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.9.

Useful outputs from the broadband SED fitting.

BAT ID	Swift ID	L_2500 Å	L_2 keV	L_bol	M_BH	α_ox	κ_4400 Å	κ_2 − 10	λ_Edd
3	SWIFTJ0002.5+0323	43.07	42.35	43.68	6.70	$- 1 . 27_{- 0.14}^{+ 0.10}$ $-1.27^{+0.10}_{-0.14}$	$5 . 59_{- 3.35}^{+ 4.92}$ $5.59^{+4.92}_{-3.35}$	$10 . 09_{- 3.60}^{+ 4.73}$ $10.09^{+4.73}_{-3.60}$	−1.20
6	SWIFTJ0006.2+2012	43.99	43.11	44.57	7.23	$- 1 . 34_{- 0.07}^{+ 0.14}$ $-1.34^{+0.14}_{-0.07}$	$5 . 86_{- 4.10}^{+ 2.94}$ $5.86^{+2.94}_{-4.10}$	$22 . 26_{- 5.22}^{+ 10.38}$ $22.26^{+10.38}_{-5.22}$	−0.84
16	SWIFTJ0029.2+1319	45.49	44.32	46.16	8.49	$- 1 . 45_{- 0.06}^{+ 0.04}$ $-1.45^{+0.04}_{-0.06}$	$8 . 12_{- 2.19}^{+ 3.38}$ $8.12^{+3.38}_{-2.19}$	$49 . 53_{- 11.80}^{+ 8.32}$ $49.53^{+8.32}_{-11.80}$	−0.50
19	SWIFTJ0034.5-7904	44.26	43.78	44.95	8.02	$- 1 . 19_{- 0.02}^{+ 0.02}$ $-1.19^{+0.02}_{-0.02}$	$6 . 56_{- 0.59}^{+ 0.54}$ $6.56^{+0.54}_{-0.59}$	$10 . 70_{- 0.80}^{+ 0.81}$ $10.70^{+0.81}_{-0.80}$	−1.25
34	SWIFTJ0051.6+2928	43.96	42.49	44.44	7.62	$- 1 . 56_{- 0.09}^{+ 0.07}$ $-1.56^{+0.07}_{-0.09}$	$4 . 63_{- 1.68}^{+ 2.22}$ $4.63^{+2.22}_{-1.68}$	$53 . 75_{- 16.65}^{+ 13.46}$ $53.75^{+13.46}_{-16.65}$	−1.36
36	SWIFTJ0051.9+1724	44.43	43.91	45.15	7.75	$- 1 . 20_{- 0.01}^{+ 0.02}$ $-1.20^{+0.02}_{-0.01}$	$7 . 38_{- 0.91}^{+ 0.59}$ $7.38^{+0.59}_{-0.91}$	$8 . 66_{- 0.50}^{+ 0.61}$ $8.66^{+0.61}_{-0.50}$	−0.77
39	SWIFTJ0054.9+2524	45.36	44.28	46.08	8.46	$- 1 . 41_{- 0.07}^{+ 0.04}$ $-1.41^{+0.04}_{-0.07}$	$9 . 13_{- 1.86}^{+ 4.19}$ $9.13^{+4.19}_{-1.86}$	$32 . 70_{- 8.44}^{+ 4.55}$ $32.70^{+4.55}_{-8.44}$	−0.56
43	SWIFTJ0059.4+3150	42.69	41.96	43.42	7.56	$- 1 . 28_{- 0.30}^{+ 0.06}$ $-1.28^{+0.06}_{-0.30}$	$8 . 96_{- 3.69}^{+ 18.44}$ $8.96^{+18.44}_{-3.69}$	$14 . 26_{- 12.71}^{+ 2.90}$ $14.26^{+2.90}_{-12.71}$	−2.32
45	SWIFTJ0101.5-0308	43.90	42.75	44.38	8.13	$- 1 . 44_{- 0.39}^{+ 0.19}$ $-1.44^{+0.19}_{-0.39}$	$4 . 19_{- 3.79}^{+ 9.42}$ $4.19^{+9.42}_{-3.79}$	$23 . 78_{- 32.21}^{+ 17.03}$ $23.78^{+17.03}_{-32.21}$	−1.93
51	SWIFTJ0105.7-1414	44.30	43.48	45.03	7.88	$- 1 . 32_{- 0.01}^{+ 0.01}$ $-1.32^{+0.01}_{-0.01}$	$8 . 37_{- 0.47}^{+ 0.48}$ $8.37^{+0.48}_{-0.47}$	$16 . 79_{- 1.29}^{+ 1.26}$ $16.79^{+1.26}_{-1.29}$	−1.03

Notes. We have reported the 2500 Å, 2 keV, and the bolometric luminosities with their errors. We also present the black hole masses (M_BH) of our sources as estimated by Mejía-Restrepo et al. (2022) in units of log (M_BH/M_⊙). Finally, we list the estimated value of the optical-to-X-ray spectral indices (α_ox; Sect. 7.3), the 2–10 keV X-ray bolometric corrections (κ_2 − 10; Sect. 7.4.1), the 4400 Å optical bolometric corrections (κ_4400 Å; Sect. 7.4.2), and the Eddington ratios (λ_Edd in log). Luminosity units: 10⁻⁴² erg s⁻¹. The table in its entirety is available at the CDS.

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