Comparison of the peak [OII] flux (top panel) and S/N (bottom panel) from the spectra of 153 MUSE-Wide DR1 [OII] emitters extracted with TDOSE based on multi-component Sérsic models of the HST F814W imaging generated with GALFIT (x-axes), and the MUSE-Wide DR1 TDOSE spectra based on single Gaussian models (y-axes). In both panels the dashed line indicates the one-to-one relation, and the red line is the best linear fit to the flux and S/N measurements with the 3σ uncertainty on the fit indicated by the shaded region.