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<ri:Resource created="2002-07-16T10:47:13Z" 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>FAUST observations in 4th Galactic Quadrant</title><shortName>J/MNRAS/313/641</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/313/641</identifier><altIdentifier>doi:10.26093/cds/vizier.73130641</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Brosch N.</name></creator><creator><name>Brook A.</name></creator><creator><name>Wisotzki L.</name></creator><creator><name>Almoznino E.</name></creator><creator><name>Prialnik D.</name></creator><creator><name>Bowyer S.,Lampton M.</name></creator><date role="Updated">2024-06-26T20:16:32Z</date><date role="Created">2002-07-16T10:47:13Z</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-astronomy</subject><subject>galaxies</subject><subject>photometry</subject><subject>ultraviolet-photometry</subject><description>The UV observations of FAUST are analysed in four sky fields (Dor, Cen, M81 and Tel), located in the general direction of the Fourth Galactic Quadrant, where 777 UV sources are detected, about 50% more than detected originally by Bowyer et al. (1993ApJ...415..875B). Ground-based objective-prism information for two of the fields were used to select the best-matching optical objects with which to identify the UV sources. Using this, and correlations with existing catalogues, reliable identifications are presented for about 75% of the sources. Most of the remaining sources have assigned optical counterparts but, lacking additional information, we offer only plausible identifications. FAUST is a wide-field telescope (7.6{deg} diameter) designed to image diffuse and point sources in the wavelength range 140-180nm. The experiment, the mission and the data are described in a previous paper by Bowyer et al., 1993ApJ...415..875B .</description><source format="bibcode">2000MNRAS.313..641B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/313/641</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/VI/99">VI/99 : Merged Log of IUE Observations (NASA-ESA, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/324/580">J/MNRAS/324/580 : FAUST sources toward NGC 4038-39 and 6752 (Daniels+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/332/441">J/MNRAS/332/441 : Hidden subluminous stars among UV sources (Formiggini+ 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/96/461">J/ApJS/96/461 : FAUST Far-UV Point Sources (Bowyer+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/111/143">J/ApJS/111/143 : Virgo cluster ultraviolet sources (Brosch+ 1997)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/313/641</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/313/641</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/313/641</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL 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47367 47371 47373-47377 47379 47393 47395 47401 47403 47420-47422 47456 47458 47493 47504-47505</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/313/641?format=ascii</footprint><waveband>UV</waveband><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/MNRAS/313/641/table2</name><description>Detected UV sources</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[BBW2000]</name><description>Source name (G1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType><flag>primary</flag></column><column><name>RAJ2000</name><description>Right ascension (J2000) (1)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000) (1)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>UVmag</name><description>UV magnitude (140-180nm)</description><unit>mag</unit><ucd>phot.mag;em.UV</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_UVmag</name><description>rms uncertainty on UVmag</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>FAUST</name><description>? FAUST number</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>n_FAUST</name><description>Last digit for double FAUST number or ? if unknown FAUST number</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column></table><table><name>J/MNRAS/313/641/table4</name><description>Identification of UV sources</description><column><name>NameID</name><description>Catalogue identifier for the proposed counterpart</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="24*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[BBW2000]</name><description>Source name (G1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>m_[BBW2000]</name><description>[ab] Multiplicity index on [BBW2000]</description><ucd>meta.code.multip</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>n_Vmag</name><description>[B] B if USNO `blue' magnitude in Vmag</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Vmag</name><description>? 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