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I.</title><shortName>J/ApJS/143/277</shortName><identifier>ivo://CDS.VizieR/J/ApJS/143/277</identifier><altIdentifier>doi:10.26093/cds/vizier.21430277</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kim D.-C.</name></creator><creator><name>Veilleux S.</name></creator><creator><name>Sanders D.B.</name></creator><date role="Updated">2017-06-26T11:50:11Z</date><date role="Created">2006-07-21T14:14:54Z</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>seyfert-galaxies</subject><subject>infrared-sources</subject><subject>infrared-photometry</subject><description>An imaging survey of the IRAS 1Jy sample of 118 ultraluminous infrared galaxies was conducted at optical (R) and near-infrared (K') wavelengths using the University of Hawaii 2.2 m telescope. The methods of observation and data reduction are described. An R and K' atlas of the entire sample is presented along with some of the basic astrometric and photometric parameters derived from these images. 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