Parsec-scale HI outflows in powerful radio galaxies

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Table 2.

Properties of images.

Source	Data	σ_noise^(a)	Beam ^(b)	Δ_v^(c)	N_ch^(d)	S_peak^(e)	S_tot^(f)
		[mJy beam⁻¹ ch⁻¹]	[mas × mas]	[km s⁻¹]		[Jy beam⁻¹]	[Jy]
3C 293	Continuum	0.19	25 × 25			0.066	0.539
	Cube	0.31	25 × 25	20.7 (41.4)	143
4C 52.37	Continuum	0.19	6 × 6			0.025	0.429
	Continuum	0.15	20 × 20			0.051	0.429
	Cube	0.58	20 × 20	21.9 (43.8)	143

Notes.

^(a)

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

^(b)

Synthesized beam as major axis and minor axis.

^(c)

Channel width in velocity of the cubes. The values in brackets represent the effective resolution because of Hanning smoothing.

^(d)

Number of channels of the cubes.

^(e)

Peak brightness of the continuum image.

^(f)

Total flux density of the continuum image.

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