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diff --git a/Zurich_group/Mountain_hut_2015/RD/mchrzasz.tex b/Zurich_group/Mountain_hut_2015/RD/mchrzasz.tex
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--- a/Zurich_group/Mountain_hut_2015/RD/mchrzasz.tex
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@@ -492,16 +492,18 @@
 
 \end{frame}
 
+
+
 \begin{frame}\frametitle{Lets pin down NP now!}
 
 
 $\Rrightarrow$ Some ideas what we can do:
 \begin{itemize}
-\item If the NP accrues in the $R_k$, it might also occur in the angular observables! $\Rightarrow$ Lets measure difference in observables like $P_5^{\prime,~\mu} - P_5^{\prime~e}$.
+\item If the NP occurs in the $R_k$, it might also occur in the angular observables! $\Rightarrow$ Lets measure difference in observables like $P_5^{\prime,~\mu} - P_5^{\prime~e}$.
 \item In the $\tau$ sector the NP is competing with a SM tree decay! We could measure: $R(\PLambda_c^{\ast})$\footnote{Please remember that protons kill a lot of background. The main criticism on $R(\PDstar)$ analysis is the background modelling}.
 \item If there exists LU breaking, one cloud also see LFV like: $\PB \to \PK \Plepton \Plepton^{\prime}$, like: $\PBplus \to \PKplus \Pmu \Pe$.
 \item Now playing the devils advocate: Maybe we are remodelling the $\PBzero \to \PKstar \Pmu \Pmu$? One could measure the partial and higher moments in this channel as well in $\PB \to \PK \Pe \Pe$, Collaboration with Roman Zwicky and Greg Cowan~\footnote{My personal opinion, we should keep as much of MoM in UZH as possible.}.
-\item Measure the angular observables of $\PBplus \to \PKplus \Pe \Pe$. 
+\item Measure the angular observables of $\PBplus \to K^{*+}_{1}\Pe \Pe$, $\PBplus \to \PKplus \Pe \Pe$ and $\Lambda^{0}_{b}\to \Lambda^{*}\Pe \Pe$ decays. 
 \end{itemize}
 
 \end{frame}
@@ -510,7 +512,10 @@
 \begin{frame}\frametitle{Lets pin down NP in Run2 data}
 $\Rrightarrow$ Some ideas what we could do with the full Run2 data:
 \begin{itemize}
-\item Well $\tau$s are more sensitive, we could start thinking of: $\PB \to \PK(\PKstar) \Ptau \Ptau$.
+\item Since decays involving $\tau$'s are more sensitive, we could start thinking in modes such as  $\PB \to \PK(\PKstar) \Ptau \Ptau$.
+\begin{itemize}
+\item Undergraduate student [Alex Daetwyler] is currently studying the sensitivity for $\PBzero \to \PKstar \Ptau \Ptau$ decays with Run 1 and 2 data. 
+\end{itemize}
 \item We should definitely update $\tau \to 3\mu$. 
 \item Some more Semi-leptonic measurements!
 \end{itemize}
@@ -518,6 +523,83 @@
 
 \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}