Supermassive Black Hole Winds in X-rays: SUBWAYS - IV. Tracing radio emission and unveiling the role of winds

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Volume 710 (June 2026)

A&A, 710 (2026) A295

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Table 1.

General parameters of the sources in the SUBWAYS sample.

ID	Target Name	R.A.	Dec.	z	D_L	log L_bol	log L_{2 − 10 keV}	log M_BH	log λ_Edd	v_out
		J2000	J2000		(Gpc)	(erg/s)	(erg/s)	(M_⊙)		(c)
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)	(10)	(11)
5	PG0804+761	08:10:58.60	+76:02:43.00	0.100	0.46	45.27	44.46±0.01	$8 . 31_{- 0.04}^{+ 0.04}$ $Mathematical equation: $ 8.31^{+0.04}_{-0.04} $$	–1.07	0.13 ± 0.01
6	PG0947+396	09:50:48.42	+39:26:50.64	0.205	1.01	45.89	44.37±0.01	$8 . 68_{- 0.10}^{+ 0.08}$ $Mathematical equation: $ 8.68^{+0.08}_{-0.10} $$	–1.24	$0 . 31_{- 0.04}^{+ 0.02}$ $Mathematical equation: $ 0.31^{+0.02}_{-0.04} $$
11	2MASXJ1051+35	10:51:44.24	+35:39:30.76	0.159	0.76	44.88	43.70±0.01	$8 . 40_{- 0.30}^{+ 0.30}$ $Mathematical equation: $ 8.40^{+0.30}_{-0.30} $$	–1.92	0.24 ± 0.01
10	PG1114+445	11:17:06.40	+44:13:33.31	0.144	0.68	45.87	44.09±0.01	$8 . 59_{- 0.09}^{+ 0.09}$ $Mathematical equation: $ 8.59^{+0.09}_{-0.09} $$	–1.26	0.07 ± 0.02
22	PG1202+281	12:04:42.12	+27:54:12.11	0.165	0.79	46.30	44.40±0.01	$8 . 61_{- 0.10}^{+ 0.08}$ $Mathematical equation: $ 8.61^{+0.08}_{-0.10} $$	–0.45	0.11±0.01
18	LBQS1338−0038	13:41:13.94	−00:53:14.97	0.237	1.19	45.27	44.52±0.01	$7 . 74_{- 0.03}^{+ 0.03}$ $Mathematical equation: $ 7.74^{+0.03}_{-0.03} $$	–0.52	0.15 ± 0.02
2	MASXJ1653+23	16:53:15.06	+23:49:42.96	0.103	0.48	45.37	43.80±0.01	$6 . 98_{- 0.30}^{+ 0.30}$ $Mathematical equation: $ 6.98^{+0.30}_{-0.30} $$	0.35	$0 . 11_{- 0.01}^{+ 0.02}$ $Mathematical equation: $ 0.11^{+0.02}_{-0.01} $$

9	PG0052+251	00:54:52.10	+25:25:37.99	0.154	0.74	45.72	44.61±0.01	$8 . 41_{- 0.09}^{+ 0.09}$ $Mathematical equation: $ 8.41^{+0.09}_{-0.09} $$	–0.83
7	2MASXJ0220–07	02:20:14.58	−07:28:59.23	0.213	1.06	46.33	44.21±0.01	$8 . 87_{- 0.30}^{+ 0.30}$ $Mathematical equation: $ 8.87^{+0.30}_{-0.30} $$	–1.89
8	WISEJ0537–02	05:37:56.30	−02:45:13.27	0.110	0.51	44.86	43.69±0.01	$7 . 73_{- 0.30}^{+ 0.30}$ $Mathematical equation: $ 7.73^{+0.30}_{-0.30} $$	–0.60
12	PG0953+414	09:56:52.40	+41:15:22.00	0.234	1.17	46.33	44.60±0.01	$8 . 24_{- 0.09}^{+ 0.06}$ $Mathematical equation: $ 8.24^{+0.06}_{-0.09} $$	–0.05
3	PG1307+085	13:09:47.00	+08:19:48.22	0.154	0.74	44.86	44.31±0.01	$7 . 90_{- 0.12}^{+ 0.12}$ $Mathematical equation: $ 7.90^{+0.12}_{-0.12} $$	–1.18
4	PG1352+183	13:54:35.72	+18:05:18.05	0.151	0.72	46.26	43.89±0.01	$8 . 42_{- 0.10}^{+ 0.08}$ $Mathematical equation: $ 8.42^{+0.08}_{-0.10} $$	–0.30
13	2MASXJ1402+26	14:02:51.19	+26:31:17.63	0.188	0.92	45.44	< 44.23	< 8.55	–1.21
15	PG1402+261	14:05:16.21	+25:55:34.13	0.164	0.79	46.34	44.03±0.01	$7 . 94_{- 0.10}^{+ 0.08}$ $Mathematical equation: $ 7.94^{+0.08}_{-0.10} $$	–0.99
17	PG1416−129	14:19:03.82	−13:10:44.78	0.129	0.59	45.74	44.17±0.01	$8 . 12_{- 0.10}^{+ 0.08}$ $Mathematical equation: $ 8.12^{+0.08}_{-0.10} $$	0.00
14	PG1425+267	14:27:35.61	+26:32:14.63	0.364	1.95	46.06	44.82±0.01	$9 . 22_{- 0.30}^{+ 0.30}$ $Mathematical equation: $ 9.22^{+0.30}_{-0.30} $$	–1.30
19	PG1427+480	14:29:43.10	+47:47:26.02	0.221	1.10	45.82	< 44.20	< 8.09	–0.41
16	PG1435−067	14:38:16.10	−06:58:21.00	0.129	0.59	45.51	43.68±0.01	$7 . 77_{- 0.10}^{+ 0.08}$ $Mathematical equation: $ 7.77^{+0.08}_{-0.10} $$	–0.40
20	SDSSJ1444+06	14:44:14.67	+06:33:06.77	0.208	1.02	45.34	44.47±0.01	$8 . 33_{- 0.30}^{+ 0.30}$ $Mathematical equation: $ 8.33^{+0.30}_{-0.30} $$	–0.94
21	HB891529+050	15:32:28.79	+04:53:58.46	0.218	1.08	45.17	44.22±0.01	$7 . 46_{- 0.30}^{+ 0.30}$ $Mathematical equation: $ 7.46^{+0.30}_{-0.30} $$	–1.47
1	PG1626+554	16:27:56.10	+55:22:32.02	0.133	0.63	46.02	44.08±0.01	$8 . 54_{- 0.10}^{+ 0.08}$ $Mathematical equation: $ 8.54^{+0.08}_{-0.10} $$	–0.66

Notes. Column 1: Reference label. Column 2: Target name. Column 3 and 4: Coordinates. Column 5: Redshift. Column 6: Luminosity distance. Column 7: Bolometric luminosity. Column 8: X-ray luminosity (derived from XMM-Newton analysis, Paper I). Column 9: SMBH mass in units of solar masses. Column 10: Eddington ratio (Paper I). Column 11: Outflow velocity in units of c (Paper III) for the UFO detected with confidence interval ≥99% (Paper I). The UFO subsample is shown before the horizontal line.

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