Fig. 9.
Evolution of the fraction of the dust obscured SFRDIR as a function of redshift. The arrows show the lower limits obtained using the lower limits discussed in Sect. 4.3.1. The points at z < 4 are obtained using a compilation of the literature from Fig. 7. The points at z > 4 are obtained using the UVLF+GSMF combined measurements from Table 2.
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