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<ri:Resource created="2009-10-12T09:18:55Z" 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>BVRIJHK photometry of red LMC supergiants</title><shortName>J/MNRAS/289/729</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/289/729</identifier><altIdentifier>doi:10.26093/cds/vizier.72890729</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Oestreicher M.O.</name></creator><creator><name>Schmidt-Kaler T.</name></creator><creator><name>Wargau W.</name></creator><date role="Updated">2024-06-25T20:17:49Z</date><date role="Created">2009-10-12T09:18:55Z</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>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><subject>late-type-stars</subject><subject>supergiant-stars</subject><description>(BV)_J_(RI)_C_ observations for 185 and additional JHK observations for 53 red supergiant candidates in the Large Magellanic Cloud (LMC) are presented. The data have been reduced discussing carefully the dependence of effective wavelengths on the spectral energy distribution of the star, which is very strong especially for the Cousins R band. Non-linear colour dependences of transformation coefficients vor the V magnitude and the R-I colour have been taken into account. The mean error of the BVRI data is 0.03 to 0.04 mag, while that of the JHK observations is 0.02mag. The MK types are not given to the stars, as the classifications given in the literature are mostly very uncertain. The spectra we have obtained for 88 of the stars will be discussed in a forthcoming paper where we will give directly physical properties like Mbol and Teff instead of MK types. 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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>Star</name><description>Identification</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType><flag>primary</flag></column><column><name>WOH</name><description>Identification number according to Westerlund et al. (1981A&amp;AS...43..267W)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>RM</name><description>Identification number according to Rebeirot et al. 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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>Star</name><description>Identification, as in file bvri.dat</description><ucd>meta.id;meta.file</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>Jmag</name><description>J magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Jmag</name><description>Error of Jmag</description><unit>mag</unit><ucd>stat.error;phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>J-H</name><description>J-H colour</description><unit>mag</unit><ucd>phot.color;em.IR.J;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_J-H</name><description>Error of J-H colour</description><unit>mag</unit><ucd>stat.error;phot.color;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>H-K</name><description>H-K colour</description><unit>mag</unit><ucd>phot.color;em.IR.H;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_H-K</name><description>Error of H-K colour</description><unit>mag</unit><ucd>stat.error;phot.color;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Rem</name><description>Remark flags</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>spFile</name><description>Spectrum file name, in "sp" subdirectory</description><ucd>meta.id;meta.file</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column></table></schema></tableset></ri:Resource>