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No Detectable One-halo Galactic Conformity Signal with Halo-mass Estimates Consistent with Weak-lensing Constraints

  • Authors: Dingyi Zhao, Yingjie Peng, Luis C. Ho, Houjun Mo, Cheqiu Lyu, Kai Wang, Yijun Wang, Tao Wang, Jing Dou, Zeyu Gao, Qiusheng Gu, Yukun Liu, Roberto Maiolino, Alvio Renzini, Bitao Wang, Yu-Chen Wang, Bingxiao Xu, Feng Yuan, Kunyao Zhao, Xingye Zhu

Dingyi Zhao et al 2026 The Astrophysical Journal Letters 1009 .

  • Provider: AAS Journals

Caption: Figure 2.

Raw one-halo conformity signals measured from the five complete samples. The upper row shows the halo-level statistic, while the lower row shows the satellite-level statistic. From left to right, the three columns use halo masses derived from the ML method, the mass-ranking AM method, and the luminosity-ranking AM method, respectively. Different colors correspond to the five complete samples defined in Figure 1. Error bars show the bootstrap uncertainties, and the dashed horizontal lines mark zero signal.

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