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Evolution of Massive Red Galaxies in Clusters from z = 1.0 to z = 0.3

  • Authors: Yen-Ting Lin, Kai-Feng Chen, Tsung-Chi Chen, Chen-Yu Chuang, Masamune Oguri

Yen-Ting Lin et al 2025 The Astronomical Journal 169 .

  • Provider: AAS Journals

Caption: Figure 6.

Similar to Figure 4, but for BCG-to-total stellar mass ratio. For a given cluster mass bin, the ratio decreases with time, because of the dramatic differences in the rates of growth between Mbcg and Mstar,tot. Also, at a given redshift, the BCG dominance decreases with cluster mass.

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