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<ri:Resource created="1997-12-09T21:03:39Z" 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>UIT near-UV bright objects catalog</title><shortName>J/ApJS/104/287</shortName><identifier>ivo://CDS.VizieR/J/ApJS/104/287</identifier><altIdentifier>doi:10.26093/cds/vizier.21040287</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Smith E.P.</name></creator><creator><name>Pica A.J.</name></creator><creator><name>Bohlin R.C.</name></creator><creator><name>Cornett R.H.</name></creator><creator><name>Fanelli M.N.,Landsman W.B.</name></creator><creator><name>O'Connell R.W.</name></creator><creator><name>Roberts M.S.</name></creator><creator><name>Smith A.M.</name></creator><creator><name>Stecher T.P.</name></creator><date role="Updated">1997-12-09T20:03:45Z</date><date role="Created">1997-12-09T21:03:39Z</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>ultraviolet-photometry</subject><description>We present a photometric catalog of 2244 objects detected by the Ultraviolet Imaging Telescope in the near-ultraviolet (NUV; 1650A&lt;lambda&lt;2900A) during the Astro-1 Space Shuttle mission. Sources in the catalog are as faint as m_nuv~18.8, or f_nuv~1.1x10^-16ergs/s/cm^2/A, but the survey is not complete to this level. Optical catalogs were used to cross identify sources and derive NUV-V colors. A majority of the objects (88%) do indeed have proposed optical identifications from catalogs, and most are stars. 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