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Table 3:

Derived parameters for the rotation curve sub-sample.
ID $\alpha_{2000}$ $\delta_{2000}$ $V_{\rm sys}$ D MV (V-I) $M_{\rm HI}$ W20 W50 W20 $_{\rm {,~turb}}$ W50 $_{\rm {,~turb}}$ i $\langle {\rm PA} \rangle$ Vvf Vpv
  (h m s) ( $\circ~~~ \hbox{$^\prime$ }~~~ \hbox{$^{\prime\prime}$ }$)  km s-1 Mpc mag   107 $M_{\odot}$  km s-1  km s-1  km s-1  km s-1 $^\circ$ $^\circ$  km s-1  km s-1
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13) (14) (15) (16)
D500-2* 10 31 43.0 +25 18 33 1259 17.9  -16.38 0.42 87.08 135 120 119 105 57 $\pm$ 6 345 68 68
D500-3 10 05 59.5 +23 52 04 1327 18.5  -15.74 0.31 6.58 96 83 84 72 55a $\pm$ 6  $\cdots$   $\cdots$  45
D512-2 14 33 20.2 +26 59 54 840 14.1  -15.22 0.80 6.96 88 74 78 65 56 $\pm$ 10 40 35 37
D564-8* 09 02 54.0 +20 04 28 478 6.5  -12.64 0.93 1.58 62 48 54 42 63 $\pm$ 7 13 25 29
D575-2* 12 52 21.9 +21 37 46 774 12.2  -15.15 0.78 31.51 146 119 129 104 57 $\pm$ 5 220 74  $\cdots$ 
D631-7* 07 57 01.8 +14 23 27 311 5.5b -14.50 0.55 14.68 113 89 100 78 59 $\pm$ 3 324 58 53
a Optical I-band inclination from Pildis et al. (1997).
b Distance as given in Karachentsev et al. (2003).
Notes: Cols. (1) to (12) as in Table 2, except that for the starred galaxies, the center position and $V_{\rm sys}$ were derived kinematically; (13) inclination angle (optical inclination for D500-3, kinematic inclination otherwise). The uncertainties given for the kinematic inclination angles represent the scatter of the values of the individual tilted-rings. For D500-3, the average uncertainty of the kinematic inclination estimates is given; (14) average position angle of the rotation curve analysis, measured counter-clockwise from north to the receding side of the galaxy; (15) maximum rotation velocity from the tilted-ring analysis of the velocity field, corrected for inclination; (16) maximum rotation velocity from the position-velocity diagram, corrected for inclination.

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