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Erik Rosolowsky edited figures/powerlawsubplots1/caption.tex
about 8 years ago
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Fits to the complementary cumulative mass distribution functions for the same (equal-area) regions used in the \citet{Adamo_2015} work. The dashed line indicates the power-law fits to the mass distributions and the solid curves indicate the fit using a truncate power-law distribution. In most cases, the truncated power law is clearly a better model, but the regions in the center of the galaxy are not well-represented by either functional model.
\ref{fig:massfits} \label{fig:massfits}