One-dimensional non-LTE Fe I abundances for each visible line in the spectrum interpolated to a microturbulence of υ_micro = 1.48 km s⁻¹. The blue line shows the best linear fit through the data, while the red dashed line denotes the mean non-LTE abundance. The black solid line denotes the cut-off in reduced equivalent width between saturated and non-saturated lines: log[W_λ/λ₀] < −4.95.