Evolution of the infrared luminosity function and its corresponding dust-obscured star formation rate density out to z ∼ 6

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Fig. 3.

Redshift evolution of the Schechter function parameters found in this work. The values determined at each redshift (Table 4) are shown as black points, with the best-fit functions (Equations (7) and (8)) depicted by black solid lines. (For details see Section 3.1.3.)

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