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<ri:Resource created="2006-09-25T08:55:15Z" 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 UV sources towards Ophiuchus</title><shortName>J/MNRAS/332/441</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/332/441</identifier><altIdentifier>doi:10.26093/cds/vizier.73320441</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Formiggini L.</name></creator><creator><name>Brosch N.</name></creator><creator><name>Almoznino E.</name></creator><creator><name>Bowyer S.</name></creator><creator><name>Lampton M.</name></creator><date role="Updated">2024-06-27T20:18:12Z</date><date role="Created">2006-09-25T08:55:15Z</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>white-dwarf-stars</subject><subject>ultraviolet-astronomy</subject><subject>photometry</subject><subject>visible-astronomy</subject><subject>trigonometric-parallax</subject><subject>proper-motions</subject><description>We present results of an analysis of a UV image in the direction of Ophiuchus, obtained with the FAUST instrument. The image contains 228 UV sources. Most of these are identified as normal early-type stars through correlations with catalogued objects. For the first time in this project we identify UV sources as such stars by selecting suitable candidates in crowded fields as the bluest objects in colour-colour diagrams using observations from the Wise Observatory. These candidates are then studied using low-resolution spectroscopy, which allows the determination of spectral types to an accuracy of about one-half class, for 60 stars. Synthetic photometry of spectral data is performed in order to predict the expected UV emission, on the basis of the photometric information. These results are used along with the Hipparcos/Tycho (&lt;I/239&gt;) information, to search for subluminous stars. The comparison of the predicted emission with the FAUST measured magnitudes allows us to select 12 stars as highly probable evolved hot stars. High signal-to-noise spectra are obtained for nine of these stars, and Balmer line profiles are compared with the prediction of atmosphere models and with the spectrum of real stellar atmospheres. Among the nine candidates, six are classified as previously unrecognized sdB stars, and two as white dwarfs. Our result indicates that indeed more bright subluminous stars are still unrecognized in the existing samples.</description><source format="bibcode">2002MNRAS.332..441F</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/332/441</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/I/239">I/239 : The Hipparcos and Tycho Catalogues (ESA 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/372/173">J/A+A/372/173 : ISOCAM observations of rho Ophiuchi cloud (Bontemps+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/438/813">J/ApJ/438/813 : Stellar population in {rho} Oph cloud core (Strom+, 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/566/993">J/ApJ/566/993 : HST/NICMOS survey of Ophiuchus cloud (Allen+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/96/461">J/ApJS/96/461 : Far-UV Point Sources from FAUST (Bowyer+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/104/101">J/ApJS/104/101 : Far-UV stellar photometry (Schmidt+, 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/112/109">J/ApJS/112/109 : Rho Oph Near IR Positions and Photometry (Barsony+, 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/316/326">J/MNRAS/316/326 : Redshifts of Ophiuchus region galaxies (Hasegawa+, 2000)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL 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29329 29341 29384-29385 29387-29389 29392-29394</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/332/441?format=ascii</footprint><waveband>UV</waveband><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/MNRAS/332/441/table1</name><description>Derived FAUST sources in the Ophiuchus field</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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