This page shows graphic outputs obtainable by using the SM macros contained in the package. In particular, this example refers to a run of VGCF on a field of the Palomar Distant Cluster Survey (Postman et al. 1996, AJ, 111, 615).
Output of macro circle_xy.sm (black circles identify detected clusters, red points show galaxies belonging to clusters):
Output of macro distributions.sm (solid line represents the cumulative distribution of densities for all galaxies in the field, dashed line refers to the cumulative distribution of densities for the fitted background):
Output of macro voronoi_holes.sm (red rectangles represent areas excluded from tessellation, green points identify galaxies belonging to clusters):