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 4.

Simultaneous fit results (θ_tor ≠ σ_tor).

Objname	Baseline	χ_r²	X-ray parameters				IR parameters
	Model		Γ	log(N_{H_tor})	θ_tor	θ_inc	σ_tor	Y	α_r	α_p	N0	τ_ν	log(P_size)
				[cm⁻²]	[°]	[°]	[°]				[#]		[μm]
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)	(10)	(11)	(12)	(13)	(14)
Seyfert 1

Mrk590	X-C/MIR-C	0.81	2.0 $_{1.94}^{2.04}$ $_{1.94}^{2.04}$	22.16 $_{22.13}^{22.24}$ $_{22.13}^{22.24}$	< 17.1	77.6 $_{72.19}^{81.63}$ $_{72.19}^{81.63}$	< 20.58	10.0 $_{9.9}^{10.4}$ $_{9.9}^{10.4}$	< 0.03	–	4.4 $_{3.4}^{5.5}$ $_{3.4}^{5.5}$	387.9 $_{262.0}^{533.7}$ $_{262.0}^{533.7}$	–
PG0804+761	X-C/MIR-TP	0.88	1.93 $_{1.89}^{1.96}$ $_{1.89}^{1.96}$	20.8 $_{20.7}^{21.3}$ $_{20.7}^{21.3}$	< 79.1	30.67 $_{26.66}^{31.96}$ $_{26.66}^{31.96}$	24.31 $_{24.09}^{24.67}$ $_{24.09}^{24.67}$	6.7 $_{6.4}^{6.9}$ $_{6.4}^{6.9}$	1.0 $_{0.92}^{1.02}$ $_{0.92}^{1.02}$	0.5 $_{0.32}^{0.52}$ $_{0.32}^{0.52}$	–	> 153.9
IRAS11119+3257	X-S/MIR-TP	0.92	2.42 $_{2.4}^{2.46}$ $_{2.4}^{2.46}$	22.89 $_{22.83}^{22.94}$ $_{22.83}^{22.94}$	< 27.8	78.23 $_{78.11}^{78.33}$ $_{78.11}^{78.33}$	12.23 $_{12.12}^{12.27}$ $_{12.12}^{12.27}$	> 39.7	0.05 $_{0.04}^{0.07}$ $_{0.04}^{0.07}$	0.5 $_{0.4}^{0.51}$ $_{0.4}^{0.51}$	–	> 154.0	0.0 $_{0.01}^{0.0}$ $_{0.01}^{0.0}$
Mrk231	X-S/MIR-TP	1.19	1.47 $_{1.4}^{1.53}$ $_{1.4}^{1.53}$	22.83 $_{22.74}^{22.91}$ $_{22.74}^{22.91}$	23.6*	> 86.99	10.21 $_{10.19}^{10.24}$ $_{10.19}^{10.24}$	> 39.0	0.5 $_{0.44}^{0.52}$ $_{0.44}^{0.52}$	< 0.01	–	> 153.3	0.19 $_{0.16}^{0.21}$ $_{0.16}^{0.21}$
Mrk1383	X-C/MIR-TP	1.08	2.11 $_{2.09}^{2.14}$ $_{2.09}^{2.14}$	20.18 $_{20.16}^{20.2}$ $_{20.16}^{20.2}$	< 13.7	62.29 $_{62.05}^{62.54}$ $_{62.05}^{62.54}$	24.34 $_{24.12}^{24.72}$ $_{24.12}^{24.72}$	4.5 $_{4.3}^{4.6}$ $_{4.3}^{4.6}$	1.0 $_{0.98}^{1.01}$ $_{0.98}^{1.01}$	0.5 $_{0.41}^{0.51}$ $_{0.41}^{0.51}$	–	> 154.3	0.6 $_{0.62}^{0.6}$ $_{0.62}^{0.6}$
Mrk1392	X-C/MIR-C	0.92	1.94 $_{1.87}^{2.01}$ $_{1.87}^{2.01}$	20.31 $_{20.25}^{20.35}$ $_{20.25}^{20.35}$	10.0 $_{1.9}^{15.3}$ $_{1.9}^{15.3}$	< 27.83	57.23 $_{49.32}^{63.45}$ $_{49.32}^{63.45}$	16.9 $_{16.4}^{18.4}$ $_{16.4}^{18.4}$	< 0.17	–	8.3 $_{7.1}^{10.3}$ $_{7.1}^{10.3}$	115.7 $_{90.3}^{178.6}$ $_{90.3}^{178.6}$	–
ESO141-G055	X-C/MIR-TP	1.04	1.94 $_{1.93}^{1.95}$ $_{1.93}^{1.95}$	21.02 $_{20.93}^{21.12}$ $_{20.93}^{21.12}$	15.5 $_{13.3}^{17.3}$ $_{13.3}^{17.3}$	69.86 $_{69.71}^{70.01}$ $_{69.71}^{70.01}$	18.06 $_{17.92}^{18.48}$ $_{17.92}^{18.48}$	2.7 $_{2.6}^{2.7}$ $_{2.6}^{2.7}$	0.5 $_{0.44}^{0.51}$ $_{0.44}^{0.51}$	> 1.46	–	132.6 $_{130.0}^{134.9}$ $_{130.0}^{134.9}$	1.3 $_{1.31}^{1.29}$ $_{1.31}^{1.29}$
NGC7213	X-S/MIR-C	1.08	1.89 $_{1.88}^{1.89}$ $_{1.88}^{1.89}$	22.14 $_{22.1}^{22.17}$ $_{22.1}^{22.17}$	23.5 $_{22.8}^{24.2}$ $_{22.8}^{24.2}$	31.77 $_{30.23}^{32.92}$ $_{30.23}^{32.92}$	17.44 $_{17.37}^{17.5}$ $_{17.37}^{17.5}$	20.3 $_{20.1}^{20.5}$ $_{20.1}^{20.5}$	0.69 $_{0.68}^{0.7}$ $_{0.68}^{0.7}$	–	6.1 $_{6.1}^{6.6}$ $_{6.1}^{6.6}$	< 66.1	–

