The properties of the obscuring material of a sample of active galactic nuclei from mid-IR and X-ray simultaneous fitting

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Table 5.

Simultaneous fit results (σ_tor = θ_tor).

Objname	Baseline	χ_r²	X-ray parameters			IR parameters							Derived quantities
	model		Γ	log(N_{H_tor})	θ_inc	σ_tor	Y	α_r	α_p	N0	τ_ν	log(P_size)	E_B − v	R_out	log(M_dust)	`CF`
				[cm⁻²]	[°]	[°]				[#]		[μm]		[pc]	[M_⊙]
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)	(10)	(11)	(12)	(13)	(14)	(15)	(16)	(17)
Seyfert 1

Mrk590	X-C/MIR-C	0.85	2.00 $_{1.96}^{2.06}$ $_{1.96}^{2.06}$	22.25 $_{22.19}^{22.3}$ $_{22.19}^{22.3}$	78.16 $_{71.63}^{79.59}$ $_{71.63}^{79.59}$	< 19.41	13.6 $_{12.64}^{14.66}$ $_{12.64}^{14.66}$	< 0.03	–	> 13.1	> 146.22	–	2.14 $_{1.53}^{2.47}$ $_{1.53}^{2.47}$	$6 . 24_{5.33}^{7.16}$ ${6.24_{5.33}^{7.16}}$	$6 . 43_{6.32}^{6.53}$ ${6.43_{6.32}^{6.53}}$	$0 . 38_{0.30}^{0.46}$ ${0.38_{0.30}^{0.46}}$
PG0804+761	X-C/MIR-TP	0.88	1.94 $_{1.88}^{1.99}$ $_{1.88}^{1.99}$	< 21.44	30.82 $_{25.07}^{33.07}$ $_{25.07}^{33.07}$	23.76 $_{23.44}^{24.17}$ $_{23.44}^{24.17}$	4.67 $_{4.46}^{4.90}$ $_{4.46}^{4.90}$	0.53 $_{0.44}^{0.62}$ $_{0.44}^{0.62}$	< 0.03	–	> 149.65	0.29 $_{0.31}^{0.24}$ $_{0.31}^{0.24}$	< 0.22	$3 . 52_{2.52}^{4.52}$ ${3.52_{2.52}^{4.52}}$	3.91*	$0 . 40_{0.39}^{0.41}$ ${0.40_{0.39}^{0.41}}$
I11119+3257	X-S/MIR-TP	0.91	2.41 $_{2.36}^{2.49}$ $_{2.36}^{2.49}$	22.88 $_{22.82}^{22.94}$ $_{22.82}^{22.94}$	78.34 $_{78.3}^{78.51}$ $_{78.3}^{78.51}$	12.05 $_{11.92}^{12.10}$ $_{11.92}^{12.10}$	> 39.63	0.04 $_{0.03}^{0.06}$ $_{0.03}^{0.06}$	0.5 $_{0.38}^{0.51}$ $_{0.38}^{0.51}$	–	> 154.12	0.0 $_{0.01}^{0.01}$ $_{0.01}^{0.01}$	$6 . 89_{6.75}^{7.02}$ $6.89_{6.75}^{7.02}$	$1 . 44_{1.37}^{1.50}$ ${1.44_{1.37}^{1.50}}$	$4 . 05_{3.93}^{4.16}$ ${4.05_{3.93}^{4.16}}$	$0 . 21_{0.20}^{0.22}$ ${0.21_{0.20}^{0.22}}$
Mrk231	X-S/MIR-TP	1.17	1.47 $_{1.43}^{1.52}$ $_{1.43}^{1.52}$	22.84 $_{22.79}^{22.88}$ $_{22.79}^{22.88}$	> 86.85	10.29 $_{10.21}^{10.56}$ $_{10.21}^{10.56}$	> 28.35	0.07 $_{0.04}^{0.12}$ $_{0.04}^{0.12}$	0.5 $_{0.39}^{0.54}$ $_{0.39}^{0.54}$	–	> 147.18	0.0 $_{0.0}^{0.03}$ $_{0.0}^{0.03}$	5.83 $_{5.61}^{6.16}$ $_{5.61}^{6.16}$	$2 . 12_{1.47}^{2.78}$ ${2.12_{1.47}^{2.78}}$	$4 . 62_{4.40}^{4.84}$ ${4.62_{4.40}^{4.84}}$	$0 . 18_{0.17}^{0.19}$ ${0.18_{0.17}^{0.19}}$
