Truncation radius measured from the RSBP along the disk mid-plane (i.e. 0 kpc) and at different heights above and below the NGC 4565 mid-plane (the horizontal axis is scaled so as to show the region around the truncation). The shaded regions denote the standard deviations of the corresponding distribution of truncation positions. The vertical dashed lines represent the mean values of the corresponding truncation radius. Top: broadband optical data values in comparison with the corresponding models. Centre: truncation radii for the disk quadrant with warp (north quadrant or upper right in Fig. 6) for the g, r, and i bands. Bottom: same as in the centre panel but for a disk quadrant with no warp feature (west quadrant or lower right in Fig. 6). In this work we detect truncations up to 4 kpc above and below the galaxy mid-plane, that is, 1 kpc higher than in ML19. The presence of a warp clearly affects the radial location of the truncation feature.