Crater coverage ρ_c against crater aperture γ_c against thermal inertia Γ in $\mathrm{J}{\mathrm{m}}^{-2}{\mathrm{s}}^{-\frac{1}{2}}{\mathrm{K}}^{-1}$ of the best solutions for asteroid (814) Tauris. All blue points correspond to acceptable solutions according to Equation (4). The red points represent the 10 best solutions among all acceptable ones. All points are grouped, except for the red point with Γ > 140, which is isolated. This point was not used to determine final parameter uncertainties.