“…As shown in [8], con sistent description of angle resolved photoemission spectra leads to the necessity to simultaneously solve a system of equations for the functions of reflection R(z, Δ, Ω 0 , Ω), transmission T(z, Δ, Ω 0 , Ω), and pho toelectron emission flux density Q(z, Δ, Ω 0 , Ω). Here, z is the layer thickness, Δ = E 0 -E is the electron energy losses, and Ω 0 = (μ 0 , ϕ 0 ) and Ω = (μ, ϕ) are the probing and viewing directions.…”