The most stringent upper limit set on the mass of a central black hole in 47 Tucanae using dynamical models

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Fig. A.1.

1D (diagonal panels) and 2D (lower-diagonal panels) marginalized, posterior distributions over the model’s free parameters. See Section 2 for a description of the parameters. Prior ranges, median values, 68%, and 99.7% CIs for each parameter are reported in Table A.1.

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