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<ri:Resource created="2002-08-06T21:35:55Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>UBV photometry of V899 Her</title><shortName>J/A+A/387/240</shortName><identifier>ivo://CDS.VizieR/J/A+A/387/240</identifier><altIdentifier>doi:10.26093/cds/vizier.33870240</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ozdemir S.</name></creator><creator><name>Demircan O.</name></creator><creator><name>Erdem A.</name></creator><creator><name>Cicek C.</name></creator><creator><name>Bulut I.</name></creator><creator><name>Soydugan F.,Soydugan E.</name></creator><date role="Updated">2002-08-06T21:36:14Z</date><date role="Created">2002-08-06T21:35:55Z</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>eclipsing-binary-stars</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><description>The data file (v899her.dat) includes photometric observations of the eclipsing binary system V899 Herculis. The observations were carried out at the Ankara University Observatory in Johnson UBV filters by using an SSP-5 photometer head attached to the 30-cm Maksutov telescope of the Observatory. Observational standard errors are 0.020m, 0.016m, and 0.021m in U, B, and V filters, respectively. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>HJDU</name><description>? Heliocentric Julian Day obtained in U filter</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>DUmag</name><description>? Differential magnitude in U filter (1)</description><unit>mag</unit><ucd>phot.mag;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>HJDB</name><description>Heliocentric Julian Day obtained in B filter</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>DBmag</name><description>Differential magnitude in B filter (1)</description><unit>mag</unit><ucd>phot.mag;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>HJDV</name><description>? Heliocentric Julian Day obtained in V filter</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>DVmag</name><description>? Differential magnitude in V filter (1)</description><unit>mag</unit><ucd>phot.mag;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>