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<ri:Resource created="2000-03-29T20:46:45Z" 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>Galaxies morphology and IR photometry II.</title><shortName>J/A+AS/120/521</shortName><identifier>ivo://CDS.VizieR/J/A+AS/120/521</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Gavazzi G.</name></creator><creator><name>Pierini D.</name></creator><creator><name>Baffa C.</name></creator><creator><name>Lisi F.</name></creator><creator><name>Hunt L.K.</name></creator><creator><name>Randone I.,Boselli A.</name></creator><date role="Updated">2013-03-06T06:34:40Z</date><date role="Created">2000-03-29T20:46:45Z</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><description>We present near-infrared H-band (1.65{mu}m) surface photometry of 297 galaxies (mostly) in the Coma Supercluster obtained with the Arcetri NICMOS3 camera, ARNICA, mounted on the Gornergrat Infrared Telescope. Magnitudes and diameters within the 21.5mag/arcsec^2^ isophote, concentration indices, and total H magnitudes are derived. Combining these observations with those obtained similarly using the Calar Alto telescopes (Paper I, &lt;J/A+AS/120/489&gt;) we find a strong positive correlation between the near-infrared concentration index and the galaxy H-band luminosity, and we analyze the consequent dependence of near-infrared growth-curves on H-band luminosity. For a description of the H band photometric system, see e.g. &lt;GCPD/59&gt;</description><source format="bibcode">1996A&amp;AS..120..521G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+AS/120/521</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+AS/120/489">J/A+AS/120/489 : Galaxies morphology and IR photometry I. (Gavazzi+ 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/142/65">J/A+AS/142/65 : Galaxies morphology and IR photometry III. (Gavazzi+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/142/73">J/A+AS/142/73 : Galaxies morphology and IR photometry IV. (Boselli+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/361/863">J/A+A/361/863 : Galaxies morphology and IR photometry V. 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