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Cited article:
S. Andreon
A&A, 409 1 (2003) 37-52
Published online: 2003-11-17
This article has been cited by the following article(s):
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Red sequence modal colour gradients across intermediate X-ray luminosity galaxy clusters
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JKCS 041: a colour-detected galaxy cluster at $z_{\mathrm{phot}}$ ~ 1.9 with deep potential well as confirmed by X-ray data
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Galaxy evolution in the high-redshift, colour-selected cluster RzCS 052 at z = 1.02
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Stellar Age versus Mass of Early‐Type Galaxies in the Virgo Cluster
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Scaling relations of the colour-detected cluster RzCS 052 at z= 1.016 and some other high-redshift clusters
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The evolution of the galaxy red sequence in simulated clusters and groups
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Evidence of Cosmic Evolution of the Stellar Initial Mass Function
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Multi-object spectroscopy of low-redshift EIS clusters
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The history of mass assembly of faint red galaxies in 28 galaxy clusters since z = 1.3
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Constraining scalar-tensor quintessence by cosmic clocks
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DARK ENERGY MODELS TOWARD OBSERVATIONAL TESTS AND DATA
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Lookback time as a test for brane cosmology
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New evidence for a linear colour-magnitude relation and a single Schechter function for red galaxies in a nearby cluster of galaxies down to M*+ 8
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The buildup of stellar mass and the 3.6μm luminosity function in clusters fromz = 1.25 toz = 0.2
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Photometric scaling relations for bulges of galaxies
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Multi-object spectroscopy of low redshift EIS clusters
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Frontiers of Cosmology
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Simulating galaxy clusters - II. Global star formation histories and the galaxy populations
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Batch discovery of ninez∼ 1 clusters using X-ray andKorR,z′ images
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Testing the Universality of the (U−V) Color‐Magnitude Relations for Nearby Clusters of Galaxies
Daniel H. McIntosh, Ann I. Zabludoff, Hans‐Walter Rix and Nelson Caldwell
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The Bimodal Galaxy Color Distribution: Dependence on Luminosity and Environment
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Constraining dark energy models using the lookback time to galaxy clusters and the age of the universe
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Galaxy evolution in clusters up toz= 1.0
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Penetrating Bars through Masks of Cosmic Dust
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Extending the Butcher-Oemler effect up toz∼ 0.7
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