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Fig. 6

image

Contributions of the different stellar populations to the NIRB. The blue, black, and red lines denote the NIRB contribution of Pop II, Pop III.1, and Pop III.2, respectively. Case A (f∗ ,III = 0.01,fesc = 0.21), case B (f∗ ,III = 0.004,fesc = 0.45), and case C (f∗ ,III = 0.002,fesc = 0.75) are denoted by dashed, solid and dotted lines, respectively.

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