Schematic representation of the DISCMINER modelling flow and capabilities. DISCMINER produces best-fit channel maps of the input data cube by modelling the disc vertical structure and orientation, stellar mass, and attributes that shape the line profile morphology, assuming that the disc emission is smooth and Keplerian. The model and data channels are then compared through three types of moment maps. Large-scale analyses of these maps allow to look into the disc dynamical and thermodynamic structure, but are also useful to reveal potential signatures driven by planetary and non-planetary mechanisms, such as meridional flows or spirallike perturbations. Small-scale analysis of residuals from these maps leads to the retrieval of the potential location of embedded planets through the detection of localised velocity perturbations and sites of enhanced velocity dispersion.