Iceline position as a function of α turbulence and initial gas surface density at 1 AU with a constant f_DG = 1% (Eq. (26)). The iceline transition is defined as T = 170 ± 10 K. The black lines mark r_ice = 0.5, 1, 2.7 and 5 AU. Higher viscosity or gas surface density leads to hotter discs, with the iceline located at greater distances from the star. The same applies to higher total dust-to-gas ratio. The gray dashed lines mark r_ice = 0.5, 1, 2.7 and 5 AU for a disc with f_DG = 3%.