Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

Matter Clustering in Astrid: Reduced Baryonic Suppression from Realistic Black Hole Dynamics

  • Authors: Yanhui Yang, 焱辉 杨, Simeon Bird, Yihao Zhou, 亦豪 周, Tiziana Di Matteo, Rupert Croft, Yueying Ni, Nianyi Chen

Yanhui Yang et al 2026 The Astrophysical Journal Letters 1007 .

  • Provider: AAS Journals

Caption: Figure 4.

AGN hard X-ray (2–10 keV) luminosity functions at z = 0. The line styles and colors are the same as in Figure 1. The SIMBA luminosity function (data from M. Habouzit et al. 2022) is also plotted for comparison. Shaded regions show observational constraints compiled by X. Shen et al. (2020) (light blue) and J. Buchner et al. (2015) (z = 0.1, gray).

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Copyright and Terms & Conditions

Additional terms of reuse