diff --git a/draft.tex b/draft.tex
index 6cdf57d..78a9d43 100644
--- a/draft.tex
+++ b/draft.tex
@@ -495,34 +495,30 @@
 
 
 %We acknowledge useful contributions from Gino Isidori, Danny van Dyk and Patrick Owen.
-%This work is supported by the Swiss National Science Foundation (SNF) under contract  
-
+%This work is supported by the Swiss National Science Foundation (SNF) under contract PZ00P2-174182.   
 
 \bibliography{references}
 
+\FloatBarrier
 
-\newpage
+\appendix
+
+%\newpage
 
 
 \section{Supplemental material}
 
 An extension of the physics case of the proposed method
 is to investigate the sensitivity to the chirality-flipped counterparts of the usual Wilson coefficients, 
-\textit{i.e.} $\WC'^{(\mu)}_9$ and $\WC'^{(\mu)}_{10}$.
-We assume the primed WCs to be fixed to the SM value for electrons mode and let free-floating the
-muon channel. In the following, we consider different NP scenarios concerning the $\WC'^{(\mu)}_i$,
-while $\WC^{(\mu,e)}_i$ are set as for \texttt{BMP}$_{\WC_{9,10}}$.
+\textit{i.e.} $\WC^{\prime (\mu)}_9$ and $\WC^{\prime(\mu)}_{10}$.
+Following the formalism discussed in this letter, the primed WCs are examined by considering in addition to the 
+\texttt{BMP}$_{\WC_{9,10}}$ three different modified NP scenarios for the muon only:
+$\WC_{9,10}^{\prime(\mu)} = \WC^{\prime \rm{SM}}_{9,10} = 0$;
+$\WC^{\prime (\mu)}_9 = \WC^{\prime (\mu)}_{10} = 0.3$; 
+and $\WC^{\prime (\mu)}_9 = - \WC^{\prime (\mu)}_{10} =  0.3$.  
+Notice that for the electron mode the $\WC_{9,10}^{\prime(e)}$ is set and fixed to the SM value $\WC^{\prime \rm{SM}}_{9,10} = 0$.
 
-Firstly, Fig.~\ref{fig:Cp_Hz} shows the fit results for different order of the analytic expansion for 
-the non-local hadronic contribution for a NP scenario with $\WC'^{(\mu)}_9 = \WC'^{(\mu)}_{10} = 0.3$, 
-and yields corresponding to the \lhcb Run II expected statistics. 
-The dependency of the determination of $\WC'^{(\mu)}_9$ and $\WC'^{(\mu)}_{10}$ on the 
-order of the expansion clearly saturates after $\mathcal{H}_\lambda[z^3]$ and allows a measurement
-of the primed Wilson coefficients for the muon decay channel $B^{0} \to K^{*0} \mumu$ independent 
-on the theoretical hadronic uncertainty.
-
-
-\begin{figure}[tbh]
+\begin{figure}[b]
 \includegraphics[width=.4\textwidth]{plots/ellipses_CpMu_Hz.pdf} 
 \caption{%
     Two-dimensional sensitivity scans for the pair of Wilson coefficients $\WC'^{(\mu)}_9$ and 
@@ -534,21 +530,27 @@
 }
 \end{figure}
 
-
+Figure~\ref{fig:Cp_Hz} shows the fit results for different order of the analytic expansion for 
+the non-local hadronic contribution for a NP scenario with $\WC'^{(\mu)}_9 = \WC'^{(\mu)}_{10} = 0.3$, 
+and yields corresponding to the \lhcb Run II expected statistics. 
+The dependency on the determination of $\WC'^{(\mu)}_9$ and $\WC'^{(\mu)}_{10}$ on the 
+order of the expansion clearly saturates after $\mathcal{H}_\lambda[z^3]$ and allows a measurement
+of the primed Wilson coefficients for the muon decay channel $B^{0} \to K^{*0} \mumu$ independent 
+on the theoretical hadronic uncertainty.
+%
 Figure~\ref{fig:Cp} shows the prospects for the sensitivity to the $\WC'^{(\mu)}_9$ and 
-$\WC'^{(\mu)}_{10}$ Wilson coefficients corresponding to the expected statistics at  \belle II
-and \lhcb upgrades [$50\,$-$\,300\,$fb$^{-1}$].
-
-
-\begin{figure}[tbh]
+$\WC'^{(\mu)}_{10}$ Wilson coefficients corresponding to the expected statistics at 
+Note that only with the full capability of the LHCb experiment it is possible 
+to start disentangling the different NP hypotheses. 
+%
+\begin{figure}[t]
 \includegraphics[width=.4\textwidth]{plots/ellipses_CpMu.pdf} 
 \caption{%
     Two-dimensional sensitivity scans for the pair of Wilson coefficients $\WC'^{(\mu)}_9$ and $\WC'^{(\mu)}_{10}$
     for three NP scenarios: (blue) $\WC'^{(\mu)}_9 = \WC'^{(\mu)}_{10} = 0$, (orange) $\WC'^{(\mu)}_9 = \WC'^{(\mu)}_{10} = 0.3$ 
     and (magenta) $\WC'^{(\mu)}_9 = - \WC'^{(\mu)}_{10} = 0.3$.
-    The contours correspond to $3\,\sigma$ statistical-only uncertainty bands expected for the \belle II 50~ab$^{-1}$ (dashed) 
-    and \lhcb Upgrade $50\,$fb$^{-1}$ (dotted) and $\,300\,$fb$^{-1}$ (solid) statistics.
-    \textbf{Figure to be updated.}
+    The contours correspond to $3\,\sigma$ statistical-only uncertainty bands expected for the LHCb Upgrade (dotted)  
+    $50\,$fb$^{-1}$ and (solid) $\,300\,$fb$^{-1}$ statistics.
     \label{fig:Cp}
 }
 \end{figure}