Source plane reconstruction of the lensed galaxies. Each row shows the morphology of one galaxy in (from left to right) rest-UV continuum, Hα emission, and rest-optical continuum. No rest-optical continuum image is available for SDSS J1038 so we show the reconstructed IRAC 3.6 μm image. In all sources the ionized gas morphology traced by Hα is similar to that of the rest-UV continuum, shown as contours of HST/ACS F814 W intensity on the Hα maps.