Counts of mock satellites generated in the parameter space. To efficiently use resources for image generation, we did not fully generate mock satellites for very bright and compact satellites, or those with large sizes. For mock satellites with half-light radii exceeding the sizes of the tiles for KiDS-like images, their detection is beyond the capabilities of KiDS and has a lower likelihood of being identified. The non-generated regions will be extrapolated in the observational selection function. The heliocentric distance d is given in kpc.