The optical-infrared relation for active galactic nuclei: The role of contaminations

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Table 3.

Median values of ratios of different estimations of luminosities for objects with $L_{disk}^{OPT} < 10^{45}$ $Mathematical equation: $ L_{\mathrm{disk}}^{\mathrm{OPT}} < 10^{45} $$ [erg/s].

Column	Low (45)	Inter 1 (30)	Inter 2 (22)	High (17)
(1) $L_{IR}^{torus} / L_{IR}^{photo}$ $Mathematical equation: $ L^{\mathrm{torus}}_{\mathrm{IR}}/L^{\mathrm{photo}}_{\mathrm{IR}} $$	0.55 ± 0.17	0.57 ± 0.14	0.64 ± 0.16	0.72 ± 0.26
(2) $L_{IR}^{torus + polar} / L_{IR}^{photo}$ $Mathematical equation: $ L_{\mathrm{IR}}^{\mathrm{torus+polar}}/L_{\mathrm{IR}}^{\mathrm{photo}} $$	0.63 ± 0.16	0.60 ± 0.12	0.68 ± 0.15	0.81 ± 0.13
(3) $L_{IR}^{torus + polar + cold} / L_{IR}^{photo}$ $Mathematical equation: $ L_{\mathrm{IR}}^{\mathrm{torus+polar+cold}}/L_{\mathrm{IR}}^{\mathrm{photo}} $$	0.71 ± 0.15	0.72 ± 0.10	0.75 ± 0.13	0.83 ± 0.12
(4) $L_{IR}^{torus + polar + cold + stellar} / L_{IR}^{photo}$ $Mathematical equation: $ L_{\mathrm{IR}}^{\mathrm{torus+polar+cold+stellar}}/L_{\mathrm{IR}}^{\mathrm{photo}} $$	0.83 ± 0.14	0.79 ± 0.11	0.85 ± 0.13	0.96 ± 0.06
(5) $L_{IR}^{torus + polar + cold + stellar + disk} / L_{IR}^{photo}$ $Mathematical equation: $ L_{\mathrm{IR}}^{\mathrm{torus+polar+cold+stellar+disk}}/L_{\mathrm{IR}}^{\mathrm{photo}} $$	1.00 ± 0.00	1.00 ± 0.00	1.00 ± 0.00	1.00 ± 0.00
(6) $L_{IR}^{torus + polar} / L_{IR}^{torus}$ $Mathematical equation: $ L_{\mathrm{IR}}^{\mathrm{torus+polar}}/L_{\mathrm{IR}}^{\mathrm{torus}} $$	1.00 ± 0.37	1.00 ± 0.88	1.00 ± 0.64	1.00 ± 2.16
(7) $L_{OPT}^{disk} / L_{OPT}^{photo}$ $Mathematical equation: $ L_{\mathrm{OPT}}^{\mathrm{disk}}/L^{\mathrm{photo}}_{\mathrm{OPT}} $$	0.53 ± 0.25	0.76 ± 0.30	0.50 ± 0.26	0.38 ± 0.28
(8) $L_{OPT}^{disk + stellar attenuated} / L_{OPT}^{photo}$ $Mathematical equation: $ L_{\mathrm{OPT}}^{\mathrm{disk+stellar\,attenuated}}/L^{\mathrm{photo}}_{\mathrm{OPT}} $$	0.97 ± 0.02	0.98 ± 0.03	0.98 ± 0.02	0.96 ± 0.02
(9) $L_{OPT}^{disk + stellar attenuated} / L_{IR}^{disk}$ $Mathematical equation: $ L_{\mathrm{OPT}}^{\mathrm{disk+stellar\,attenuated}}/L_{\mathrm{IR}}^{\mathrm{disk}} $$	1.82 ± 62.94	1.31 ± 5.91	1.95 ± 13.29	2.53 ± 713.33

Notes. The errors are the median absolute deviation errors. The particular luminosity estimates are described in Sect. 4.3.

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