A multiwavelength characterization of the obscuring medium at the center of NGC 6300

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Volume 697 (May 2025)

A&A, 697 (2025) A78

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Table B.1.

X-ray fitting results for NGC 6300

Parameter		`borus02`	`UXCLUMPY`	`XClumpy`
χ²/d.o.f		2470/2571	2470/2571	2462/2562
χ_Red²		0.96	0.96	0.96
Tσ¹		1.43σ	1.43σ	1.43σ

kT₁²		0.78 $_{- 0.08}^{+ 0.08}$ $_{-0.08}^{+0.08}$	0.78 $_{- 0.08}^{+ 0.08}$ $_{-0.08}^{+0.08}$	0.78 $_{- 0.08}^{+ 0.08}$ $_{-0.08}^{+0.08}$
kT₂³		0.11 $_{- 0.00}^{+ 0.00}$ $_{-0.00}^{+0.00}$	0.12 $_{- 0.00}^{+ 0.00}$ $_{-0.00}^{+0.00}$	0.10 $_{- 0.00}^{+ 0.00}$ $_{-0.00}^{+0.00}$

apec norm⁴ ( × 10⁻⁴)		6.97 $_{- 1.13}^{+ 1.33}$ $_{-1.13}^{+1.33}$	6.15 $_{- 1.28}^{+ 1.89}$ $_{-1.28}^{+1.89}$	6.69 $_{- 1.07}^{+ 1.34}$ $_{-1.07}^{+1.34}$
Γ⁵		1.76 $_{- 0.05}^{+ 0.05}$ $_{-0.05}^{+0.05}$	1.82 $_{- 0.06}^{+ 0.03}$ $_{-0.06}^{+0.03}$	1.76 $_{- 0.05}^{+ 0.05}$ $_{-0.05}^{+0.05}$
N_H, av⁶ ×10²⁴ cm⁻²		2.64 $_{- 0.62}^{+ 1.09}$ $_{-0.62}^{+1.09}$	…	…
f_s⁷ ×10⁻²		0.11 $_{- 0.02}^{+ 0.02}$ $_{-0.02}^{+0.02}$	0.44 $_{- 0.14}^{+ 0.48}$ $_{-0.14}^{+0.48}$	0.09 $_{- 0.02}^{+ 0.02}$ $_{-0.02}^{+0.02}$
C_F⁸		0.59 $_{- 0.10}^{+ 0.12}$ $_{-0.10}^{+0.12}$	…	…
cos(θ_i)⁹		0.50 $_{- 0.07}^{+ 0.10}$ $_{-0.07}^{+0.10}$	…	…
θ_i¹⁰		…	0 $_{- }^{+ }$ $_{-}^{+}$	53.77 $_{- 7.55}^{+ 6.08}$ $_{-7.55}^{+6.08}$
CTKcover¹¹		…	0.60 $_{- 0.21}^{+ }$ $_{-0.21}^{+}$	…
TORσ¹²		…	24.14 $_{- 4.96}^{+ 37.33}$ $_{-4.96}^{+37.33}$	…
σ¹³		…	…	28.94 $_{- 5.75}^{+ 9.46}$ $_{-5.75}^{+9.46}$

