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A Census of Quiescent Galaxies across 0.5 < z < 8 with JWST/MIRI: Mass-dependent Number Density Evolution of Quiescent Galaxies in the Early Universe

  • Authors: Tiancheng Yang, Tao Wang, Ke Xu, Hanwen Sun, Luwenjia Zhou, Lizhi Xie, Gabriella De Lucia, Claudia del P. Lagos, Kai Wang, Fabio Fontanot, Qi Guo, Yuxuan Wu, Shiying Lu, Longyue Chen, Michaela Hirschmann

Tiancheng Yang et al 2026 The Astrophysical Journal Letters 1000 .

  • Provider: AAS Journals

Caption: Figure 1.

The UVJ color–color diagram for the photometric sample with M > 109.0 M. The comoving volume is nearly constant across all redshift slices (except for the highest-redshift bin), allowing for a direct comparison of the number density evolution of QGs and SFGs. The orange line denotes our inclusive preselection boundary (defined in Equations (1) and (2)). The solid black line indicates the standard UVJ criterion proposed by R. J. Williams et al. (2009), while the dashed black line shows an extended criterion (lowering the U − V threshold to 0.85). This extended cut is designed to include high-redshift PSBs, though it introduces substantial contamination from SFGs. This diagram does not include contamination removed in Section 3.2.

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