diff --git a/Manuscript/EPAWTFT.tex b/Manuscript/EPAWTFT.tex
index 441593f..b43d39b 100644
--- a/Manuscript/EPAWTFT.tex
+++ b/Manuscript/EPAWTFT.tex
@@ -331,14 +331,14 @@ Expanding the wave function and energy as power series in $\lambda$ as
 \end{align}
 \end{subequations}
 and solving the corresponding perturbation equations up to a given order $k$, then 
-yields approximate solutions to Eq.~\eqref{eq:SchrEq} \titou{by setting $\lambda = 1$}.
+yields approximate solutions to Eq.~\eqref{eq:SchrEq} by setting $\lambda = 1$.
 
 % MATHEMATICAL REPRESENTATION
 Mathematically, Eq.~\eqref{eq:E_expansion} corresponds to a Taylor series expansion of the exact energy
 around the reference system $\lambda = 0$.
 The energy of the target ``physical'' system is then recovered at the point $\lambda = 1$.
 However, like all series expansions, the Eq.~\eqref{eq:E_expansion} has a radius of convergence $\rc$. 
-When $\rc \titou{\le} 1$, the Rayleigh--Sch\"{r}odinger expansion will diverge
+When $\rc \le 1$, the Rayleigh--Sch\"{r}odinger expansion will diverge
 for the physical system.
 The value of $\rc$ can vary significantly between different systems and strongly depends on the particular decomposition
 of the reference and perturbation Hamiltonians in Eq.~\eqref{eq:SchrEq-PT}.\cite{Mihalka_2017b}
@@ -377,7 +377,7 @@ We will demonstrate how the choice of reference Hamiltonian controls the positio
 ultimately determines the convergence properties of the perturbation series.
 
 
-\titou{Practically, to locate EPs in a more complicated systems, one must solve simultaneously the following equations:\cite{Cejnar_2007}
+Practically, to locate EPs in a more complicated systems, one must simultaneously solve\cite{Cejnar_2007}
 \begin{subequations}
 \begin{align}
 	\label{eq:PolChar}
@@ -388,9 +388,11 @@ ultimately determines the convergence properties of the perturbation series.
 \end{align}
 \end{subequations}
 where $\hI$ is the identity operator.
-Equation \eqref{eq:PolChar} is the well-known secular equation providing us with the (eigen)energies of the system. 
-If an energy is also solution of Eq.~\eqref{eq:DPolChar}, then this energy value is, at least, two-fold degenerate. 
-These degeneracies can be conical intersections between two states with different symmetries for real values of $\lambda$ \cite{Yarkony_1996} or EPs between two states with the same symmetry for complex values of $\lambda$.}
+Equation \eqref{eq:PolChar} is the well-known secular equation providing the (eigen)energies of the system. 
+If the energy is also solution of Eq.~\eqref{eq:DPolChar}, then this energy value is at least two-fold degenerate. 
+These degeneracies can be conical intersections between two states with different symmetries 
+for real values of $\lambda$\cite{Yarkony_1996} or EPs between two states with the 
+same symmetry for complex values of $\lambda$.
 
 
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