A possible two-fold scenario for the disc-corona of the luminous active galactic nucleus 1H 0419-577: A high-density disc or a warm corona

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Fig. C.1.

Data-to-model ratio of the fits using the REXCOR model grids for the May 2018 (black) and November 2018 (blue) simultaneous XMM-Newton and NuSTAR spectra. The inferred parameter values are reported in Table C.1. Top left panel: Model calculated for a spin of 0.99 and a hot corona height of 5 R_g (χ²/d.o.f.=1871.5/1437). Top right panel: Model calculated for a spin of 0.99 and a hot corona height of 20 R_g (χ²/d.o.f. = 1864.8/1437). Bottom left panel: Model calculated for a spin of 0.90 and a hot corona height of 5 R_g (χ²/d.o.f. = 1957.1/1437). Bottom right panel: Model calculated for a spin of 0.90 and a hot corona height of 20 R_g (χ²/d.o.f. = 1970.8/1437).

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