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<ri:Resource created="2006-01-28T11:53:11Z" 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>byH{alpha} photometry of NGC 3766</title><shortName>J/ApJ/622/1052</shortName><identifier>ivo://CDS.VizieR/J/ApJ/622/1052</identifier><altIdentifier>doi:10.26093/cds/vizier.16221052</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>McSwain M.V.</name></creator><creator><name>Gies D.R.</name></creator><date role="Updated">2017-10-09T13:34:19Z</date><date role="Created">2006-01-28T11:53:11Z</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>open-star-clusters</subject><subject>be-stars</subject><subject>visible-astronomy</subject><subject>medium-band-photometry</subject><subject>h-alpha-photometry</subject><description>We describe a technique to identify Be stars in open clusters using Stroemgren b, y, and narrowband H{alpha} photometry. We first identify the B-type stars of the cluster using a theoretical isochrone fit to the (b-y, y) color-magnitude diagram. The strongest Be stars are easily identified in a (b-y, y-H{alpha}) color-color diagram, but those with weaker H{alpha} emission (classified as possible Be star detections) may be confused with evolved or foreground stars. Here we present such photometry plus H{alpha} spectroscopy of members of the cluster NGC 3766 to demonstrate the accuracy of our technique.</description><source format="bibcode">2005ApJ...622.1052M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/622/1052</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/A+AS/119/271">J/A+AS/119/271 : Be stars uvby{beta} photometry (Fabregat+, 1996)</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/ApJ/622/1052</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/622/1052</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/622/1052</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/622/1052</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/622/1052</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/622/1052</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/ApJ/622/1052/table1 (Photometry of NGC 3766)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/622/1052/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/622/1052/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/622/1052/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>173.9969167</ra><dec>-61.4873056</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/37901 37912</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/622/1052?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/622/1052/table1</name><description>Photometry of NGC 3766</description><column><name>Code</name><description>Stellar type (1)</description><dataType xsi:type="vs:VOTableType" arraysize="3*">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>Seq</name><description>Star identification number in NGC 3766</description><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RAJ2000</name><description>Hour of Right Ascension (J2000)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Degree of Declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>ymag</name><description>Stromgren y band magnitude</description><unit>mag</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_ymag</name><description>Error in ymag</description><unit>mag</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>b-y</name><description>Stromgren (b-y) color index</description><unit>mag</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_b-y</name><description>Error in b-y</description><unit>mag</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>y-Ha</name><description>The (y-H{alpha}) color index</description><unit>mag</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_y-Ha</name><description>Error in y-Ha</description><unit>mag</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>WEBDA</name><description>? 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