diff --git a/main.tex b/main.tex
index 2babbeb..f104107 100644
--- a/main.tex
+++ b/main.tex
@@ -121,7 +121,7 @@ code-for-last-col = \color{blue}
 \begin{frame}[fragile]{Homogenous Spherical Spaces --- Results}
 	\begin{itemize}
 		\pause
-		\item For the majority of groups $\Gamma$, the anisotropies $\frac{\delta T}{T}$ do not coincide with observations.
+		\item For the majority of groups $\Gamma$, the anisotropies $\textcolor{purple}{\frac{\delta T}{T}}$ do not coincide with observations.
 		      \pause
 		\item The only groups for which they do are $\Gamma = O^*$ and $\Gamma = I^*$ — the \textcolor{red}{binary octahedral} and \textcolor{red}{binary icosahedral} groups of order 48 and 120 respectively.
 		      \pause
@@ -237,7 +237,7 @@ code-for-last-col = \color{blue}
 
 	\pause
 	\begin{enumerate}
-		\item We can infer the shape of the universe from its spectrum.
+		\item We can infer the \textcolor{blue}{shape} of the universe from its \textcolor{blue}{spectrum}.
 
 		      \pause
 		\item There are two homogeneous spherical manifolds obtained as $\S^3/\Gamma$ which produce CMB similar to observations.
@@ -246,7 +246,7 @@ code-for-last-col = \color{blue}
 		\item Inhomogeneous spherical spaces exhibit varied behavior of CMB anisotropies.
 
 		      \pause
-		\item Statistical test results suggest possibilities of finite multi-connected topology.
+		\item Statistical test results suggest possibilities of \textcolor{red}{finite multi-connected} topology.
 	\end{enumerate}
 \end{frame}