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.4.

Spectral fitting results of Compton-thick sources only using the UXCLUMPY model.

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

		Γ_soft	N_soft	kT	N_APEC	Γ	N_H^eq	N_H^los	θ_inc	(σ_torus)	N_UXCLUMPY	χ²/dof
			×10⁻⁵	keV	×10⁻⁵		×10²² cm⁻²	×10²² cm⁻²	deg.		×10⁻³
ESO420-013	C,N	$3 . 35_{- 0.24}^{+ 0.40}$ $3.35^{+0.40}_{-0.24}$	$5 . 14_{- 2.43}^{+ 2.06}$ $5.14^{+2.06}_{-2.43}$	$0 . 86_{- 0.07}^{+ 0.08}$ $0.86^{+0.08}_{-0.07}$	$2 . 55_{- 1.21}^{+ 0.44}$ $2.55^{+0.44}_{-1.21}$	$1 . 53_{- 0.28}^{+ 0.27}$ $1.53^{+0.27}_{-0.28}$	-	> 292	90(f)	30(f)	$0 . 89_{- 0.11}^{+ 1.42}$ $0.89^{+1.42}_{-0.11}$	100.83/95
UGC01214	X,N	$3 . 61_{- 0.16}^{+ 0.20}$ $3.61^{+0.20}_{-0.16}$	$9 . 61_{- 1.01}^{+ 0.91}$ $9.61^{+0.91}_{-1.01}$	$0 . 88_{- 0.09}^{+ 0.10}$ $0.88^{+0.10}_{-0.09}$	$1 . 58_{- 0.58}^{+ 0.60}$ $1.58^{+0.60}_{-0.58}$	$2 . 33_{- 0.22}^{+ 0.31}$ $2.33^{+0.31}_{-0.22}$	-	> 345	90(f)	30(f)	$16 . 46_{- 7.91}^{+ 21.70}$ $16.46^{+21.70}_{-7.91}$	85.17/72
2MASXJ04405494-0822221	X,N	-	-	$0 . 38_{- 0.12}^{+ 0.33}$ $0.38^{+0.33}_{-0.12}$	0.22 $_{- 0.14}^{+ 0.18}$ $^{+0.18}_{-0.14}$	$2 . 17_{- 0.21}^{+ 0.20}$ $2.17^{+0.20}_{-0.21}$	-	> 298	90(f)	30(f)	18.57 $_{- 6.90}^{+ 11.21}$ $^{+11.21}_{-6.90}$	80.91/58
IC4769	X	-	-	0.75 $_{- 0.10}^{+ 0.10}$ $^{+0.10}_{-0.10}$	0.38 $_{- 0.11}^{+ 0.11}$ $^{+0.11}_{-0.11}$	$2 . 01_{- 0.32}^{+ 0.34}$ $2.01^{+0.34}_{-0.32}$	-	> 142	90(f)	30(f)	5.12 $_{- 2.97}^{+ 6.47}$ $^{+6.47}_{-2.97}$	71.42/55
IC4995	X,N	5.53 $_{- 1.62}^{+ 3.15}$ $^{+3.15}_{-1.62}$	0.81 $_{- 0.69}^{+ 1.41}$ $^{+1.41}_{-0.69}$	0.79 $_{- 0.14}^{+ 0.16}$ $^{+0.16}_{-0.14}$	0.73 $_{- 0.42}^{+ 0.44}$ $^{+0.44}_{-0.42}$	2.38 $_{- 0.11}^{+ 0.27}$ $^{+0.27}_{-0.11}$	-	> 363	90(f)	30(f)	$36 . 6_{- 11.53}^{+ 28.17}$ $36.6^{+28.17}_{-11.53}$	86.72/53

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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