ultraviolet Source Catalogs (Voyer+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/570/A69">J/A+A/570/A69 : GALEX Ultraviolet Virgo Cluster Survey. IV. 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