The ATESP 5 GHz radio survey - IV. 19, 38, and 94 GHz observations and radio spectral energy distributions

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Volume 621 (January 2019)

A&A, 621 (2019) A19

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Table 5.

Intrinsic luminosity and linear size.

Name	z	P_5 GHz	P_1.4 GHz		LS
		W Hz⁻¹	W Hz⁻¹		kpc
src01	0.54	24.71	25.10	−0.71	120.0
src06	0.44	24.68	25.02	−0.62	320.2
src07	0.61	24.17	24.66	−0.89	39.9
src15	1.17	26.55	27.02	−0.86	110.5
src18	0.03	21.46	21.74	−0.51	10.1
src23	0.43	24.48	24.92	−0.79	19.6
src25	1.64	26.40	26.83	−0.78	196.4
src02	0.19	24.41	24.48	−0.12	12.7
src04	0.40	24.22	24.47	−0.45	196.3
src08	0.37	24.67	24.93	−0.48	18.7
src10	0.35	23.36	23.51	−0.28	< 9.9^b
src13	0.61	24.42	24.67	−0.45	8.6
src14	0.13	22.83	23.06	−0.41	10.9
src17	0.03	21.31	21.37	−0.11	9.6
src19	0.59	24.09	24.24	−0.26	12.1
src20	0.30	23.44	23.70	−0.48	< 8.9^c
src27	1.58	24.99	25.15	−0.29	< 33.9
src28	0.73	23.32	23.45	−0.24	< 14.1^a
src09	1.25	24.35	24.21	0.25	< 17.1^b
src11	0.15	22.63	22.56	0.12	19.9
src12	0.25	23.38	23.34	0.06	4.0
src16	0.03	21.84	21.67	0.31	3.6
src21	0.36	23.33	23.11	0.40	32.7
src22	1.40	24.21	23.44	1.39	5.1
src24	0.56	23.43	23.31	0.70	< 12.9^b
src26	0.44	23.41	23.30	0.19	< 11.4^b

Notes.

Columns 1–6: source name; redshift; rest-frame luminosity at 5 and 1.4 GHz; spectral index used to compute rest-frame luminosity; linear size in kpc. Sources are divided into three groups based on the spectral index: (from top to bottom) steep-, flat-, and inverted-spectrum sources.

^(a)

These sources appear as resolved at 0.6 arcsec resolution. For these sources we can infer a lower limit in size equal to one third of the quoted values (see Sect. 3 for more details).

^(b)

These sources appear as resolved at 0.15 arcsec resolution. For these sources we can infer a lower limit in size equal to one tenth of the quoted values (see Sect. 3 for more details).

^(c)

This source appears as unresolved down to 0.15 arcsec. This gives a more stringent size upper limit of < 1 kpc (see Sect. 3 for more details).

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