Fig. D.1.

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Few example RCs for which either dynamical masses are unexpected or are a DM fraction. The color codes are as follows: Observed RC is shown by brown squares with the error bars connected with a black line; the orange and blue curves indicate the stellar and baryonic mass velocity curves derived assuming Freeman (1970) disk for given total M* and Mbar. The vertical red, light blue, and dashed blue lines represent the Re, Ropt, and Rout respectively. From left to right: first and second type of RCs seem to have either overestimated baryonic mass or wrong RC, which leads to smaller dynamical masses than baronic masses, and thus a negative DM fraction. The third type of RCs are announced declining, thus giving us fDM(<Ropt) > fDM(<Rout), which is generally not seen in the local SFGs. The fourth type of RCs are disturbed, thus discarded from the analysis.
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