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<ri:Resource created="1999-02-27T20:25:14Z" 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>Magellanic clouds ultraviolet observations</title><shortName>J/AJ/116/180</shortName><identifier>ivo://CDS.VizieR/J/AJ/116/180</identifier><altIdentifier>doi:10.26093/cds/vizier.51160180</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Parker J.W.</name></creator><creator><name>Hill J.K.</name></creator><creator><name>Cornett R.H.</name></creator><creator><name>Hollis J.</name></creator><creator><name>Zamkoff E.</name></creator><creator><name>Bohlin R.C.,O'Connell R.W.</name></creator><creator><name>Neff S.G.</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">2023-04-06T16:50:30Z</date><date role="Created">1999-02-27T20:25:14Z</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>magellanic-clouds</subject><subject>ultraviolet-photometry</subject><description>The catalog is derived from wide-field far-ultraviolet (FUV; 1300-1800{AA}) images of the Large and Small Magellanic Clouds (LMC, SMC) obtained by the Ultraviolet Imaging Telescope (UIT) during the Astro-1 (1990 December 1-10) and Astro-2 (1995 March 2-18) missions. The FUV magnitudes are derived from point-spread function photometry for 37,333 stars in the LMC (the UIT FUV magnitudes for 11,306 stars in the SMC were presented by Cornett et al. (1997AJ....113.1011C), with a completeness limit of m_UV_ ~ 15mag and a detection limit of m_UV_ ~ 17.5. 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