Redshift distribution of miniJPAS galaxies (left panel) and AMICO cluster detections (central panel; blue and red histograms for detections with S/N > 2.5 and S/N > 3, respectively). The large fluctuations in the number of galaxies and clusters are physical and are due to large-scale structure of the field, as confirmed by the spectroscopic redshifts (Bonoli et al. 2021). The right panel shows the distribution of signal-to-noise ratio of the detections.