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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 5.

Similar to Figure 4, but for the stellar mass assembly history of BCGs. There appears to be a halt in BCG stellar mass growth at z ≲ 0.6. It is also seen that the BCGs in the high cluster mass bin do not experience much growth from z = 0.99 to z = 0.3.

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