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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 3.

Best-fitting constant amplitudes obtained by fitting a horizontal line to each raw conformity curve shown in Figure 2. The left panel shows the halo-level results and the right panel shows the satellite-level results. Blue, green, and orange lines correspond to the ML, mass-ranking AM, and luminosity-ranking AM halo masses, respectively. Error bars indicate the 1σ uncertainties of the fitted constant amplitudes. The fitted amplitudes depend systematically on the adopted halo-mass method.

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