Computational Notes on the Numerical Analysis of Galactic Rotation   Curves
  In this paper we present a brief discussion on the salient points of the computational analysis that are at the basis of the paper \cite{StSc}. The computational and data analysis have been made with the software Mathematica$^\circledR$ and presented at Mathematica Italia User Group Meeting 2011. 
G. Scelza, A. Stabile
astro-ph.GA