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Table A.2.

Main properties for the sample of massive nearby spirals studied in this work.

Galaxy log10(M/M) ϵM, low ϵM, up log10(Mhalo/M) ϵMhalo, low ϵMhalo, up vflat ϵvflat Reff ϵReff
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11)
NGC 7331 10.78 10.69 10.84 12.38 12.21 12.60 239.00 5.40 3.99 0.41
NGC 5985 10.91 10.55 11.10 12.21 12.12 12.28 293.60 8.60 10.71 2.67
UGC 03205 10.94 10.85 11.00 12.12 11.95 12.33 219.60 8.60 5.35 1.07
UGC 11914 10.95 10.82 11.04 13.04 12.44 13.67 288.10 10.50 3.12 0.94
UGC 05253 10.95 10.81 11.05 12.16 12.08 12.27 213.70 7.10 4.28 1.07
NGC 5907 10.96 10.87 11.01 12.02 11.93 12.16 215.00 2.90 7.88 0.41
NGC 2998 10.98 10.85 11.07 12.01 11.91 12.13 209.90 8.10 7.06 1.06
NGC 2841 11.00 10.95 11.04 12.54 12.42 12.69 284.80 8.60 5.51 0.55
NGC 3992 11.01 10.93 11.07 12.15 12.03 12.30 241.00 5.20 9.99 0.97
UGC 12506 11.12 10.95 11.19 12.14 11.96 12.33 234.00 16.80 12.36 1.24
NGC 5371 11.13 10.94 11.26 11.64 11.53 11.74 209.50 3.90 9.80 2.45
UGC 09133 11.15 11.04 11.24 12.22 12.18 12.25 226.80 4.20 5.92 1.18
NGC 2955 11.17 11.11 11.22 12.13 11.80 12.48 (a) (a) 7.22 0.72
UGC 02953 11.18 11.03 11.28 12.29 12.22 12.36 264.90 6.00 5.03 1.51
NGC 6195 11.21 11.15 11.26 12.16 11.94 12.42 251.70 9.30 9.52 0.95
UGC 11455 11.22 11.11 11.31 12.61 12.43 12.84 269.40 7.40 10.06 1.51
NGC 0801 11.23 11.18 11.28 12.00 11.90 12.14 220.10 6.20 7.76 0.78
NGC 6674 11.24 11.15 11.32 12.42 12.32 12.56 241.30 4.90 7.75 1.54
UGC 02885 11.37 11.30 11.43 12.62 12.48 12.79 289.50 12.00 12.20 1.22
UGC 02487 11.39 11.33 11.45 12.58 12.52 12.67 332.00 3.50 9.63 1.45
ESO 563-G021 11.40 11.33 11.46 12.93 12.70 13.21 314.60 11.70 10.59 1.59

Notes. (1) Galaxy name; (2)-(4) stellar mass and related lower and upper uncertainties from PFM19; (5)-(7) halo mass and related lower and higher uncertainties from PFM19; (8)-(9) velocity of the flat part of the rotation curve (in  km s−1) and the related uncertainty from Lelli et al. (2016); (10)-(11) effective radius (in  kpc) and related uncertainty from Lelli et al. (2016).

(a)

The rotation curve of NGC 2955 does not have a well-defined flat part, thus its vflat is not reported in Lelli et al. (2016).

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