diff --git a/Zurich_group/Mountain_hut_2015/RD/images/MCData_correction.png b/Zurich_group/Mountain_hut_2015/RD/images/MCData_correction.png
new file mode 100644
index 0000000..5794d9e
--- /dev/null
+++ b/Zurich_group/Mountain_hut_2015/RD/images/MCData_correction.png
Binary files differ
diff --git a/Zurich_group/Mountain_hut_2015/RD/images/sWeights_MCData_correction.png b/Zurich_group/Mountain_hut_2015/RD/images/sWeights_MCData_correction.png
new file mode 100644
index 0000000..1720c79
--- /dev/null
+++ b/Zurich_group/Mountain_hut_2015/RD/images/sWeights_MCData_correction.png
Binary files differ
diff --git a/Zurich_group/Mountain_hut_2015/RD/mchrzasz.tex b/Zurich_group/Mountain_hut_2015/RD/mchrzasz.tex
index 20ca7dd..ed09c9f 100644
--- a/Zurich_group/Mountain_hut_2015/RD/mchrzasz.tex
+++ b/Zurich_group/Mountain_hut_2015/RD/mchrzasz.tex
@@ -452,6 +452,85 @@
 
 \end{frame} 
 
+
+\begin{frame}\frametitle{Angular analysis of $\PBzero \to \PKstar [\Pmuon \APmuon,\Pelectron \APelectron]$\\ \texttt{\begin{small} F.Lionetto, N.Serra, R.Silva Coutinho \end{small}}}
+
+
+$\Rrightarrow$ LFV measurements using $\PBzero \to \PKstar \Pelectron \APelectron (R_{K^{*}})$ are under way, \footnote{Similarly LU tests for $R_{\phi}$ are also being performed.} so it seems a good idea to study their angular observables.
+
+\begin{columns}
+\column{0.02\textwidth}
+{~}
+\column{0.47\textwidth}
+\begin{itemize}
+\item Analysis at an initial stage. 
+\item Plan is to perform the MoM for sensitive observables
+\begin{itemize}
+\item $1.1 < q^{2} < 6.0\,$GeV$^{2}/c^{4}$
+\item $q^{2} > 15$GeV\,$^{2}/c^{4}$
+\end{itemize}
+\item Studying smearing tool to reproduce Bremsstrahlung effects in muons.
+
+\end{itemize}
+
+\column{0.4\textwidth}
+\includegraphics[width=0.95\textwidth]{images/sWeights_MCData_correction.png}\\
+\includegraphics[width=0.95\textwidth]{images/MCData_correction.png}
+
+\column{0.02\textwidth}
+{~}
+\end{columns}
+\end{frame}
+
+\begin{frame}\frametitle{Moments analysis of $\PBzero \to \PKstar(14X0) [\Pmuon \APmuon,\Pelectron \APelectron]$\\ \texttt{\begin{small} N.Serra, R.Silva Coutinho \end{small}}}
+
+$\Rrightarrow$ Similar methodology used in the ($S,P,D$)-wave analysis performed by Espen, but extended to electrons.
+
+\begin{columns}
+\column{0.02\textwidth}
+{~}
+\column{0.47\textwidth}
+\begin{itemize}
+\item Several tools used are shared with Federica's analysis.
+\item Revised selection (wrt the $R_{K^{*}}$ analysis) optimised for the phase-space. 
+\item Currently working on simulated studies to verify the sensitivity (and even feasibility) of the analysis.
+
+\end{itemize}
+
+\column{0.5\textwidth}
+\includegraphics[width=5.5cm,height=4cm]{images/ROC_uBoost.png}
+
+\column{0.02\textwidth}
+{~}
+\end{columns}
+\end{frame}
+
+\begin{frame}\frametitle{Lepton flavour violation in $\PB \to \PK \Plepton \Plepton^{\prime}$ decays\\ \texttt{\begin{small} M.Chrzaszcz \end{small}}}
+
+\begin{columns}
+\column{0.02\textwidth}
+{~}
+\column{0.47\textwidth}
+\begin{itemize}
+
+\item Several groups concentrate their affords in $\PBzero \to \PK \Ptau \Pmu$.
+\item However, $\PB \to \PK \Pelectron \APmuon$ decays might be a better candidate.
+\begin{itemize}
+\item Factor of $10$ lost because of the hierarchical structure of NP, but you can this back because of $\tau$ branching fraction.
+\item ... and still you do not have the neutrinos to worry about.
+\end{itemize}
+\item Currently working on the MVA optimisation.
+\end{itemize}
+
+\column{0.5\textwidth}
+\includegraphics[width=1.1\textwidth]{images/ROC_Kmue.pdf}
+
+\column{0.02\textwidth}
+{~}
+\end{columns}
+\end{frame}
+
+
 %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
 \begin{frame}
 
