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Fig. 6.

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Evolution with redshift of the B-band luminosity functions of star-forming and quiescent galaxies (solid lines in left and right panels, respectively) from miniJPAS. The shaded areas exhibit the uncertainties in the luminosity functions obtained with our methodology. The dash-dot lines show the B-band luminosity functions before correcting of Eddington bias effects. The dashed and dotted lines point the absolute magnitude range in which our sample is affected by incompleteness after and before correcting for Eddington bias effects, respectively.

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