The mass quenching determination dependence on the gas accretion. The x-axis represents the mass of a galaxy at which it starts quenching, plotted against γ, which depicts the rate of gas accretion by the galaxy. Each dot represents a possible solution as posterior samples from the Multinest fitting. The colour background shows smoothed distribution of the posterior points. The solid black line given by (log₁₀γ = 110.75−11.25log₁₀(M_cap/M_⊙)), shows that a galaxy that accretes gas in high quantities quenches at a lower mass compared to a galaxy that does not accrete a lot of gas.