[OIII] 88 μm-SFR relation. The blue line shows the metal-poor local dwarf galaxies relation from De Looze et al. (2014). The green line corresponds to the high-redshift observed relation proposed by Harikane et al. (2020) while the red line corresponds to simulation results from Arata et al. (2020) both at z = 6 − 9. We translate our [OIII]λ5007 luminosities into [OIII] 88 μm using a mean ratio of 1.9 derived from CLOUDY HII-region models at an electron density of n_e = 100 cm⁻³ shown as a black dotted line. The gray area is the dispersion in the translation with gas-phase metallicity.