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Toward Determining the Number of Observable Supermassive Black Hole Shadows

  • Authors: Dominic W. Pesce, Daniel C. M. Palumbo, Ramesh Narayan, Lindy Blackburn, Sheperd S. Doeleman, Michael D. Johnson, Chung-Pei Ma, Neil M. Nagar, Priyamvada Natarajan, and Angelo Ricarte

2021 The Astrophysical Journal 923 260.

  • Provider: AAS Journals

Caption: Figure 16.

Comparison of the ERDF prescription used in this paper with the empirical modeling from Aird et al. (2018), with each panel showing a different choice of redshift. In each panel, the colored lines and corresponding shaded regions show the constraints from Aird et al. (2018) for a range of SMBH masses, as labeled in the legend at the lower right; the black dashed and dotted lines show our ERDF prescription (see Equation (12)) for example SMBH masses of 106 and 109 M, respectively, as labeled in the legend at the lower left. All panels share the same horizontal and vertical axis ranges, which are explicitly labeled in the left panel.

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