Broad iron line as a relativistic reflection from warm corona in AGNs

Open Access

Fig. 6.

Black hole disk images computed by GYOTO from the TITAN local angle dependent spectra, for two different spins. Images are computed at 6.4 keV and at θ_obs = 15° – almost face-on. The black hole mass is set to 10⁸ M_⊙. The map is created for monochromatic luminosity νL_ν in erg s⁻¹ px⁻¹, and the X and Y axes are in units of r_g with the SMBH center as the origin.

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