How to constrain mass and spin of supermassive black holes through their disk emission

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Table 2

Parameters of the functions g₁ and g₂ in Eqs. (12) and (13), written as a general functional (14), in the case with the viewing angle 0^°.

Parameters	α_g	β_g	γ_g	δ_g	ϵ_g	ζ_g	ι_g
g₁	1001.3894	−0.061735	−381.64942	8282.077258	−40 453.436	66 860.08872	−34 974.1536
g₂	2003.6451	−0.166612	−737.3402	16 310.0596	−80 127.1436	132 803.23932	−69 584.31533

Notes. Using KERRBB results, it is possible to find similar equations for the cases with the disk inclination angle > 0^°.

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