PSFs measured from the broad Hα and Hβ lines from DELS J0411–0907 (top) and VDES J0020–3653 (bottom), from the N&B quasar subtraction, as described in Section 2.3.3. These were created from the best fit quasar cube, which is the peak quasar spectrum scaled in flux to match the observed broad line flux in each spaxel. The relative intensity here depicts this scaling factor, which is the amount of flux in each spaxel relative to the brightest spaxel. We created two PSFs for each quasar, one from each of Hα and Hβ, as the PSF varies with wavelength.