Distributions for the number of bright PBHs above the NuSTAR point source detection limit for different levels of turbulence in the CMZ (0–5 km s⁻¹) and for different DM profiles (NFW, Einasto). Each distribution is derived from 1000 independent Monte Carlo realizations. The orange histograms represent the model with only a bulge and DM halo. The green histograms correspond to the case in which the MB 1D velocity dispersion has been increased by 25% to correct for the missing Galactic disk contribution (see Fig. 3). The uniform gas distribution within resolution element is assumed.