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diff --git a/Zurich_group/Mountain_hut_2015/QEE/mchrzasz.pdf b/Zurich_group/Mountain_hut_2015/QEE/mchrzasz.pdf
index ca7286e..84d82f4 100644
--- a/Zurich_group/Mountain_hut_2015/QEE/mchrzasz.pdf
+++ b/Zurich_group/Mountain_hut_2015/QEE/mchrzasz.pdf
Binary files differ
diff --git a/Zurich_group/Mountain_hut_2015/QEE/mchrzasz.tex b/Zurich_group/Mountain_hut_2015/QEE/mchrzasz.tex
index a66c01a..7b27d3c 100644
--- a/Zurich_group/Mountain_hut_2015/QEE/mchrzasz.tex
+++ b/Zurich_group/Mountain_hut_2015/QEE/mchrzasz.tex
@@ -287,6 +287,36 @@
 
 \end{frame}
 
+\begin{frame}\frametitle{What could we do?}
+
+$\Rrightarrow$ For starters we should start by measurement of $\PZ$ cross section.\\
+$\Rightarrow$ Relativity simple, you don't need much data.\\
+$\Rightarrow$ Important for MC tuning.\\
+$\Rrightarrow$ More interesting: Tripple Gauge Boson Couplings:\\{~}\\
+\begin{columns}
+
+\column{3in}
+\begin{itemize}
+\item Clear SM prediction.
+\item Sensitive to anomalous couplings!
+\item ATLAS observed a small but consistent deviation in this measurement.
+\end{itemize}
+
+\column{2in}
+\includegraphics[width=0.9\textwidth]{{images/DibosonGeneric.eps}.jpg}
+
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+
+
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+
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+
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+
+
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diff --git a/Zurich_group/Mountain_hut_2015/RD/mchrzasz.tex b/Zurich_group/Mountain_hut_2015/RD/mchrzasz.tex
index 7761983..b5d5123 100644
--- a/Zurich_group/Mountain_hut_2015/RD/mchrzasz.tex
+++ b/Zurich_group/Mountain_hut_2015/RD/mchrzasz.tex
@@ -454,7 +454,7 @@
 \begin{frame}\frametitle{Plans for the future?}
 $\Rrightarrow$ So let's list the hints of NP we have:
 \begin{itemize}
-\item The famous $P_56{\prime}$ anomaly ($3.7~\sigma$).
+\item The famous $P_5^{\prime}$ anomaly ($3.7~\sigma$).
 \item The $R_k$ anomaly ($2.7~\sigma$). 
 \item The $R(\PDstar)$ anomaly ($2.1~\sigma$)\footnote{This anomaly was also observed by Babar and Belle with $2.7~\sigma$ and $2.0\sigma$ significance.}.
 \end{itemize}
@@ -478,12 +478,13 @@
 \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 $\PBplus \to \PKplus \Pe \Pe$. 
 \end{itemize}
 
 \end{frame}
 
 
-\begin{frame}\frametitle{Lets pin down NP in run2 data}
+\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: $\PB \to \PK(\PKstar) \Ptau \Ptau$.
@@ -498,6 +499,7 @@
 
 
 \begin{enumerate}
+\item Future analysis will be more challenging!
 \item Run1 data analysis program is still rich in NP searches.
 \item Many analysis are in the pipe line. 
 \item We should maximize the coverage of the mentioned topics.