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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 D1.

Stellar size–mass relation of galaxies at 2.2 < z < 3.0. The solid curves show the best-fitting broken power-law relations obtained from three different samples: the sample including COSMOS galaxies at 2.2 < z < 2.8 (blue), the COSMOS-only subsample at 2.2 < z < 2.8 (black), and the sample excluding COSMOS galaxies in this redshift interval (red). The filled circles mark the pivot mass (﹩\mathrm{log}{M}_{{\rm{p}}}﹩) of each fit.

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