From binary to singular: The AGN PSO J334.2028+1.4075 under the high-resolution scope

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Table 2.

Characteristics of modelfit components.

ν [GHz] ^(a)	Array	Component	S_comp [mJy] ^(b)	b_comp [mas] ^(c)	T_b [10⁸ K] ^(d)
1.7	EVN		7.15 ± 0.72	6.58 ± 0.68	2.2 ± 0.5
4.38	VLBA	SE	2.43 ± 0.24	1.53 ± 0.49	2.0 ± 1.3
		NW	2.64 ± 0.26	1.23 ± 0.49	3.4 ± 2.7
7.40	VLBA	SE	1.71 ± 0.17	0.8 ± 0.29	1.8 ± 1.4
		NW	1.75 ± 0.18	0.9 ± 0.29	1.5 ± 1.0
8.67	VLBA	SE	1.97 ± 0.2	0.59 ± 0.17	2.8 ± 1.6
		NW	2.03 ± 0.2	0.83 ± 0.17	1.5 ± 0.6
15.37	VLBA	SE	0.95 ± 0.1	0.16 ^(*)	> 6.0 ^(*)
		NW	0.8 ± 0.08	0.38 ± 0.1	0.9 ± 0.4

Notes.

^(a)

Frequency of the observation.

^(b)

Flux density of the component.

^(c)

Size of the component (FWHM).

^(d)

Brightness temperature.

^(*)

Component is unresolved based on Eq. (2) from Kovalev et al. (2005).

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