Evolution over redshift of the star formation rate density. We used the same colour scheme as Fig. 8, where grey corresponds to measurements based on UV, blue to Hα and orange to [O III] and [O III]+Hβ. The black line corresponds to the results of the review Madau & Dickinson (2014), which compiles the state-of-the-art measurements of the time. All the results have an integration lower limit of 0.24 − 0.30 M_⊙ yr⁻¹ Mpc⁻³ and are IMF-corrected to Chabrier (2003). The z ∼ 7 − 9 orange points correspond to GLIMPSE measurements, where the bright orange uses the standard 0.3 M_⊙ yr⁻¹ Mpc⁻³ lower integration limit and the light orange uses the deep 0.005 M_⊙ yr⁻¹ lower integration limit (approximately corresponding to L_Hα ∼ 10³⁹ erg s⁻¹). The non-exhaustive compilation of UV, Hα and [O III]+Hβ based measurements, including this work, are listed in Table E.1.