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<ri:Resource created="2007-06-17T11:42:05Z" 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>Haffner 19 UBV(RI)_c_ photometry</title><shortName>J/other/RMxAA/38</shortName><identifier>ivo://CDS.VizieR/J/other/RMxAA/38.141</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Moreno-Corral M.A.</name></creator><creator><name>Chavarria-K C.</name></creator><creator><name>de Lara E.</name></creator><date role="Updated">2017-11-28T13:21:35Z</date><date role="Created">2007-06-17T11:42:05Z</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>ccd-photometry</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>Wide-band photometry</subject><description>We present broad-band UBV(RI)_c_ CCD imagery of 334 stars in the direction of the Galactic cluster Haffner 19. The sample is complete to m{lambda}=19 ({lambda} = U, B, V, R, I). We reliably establish the cluster membership for 102 stars based upon their locations in the (V, B-V), (V, V-I), (I, R-I), (U-B, B-V), and (V-R, V-I) diagrams, thus increasing three-fold the number of known cluster members. With the Q-method we determine the MK spectral types of the 33 brightest stars, confirming that 29 belong to the cluster's young population (15 B0-B1 and 14 B2- B9 main sequence stars). 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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>MCD</name><description>Simbad designation, Cl* Haffner 19 MCD NNNa</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>Seq</name><description>Sequential number (as in original table)</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>n_Seq</name><description>[*] star belongs to inner region of Haffner 19</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Name</name><description>Other name (1)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>Xpos</name><description>X position (2)</description><unit>pix</unit><ucd>pos.cartesian.x</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ypos</name><description>Y position (2)</description><unit>pix</unit><ucd>pos.cartesian.y;instr.det</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Vmag</name><description>? 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