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H I Depletion Begins Well Beyond the Virial Radius: A FAST Stacking Study of 36 Galaxy Clusters to 5 × R200

  • Authors: Cheng Cheng, Chuan-Peng Zhang, Edo Ibar, Rory Smith, Weiwei Xu, Hyowon Kim, Jia-Sheng Huang, Wei Zhang, Pei Zuo, Hugo Méndez-Hernández, Juan Molina, Ming Zhu, Qian Yu

Cheng Cheng et al 2026 The Astrophysical Journal 1009 .

  • Provider: AAS Journals

Caption: Figure 2.

Left: redshift versus M* of the member galaxies we selected. The stellar mass lower than 109M is not complete to a redshift of 0.06. The dashed purple line shows the stellar mass for a target with r = 20 AB mag and g − r = 0.5 at each redshift, which is roughly the detection limit of the DESI spectroscopic sample. Right: histogram of the stellar mass at different R/R200. The stellar mass distributions for galaxies at different radii are similar.

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