The radio-loud AGN population at z ≳ 1 in the COSMOS field - I. selection and spectral energy distributions

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Table 5

The radio-loud AGN population in the COSMOS field at z ≳ 1.


ID	Redshift	Radio				log M_∗	Dust		UV


	z _phot	L _FIRST	L _NVSS	radio class	radio morph	M _⊙	L _{IR exc.}	α _{8 − 24}	L _UV


1	1.1577^s	32.07	32.23	LP	compact	11.31	45.74	−0.87	43.51
2	1.767	32.76	32.82	HP	FR II	10.67	<43.96		<42.00
3	1.983	32.59	<32.77	HP	compact	10.79	44.15	>−0.42	42.98
4	1.104	32.48	32.47	LP	compact	10.32	44.41	0.62	<41.43
5	0.9707^s	32.13	32.24	LP	FR II	11.17	44.22	−0.53	43.80
6	1.963	32.75	32.84	HP	FR II	10.85	43.79	>−0.38	43.47
7	1.384	32.76	32.85	HP	FR II	10.89	<43.49		42.19
8	0.8357^s	32.50	32.61	HP	FR II	11.59	<44.10		<42.20
9	2.152	33.34	33.37	HP	FR II	10.60	<44.15		42.83
11	1.018	32.58	32.73	HP	FR II	10.69	<43.44		42.23^m
12	1.860	32.84		HP	compact	10.49	<43.66		42.38
13	1.018	32.22		LP	FR II	10.16	<43.16		41.88^m
14	1.377	33.06	33.11	HP	compact	10.92	43.87	>−0.12	42.34
15	1.015	31.97	32.45	LP	FR II	10.76	<43.15		<42.06
16	0.8442^s	31.90	<31.88	LP	compact	10.78	43.26	>−0.59	<42.22
17	1.391	32.81	32.80	HP	FR II	10.89	<43.83		42.87
18	1.193	32.84	32.92	HP	FR II	10.94	44.71	0.43	43.30
19	0.932	31.61	<31.99	LP	compact	11.26	43.66	>0.91	<42.20
20	1.016	32.89	32.92	HP	FR II	10.33	<43.52		42.33^m
21	0.894	31.97	32.18	LP	compact	10.71	<43.42		42.20^m
23	0.8393^s	32.64	32.90	HP	FR II	10.50	<43.30		42.25^m
24	2.006	32.73	32.86	HP	compact	11.08	44.69	>0.66	42.91
25	0.825	31.99	32.05	LP	FR I/FR II	11.17	43.27	>2.50	<41.98
26	0.830	31.88	31.83	LP	compact	11.04	<43.32		<42.07
27	2.523	33.35	33.42	HP	compact	10.68	<44.17		43.22
28	1.788	32.67	32.95	HP	FR II	10.51	44.12	−0.23	43.30
29	1.4050^s	32.68	33.03	HP	compact	QSO	45.27	−0.92	45.69
30	2.268	33.13	33.14	HP	extended	10.74	<44.16		42.53^m
31	1.698	32.77	32.75	HP	extended	10.65	<44.06		42.57
32	1.067	32.17	32.23	LP	extended	10.08	<43.59		42.05^m
34	1.402	32.95	32.86	HP	extended	10.65	44.61	−1.08	<42.63
35	1.80	33.70	33.69	HP	compact	QSO	44.89	−0.78	44.66
36	2.255	33.89	33.90	HP	compact	10.91	<44.09		43.37
37	1.3176^s	33.70	33.72	HP	FR II	QSO	45.47	−0.95	45.55
38	2.355	34.17	34.24	HP	FR II	11.09	44.42	>0.58	43.70
39	1.851	33.52	33.52	HP	compact	10.94	<43.94		42.34^m
40	1.110	33.08	33.23	HP	FR II	10.70	<43.51		<42.24
41	1.028	32.96	32.96	HP	extended	10.22	44.69	0.15	43.27
42	1.137	33.02	33.00	HP	compact	10.75	<43.66		42.58^m
43	1.247	33.27	33.40	HP	FR II	11.03	<43.63		42.68^m
44	1.062	33.97	33.96	HP	FR II	10.61	44.37	0.53	43.12
45	0.918	33.07	33.21	HP	FR II	10.74	<43.35		42.28^m
46	0.8784^s	32.77	32.88	HP	FR II	10.47	<43.29		42.27^m


