BASS - XLIII. Optical, UV, and X-ray emission properties of unobscured Swift/BAT active galactic nuclei

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Volume 691 (November 2024)

A&A, 691 (2024) A203

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Table A.5.

Results of the X-ray spectral fitting (Sect. 4).

BAT ID	Swift ID	Γ	F_2 − 10	Model	Statistic/dof
2	SWIFTJ0001.6-7701	$1 . 55_{- 0.64}^{+ 1.01}$ $1.55_{-0.64}^{+1.01}$	$2 . 90_{- 0.44}^{+ 0.48}$ $2.90_{-0.44}^{+0.48}$	A1 + `ZXIPCF`	86.84/113
3	SWIFTJ0002.5+0323	$1 . 97_{- 0.16}^{+ 0.24}$ $1.97_{-0.16}^{+0.24}$	$3 . 19_{- 0.34}^{+ 0.37}$ $3.19_{-0.34}^{+0.37}$	A2	134.4/148
6	SWIFTJ0006.2+2012	$2 . 34_{- 0.04}^{+ 0.03}$ $2.34_{-0.04}^{+0.03}$	$10 . 8_{- 0.21}^{+ 0.21}$ $10.8_{-0.21}^{+0.21}$	A1	796.5/597
10	SWIFTJ0021.2-1909	$1 . 60_{- 0.18}^{+ 0.18}$ $1.60_{-0.18}^{+0.18}$	$9 . 03_{- 0.48}^{+ 0.50}$ $9.03_{-0.48}^{+0.50}$	B1	360.5/445
14	SWIFTJ0026.5-5308	$1 . 70_{- 0.23}^{+ 0.35}$ $1.70_{-0.23}^{+0.35}$	$1 . 97_{- 0.23}^{+ 0.25}$ $1.97_{-0.23}^{+0.25}$	A1	130.7/139
16	SWIFTJ0029.2+1319	$2 . 20_{- 0.17}^{+ 0.17}$ $2.20_{-0.17}^{+0.17}$	${5.44}_{- 0.21}^{+ 0.22}$ ${5.44}_{-0.21}^{+0.22}$	A2	335.2/397
19	SWIFTJ0034.5-7904	$2 . 36_{- 0.07}^{+ 0.11}$ $2.36_{-0.07}^{+0.11}$	${6.14}_{- 0.21}^{+ 0.22}$ ${6.14}_{-0.21}^{+0.22}$	A2	390.3/390
34	SWIFTJ0051.6+2928	$1 . 99_{- 0.23}^{+ 0.25}$ $1.99_{-0.23}^{+0.25}$	${1.71}_{- 0.13}^{+ 0.13}$ ${1.71}_{-0.13}^{+0.13}$	A2	197.3/253
36	SWIFTJ0051.9+1724	$1 . 91_{- 0.03}^{+ 0.10}$ $1.91_{-0.03}^{+0.10}$	${16.6}_{- 0.40}^{+ 0.40}$ ${16.6}_{-0.40}^{+0.40}$	A2	564.5/578
39	SWIFTJ0054.9+2524	$1 . 97_{- 0.15}^{+ 0.18}$ $1.97_{-0.15}^{+0.18}$	${5.58}_{- 0.23}^{+ 0.24}$ ${5.58}_{-0.23}^{+0.24}$	A2	328.9/403

Notes. We have reported the main outputs of the fitting here, including the best-fit values of the photon index, the 2–10 keV intrinsic fluxes with errors, the model used to get the best fit, and the value of the statistic and the degrees of freedom of the fit. Flux units: 10⁻¹² erg cm⁻² s⁻¹. The table in its entirety is available at the CDS.

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