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Table 4:

Derived quantities from the harmonic decomposition.

Galaxy
$\langle A_{\rm r}\rangle$ $\langle A_{\rm r,1~kpc}\rangle$ $\langle A_{\rm r}\rangle$/ $v_{\rm rot}$ $\langle M_{\rm res}\rangle$ $\langle A_{\rm r,c}\rangle$ $\langle A_{\rm r,c,1~kpc}\rangle$ $\langle A_{\rm r,c}\rangle$/ $v_{\rm rot}$ $\langle M_{\rm res,c}\rangle$ $r_{\rm max}$
  [ \ensuremath{\mbox{km}~\mbox{s}^{-1}}] [ \ensuremath{\mbox{km}~\mbox{s}^{-1}}] [%] [ \ensuremath{\mbox{km}~\mbox{s}^{-1}}] [ \ensuremath{\mbox{km}~\mbox{s}^{-1}}] [%] [ \ensuremath{\mbox{km}~\mbox{s}^{-1}}] [kpc]  
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10)

NGC 2366
$2.91^{\rm +4.09}_{-1.06}$ $1.50^{\rm +0.42}_{-0.87}$ 5.8 2.15 $4.81^{\rm +2.32}_{-1.83}$ $2.08^{\rm +0.66}_{-0.67}$ 9.6 1.89 4.1

ESO 059-G001
$0.77^{\rm +0.51}_{-0.09}$ $0.77^{\ldots}_{\ldots}$ 1.1 0.43 $1.45^{\rm +0.62}_{-0.61}$ $1.17^{\ldots}_{\ldots}$ 2.1 0.37 3.2

ESO 215-G?009
... ... ... ... $6.57^{\rm +1.64}_{-1.38}$ $5.42^{\rm +2.79}_{-3.03}$ 8.5 1.99 7.3

NGC 4861
$1.54^{\rm +0.94}_{-0.46}$ $0.78^{\ldots}_{\ldots}$ 3.3 1.04 $2.60^{\rm +0.78}_{-0.28}$ $1.02^{\ldots}_{\ldots}$ 5.7 1.07 7.1

NGC 5408
$2.15^{\rm +2.62}_{-0.88}$ $2.50^{\ldots}_{\ldots}$ 4.1 1.92 $4.08^{\rm +2.63}_{-1.79}$ $2.54^{\ldots}_{\ldots}$ 7.7 1.30 6.9

IC 5152
$2.35^{\rm +2.27}_{-1.24}$ $1.63^{\rm +0.99}_{-1.24}$ 5.3 1.17 $5.38^{\rm +0.10}_{-0.64}$ $5.38^{\rm +0.10}_{-0.64}$ 12.2 1.07 3.9
Notes: (1) The name of the galaxy; (2) the median of the quadratically-added amplitude of the non-circular motions (unconstrained case), averaged over the entire radial range, the errors indicate the lower and upper quartile; (3) same as (2), but averaged over the inner 1 kpc only; (4) the percentage the non-circular motions contribute to the maximum rotation velocity; (5) the median of the reswri absolute residual velocity field after the harmonic decomposition; (6), (7), (8), (9) the same as (2), (3), (4), (5), but for the constrained case; (10) maximum radius for the averaging of the quadratically-added amplitudes.

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