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Overmassive Supermassive Black Holes in SDSS Close Galaxy Pairs

  • Authors: Maggie C. Huber, Julia M. Comerford, Joseph Simon

Maggie C. Huber et al 2026 The Astrophysical Journal 1008 .

  • Provider: AAS Journals

Caption: Figure 5.

Normalized histograms showing the distribution of SMBH mass ratio q (Equation (12)) calculated from Mσ (light blue) and MMb (dark blue). Panel (a) uses the MMb and Mσ from N. J. McConnell & C.-P. Ma (2013), and panel (b) uses the MMb and Mσ from J. Kormendy & L. C. Ho (2013). The solid black line at q = 0.25 divides major and minor SMBH mergers, and the relative fractions of major (fmajor) and minor (fminor) SMBH mergers predicted by each scaling relation are shown as percentages of the total close-pair sample. The Kolmogorov–Smirnov (K-S) statistic (D) between the distributions and the associated p-values are also shown. D is greater in panel (a), indicating a larger statistical difference in the q distributions obtained from the N. J. McConnell & C.-P. Ma (2013) scaling relations (likely as a result of the differences in morphology and M dynamic range described in Section 2.4). The MMb scaling relations predict a greater fraction of major SMBH pairs than the Mσ scaling relations.

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