Mrk1383	X-C/MIR-TP	0.99	2.10 $_{2.05}^{2.12}$ $_{2.05}^{2.12}$	20.6 $_{20.58}^{20.66}$ $_{20.58}^{20.66}$	75.13 $_{74.83}^{75.30}$ $_{74.83}^{75.30}$	17.6 $_{17.23}^{17.86}$ $_{17.23}^{17.86}$	< 2.03	0.07 $_{0.05}^{0.14}$ $_{0.05}^{0.14}$	< 0.01	–	> 153.31	0.99 $_{1.01}^{0.98}$ $_{1.01}^{0.98}$	< 0.33	$1 . 49_{0.38}^{2.60}$ ${1.49_{0.38}^{2.60}}$	$3 . 94_{3.92}^{3.96}$ ${3.94_{3.92}^{3.96}}$	$0 . 30_{0.29}^{0.31}$ ${0.30_{0.29}^{0.31}}$
Mrk1392	X-C/MIR-C	0.92	1.93 $_{1.89}^{1.99}$ $_{1.89}^{1.99}$	< 21.86	< 23.46	57.5 $_{51.07}^{60.97}$ $_{51.07}^{60.97}$	16.91 $_{16.50}^{18.07}$ $_{16.50}^{18.07}$	< 0.1	–	8.27 $_{7.08}^{10.13}$ $_{7.08}^{10.13}$	114.92 $_{92.38}^{182.98}$ $_{92.38}^{182.98}$	–	2.03 $_{1.71}^{2.38}$ $_{1.71}^{2.38}$	$2 . 19_{1.59}^{2.80}$ ${2.19_{1.59}^{2.80}}$	$5 . 95_{5.84}^{6.07}$ ${5.95_{5.84}^{6.07}}$	$0 . 95_{0.92}^{0.97}$ ${0.95_{0.92}^{0.97}}$
ESO141-G055	X-C/MIR-TP	1.03	1.94 $_{1.93}^{1.95}$ $_{1.93}^{1.95}$	21.04 $_{20.9}^{21.13}$ $_{20.9}^{21.13}$	69.86 $_{69.57}^{70.20}$ $_{69.57}^{70.20}$	17.79 $_{17.57}^{18.13}$ $_{17.57}^{18.13}$	2.72 $_{2.68}^{2.76}$ $_{2.68}^{2.76}$	0.05 $_{0.02}^{0.1}$ $_{0.02}^{0.1}$	0.5 $_{0.42}^{0.87}$ $_{0.42}^{0.87}$	–	107.07 $_{105.06}^{109.07}$ $_{105.06}^{109.07}$	1.6 $_{1.62}^{1.58}$ $_{1.62}^{1.58}$	< 0.21	$0 . 86_{0.40}^{1.33}$ ${0.86_{0.40}^{1.33}}$	$5 . 99_{5.89}^{6.09}$ ${5.99_{5.89}^{6.09}}$	$0 . 30_{0.31}^{0.32}$ ${0.30_{0.31}^{0.32}}$
NGC7213	X-S/MIR-C	1.08	1.89 $_{1.88}^{1.89}$ $_{1.88}^{1.89}$	22.13 $_{22.05}^{22.16}$ $_{22.05}^{22.16}$	31.67 $_{29.84}^{32.61}$ $_{29.84}^{32.61}$	23.46 $_{23.33}^{23.60}$ $_{23.33}^{23.60}$	20.02 $_{18.33}^{21.70}$ $_{18.33}^{21.70}$	0.64 $_{0.63}^{0.65}$ $_{0.63}^{0.65}$	–	5.85 $_{5.62}^{5.89}$ $_{5.62}^{5.89}$	< 59.32	–	4.81 $_{4.74}^{4.87}$ $_{4.74}^{4.87}$	$0 . 49_{0.32}^{0.67}$ ${0.49_{0.32}^{0.67}}$	$3 . 07_{2.98}^{3.16}$ ${3.07_{2.98}^{3.16}}$	$0 . 54_{0.52}^{0.56}$ ${0.54_{0.52}^{0.56}}$

