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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 A1.

Top: the relative deviation of the estimated Sérsic index (﹩{n}^{{\prime} }﹩) from the true Sérsic index (n) as a function of ﹩{n}^{{\prime} }﹩, defined as ﹩(n-{n}^{{\prime} })/n﹩. The vertical grid lines separate ﹩{n}^{{\prime} }﹩ bins. Boxes show median (central horizontal line), interquartile range (IQR; box edges), and the maximum/minimum within 1.5 × IQR (whiskers). Bottom: the relative deviation of the estimated ﹩{R}^{{\prime} }﹩ from the true R as a function of ﹩{R}^{{\prime} }﹩, defined as ﹩(R-{R}^{{\prime} })/R﹩. Outliers beyond 1.5 × IQR (∼1.5%) are excluded for clarity in all plots.

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