Towards a complete census of luminous Compton-thick active galactic nuclei in the Local Universe

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Volume 692 (December 2024)

A&A, 692 (2024) A250

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Table A.2.

Spectral fitting results using the simple power-law model.

Source name	Mission¹	PHABS_GAL * (APEC + PHABS * PO + GA) model parameters

		kT	N_APEC	Γ_{soft PO}	N_{soft PO}	Γ_{hard PO}	N_H	N_{hard PO}	FeK line (EW)	χ²/dof
		keV	×10⁻⁵		×10⁻⁵		×10²²cm⁻²	×10⁻³	eV
2MASXJ01500266-0725482	X,N	-	-	-	-	$2 . 11_{- 0.10}^{+ 0.10}$ $2.11^{+0.10}_{-0.10}$	$0 . 091_{- 0.33}^{+ 0.34}$ $0.091^{+0.34}_{-0.33}$	$0 . 36_{- 0.06}^{+ 0.08}$ $0.36^{+0.08}_{-0.06}$	$6 . 43_{- 0.10}^{+ 0.25}$ $6.43^{+0.25}_{-0.10}$ ( $290_{- 150}^{+ 190})$ $290^{+190}_{-150})$	115.99/103
NGC3094	X,N	$0 . 77_{- 0.12}^{+ 0.10}$ $0.77^{+0.10}_{-0.12}$	$0 . 87_{- 0.35}^{+ 0.74}$ $0.87^{+0.74}_{-0.35}$	-	-	$1 . 92_{- 0.28}^{+ 0.41}$ $1.92^{+0.41}_{-0.28}$	< 0.14	$0 . 021_{- 0.011}^{+ 0.018}$ $0.021^{+0.018}_{-0.011}$	-	48.89/40
UGC04145	X	$0 . 68_{- 0.13}^{+ 0.11}$ $0.68^{+0.11}_{-0.13}$	$1 . 24_{- 0.64}^{- 0.69}$ $1.24^{-0.69}_{-0.64}$	-	-	$2 . 43_{- 0.83}^{+ 1.55}$ $2.43^{+1.55}_{-0.83}$	< 1.16	$0 . 019_{- 0.010}^{+ 0.073}$ $0.019^{+0.073}_{-0.010}$	-	6.7/8

Notes.⁽¹⁾X:XMM-Newton data have been used , C: Chandra data have been used, N: NuSTAR data have been used

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