Gallery of young systems detected with NACO and reduced with PIPPIN. Each panel shows the polarised light on a logarithmic scale ranging between different values to highlight sub-structures. The highest degree of IP correction is used where possible. Scale bars in the lower-left corners of each panel indicate 100 AU at each object’s distance. HD 169142, R CrA, and Parsamian 21 are shown in the H band, MP Mus is shown in the IB_2.06 filter, and the other panels use Ks-band observations. Mon R2 IRS 3 shows the median I_q image because the Stokes U component was not observed. The images of YLW 16A and Elia 2-21 present the first polarised light detections in the NACO observations.