Fig. 5.

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Estimated growth history of PSO J0309+27 (red star). Solid lines represent the best fit cases, under which the corresponding λEdd and η are reported. The shaded horizontal regions correspond to the expected mass ranges of Pop III remnants BHs (Mseed ≤ 102 M⊙, grey), stellar dynamical processes (Mseed ≥ 103 − 104 M⊙, cyan), and direct collapse BHs (Mseed ∼ 104 − 106 M⊙, dark cyan). The values of the different seed black holes are taken from Valiante et al. (2016).
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