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The Bigfoot: A Footprint of a Coma Cluster Progenitor at z = 3.98

  • Authors: Hanwen Sun, Tao Wang, Emanuele Daddi, Qiaoyang Hao, Ke Xu, David Elbaz, Luwenjia Zhou, Houjun Mo, Huiyuan Wang, Longyue Chen, Yangyao Chen, Shuowen Jin, Yipeng Lyu, Nikolaj Sillassen, Kai Wang, Tiancheng Yang

Hanwen Sun et al 2025 The Astrophysical Journal Letters 993 .

  • Provider: AAS Journals

Caption: Figure A1.

The RGB composite color image of the most massive protocluster core (0217A). The red, green, and blue channels correspond to the JWST/NIRCam F444W, F277W, and F150W filters, respectively. Member galaxies are overlaid as open circles: massive SFGs (M* > 1010M⊙) in yellow, low-mass SFGs (M* < 109M⊙) in cyan, and quiescent galaxies (QGs, including both passive galaxies and poststarburst galaxies) in red.

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