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

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Table 1.

Map properties of the clean images shown in Figs. 1 and 3, as well as the reanalyzed VLBA images from Mooley et al. (2018).

ν [GHz] ^(a)	Array ^(b)	S_tot [mJy] ^(c)	S_peak [mJy beam⁻¹] ^(d)	σ [mJy beam⁻¹] ^(e)	b_maj [mas] ^(f)	b_min [mas] ^(g)	PA [°] ^(h)
1.5	VLA	35.41	14.7	0.04	1665	1218	−30.5
6.2	VLA	11.48	4.52	0.01	422.4	340.6	−35.4
1.7	EVN	6.8	2.1	0.035	3.4	3.4	0
4.38	VLBA	4.83	2.54	0.049	5.86	2.46	11.2
7.40	VLBA	3.24	1.41	0.036	3.48	1.46	12.1
8.67	VLBA	3.45	1.56	0.06	2.13	0.86	−0.27
15.37	VLBA	1.19	0.85	0.036	1.29	0.48	−3.99

Notes.

^(a)

Observing frequency.

^(b)

Interferometer array performing the observation.

^(c)

Total flux density.

^(d)

Peak brightness.

^(e)

rms noise.

^(f)

Beam major axis.

^(g)

Beam minor axis.

^(h)

Beam position angle.

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