Seyfert 2

UM146	X-C/MIR-C	0.66	2.13 $_{1.98}^{2.26}$ $_{1.98}^{2.26}$	23.06 $_{22.97}^{23.15}$ $_{22.97}^{23.15}$	< 42.77	> 54.73	> 91.18	1.2 $_{1.15}^{1.25}$ $_{1.15}^{1.25}$	–	4.0 $_{3.33}^{5.46}$ $_{3.33}^{5.46}$	138.0 $_{94.97}^{263.22}$ $_{94.97}^{263.22}$	–	3.92 $_{3.35}^{4.47}$ $_{3.35}^{4.47}$	$2 . 67_{2.25}^{3.10}$ ${2.67_{2.25}^{3.10}}$	$4 . 66_{4.56}^{4.76}$ ${4.66_{4.56}^{4.76}}$	> 0.84
NGC788	X-C/MIR-C	0.88	1.58 $_{1.50}^{1.64}$ $_{1.50}^{1.64}$	23.64 $_{23.59}^{23.69}$ $_{23.59}^{23.69}$	> 73.9	< 45.69	13.28 $_{11.82}^{14.49}$ $_{11.82}^{14.49}$	1.0 $_{0.52}^{1.22}$ $_{0.52}^{1.22}$	–	6.23 $_{5.46}^{7.39}$ $_{5.46}^{7.39}$	169.2 $_{127.43}^{237.26}$ $_{127.43}^{237.26}$	–	1.69 $_{1.41}^{1.95}$ $_{1.41}^{1.95}$	$0 . 74_{0.30}^{1.19}$ ${0.74_{0.30}^{1.19}}$	$3 . 94_{3.75}^{4.12}$ ${3.94_{3.75}^{4.12}}$	> 0.84
NGC1358	X-S/MIR-C	0.66	1.69 $_{1.63}^{1.78}$ $_{1.63}^{1.78}$	24.23 $_{24.21}^{24.27}$ $_{24.21}^{24.27}$	< 38.81	< 67.26	> 78.09	0.65 $_{0.27}^{0.88}$ $_{0.27}^{0.88}$	–	8.77 $_{6.16}^{11.45}$ $_{6.16}^{11.45}$	< 260.87	–	> 7.95	$7 . 67_{5.11}^{10.23}$ ${7.67_{5.11}^{10.23}}$	$6 . 48_{6.25}^{6.71}$ ${6.48_{6.25}^{6.71}}$	> 0.84
Mrk78	X-C/MIR-C	1.01	1.40 $_{1.32}^{1.52}$ $_{1.32}^{1.52}$	23.56 $_{23.51}^{23.62}$ $_{23.51}^{23.62}$	59.73 $_{40.97}^{72.83}$ $_{40.97}^{72.83}$	41.29 $_{26.98}^{64.67}$ $_{26.98}^{64.67}$	32.12 $_{27.45}^{35.55}$ $_{27.45}^{35.55}$	1.1 $_{0.82}^{1.22}$ $_{0.82}^{1.22}$	–	5.9 $_{4.25}^{7.47}$ $_{4.25}^{7.47}$	187.01 $_{118.36}^{280.95}$ $_{118.36}^{280.95}$	–	4.92 $_{4.59}^{5.26}$ $_{4.59}^{5.26}$	$3 . 78_{2.35}^{5.20}$ ${3.78_{2.35}^{5.20}}$	$5 . 22_{5.04}^{5.40}$ ${5.22_{5.04}^{5.40}}$	> 0.86
[4pt] Mrk1210	X-C/MIR-TP	0.92	1.67 $_{1.63}^{1.72}$ $_{1.63}^{1.72}$	23.3 $_{23.28}^{23.32}$ $_{23.28}^{23.32}$	39.21 $_{38.52}^{40.59}$ $_{38.52}^{40.59}$	60.02 $_{59.38}^{60.59}$ $_{59.38}^{60.59}$	20.0 $_{19.76}^{20.21}$ $_{19.76}^{20.21}$	< 0.01	0.5 $_{0.33}^{0.53}$ $_{0.33}^{0.53}$	–	80.5 $_{76.54}^{83.83}$ $_{76.54}^{83.83}$	0.11 $_{0.05}^{0.17}$ $_{0.05}^{0.17}$	< 0.07	$1 . 84_{1.55}^{2.12}$ ${1.84_{1.55}^{2.12}}$	$4 . 86_{4.72}^{4.99}$ ${4.86_{4.72}^{4.99}}$	$0 . 87_{0.86}^{0.88}$ ${0.87_{0.86}^{0.88}}$
