Figure 6
Variation with redshift of (a) LIR/LFUV ratio, (b) Hα SFR, (c) mass, (d) specific Hα-derived SFR. The gap centred on z = 0.16 shows where the wavelength of the atmospheric O2 band (Fraunhofer A-line) overlaps with redshifted wavelength of the Hα emission line. For this reason, we cannot use Hα emission-line measurements that fall into this redshift range, leading us to omit these data from our analysis.

Variation with redshift of (a) LIR/LFUV ratio, (b) Hα SFR, (c) mass, (d) specific Hα-derived SFR. The gap centred on z = 0.16 shows where the wavelength of the atmospheric O2 band (Fraunhofer A-line) overlaps with redshifted wavelength of the Hα emission line. For this reason, we cannot use Hα emission-line measurements that fall into this redshift range, leading us to omit these data from our analysis.

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