Fig. 9.

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Excess of massive log(M⋆/M⊙)≳10.5 galaxies around the MQN01 QSO. Left panel: cumulative stellar mass function of the MQN01 spectroscopic sample in proximity to the QSO (black stars) compared to the control-field sample (orange diamonds) and the expectations for blank fields from the COSMOS survey (3.0 < z < 3.5, Weaver et al. 2023, gray). Right panel: same as the left panel, but normalized to the value of the cumulative mass function at M⋆ = 109.8 M⊙, corresponding to the 90% completeness limit of the MQN01 spectroscopic sample.
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