J105943+65040	X-C/MIR-S	0.44	1.79 $_{1.65}^{1.90}$ $_{1.65}^{1.90}$	22.82 $_{22.65}^{22.94}$ $_{22.65}^{22.94}$	< 21.14	25.0 $_{23.53}^{26.1}$ $_{23.53}^{26.1}$	< 10.3	> 0.03	< 0.03	–	> 171.67	–	$3 . 80_{3.39}^{4.38}$ $3.80_{3.39}^{4.38}$	$2 . 79_{2.39}^{3.19}$ ${2.79_{2.39}^{3.19}}$	> 7.54	$0 . 42_{0.40}^{0.44}$ ${0.42_{0.40}^{0.44}}$
NGC4939	X-C/MIR-TP	0.98	1.62 $_{1.56}^{1.73}$ $_{1.56}^{1.73}$	23.67 $_{23.62}^{23.71}$ $_{23.62}^{23.71}$	< 26.39	75.12 $_{72.21}^{76.94}$ $_{72.21}^{76.94}$	20.85 $_{20.39}^{21.32}$ $_{20.39}^{21.32}$	< 0.01	< 0.02	–	83.3 $_{76.93}^{85.81}$ $_{76.93}^{85.81}$	> 1.0	< 0.07	$0 . 78_{0.64}^{0.92}$ ${0.78_{0.64}^{0.92}}$	1.69*	$0 . 97_{0.95}^{0.98}$ ${0.97_{0.95}^{0.98}}$
IC4518W	X-C/MIR-TP	0.8	1.70 $_{1.59}^{1.79}$ $_{1.59}^{1.79}$	23.14 $_{23.07}^{23.2}$ $_{23.07}^{23.2}$	> 79.41	12.22 $_{11.63}^{15.82}$ $_{11.63}^{15.82}$	> 38.72	0.96 $_{0.9}^{1.01}$ $_{0.9}^{1.01}$	< 0.04	–	83.44 $_{81.76}^{89.03}$ $_{81.76}^{89.03}$	> 1.0	$12 . 65_{12.25}^{13.08}$ $12.65_{12.25}^{13.08}$	$3 . 0_{2.8}^{3.2}$ ${3.0_{2.8}^{3.2}}$	2.02*	$0 . 21_{0.20}^{0.27}$ ${0.21_{0.20}^{0.27}}$
ESO138-G1	X-C/MIR-C	0.95	2.06 $_{2.00}^{2.11}$ $_{2.00}^{2.11}$	23.29 $_{23.23}^{23.34}$ $_{23.23}^{23.34}$	60.06 $_{54.92}^{67.73}$ $_{54.92}^{67.73}$	< 16.56	> 54.22	1.99 $_{1.92}^{2.03}$ $_{1.92}^{2.03}$	–	4.83 $_{3.63}^{6.64}$ $_{3.63}^{6.64}$	306.01 $_{170.92}^{529.97}$ $_{170.92}^{529.97}$	–	4.32 $_{3.94}^{4.50}$ $_{3.94}^{4.50}$	$1 . 3_{0.6}^{2.0}$ ${1.3_{0.6}^{2.0}}$	$2 . 71_{2.60}^{2.82}$ ${2.71_{2.60}^{2.82}}$	$0 . 35_{0.31}^{0.40}$ ${0.35_{0.31}^{0.40}}$
NGC6300	X-S/MIR-TP	0.89	1.90 $_{1.86}^{1.94}$ $_{1.86}^{1.94}$	24.42 $_{24.37}^{24.47}$ $_{24.37}^{24.47}$	81.31 $_{80.79}^{82.33}$ $_{80.79}^{82.33}$	14.17 $_{13.55}^{14.34}$ $_{13.55}^{14.34}$	> 39.73	1.38 $_{1.35}^{1.42}$ $_{1.35}^{1.42}$	0.5 $_{0.4}^{0.52}$ $_{0.4}^{0.52}$	–	> 153.23	> 1.0	$13 . 44_{13.12}^{13.76}$ $13.44_{13.12}^{13.76}$	$1 . 03_{0.99}^{1.08}$ ${1.03_{0.99}^{1.08}}$	$3 . 45_{3.34}^{3.55}$ ${3.45_{3.34}^{3.55}}$	$0 . 24_{0.23}^{0.25}$ ${0.24_{0.23}^{0.25}}$
