Total mass of the outflowing gas showed in bins of temperature-density, after 250 Myr for the noCR, Isodiff, κ = 3 × 10²⁸ cm² s⁻¹ and Streaming boost runs as indicated in the corresponding panels. We use a lower threshold of 10 km s⁻¹ to detect the outflowing gas, selected only above 2 kpc from the disc plane. Without CR injection, the densest (10⁻⁴ − 10⁻³ cm⁻³) component of the outflowing gas has temperatures of 10⁵ − 10^5.5 K. When including CR injection with transport, that component is colder (10⁴ K) and denser (10⁻⁴ − 10⁻² cm⁻³). In the Advection case, the wind component is almost nonexistent. The wind component is very weak with CR streaming but with similar temperatures to simulations with CR diffusion. The upper left part of the phase diagram corresponds to gas of the intergalactic medium at the outer edges of the disc.