Comparison of the SFR values derived for our sample galaxies obtained via SED fitting (see Sec. 2.2 for details) and from the [O II] luminosity of each galaxy (see Sec. 3.3.1). The black squares show the SFR values for galaxies in our final sample, and the gray dots show the SFR values for galaxies in the preliminary sample, for the subset of galaxies at z ≲ 1.48, where the [O II] doublet falls well within the MUSE wavelength range. The red line shows the identity for reference. Table D.1 provides these measurements for each galaxy in our final sample.