Fig. 4
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Comparison of simulated IMBH candidates in Model B with observational data. (a) Corner plot showing the GCs (purple) and NSCs (orange) clusters in our simulations hosting an IMBH at z = 0, compared to observations of potential IMBHs in Milky Way globular clusters and G1. (b) One-dimensional IMBH mass distribution, compared to estimated masses for G1 and 47 Tuc.
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