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<ri:Resource created="1997-12-09T19:09:04Z" 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>Hickson Compact Groups of Galaxies I.</title><shortName>J/A+AS/117/39</shortName><identifier>ivo://CDS.VizieR/J/A+AS/117/39</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Allam S.</name></creator><creator><name>Assendorp R.</name></creator><creator><name>Longo G.</name></creator><creator><name>Braun M.</name></creator><creator><name>Richter G.</name></creator><date role="Updated">1997-12-09T18:09:07Z</date><date role="Created">1997-12-09T19:09:04Z</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>galaxy-clusters</subject><subject>galaxies</subject><subject>infrared-sources</subject><description>The Far Infrared (FIR) properties of galaxies which are members of compact groups bear relevant information on the dynamical status and the physical properties of these structures. All studies published so far have been undermined by the poor sensitivity and spatial resolution of the IRAS-PSC and IRAS Sky Survey data. We used the HIRAS software available at the IRAS server at the Laboratory for Space Research in Groningen to fully exploit the redundancy of the IRAS data and to approach the theoretical diffraction limit of IRAS. Among the 97 groups which were observed by IRAS, 62 were detected in at least one band, while reliable upper limits were derived for all the others. Among the detected groups, 49 were fully or partially resolved, i.e. it was possible to discriminate which member or members emit most of the FIR light. At 60{mu}m, for instance, 87 individual sources were detected in 62 groups. In order to ease the comparison with data obtained at other wavelengths - and in particular in the X and radio domains - we give co-added and HIRAS maps for all the detected groups.</description><source format="bibcode">1996A&amp;AS..117...39A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+AS/117/39</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/VII/85">VII/85 : Catalogue of compact groups of galaxies (Hickson, 1982)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/125">II/125 : IRAS catalogue of Point Sources, Version 2.0 (IPAC 1986)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/380/30">J/ApJ/380/30 : LF of Compact Groups (Mendes de Oliveira+ 1991)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/399/353">J/ApJ/399/353 : Radial velocities in Hickson Compact Groups (Hickson+ 1992)</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+AS/117/39</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+AS/117/39</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+AS/117/39</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+AS/117/39</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+AS/117/39</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+AS/117/39</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>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+AS/117/39/table2</name><description>Flux and upper limits for galaxies which are members of the Hickson's Groups.</description><column><name>n_F60</name><description>Note on F60 (2)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>n_F100</name><description>Note on F100 (2)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>Com</name><description>Comments</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="31*">char</dataType></column><column><name>e_F100</name><description>? rms uncertainty on F100</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><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>HCG</name><description>Identification accordingly to Hickson (1982) (1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>Mtype</name><description>Morphological type of the galaxy accordingly to Hickson (1993)</description><ucd>src.morph.type</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>l_F12</name><description>Upper limit on F12</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>F12</name><description>? Flux at 12{mu}m</description><unit>Jy</unit><ucd>phot.flux.density;em.IR.8-15um</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>n_F12</name><description>Note on F12 (2)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>e_F12</name><description>? rms uncertainty on F12</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>l_F25</name><description>Upper limit on F25</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>F25</name><description>? Flux at 25{mu}m</description><unit>Jy</unit><ucd>phot.flux.density;em.IR.15-30um</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>n_F25</name><description>Note on F25 (2)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>e_F25</name><description>? rms uncertainty on F25</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>l_F60</name><description>Upper limit on F60</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>F60</name><description>? 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