Figure 12 from Toward Determining the Number of Observable Supermassive Black Hole Shadows

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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 12.

Example SEDs produced from the model described in Appendix A plotted for a range of accretion rates. The left panel shows SEDs for an SMBH mass similar to that of M87 (6.5 × 10⁹ M_⊙; Event Horizon Telescope Collaboration et al. 2019f), and the right panel shows SEDs for an SMBH mass similar to that of Sgr A* (4 × 10⁶ M_⊙; Do et al. 2019; Gravity Collaboration et al. 2019).

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