C_flux¹⁴	`Suzaku`— 17/10/2007	1.09 $_{- 0.04}^{+ 0.05}$ $_{-0.04}^{+0.05}$	1.24 $_{- 0.18}^{+ 0.21}$ $_{-0.18}^{+0.21}$	1.13 $_{- 0.03}^{+ 0.03}$ $_{-0.03}^{+0.03}$
	`Chandra`— 03/06/2009	0.91 $_{- 0.06}^{+ 0.07}$ $_{-0.06}^{+0.07}$	1.03 $_{- 0.16}^{+ 0.19}$ $_{-0.16}^{+0.19}$	0.95 $_{- 0.06}^{+ 0.07}$ $_{-0.06}^{+0.07}$
	`Chandra`— 07/06/2009	1.14 $_{- 0.07}^{+ 0.08}$ $_{-0.07}^{+0.08}$	1.29 $_{- 0.18}^{+ 0.22}$ $_{-0.18}^{+0.22}$	1.19 $_{- 0.06}^{+ 0.07}$ $_{-0.06}^{+0.07}$
	`Chandra`— 09/06/2009	0.96 $_{- 0.07}^{+ 0.07}$ $_{-0.07}^{+0.07}$	1.11 $_{- 0.18}^{+ 0.22}$ $_{-0.18}^{+0.22}$	1.01 $_{- 0.06}^{+ 0.06}$ $_{-0.06}^{+0.06}$
	`Chandra`— 10/06/2009	1.09 $_{- 0.07}^{+ 0.08}$ $_{-0.07}^{+0.08}$	1.23 $_{- 0.17}^{+ 0.21}$ $_{-0.17}^{+0.21}$	1.14 $_{- 0.07}^{+ 0.07}$ $_{-0.07}^{+0.07}$
	`Chandra`— 14/06/2009	1.09 $_{- 0.07}^{+ 0.08}$ $_{-0.07}^{+0.08}$	1.27 $_{- 0.21}^{+ 0.25}$ $_{-0.21}^{+0.25}$	1.15 $_{- 0.07}^{+ 0.05}$ $_{-0.07}^{+0.05}$
	`NuSTAR`— 25/02/2013	1	1	1
	`NuSTAR`— 24/01/2016	0.85 $_{- 0.03}^{+ 0.03}$ $_{-0.03}^{+0.03}$	0.88 $_{- 0.06}^{+ 0.08}$ $_{-0.06}^{+0.08}$	0.83 $_{- 0.04}^{+ 0.03}$ $_{-0.04}^{+0.03}$
	`NuSTAR`— 24/08/2016	0.93 $_{- 0.03}^{+ 0.03}$ $_{-0.03}^{+0.03}$	1.00 $_{- 0.07}^{+ 0.08}$ $_{-0.07}^{+0.08}$	0.95 $_{- 0.02}^{+ 0.02}$ $_{-0.02}^{+0.02}$
	`Chandra`— 26/04/2020	0.41 $_{- 0.05}^{+ 0.05}$ $_{-0.05}^{+0.05}$	0.49 $_{- 0.11}^{+ 0.10}$ $_{-0.11}^{+0.10}$	0.40 $_{- 0.03}^{+ 0.03}$ $_{-0.03}^{+0.03}$

N_H, l.o.s.¹⁵	`Suzaku`— 17/10/2007	20.57 $_{- 0.52}^{+ 0.54}$ $_{-0.52}^{+0.54}$	19.30 $_{- 0.57}^{+ 0.34}$ $_{-0.57}^{+0.34}$	20.57 $_{- 0.65}^{+ 1.46}$ $_{-0.65}^{+1.46}$
	`Chandra`— 03/06/2009	19.60 $_{- 0.97}^{+ 1.03}$ $_{-0.97}^{+1.03}$	18.63 $_{- 1.04}^{+ 0.71}$ $_{-1.04}^{+0.71}$	19.71 $_{- 1.12}^{+ 1.17}$ $_{-1.12}^{+1.17}$
	`Chandra`— 07/06/2009	18.43 $_{- 0.76}^{+ 0.81}$ $_{-0.76}^{+0.81}$	17.84 $_{- 1.15}^{+ 0.74}$ $_{-1.15}^{+0.74}$	18.54 $_{- 0.86}^{+ 0.91}$ $_{-0.86}^{+0.91}$
	`Chandra`— 09/06/2009	20.17 $_{- 0.94}^{+ 1.00}$ $_{-0.94}^{+1.00}$	19.21 $_{- 0.94}^{+ 0.62}$ $_{-0.94}^{+0.62}$	20.32 $_{- 1.06}^{+ 1.11}$ $_{-1.06}^{+1.11}$
	`Chandra`— 10/06/2009	18.84 $_{- 0.85}^{+ 0.90}$ $_{-0.85}^{+0.90}$	18.04 $_{- 1.04}^{+ 0.71}$ $_{-1.04}^{+0.71}$	19.01 $_{- 0.97}^{+ 0.98}$ $_{-0.97}^{+0.98}$
	`Chandra`— 14/06/2009	20.54 $_{- 0.91}^{+ 0.96}$ $_{-0.91}^{+0.96}$	19.44 $_{- 0.83}^{+ 0.56}$ $_{-0.83}^{+0.56}$	20.94 $_{- 0.95}^{+ 1.02}$ $_{-0.95}^{+1.02}$
	`NuSTAR`— 25/02/2013	15.50 $_{- 1.08}^{+ 1.05}$ $_{-1.08}^{+1.05}$	14.33 $_{- 1.03}^{+ 1.21}$ $_{-1.03}^{+1.21}$	15.47 $_{- 1.29}^{+ 1.36}$ $_{-1.29}^{+1.36}$
	`NuSTAR`— 24/01/2016	16.22 $_{- 1.09}^{+ 1.09}$ $_{-1.09}^{+1.09}$	15.26 $_{- 1.49}^{+ 1.17}$ $_{-1.49}^{+1.17}$	15.89 $_{- 1.12}^{+ 1.36}$ $_{-1.12}^{+1.36}$
	`NuSTAR`— 24/08/2016	13.80 $_{- 0.99}^{+ 0.93}$ $_{-0.99}^{+0.93}$	12.57 $_{- 0.82}^{+ 0.75}$ $_{-0.82}^{+0.75}$	13.48 $_{- 0.99}^{+ 1.05}$ $_{-0.99}^{+1.05}$
	`Chandra`— 26/04/2020	21.75 $_{- 1.87}^{+ 2.06}$ $_{-1.87}^{+2.06}$	20.79 $_{- 2.08}^{+ 2.43}$ $_{-2.08}^{+2.43}$	21.96 $_{- 2.32}^{+ 2.31}$ $_{-2.32}^{+2.31}$

