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<ri:Resource created="1997-12-09T19:41:07Z" 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>NGC 2366, NGC 2403 &amp; NGC 4236 HK' photometry</title><shortName>J/A+AS/125/293</shortName><identifier>ivo://CDS.VizieR/J/A+AS/125/293</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Pierini D.</name></creator><creator><name>Gavazzi G.</name></creator><creator><name>Boselli A.</name></creator><creator><name>Tuffs R.</name></creator><date role="Updated">1997-12-09T18:41:10Z</date><date role="Created">1997-12-09T19:41:07Z</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>galaxies</subject><subject>photometry</subject><subject>infrared-photometry</subject><description>Near Infrared H and K' surface photometry of the three nearby galaxies NGC 2366, NGC 2403 and NGC 4236, used as local calibrators of the Tully-Fisher relation, was obtained using the 256^2^ NICMOS3 IR array MAGIC attached to the 2.2 m telescope of Calar Alto. The present measurements are compared with the aperture photometry available in the literature. Surface brightness profiles and integrated magnitudes are given.</description><source format="bibcode">1997A&amp;AS..125..293P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+AS/125/293</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</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/125/293</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+AS/125/293</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+AS/125/293</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+AS/125/293</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+AS/125/293</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+AS/125/293</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>Optical</waveband><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+AS/125/293/table4</name><description>Differential and integrated magnitudes derived along elliptical annuli</description><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>NGC</name><description>NGC name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>PA</name><description>Position angle of the galaxy major axis (measured Eastwards from North)</description><unit>deg</unit><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Eps</name><description>Ellipticity (1-(b/a)) of the rings</description><ucd>src.ellipticity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Rad</name><description>Major semiaxis of the elliptical annulus</description><unit>arcsec</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SuBrH</name><description>? H band surface brightness</description><unit>mag/arcsec</unit><ucd>phot.mag.sb;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Hmag</name><description>? Integrated H magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SuBrK'</name><description>? K' band surface brightness</description><unit>mag/arcsec</unit><ucd>phot.mag.sb;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>K'mag</name><description>? Integrated K' magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>