Seyfert 2

UM146	X-C/MIR-C	0.66	2.10 $_{1.97}^{2.24}$ $_{1.97}^{2.24}$	23.05 $_{22.96}^{23.13}$ $_{22.96}^{23.13}$	27.8*	< 39.35	> 57.63	> 91.1	1.2 $_{1.14}^{1.25}$ $_{1.14}^{1.25}$	–	4.0 $_{3.3}^{5.4}$ $_{3.3}^{5.4}$	138.1 $_{93.3}^{258.8}$ $_{93.3}^{258.8}$	–
NGC788	X-C/MIR-C	0.88	1.58 $_{1.49}^{1.64}$ $_{1.49}^{1.64}$	23.69 $_{23.62}^{23.75}$ $_{23.62}^{23.75}$	> 10.0	> 69.25	37.08 $_{19.05}^{64.44}$ $_{19.05}^{64.44}$	13.3 $_{11.7}^{14.4}$ $_{11.7}^{14.4}$	1.0 $_{0.31}^{1.2}$ $_{0.31}^{1.2}$	–	5.9 $_{4.8}^{8.0}$ $_{4.8}^{8.0}$	164.9 $_{112.6}^{269.1}$ $_{112.6}^{269.1}$	–
NGC1358	X-S/MIR-C	0.67	1.66 $_{1.57}^{1.77}$ $_{1.57}^{1.77}$	24.24 $_{24.2}^{24.27}$ $_{24.2}^{24.27}$	< 57.8	< 57.3	65.19*	> 80.8	0.65 $_{0.31}^{0.86}$ $_{0.31}^{0.86}$	–	7.4 $_{5.4}^{11.8}$ $_{5.4}^{11.8}$	< 249.6	–
Mrk78	X-C/MIR-C	1.01	1.44 $_{1.35}^{1.54}$ $_{1.35}^{1.54}$	23.57 $_{23.51}^{23.62}$ $_{23.51}^{23.62}$	> 9.0	59.68 $_{39.09}^{70.01}$ $_{39.09}^{70.01}$	41.12 $_{29.86}^{62.95}$ $_{29.86}^{62.95}$	32.1 $_{26.9}^{35.6}$ $_{26.9}^{35.6}$	1.1 $_{0.81}^{1.22}$ $_{0.81}^{1.22}$	–	5.9 $_{4.2}^{7.5}$ $_{4.2}^{7.5}$	187.8 $_{118.1}^{280.6}$ $_{118.1}^{280.6}$	–
Mrk1210	X-C/MIR-TP	0.93	1.68 $_{1.62}^{1.74}$ $_{1.62}^{1.74}$	23.3 $_{23.28}^{23.32}$ $_{23.28}^{23.32}$	80.0*	39.24 $_{38.44}^{41.26}$ $_{38.44}^{41.26}$	60.0 $_{59.31}^{60.56}$ $_{59.31}^{60.56}$	20.0 $_{19.8}^{20.2}$ $_{19.8}^{20.2}$	< 0.01	0.5 $_{0.31}^{0.53}$ $_{0.31}^{0.53}$	–	80.3 $_{76.5}^{83.8}$ $_{76.5}^{83.8}$	0.11 $_{0.05}^{0.17}$ $_{0.05}^{0.17}$
J105943+65040	X-C/MIR-S	0.44	1.79 $_{1.65}^{1.89}$ $_{1.65}^{1.89}$	22.82 $_{22.7}^{22.93}$ $_{22.7}^{22.93}$	27.9*	< 20.98	25.0 $_{24.23}^{26.12}$ $_{24.23}^{26.12}$	< 10.3	> 0.02	< 0.03	–	> 172.5	–
NGC4939	X-C/MIR-TP	0.98	1.61 $_{1.54}^{1.72}$ $_{1.54}^{1.72}$	23.67 $_{23.63}^{23.73}$ $_{23.63}^{23.73}$	23.0*	< 26.38	75.0 $_{72.23}^{77.02}$ $_{72.23}^{77.02}$	20.8 $_{20.4}^{21.3}$ $_{20.4}^{21.3}$	< 0.01	< 0.02	–	83.3 $_{77.0}^{85.7}$ $_{77.0}^{85.7}$	> 1.0
IC4518W	X-C/MIR-TP	0.92	1.7 $_{1.59}^{1.81}$ $_{1.59}^{1.81}$	23.14 $_{23.07}^{23.2}$ $_{23.07}^{23.2}$	10.0*	> 85.64	11.81 $_{11.31}^{13.01}$ $_{11.31}^{13.01}$	> 39.5	0.10 $_{0.06}^{0.20}$ $_{0.06}^{0.20}$	< 0.02	–	74.0 $_{69.0}^{79.9}$ $_{69.0}^{79.9}$	0.12 $_{0.14}^{0.09}$ $_{0.14}^{0.09}$
