as an

paper/paper.tex

@@ -747,7 +747,7 @@ \section{Discussion}
 Figure \ref{fig:mass} shows the enclosed mass as a function of radius
 for different dark matter halos together with the \tol's dynamical
 mass estimate. 
-{\bf This should be considered an upper bound as lower values
+{\bf This should be considered as an upper bound as lower values
   could be achieved if one considers instead a cored DM profile.}
 {\bf Realistic mass estimates could only be achieved by detailed mass
   modelling once \tol's detailed kinematic information becomes