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Table B.1.

3DB input parameters and characteristics of data cubes.

Galaxy Beam Δv σch σtot Rmax ΔR centre RA centre DEC Vsys norm
(″) ( km s−1) (mJy beam−1) (kpc) (pc) (hh mm ss.s) (dd mm ss) ( km s−1)
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10)
DDO 154 21 × 21 2.6 1.366 6.3 8.3 412 12 54 6.35 27 09 0.5 375.2 L
IC 2574 22 × 22 2.6 1.793 10 9.6 418 10 28 23.5 68 24 44 44.9 L
NGC 0925 9 × 9 2.6 0.820 5.002 16.1 401 02 27 16.9 33 34 45 546.3 L
NGC 2403 27 × 27 5.2 0.0326 0.154 19 413 07 36 51.4 65 36 09 133.2 L
NGC 2841 6.06 × 5.79 5.2 0.3917 2.745 46.8 410 09 22 02.6 50 58 35 633.7 A
NGC 2976 23 × 23 5.2 0.934 3.769 3.2 400 09 47 15.4 67 54 59 1.1 L
NGC 3198 7.64 × 5.62 5.2 0.382 0.198 31.4 474 10 19 54.9 45 32 59 657 A
NGC 4736 18 × 18 5.2 0.895 4.502 7.8 410 12 50 53.0 41 07 14 306.7 L
NGC 5055 9 × 9 5.2 0.499 2.839 33.3 432 13 15 49.3 42 01 45 496.7 L
NGC 6946 15 × 15 2.6 1.556 10.179 14.5 402 20 34 52.3 60 09 14 48.7 L
NGC 7331 4.94 × 4.6 5.2 0.505 3.318 24.8 357 22 37 04.0 34 24 56 818.3 A
NGC 7793 24 × 24 2.6 2.343 16.634 7.14 420 23 57 49.8 −32 35 28 226.2 A

Notes. The table lists: (1) beam size of the data cube (NGC 2841, NGC 3198, and NGC 7331 are at the original resolution); (2) channel width; (3) noise in the channels; (4) noise in the total map; (5) outermost fitted radius; (6) sampling radius; (7,8) centre coordinate; (9) systemic velocity; and (10) normalisation method (L=local, A=azimuthal).

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