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Probing Dark Matter Halos of High-redshift Quasars via Wide-field Clustering

  • Authors: Hao Meng, 皓 蒙, Guangping Ye, 广平 叶, Huanian Zhang, 华年 张

Hao Meng et al 2026 The Astrophysical Journal Letters 1009 .

  • Provider: AAS Journals

Caption: Figure 6.

The scaling relation between the observed quasar bolometric luminosity and its derived host halo mass: (a) typical mass, (b) minimum mass. The error bars of Lbol represent the observed range of the quasar luminosity, while the error bars of Mh denote the measurement uncertainties. The gray solid line and shaded region in panel (a) represent the theoretical Lbol–Mtyp relation at z ≈ 6 from simulations (E. Pizzati et al. 2024b).

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