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<ri:Resource created="2007-02-08T11:42:50Z" 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>IR fluxes of solar-type stars</title><shortName>J/ApJ/555/932</shortName><identifier>ivo://CDS.VizieR/J/ApJ/555/932</identifier><altIdentifier>doi:10.26093/cds/vizier.15550932</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Spangler C.</name></creator><creator><name>Sargent A.I.</name></creator><creator><name>Silverstone M.D.</name></creator><creator><name>Becklin E.E.</name></creator><creator><name>Zuckerman B.</name></creator><date role="Updated">2022-05-11T09:32:56Z</date><date role="Created">2007-02-08T11:42:50Z</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>pre-main-sequence-stars</subject><subject>infrared-sources</subject><description>Using ISO-ISOPHOT, we carried out a survey of almost 150 stars to search for evidence of emission from dust orbiting young main-sequence stars, both in clusters and isolated systems. Over half of the detections are new examples of dusty stellar systems and demonstrate that such dust can be detected around numerous stars older than a few times 10^6^yr. Fluxes at 60 and either 90 or 100{mu}m or the new excess sources together with improved fluxes for a number of IRAS-identified sources are presented. 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IRAS flux density at 12{mu}m</description><unit>mJy</unit><ucd>phot.flux.density;em.IR.8-15um</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>l_S25um1</name><description>Limit flag on S25um1</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>S25um1</name><description>? IRAS flux density at 25{mu}m</description><unit>mJy</unit><ucd>phot.flux.density;em.IR.15-30um</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>l_S60um1</name><description>Limit flag on S60um1</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>S60um1</name><description>? IRAS flux density at 60{mu}m</description><unit>mJy</unit><ucd>phot.flux.density;em.IR.30-60um</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>l_S100um1</name><description>Limit flag on S100um1</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">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>Field</name><description>Field (1)</description><ucd>obs.field</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">char</dataType></column><column><name>Name</name><description>Target name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>l_S12um1</name><description>Limit flag on S12um1</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>S100um1</name><description>? IRAS flux density at 100{mu}m</description><unit>mJy</unit><ucd>phot.flux.density;em.IR.60-100um</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>l_S60um2</name><description>Limit flag on S60um2</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>S60um2</name><description>ISO flux density at 60{mu}m (2)</description><unit>mJy</unit><ucd>phot.flux.density;em.IR.30-60um</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>l_S90um2</name><description>Limit flag on S90um2</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>S90um2</name><description>ISO flux density at 90{mu}m (2)</description><unit>mJy</unit><ucd>phot.flux.density;em.IR.60-100um</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>n_S90um2</name><description>[b] if chopped upper limit at 100{mu}m</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>fd</name><description>Factional excess luminosity</description><ucd>phys.luminosity;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Notes</name><description>? Notes in notes.dat file</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>IRAS</name><description>Display the data of the IRAS sources close to this position</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>_RA</name><description>Right Ascension (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Declination (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table><table><name>J/ApJ/555/932/notes</name><description>Notes to tables 6 and 7</description><column><name>Note</name><description>Note number</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType">int</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>Text</name><description>Text of the note</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="77*">char</dataType></column></table></schema></tableset></ri:Resource>