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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 4.

Redshift evolution of total stellar mass contained in red member galaxies, for three sets of clusters whose z = 0.3 masses lie in the ranges ﹩\mathrm{log}{M}_{200m}/({h}^{-1}\,{M}_{\odot })=14.2-14.4﹩ (blue squares), 14.4–14.6 (green triangles), and ≥14.6 (red solid points). For each set, the points from lower left to upper right show how Mstar,tot evolves with redshift. In other words, the x-axis not only shows the cluster mass, but can also be regarded as the arrow of time (for a given cluster set). The offset of three sets of data points reflects the true halo masses derived from the merger trees (i.e., not artificially adjusted for clarity of presentation).

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