Evolution of spectral parameters as a function of the Compton parameter y from the compps fits (color-coding as in Fig. 2). The overall trends of L_dbb/L_c ratio (top panel) and the reflection amplitude Ω/2π (middle panel) show qualitatively similar behavior to the nthcomp fits. We also see how the electron temperature kT_e (bottom panel) increases when the flux drops below the critical limit of F_x ≲ 10^-8 erg cm^-2 s^-1. The kT_e increase may be caused by the change of geometry and seed photon source: disk truncation leads to fewer disk photons entering the Comptonized region, resulting in less efficient cooling of the electrons and thus higher equilibrium temperatures.