Notes. The models are constructed as plabs⋅tbabs⋅(DE + RR + SR), where DE denotes the direct emission (i.e., the sum of hot-corona Comptonization and unscattered thermal disk emission, including reflected returning radiation); RR is the relativistic reflection component; and SR is the static reflection component. In all models, SR is computed as xilconv⋅DE and RR is computed as relconv⋅comppsc⋅xilconv⋅DE, except for model 4, in which the relativistic reflection component is not included. As indicated in the DE terms, reflection of returning radiation is treated as elastic in model 1 and with xillverNS in models 2–5. comppsc represents the hot corona Comptonization, affecting both the disk emission and the disk reflection. In model 3, thcomp represents warm corona Comptonization.