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<ri:Resource created="1997-12-09T20:02:10Z" 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>Montreal Blue Galaxy Survey</title><shortName>J/AJ/105/35</shortName><identifier>ivo://CDS.VizieR/J/AJ/105/35</identifier><altIdentifier>doi:10.26093/cds/vizier.51050035</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>COZIOL R.</name></creator><creator><name>DEMERS S.</name></creator><creator><name>PENA M.</name></creator><creator><name>TORRES-PEIMBERT S.</name></creator><creator><name>FONTAINE G.,WESEMAEL F.</name></creator><creator><name>LAMONTAGNE R.</name></creator><date role="Updated">2023-04-06T16:49:27Z</date><date role="Created">1997-12-09T20:02:10Z</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>ultraviolet-sources</subject><description>We describe and present the first results of a UV-bright galaxy survey using the Montreal-Cambridge-Tololo (MCT) plate collection. Visual inspection of 57 CTIO Curtis Schmidt plates, covering more than 1300 sq. deg., has resulted in the identification of 95 UV-bright galaxies brighter than B = 15.5. Even though 80% of these objects are IRAS sources, barely 20% have their nature already established. The initial result of our survey shows that the bulk of our UV-bright candidates are narrow emission-line galaxies commonly known as starburst or HII galaxies. The fraction of AGNs found is somewhat less than 10%, but comparable to what has been found by the Markarian survey. We expect to find approximately 500 UV-bright galaxies in the 7000 sq. deg. of The MCT Survey with b &lt; -40 deg. As we go further south, a large number of bright new objects will be discovered.</description><source format="bibcode">1993AJ....105...35C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/105/35</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/108/405">J/AJ/108/405 : Montreal Blue Galaxy Survey. II. 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