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Fig. 15.

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Evolution of the star formation rate density with redshift using different integration limits for the LF. Brown (red) crosses show results of integrating the best-fit Schechter (modified Schechter) functions log(L) from 41 (39.5) to 44 erg s−1. Solid blue, orange, and green curves indicate the critical SFRDs obtained by assuming a clumping factor of 3 and fescp = 3%, 8%,  and 25%, respectively. The solid green curve, having fescp = 8%, indicates the best likely match with our SFRD points in the luminosity range of 41 < log(L) < 44 (see details in the text).

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