@@ -523,82 +602,6 @@
 
 \end{frame}
 
-\begin{frame}\frametitle{Angular analysis of $\PBzero \to \PKstar [\Pmuon \APmuon,\Pelectron \APelectron]$\\ \texttt{\begin{small} F.Lionetto, N.Serra, R.Silva Coutinho \end{small}}}
-
-
-$\Rrightarrow$ LFV measurements using $\PBzero \to \PKstar \Pelectron \APelectron (R_{K^{*}})$ are under way, \footnote{Similarly LU tests for $R_{\phi}$ are also being performed.} so it seems a good idea to study their angular observables.
-
-\begin{columns}
-\column{0.02\textwidth}
-{~}
-\column{0.47\textwidth}
-\begin{itemize}
-\item Analysis at an initial stage. 
-\item Plan is to perform the MoM for sensitive observables
-\begin{itemize}
-\item $1.1 < q^{2} < 6.0\,$GeV$^{2}/c^{4}$
-\item $q^{2} > 15$GeV\,$^{2}/c^{4}$
-\end{itemize}
-\item Studying smearing tool to reproduce Bremsstrahlung effects in muons.
-
-\end{itemize}
-
-\column{0.4\textwidth}
-\includegraphics[width=4cm,height=2.5cm]{images/sWeights_MCData_correction.pdf}\\
-\includegraphics[width=4cm,height=2.5cm]{images/MCData_correction.pdf}
-
-\column{0.02\textwidth}
-{~}
-\end{columns}
-\end{frame}
-
-\begin{frame}\frametitle{Moments analysis of $\PBzero \to \PKstar(14X0) [\Pmuon \APmuon,\Pelectron \APelectron]$\\ \texttt{\begin{small} N.Serra, R.Silva Coutinho \end{small}}}
-
-$\Rrightarrow$ Similar methodology used in the ($S,P,D$)-wave analysis performed by Espen, but extended to electrons.
-
-\begin{columns}
-\column{0.02\textwidth}
-{~}
-\column{0.47\textwidth}
-\begin{itemize}
-\item Several tools used are shared with Federica's analysis.
-\item Revised selection (wrt the $R_{K^{*}}$ analysis) optimised for the phase-space. 
-\item Currently working on simulated studies to verify the sensitivity (and even feasibility) of the analysis.
-
-\end{itemize}
-
-\column{0.5\textwidth}
-\includegraphics[width=5.5cm,height=4cm]{images/ROC_uBoost.png}
-
-\column{0.02\textwidth}
-{~}
-\end{columns}
-\end{frame}
-
-\begin{frame}\frametitle{Lepton flavour violation in $\PB \to \PK \Plepton \Plepton^{\prime}$ decays\\ \texttt{\begin{small} M.Chrzaszcz \end{small}}}
-
-\begin{columns}
-\column{0.02\textwidth}
-{~}
-\column{0.47\textwidth}
-\begin{itemize}
-
-\item Several groups concentrate their affords in $\PBzero \to \PK \Ptau \Pmu$.
-\item However, $\PB \to \PK \Pelectron \APmuon$ decays might be a better candidate.
-\begin{itemize}
-\item Factor of $10$ lost because of the hierarchical structure of NP, but you can this back because of $\tau$ branching fraction.
-\item ... and still you do not have the neutrinos to worry about.
-\end{itemize}
-\item Currently working on the MVA optimisation.
-\end{itemize}
-
-\column{0.5\textwidth}
-\includegraphics[width=1.1\textwidth]{images/ROC_Kmue.pdf}
-
-\column{0.02\textwidth}
-{~}
-\end{columns}
-\end{frame}
 
 \begin{frame}\frametitle{Summary}