Fig. 6
Contribution to the cosmic SFRD of galaxies with SFR ≥ 1.4 × 10-6 M⊙/yr (corresponding to UV luminosity LUV ≳ 1015 W Hz−1 when adopting the calibration given in Kennicutt 1998) as a function of redshift (solid line). Dashed line indicates the contribution of galaxies dominated by the quiescent mode of star formation, while dotted line indicates the contribution of galaxies dominated by the burst mode of star formation.
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