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Table B.1.

Scale heights and amplitudes of thin and thick radio discs; effective radii in the radio continuum.

Galaxy w1 w2 h1 h2 re h1 h2
(mJy beam−1) (arcsec) (arcsec) (arcsec) (kpc) (kpc)
N0891 2.81±0.94 0.88±0.22 2.86±0.26 22.77±2.05 132.40±4.33 0.13±0.01 1.00±0.09
N2683 0.26±0.04 0.17±0.05 8.86±4.76 21.64±2.52 86.41±1.88 0.27±0.14 0.66±0.08
N2820a 1.53±0.43 0.60±0.22 2.86±0.66 10.29±0.85 30.31±1.13 0.37±0.08 1.32±0.11
N3003 0.85±0.05 0.27±0.06 2.54±0.50 12.20±1.52 56.35±3.89 0.31±0.06 1.50±0.19
N3044a 3.19±1.34 0.65±0.42 3.69±0.95 10.77±2.05 24.24±1.05 0.36±0.09 1.06±0.20
N3079c 4.86±0.20 0.28±0.22 5.41±0.86 13.57±4.03 49.58±1.87 0.54±0.09 1.36±0.40
N3432 0.49±0.14 0.18±0.10 5.83±1.88 20.36±1.58 76.38±3.40 0.27±0.09 0.93±0.07
N3448 0.88±0.18 0.73±0.33 3.41±1.40 7.96±0.84 32.07±1.60 0.41±0.17 0.95±0.10
N3556a 0.48±0.05 0.15±0.14 13.05±5.19 31.57±6.86 125.70±11.70 0.89±0.35 2.16±0.47
N3628b 2.12±0.12 0.24±0.14 6.53±1.82 23.10±5.77 54.55±1.79 0.27±0.08 0.95±0.24
N3735c 2.37±0.88 0.02±0.03 5.13±0.72 23.62±3.54 29.36±0.86 1.04±0.15 4.81±0.72
N4013 0.80±0.60 0.13±0.02 1.11±0.19 10.67±0.32 85.87±4.46 0.09±0.01 0.83±0.02
N4096b 0.57±0.09 0.16±0.01 2.53±0.64 22.24±1.53 64.47±2.92 0.13±0.03 1.11±0.08
N4157 0.98±0.09 0.10±0.10 8.90±1.58 17.25±4.28 75.38±2.54 0.67±0.12 1.30±0.32
N4217a 1.18±0.17 0.48±0.20 2.95±0.97 11.29±1.95 59.57±1.90 0.29±0.10 1.13±0.19
N4302 0.44±0.15 0.17±0.04 1.59±0.30 9.90±0.89 73.22±1.81 0.15±0.03 0.93±0.08
N4388 2.71±0.22 0.09±0.18 5.07±1.17 10.25±1.56 42.53±2.00 0.41±0.09 0.82±0.13
N4565 0.22±0.01 0.08±0.09 10.48±3.43 14.38±1.02 213.30±4.36 0.60±0.20 0.83±0.06
N4631a 4.52±0.10 1.17±0.11 4.90±0.56 28.58±0.99 100.00±10.00 0.18±0.02 1.03±0.04
N4666 3.62±0.28 0.88±0.36 6.88±1.34 19.14±2.61 43.33±1.37 0.92±0.18 2.55±0.35
N5775 1.76±0.56 0.29±0.06 5.65±0.29 22.59±4.27 80.08±5.18 0.79±0.04 3.17±0.60
N5907a 0.41±0.08 0.01±0.02 10.29±1.62 24.78±3.62 140.40±4.43 0.84±0.13 2.02±0.29

Notes. Results refer to 3 GHz radio continuum emission at 7 arcsec FWHM angular resolution. For NGC 4631, the effective radius was estimated without fit.

(a)

Both haloes individually fitted;

(b)

only northern halo (z>0);

(c)

only southern halo (z<0).

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