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Table 5.

Fit results for the three models par, wedge, and const.

Galaxy a b c αc AICa δmeda AICb δmedb AICc δmedc NPoints
[kpc−2] [kpc−1] [deg] [deg] [deg] [deg]
NGC 891 0.108 ± 0.012 0.48 ± 0.07 1.03±0.07 44 ± 2 554 17.2 563 18.9 529 15.3 148
NGC 3044 0.064 ± 0.008 0.36±0.05 0.56 ± 0.06 61 ± 3 64 7.2 57 7.6 71 13.5 29
NGC 3079 0.022 ± 0.009 0.17 ± 0.08 0.36 ± 0.16 70 ± 8 403 36.5 402 35.1 409 42.4 68
NGC 3448 0.305 ± 0.066 0.86 ± 0.27 0.46 ± 0.07 65 ± 3 20 10.3 20 7.3 20 8.9 9
NGC 3735 2.18±0.68 25 ± 7 122 21.4 128 14.7 104 15.9 22
NGC 4157 0.107 ± 0.061 0.47 ± 0.35 0.86 ± 0.31 49 ± 10 91 24.3 90 20.7 91 28.4 19
NGC 4217 0.020 ± 0.004 0.19 ± 0.04 0.66±0.06 57 ± 2 114 10.9 102 7.3 87 7.7 26
NGC 4631 0.143 ± 0.014 0.38 ± 0.05 0.95±0.04 46 ± 1 573 13.2 585 14.5 462 4.7 105
NGC 4666 0.08 ± 0.09 86 ± 5 146 26.1 147 26.7 146 25.4 37
NGC 5775 0.010 ± 0.002 0.12 ± 0.03 0.58 ± 0.10 60 ± 4 110 21.6 109 19.8 110 16.1 36

Notes. We report fit parameters a (par), b (wedge), and c (const) including parameter uncertainties, AIC scores (AICa, b, c), and the absolute residual median of the best-fitting solutions ( δ med a , b , c $ \delta_{\mathrm{med}}^{a,b,c} $). Additionally, we transform the slope of the const model to the angle measured from the disc (in the first quadrant) in decimal degrees (αc) and report the number of data point after the box average (NPoints) that were used as modelling input. Galaxies with a significant model preference and the preferred model parameter are marked in bold font.

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