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A Bending in the Size–Mass Relation of Star-forming Galaxies across 0.5 < z < 6.0 at a Critical Stellar Mass of 1010M⊙ Revealed by JWST

  • Authors: Longyue Chen, Tao Wang, Hanwen Sun, Ke Xu, Luwenjia Zhou, Tiancheng Yang, Maxime Tarrasse, Houjun Mo, Zhaozhou Li, Yangyao Chen, Avishai Dekel, Emanuele Daddi, Xuheng Ding, Mauro Giavalisco, David Elbaz

Longyue Chen et al 2026 The Astrophysical Journal Letters 1002 .

  • Provider: AAS Journals

Caption: Figure 4.

Size–mass relations fitted by a broken power-law model for SFGs at 0.5 < z < 6.0 and a mixture model for QGs at 0.5 < z < 4.0 (same symbols as in Figure 3). At z  >  4.0, the lack of low-mass QGs results in an unconstrained mixture model fit so the mixture model is not applicable. Gray dashed lines represent the relations fitted by a single power law shown in Figure 3 for comparison.

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