Example of unweighted models simulating an outflow with the spatial and spectral resolution of a galaxy observed with MUSE at z = 0.001. From left to right: Line-velocity integrated map, LOS velocity map, and velocity dispersion map. Top panels: full biconical model with P.A. = 40°, inclination with respect to the plane of the sky of β = 85°, a constant radial velocity of 1200 km s⁻¹, and a cone semi-aperture of θ_OUT = 30°. Bottom panels: single hollow conical model with P.A. = 90°, β = 65°, and inner and outer semi-aperture θ_IN = 25° ,θ_OUT = 35°. Both models have been convolved with a spatial PSF = 0.3″ and no spectral convolution.