COSMOS-FR I 1	0.8827^s	31.78	<31.93	LP	compact	10.08	<43.31		<41.92
COSMOS-FR I 2	1.33	32.02	32.40	LP	extended	11.00	<43.65		42.53
COSMOS-FR I 3	2.20	33.10	33.19	HP	compact	10.59	45.27	−0.01	43.21
COSMOS-FR I 4	1.37	32.77	32.86	HP	FR I	11.16	<43.55		42.71
COSMOS-FR I 5	2.01	32.47	32.89	HP	compact	11.49	44.76	>0.49	<43.00
COSMOS-FR I 11	1.57	32.18	<32.52	LP	compact	10.98	<43.80		<42.11
COSMOS-FR I 13	1.19	32.02	32.22	LP	compact	10.72	44.23	−0.41	42.65^m
COSMOS-FR I 16	0.9687^s	32.38	32.27	LP	compact	10.74	43.60	>−0.12	42.42^m
COSMOS-FR I 18	0.92	32.22	32.28	LP	extended	10.02	<43.96		<42.23
COSMOS-FR I 20	0.88	31.66	<31.93	LP	extended	11.03	<43.02		42.25^m
COSMOS-FR I 22	1.30	32.38	<32.34	LP	compact	11.16	43.87	>0.66	<41.79
COSMOS-FR I 25	1.33	32.29	32.39	LP	compact	10.75	43.75	>0.26	42.87^m
COSMOS-FR I 26	1.09	32.02	32.25	LP	extended	11.12	<43.45		42.50^m
COSMOS-FR I 28	2.90	32.99	33.13	HP	compact	11.38	44.28	>0.22	<43.35
COSMOS-FR I 29	1.32	32.28	32.31	LP	compact	10.03	<43.68		42.83
COSMOS-FR I 30	1.06	31.83	32.11	LP	compact	11.03	<43.47		<41.81
COSMOS-FR I 31	0.9132^s	32.14	32.18	LP	compact	10.75	<43.35		42.86
COSMOS-FR I 34	1.55	32.84	32.77	HP	compact	10.99	<44.04		42.82
COSMOS-FR I 36	1.07	32.23	32.25	LP	compact	10.83	43.46	>0.20	<41.91
COSMOS-FR I 38	1.30	32.94	33.00	HP	compact	10.65	43.77	0.45	43.03
COSMOS-FR I 39	1.10	31.90	<32.16	LP	compact	10.88	<43.20		<42.23
COSMOS-FR I 52	0.7417^s	31.54	<31.73	LP	compact	10.78	43.33	0.61	42.96
COSMOS-FR I 70	2.32	33.12	33.18	HP	compact	10.65	44.07	>-0.50	43.54
COSMOS-FR I 202	1.31	31.98	32.46	LP	extended	10.86	<43.66		42.21
COSMOS-FR I 219	1.03	31.96	<32.09	LP	compact	10.67	<43.32		42.69^m
COSMOS-FR I 224	1.10	32.28	32.27	LP	extended	10.71	<43.53		42.53^m
COSMOS-FR I 228	1.31	32.25	32.51	LP	compact	11.06	<43.64		<41.91
COSMOS-FR I 234	1.10	32.41	32.48	LP	FR I	10.83	<43.52		<42.02
COSMOS-FR I 236	2.1318^s	33.29	33.29	HP	compact	QSO	45.45	−1.01	45.60
COSMOS-FR I 258	0.9009^s	31.90	32.12	LP	compact	10.64	<43.41		43.27
COSMOS-FR I 285	1.10	32.23	32.31	LP	extended	10.43	43.73	−0.22	43.08

Notes. Column description: (1) ID number of the object; (2) photometric or spectroscopic (if available) redshift; (3), (4) FIRST and NVSS radio luminosities; (5) classification based on the radio power: low or high power (LP or HP) radio sources; (6) radio morphology based on the VLA-COSMSO images; (7) the total stellar mass of the galaxy in M_⊙; (8), (9) the infrared excess luminosity (in erg s^-1) and the spectral index measured on the infrared excess at 8 and 24 μm; (10) UV luminosity at 2000 Å in the rest frame in erg s^-1. The marginal UV excesses are marked with a ^m. The QSO are the spectroscopically-confirmed and photometrically-defined quasars.

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