Compton-thick AGN in the NuSTAR Era X: Analysing seven local CT-AGN candidates

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Volume 676 (August 2023)

A&A, 676 (2023) A103

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Table A.1.

Summary of best-fit solutions of NuSTAR data using different models for NGC 4180

Model	MyTorus	MyTorus	borus02
					Edge-on	Face-on
χ²/dof					76/64	84/64	76/62
C_Ins^a				1.47	1.48	1.47
Γ			1.66	1.40	1.55
C_Tor		—	—	0.88
θ_Inc	—	—	49
N_H,z					6.10	1.49	1.78
N_H,S				1.97	3.98	1.74
f_s10⁻²			0.40	0.55	2.27
F_{2 − 10keV}		1.34	1.30	1.33
F_{10 − 50keV}	4.49	4.73	4.54
L_{2 − 10keV}^b					11.01	2.72	3.21
L_{10 − 50keV}^c				19.05	7.14	6.63

Notes. We summarise here the best-fits of NuSTAR spectra using different torus models between 3 and 50 keV, referred in Section 4.2. The statistics and degrees of freedom for each fit are also reported. The parameters are reported as in Table 2 if not mentioned otherwise.

C_Ins is the ratio of cross-normalisation constant between two NuSTAR observations through their FPMA detectors.

Intrinsic luminosity between 2 and 10 keV in 10⁴¹ erg s⁻¹.

Intrinsic luminosity between 10 and 50 keV in 10⁴¹ erg s⁻¹.

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