Deciphering the imprint of active galactic nucleus feedback in Seyfert galaxies - Nuclear-scale molecular gas deficits

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Table B.1.

L_X values obtained from X-ray spectral fitting.

Source	OBSID	Exptime	Model	log₁₀(L_X)	kT(keV)	Γ	N_H	f_cov	χ/dof
NGC2782	3014	29.58	M3	$39 . 5_{0.5}^{0.3}$ ${39.5_{0.5}^{0.3}}$	1.020.05	1.8^*	$3 . 6_{- 3.5}^{+ 6.6}$ $\rm{3.6_{-3.5}^{+6.6}}$	0.8 ± 0.2	13.6/19
NGC3718	0795730101/3993	16.14/0.5	M1	40.64 ± 0.01/40.84 ± 0.01		1.7 ± 0.1	0.90 ± 0.05	0.98 ± 0.01	182.0/200
NGC4321	0106860201/14230	1.0/78.8	M2	40.4 ± 0.2/ $39 . 2_{- 0.2}^{+ 0.7}$ ${39.2_{-0.2}^{+0.7}}$	$0 . 65_{- 0.03}^{+ 0.09}$ ${0.65_{-0.03}^{+0.09}}$	1.8^*	$76_{- 38}^{+ 113}$ $\rm{76_{-38}^{+113}}$	0.6 ± 0.2	107.1/86
NGC4569	0200650101/5911	40.0/29.9	M2	39.64 ± 0.06/39.22 ± 0.07	0.760.01	1.8^*	16.8 ± 0.5	0.4 ± 0.1	221.3/152
NGC4579	0790840201/807	17.1/31.4	M3	41.42 ± 0.01/41.29 ± 0.01	0.840.06	1.76 ± 0.01	1.20 ± 0.05	0.68 ± 0.01	1081.0/994

Notes. Table of the results for the X-ray spectral fitting. N_H are in units of 10²² cm⁻². M1: pcfabs × powerlaw, M2: apec + pcfabs × powerlaw, M3: apec + pexmon + pcfabs× powerlaw.

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