Mapping the neutral atomic hydrogen gas outflow in the restarted radio galaxy 3C 236

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Table 2.

Image properties.

Data	σ^a_noise (mJy beam⁻¹ ch⁻¹)	Beam^b	Δυ^c (km s⁻¹)	N^d_ch	S^e_peak (Jy beam⁻¹)	S^f_tot (Jy)
VLBI

Continuum	0.23	20 mas × 20 mas	–	1	0.145 ± 0.020	1.35 ± 0.20
Cube	0.37	20 mas × 20 mas	21.7 (43.4)	143	–	–

VLA

Continuum	2.1	1″.7 × 1″.2, −67°	–	1	2.883 ± 0.086	3.37 ± 0.10
Cube (VLBI)	1.1	2″.0 × 1″.5, −81°	21.7 (43.4)	157	–	–
Cube (WSRT)	1.1	2″.0 × 1″.5, −81°	20.0 (40.0)	186	–	–

Notes.

^(a)

Noise level. For the cubes, this value represents the average value over all channels.

^(b)

Synthesized beam as major axis, minor axis, and the position angle.

^(c)

Channel width in velocity of the cubes after re-sampling. The value in brackets corresponds to the effective resolution after Hanning-smoothing.

^(d)

Number of channels of the cubes.

^(e)

Total flux density of the continuum image.

^(f)

Peak flux density of the continuum image.

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