ESO103-G35	X-C/MIR-C	1.04	1.80 $_{1.78}^{1.81}$ $_{1.78}^{1.81}$	23.24 $_{23.23}^{23.24}$ $_{23.23}^{23.24}$	34.84 $_{26.58}^{49.49}$ $_{26.58}^{49.49}$	> 65.1	14.28 $_{13.8}^{14.71}$ $_{13.8}^{14.71}$	0.5 $_{0.14}^{0.58}$ $_{0.14}^{0.58}$	–	3.96 $_{3.7}^{4.28}$ $_{3.7}^{4.28}$	175.82 $_{153.66}^{204.31}$ $_{153.66}^{204.31}$	–	$6 . 72_{6.52}^{6.90}$ $6.72_{6.52}^{6.90}$	$1 . 90_{1.39}^{2.41}$ ${1.90_{1.39}^{2.41}}$	$5 . 21_{5.11}^{5.31}$ ${5.21_{5.11}^{5.31}}$	$0 . 90_{0.88}^{0.91}$ ${0.90_{0.88}^{0.91}}$
IC5063	X-C/MIR-C	0.87	1.80 $_{1.78}^{1.83}$ $_{1.78}^{1.83}$	23.33 $_{23.31}^{23.35}$ $_{23.31}^{23.35}$	73.06 $_{69.82}^{74.06}$ $_{69.82}^{74.06}$	< 16.19	> 93.31	2.06 $_{2.03}^{2.09}$ $_{2.03}^{2.09}$	–	> 14.36	> 735.26	–	$3 . 12_{2.94}^{3.28}$ $3.12_{2.94}^{3.28}$	$5 . 85_{4.88}^{6.83}$ ${5.85_{4.88}^{6.83}}$	$3 . 94_{3.88}^{4.00}$ ${3.94_{3.88}^{4.00}}$	$0 . 43_{0.41}^{0.46}$ ${0.43_{0.41}^{0.46}}$
PKS2356-61	X-C/MIR-C	0.67	1.86 $_{1.78}^{1.95}$ $_{1.78}^{1.95}$	23.13 $_{23.07}^{23.20}$ $_{23.07}^{23.20}$	< 21.51	50.37 $_{41.06}^{58.14}$ $_{41.06}^{58.14}$	19.24 $_{15.47}^{23.33}$ $_{15.47}^{23.33}$	< 0.56	–	6.94 $_{4.65}^{9.88}$ $_{4.65}^{9.88}$	169.26 $_{98.16}^{332.3}$ $_{98.16}^{332.3}$	–	$6 . 09_{5.65}^{6.52}$ $6.09_{5.65}^{6.52}$	$8 . 45_{4.95}^{11.95}$ ${8.45_{4.95}^{11.95}}$	$6 . 71_{6.55}^{6.86}$ ${6.71_{6.55}^{6.86}}$	$0 . 95_{0.92}^{0.97}$ ${0.95_{0.92}^{0.97}}$

Notes. Column (1): Source name. Column (2): Baseline model used. Column (3): Reduced χ² (χ²/d.o.f.). Columns (4–6): Final reflection parameter values per model. Columns (7–13): Final dust parameter values per model. Column (14): Color excess for the foreground extinction. The asterisk next to the value indicates that the parameter is not constrained. For each parameter, we report the value obtained from the best fit, accompanied by the minimum and maximum values calculated at +/– 1σ. The outer radius is calculated as R_out = Y * R_in = Y * 1.3 * (L_bol/10⁴⁶)^1/2.

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