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ivo-id="ivo://CDS">CDS</publisher><creator><name>Tsalmantza P.</name></creator><creator><name>Kontizas E.</name></creator><creator><name>Cambresy L.</name></creator><creator><name>Genova F.</name></creator><creator><name>Dapergolas A.,Kontizas M.</name></creator><date role="Updated">2018-01-05T08:55:54Z</date><date role="Created">2007-01-01T22:36:05Z</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>galaxies</subject><subject>giant-stars</subject><subject>infrared-photometry</subject><description>This study focuses on very luminous (M_bol_&lt;-6.0mag) AGB stars with J-Ks&gt;1.5mag and H-Ks&gt;0.4mag in the LMC, SMC, M 31, and M 33 from 2MASS data.</description><source 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