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I.</title><shortName>J/A+A/487/453</shortName><identifier>ivo://CDS.VizieR/J/A+A/487/453</identifier><altIdentifier>doi:10.26093/cds/vizier.34870453</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ascaso B.</name></creator><creator><name>Moles M.</name></creator><creator><name>Aguerri J.A.L.</name></creator><creator><name>Sanchez-Janssen R.</name></creator><creator><name>Varela J.</name></creator><date role="Updated">2018-01-05T08:56:06Z</date><date role="Created">2010-10-07T13:46:48Z</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>galaxy-clusters</subject><subject>galaxies</subject><subject>photometry</subject><subject>redshifted</subject><description>Using data from five clusters of galaxies within the redshift range 0.15&lt;=z&lt;=0.25, imaged with the Nordic Optical Telescope (NOT) in the central ~1Mpc^2^ in very good seeing conditions, we have performed an exhaustive inspection of their bright galaxy population. That range of redshift, where only a small amount of data with the required resolution and quality is available, is particularly important for the understanding of the formation and evolution of clusters of galaxies. We have inspected the color-magnitude relation (CMR) for those clusters and measured the blue fraction of galaxies in their cores to check for evidence of evolution as found in other works. 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