ESO138-G1	X-C/MIR-C	0.94	2.04 $_{1.99}^{2.1}$ $_{1.99}^{2.1}$	23.31 $_{23.24}^{23.37}$ $_{23.24}^{23.37}$	< 9.7	60.0 $_{44.34}^{64.06}$ $_{44.34}^{64.06}$	< 25.4	> 52.8	1.99 $_{1.94}^{2.02}$ $_{1.94}^{2.02}$	–	4.8 $_{3.6}^{6.3}$ $_{3.6}^{6.3}$	306.1 $_{169.6}^{503.3}$ $_{169.6}^{503.3}$	–
NGC6300	X-S*/MIR-TP	0.89	1.9 $_{1.85}^{1.94}$ $_{1.85}^{1.94}$	24.46 $_{24.38}^{24.5}$ $_{24.38}^{24.5}$	12.7 $_{11.5}^{15.8}$ $_{11.5}^{15.8}$	81.58 $_{79.44}^{83.13}$ $_{79.44}^{83.13}$	14.1 $_{13.67}^{14.28}$ $_{13.67}^{14.28}$	> 39.7	1.39 $_{1.35}^{1.43}$ $_{1.35}^{1.43}$	0.5 $_{0.39}^{0.52}$ $_{0.39}^{0.52}$	–	> 153.2	> 1.0
ESO103-G35	X-C/MIR-C	1.04	1.8 $_{1.79}^{1.81}$ $_{1.79}^{1.81}$	23.24 $_{23.23}^{23.25}$ $_{23.23}^{23.25}$	> 76.3	34.57 $_{26.56}^{43.61}$ $_{26.56}^{43.61}$	> 59.61	14.3 $_{13.8}^{14.8}$ $_{13.8}^{14.8}$	0.5 $_{0.17}^{0.58}$ $_{0.17}^{0.58}$	–	4.0 $_{3.8}^{4.8}$ $_{3.8}^{4.8}$	176.5 $_{156.9}^{228.6}$ $_{156.9}^{228.6}$	–
IC5063	X-C/MIR-C	0.86	1.8 $_{1.77}^{1.83}$ $_{1.77}^{1.83}$	23.33 $_{23.31}^{23.35}$ $_{23.31}^{23.35}$	< 10.3	72.83 $_{69.59}^{74.04}$ $_{69.59}^{74.04}$	< 16.36	> 93.2	2.06 $_{2.03}^{2.09}$ $_{2.03}^{2.09}$	–	> 14.4	> 735.3	–
PKS2356-61	X-C/MIR-C	0.67	1.86 $_{1.78}^{1.94}$ $_{1.78}^{1.94}$	23.12 $_{23.05}^{23.18}$ $_{23.05}^{23.18}$	> 38.0	< 21.7	50.83 $_{46.03}^{60.85}$ $_{46.03}^{60.85}$	19.3 $_{18.3}^{23.4}$ $_{18.3}^{23.4}$	< 0.57	–	6.9 $_{4.6}^{9.7}$ $_{4.6}^{9.7}$	166.8 $_{96.5}^{309.7}$ $_{96.5}^{309.7}$	–

Notes. Column (1): Source name. Column (2): Baseline model used (Combination X-ray model/IR model). The asterisk next to model indicates that N_{H_tor} ≤ N_{H_los}. Column (3): Reduced χ² (χ²/d.o.f.). Columns (4–7): Final reflection parameter values per model (see Table 2). Columns (8–14): Final dust parameter values per model (see Table 1). The asterisk next to the value indicates that the parameter is not constrained. The confidence range of error calculated here is 1σ. For each parameter, we report the value obtained from the best fit, accompanied by the minimum and maximum values calculated at +/– 1σ.

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