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<ri:Resource created="1999-05-01T22:22:59Z" 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>1.49 GHz atlas of the IRAS bright galaxies</title><shortName>J/ApJS/73/359</shortName><identifier>ivo://CDS.VizieR/J/ApJS/73/359</identifier><altIdentifier>doi:10.26093/cds/vizier.20730359</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Condon J.J.</name></creator><creator><name>Helou G.</name></creator><creator><name>Sanders D.B.</name></creator><creator><name>Soifer B.T.</name></creator><date role="Updated">2013-03-05T06:37:27Z</date><date role="Created">1999-05-01T22:22:59Z</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>radio-continuum-emission</subject><subject>infrared-sources</subject><subject>galaxies</subject><subject>radio-galaxies</subject><description>This catalog contains 1.49 GHz VLA observations of sources from the IRAS Bright Galaxy Sample. The original IRAS Bright Galaxy Sample (Soifer et al., 1987ApJ...320..238S) comprises 324 extragalactic objects with 60 micron flux densities above 5.4 Jy. It is the infrared analog of the radio 3CR or optical Shapley-Ames samples. Recalibration of the IRAS flux densities led to a revised Bright Galaxy Sample (Soifer et al., 1989AJ.....98..766S) containing 313 sources stronger than 5.24 Jy at 60 microns. Only one source from these samples was not detected (NGC1377) at 1.49 GHz. For most sources, multiple observations were conducted with different synthesized beam areas. Thus, for a given galaxy there may be several rows in the table reporting data at different angular resolution or reporting different radio components of the object. A low-resolution observation was used to yield an accurate total flux density and a high-resolution observation was used to resolve the brightest components clearly. 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Radio minus infrared declination offset (6)</description><unit>arcsec</unit><ucd>pos.eq.dec;arith.diff</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>S1.49p</name><description>? Peak flux density at 1.49 GHz (7)</description><unit>mJy</unit><ucd>phot.flux.density;em.radio.750-1500MHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>S1.49i</name><description>? Integrated flux density at 1.49 GHz (7)</description><unit>mJy</unit><ucd>phot.flux.density;em.radio.750-1500MHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>l_MajAxis</name><description>[ &lt;] Flagged if major axis is an upper limit (8)</description><ucd>meta.code.error;phys.angSize</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>MajAxis</name><description>? 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