Fig. 8
Top panels: posterior luminosity function of star-forming galaxies in ALHAMBRA, Φ (z,MB | SF), differential (left) and binned (right) version with Δz = 0.05 and ΔMB = 0.3. Bottom panels: median luminosity function model for star-forming galaxies, differential (left) and binned (right) version. These luminosity functions are complete for I0 ≤ 24 galaxies.
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