adsabs/AstroCLIMB huggingface dataset:
Paper: A 13 Billion Year View of Galaxy Growth: Metallicity Gradient Evolution from the Local Universe to z = 9 with JWST and Archival Surveys
Authors: Zihao Li, Zheng Cai, Xin Wang, Zhaozhou Li, Avishai Dekel, Kartick C. Sarkar, Eduardo Bañados, Fuyan Bian, Aklant K. Bhowmick, Laura Blecha, Sarah E. I. Bosman, Jaclyn B. Champagne, Xiaohui Fan, Emmet Golden-Marx, Hyunsung D. Jun, Mingyu Li, Xiaojing Lin, Weizhe Liu, Fengwu Sun, Maxime Trebitsch, Fabian Walter, Feige Wang, Yunjing Wu, Jinyi Yang, Huanian Zhang, Shiwu Zhang, Mingyang Zhuang, Siwei Zou
Figure caption: The MZGR for individual galaxies in four redshift bins. The red shadows represent the 1σ confidence interval of the linear regression. For z ≤ 0.1 measurements, regressions are performed within two stellar mass bins, ﹩\mathrm{log}({M}_{* }/{M}_{\odot })\leqslant 9﹩ and ﹩\mathrm{log}({M}_{* }/{M}_{\odot })\gt 9﹩, while high-redshift measurements are performed across the entire mass range. The error bar on the bottom left of each figure represents the median uncertainty in stellar masses and gradients. The pre-JWST observations are shown as gray circles (A. M. Swinbank et al. 2012; T. Jones et al. 2013; I. T. Ho et al. 2015; L. Sánchez-Menguiano et al. 2016; E. Wuyts et al. 2016; D. Carton et al. 2018; N. M. Förster Schreiber et al. 2018; F. Bresolin 2019; M. Curti et al. 2020a; R. C. Simons et al. 2021; T. Li et al. 2025); NGDEEP and recent JWST MSA-3D (M. Ju et al. 2025) observations are highlighted in red and blue, respectively.