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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 8.

Normalized histograms showing the distribution of SMBH mass ratio q (Equation (12)) calculated from inferred quantities MM﹩{}_{{\rm{b}},{\rm{\inf }}}﹩ (Equations (8) and (9)) and Mσinf (Equation (11)) in light blue and MMb and Mσ in dark blue. Panels (a) and (c) use the N. J. McConnell & C.-P. Ma (2013) scaling relations and panels (b) and (d) use the J. Kormendy & L. C. Ho (2013) relations. 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 K-S test statistic and p-values between the light and dark blue distributions are shown in the upper-right corners of each panel. MM﹩{}_{{\rm{b}},{\rm{\inf }}}﹩ predicts a greater fraction of major SMBH mergers than MMb, while Mσinf predicts a greater fraction of minor mergers than Mσ.

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