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Fig. 2.


Spectral energy distribution fits minimising the χ2-statistic for each of the spectroscopically identified host-galaxies. In each panel, we plot the solutions including and excluding nebular emission lines to show its impact on the derived stellar masses. Blue (red) data points refer to included (excluded) magnitudes, with vertical and horizontal error-bars indicating the uncertainty in the photometry and the FWHM of each filter, respectively. Grey squares refer to the transmission-weighted flux in each filter, calculated based on the best-fit SED solution. Upper limits are denoted by triangles. Each panel text displays the LEPHARE best fit reddening before we apply the stellar-to-nebular conversion (Eq. (4)), and the resulting stellar mass.

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