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Table 1

Properties of the 10 selected extscmo extscria simulations at z = 0.

(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12)
Name Symbol log 10(M) log 10(MHI) log 10(M200) M V q Rout vout,H i W50/ 2 σ
[M] [M] [M] [mag] [kpc] [km s-1] [km s-1] [km s-1] [km s-1]

M-1 6.56 7.48 9.97 –12.35 0.49 1.68 21.66 36.16 14.30 10.84
M-2 6.59 7.29 9.95 –12.52 0.63 1.21 39.87 36.43 24.35 18.51
M-3 6.87 7.31 9.93 –12.77 0.74 1.13 19.45 33.81 15.00 12.95
M-4 7.41 7.83 10.00 –13.92 0.41 2.37 17.04 37.60 18.58 12.55
M-5 7.55 7.34 10.01 –14.35 0.53 1.09 41.69 43.10 41.53 18.89
M-6 7.71 7.94 10.55 –14.93 0.76 1.93 39.04 52.72 27.02 21.60
M-7 8.00 8.49 10.41 –15.69 0.58 4.18 36.31 46.96 21.57 19.79
M-8 8.33 8.64 10.47 –16.50 0.61 4.87 45.79 54.49 29.33 26.49
M-9 8.53 8.59 10.42 –16.75 0.60 3.43 40.54 52.38 37.50 25.09
M-10 9.07 8.66 10.84 –18.17 0.56 4.15 53.94 67.30 38.27 33.94

Notes. (1) The name of the simulation, (2) the symbol used throughout the plots, (3) the stellar mass, (4) the H i mass, (5) the halo virial mass, (6) the total V-band magnitude, (7) the intrinsic flattening of the H i, (8) the H i radius, (9) the outermost value of the rotation curve, (10) the maximum circular velocity of the halo, (11) the half-width-half-max of the H i, and (12) the velocity dispersion of the stars at Rout.

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