3′′× 3′′ HST-ACS images of the sample presented in this paper, with a spatial scale of 3′′× 3′′ for each object. For XID178 and XID5627, the white contours represent the narrow component of the [O iii] λ5007 emission line profile, while the yellow contours represent the broad component; for XID5330, the white contours represent the single Gaussian component of [O iii] λ5007. All contours are at 50%, 75%, and 95% levels. The SINFONI data are not corrected for astrometry.