log( $f l u x_{2 - 10 keV}$ $flux_{2-10\rm{keV}}$ )¹⁶		-10.38 $_{- 0.06}^{+ 0.06}$ $_{-0.06}^{+0.06}$	-10.34 $_{- 0.07}^{+ 0.07}$ $_{-0.07}^{+0.07}$	-10.41 $_{- 0.04}^{+ 0.05}$ $_{-0.04}^{+0.05}$
log( $f l u x_{10 - 40 keV}$ $flux_{10-40\rm{keV}}$ )¹⁷		-10.29 $_{- 0.06}^{+ 0.06}$ $_{-0.06}^{+0.06}$	-10.29 $_{- 0.08}^{+ 0.07}$ $_{-0.08}^{+0.07}$	-10.29 $_{- 0.04}^{+ 0.04}$ $_{-0.04}^{+0.04}$
log( $l u m_{2 - 10 keV}$ $lum_{2-10\rm{keV}}$ )¹⁸		42.10 $_{- 0.06}^{+ 0.06}$ $_{-0.06}^{+0.06}$	42.14 $_{- 0.07}^{+ 0.07}$ $_{-0.07}^{+0.07}$	42.07 $_{- 0.05}^{+ 0.03}$ $_{-0.05}^{+0.03}$
log( $l u m_{10 - 40 keV}$ $lum_{10-40\rm{keV}}$ )¹⁹		42.19 $_{- 0.06}^{+ 0.06}$ $_{-0.06}^{+0.06}$	42.19 $_{- 0.07}^{+ 0.07}$ $_{-0.07}^{+0.07}$	42.19 $_{- 0.05}^{+ 0.03}$ $_{-0.05}^{+0.03}$

⁽¹⁾

The Tension value for the “true” model.

^(2,3)

Apec model temperature of the two mediums in units of keV.

⁽⁴⁾

Apec normalization.

⁽⁵⁾

Powerlaw photon index.

⁽⁶⁾

Average hydrogen column density of the torus in units of 10²⁴ cm⁻².

⁽⁷⁾

Fraction of primary emission getting scattered instead of being absorbed, by the obscuring material.

⁽⁸⁾

Covering factor of the torus, from borus02.

⁽⁹⁾

Cosine of the inclination angle, from borus02.

⁽¹⁰⁾

Inclination angle in degree, from UXCLUMPY and XClumpy.

⁽¹¹⁾

Covering factor of inner thick ring of clouds, from UXCLUMPY.

⁽¹²⁾

Cloud dispersion in degrees, from UXCLUMPY.

⁽¹³⁾

Dispersion of torus clouds, from XClumpy.

⁽¹⁴⁾

Cross normalization constant between the observations. C_flux is fixed to 1 for NuSTAR observation of 2013.

⁽¹⁵⁾

LOS hydrogen column density in units of 10²² cm⁻².

^(16,17)

Average intrinsic flux within the given energy range.

^(18,19)

Average intrinsic luminosity within the given energy range.

^(*)

The upper and/or lower limits of uncertainty have reached the parameter boundary.

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