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\author{ {M.Chrzaszcz} (CERN)}
\institute{UZH}
\title[Mass Calibration]{Mass Calibration}
\date{28 March 2018}


\begin{document}
\tikzstyle{every picture}+=[remember picture]

{
\setbeamertemplate{sidebar right}{\llap{\includegraphics[width=\paperwidth,height=\paperheight]{bubble2}}}
\begin{frame}[c]%{\phantom{title page}}
\begin{center}
\begin{center}
	\begin{columns}
		\begin{column}{0.75\textwidth}
			\flushright\bfseries \Huge {Mass Calibration}
		\end{column}
                \begin{column}{0.02\textwidth}
                  {~}
                  \end{column}
                \begin{column}{0.23\textwidth}
                 % \hspace*{-1.cm}
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	\quad
	\vspace{3em}
\begin{columns}
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\flushright \vspace{-1.8em} { \Large Marcin Chrzaszcz\\\vspace{-0.1em} \vspace{-0.1em} }

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\vspace{0.2em}


\vspace{1em}

\vspace{0.5em}

	\textcolor{normal text.fg!50!Comment}{$\PBzero \to \PKstar \Pmuon \APmuon$ meeting, CERN\\28 March 2018
}
\end{center}
\end{frame}
}


\begin{frame}{Mass Calibration - why? }

\ARROW In the fit for rare mode $\PBd \to \PKstar \Pmu \Pmu$ we cannot leave the mass shape floating as we do for $\PBd \to \PKstar \PJpsi$\\
\ARROW To many free parameters!\\
\ARROW We need to obtain the mass-shape from data: $\PBd \to \PKstar \PJpsi$\\
\ARROW Than account for difference due kinematics.


\end{frame}


\begin{frame}{Mass Calibration -Procedure}

\begin{itemize}
\item Perform fit (2CB)to data with $\PBd \to \PKstar \PJpsi$\\
\begin{itemize}
\item After Preselection+BDT cut.
\end{itemize}
\end{itemize}
\begin{center}
\includegraphics[angle=-90,width=0.7\textwidth]{{images/Jpsi_fit_data_2016}.pdf}
\end{center}


\end{frame}



\begin{frame}{Mass Calibration -Procedure 2}

\begin{itemize}
\item Perform fit to MC with $\PBd \to \PKstar \Pmu \Pmu$ \texttt{FLATQ2} in $\PJpsi$ mass window.
\begin{itemize}
\item After Preselection+BDT cut.
\end{itemize}
\end{itemize}
\begin{center}
\includegraphics[angle=-90,width=0.7\textwidth]{{images/Jpsi_fit_MC_2016}.pdf}
\end{center}


\end{frame}



\begin{frame}{Mass Calibration -Procedure 3}

\begin{itemize}
\item We fix now all the parameters besides the widths of CB.
\item We parametrize the width:
\begin{equation}
\sigma^{\rm MC}_{q^2}= \sigma^{\rm MC}_{\PJpsi} \times S_{q^2}
\end{equation}
\item Only free parameters is the $S_{q^2}$.
\item To obtain the data prediction for given $q^2$ the $S_{q^2}$ is applied to signal pdf from $\PBd \to \PKstar \Pmu \Pmu$.
\end{itemize}



\end{frame}





\begin{frame}{Fits to MC}

\begin{center}
\includegraphics[angle=-90,width=0.49\textwidth]{images/KstarMuMu_0.1_0.98_2016.pdf}
\includegraphics[angle=-90,width=0.49\textwidth]{images/KstarMuMu_1.1_2.5_2016.pdf}\\
\includegraphics[angle=-90,width=0.49\textwidth]{images/KstarMuMu_2.5_4_2016.pdf}
\includegraphics[angle=-90,width=0.49\textwidth]{images/KstarMuMu_4_6_2016.pdf}

\end{center}

\end{frame}

\begin{frame}{Fits to MC}

\begin{center}
\includegraphics[angle=-90,width=0.49\textwidth]{images/KstarMuMu_6_8_2016.pdf}
\includegraphics[angle=-90,width=0.49\textwidth]{images/KstarMuMu_11_12.5_2016.pdf}\\
\includegraphics[angle=-90,width=0.49\textwidth]{images/KstarMuMu_15_17_2016.pdf}
\includegraphics[angle=-90,width=0.49\textwidth]{images/KstarMuMu_17_19_2016.pdf}

\end{center}

\end{frame}


\begin{frame}{Scaling factor -results}

\begin{center}
\includegraphics[angle=-90,width=0.49\textwidth]{images/S_factor_1GeV.pdf}
\includegraphics[angle=-90,width=0.49\textwidth]{images/S_factor_2GeV.pdf}\\
\end{center}

\end{frame}

\begin{frame}{Scaling factor -crosscheck}
\ARROW This is the same procedure as was in Run1 analysis.\\
\ARROW Let's repeat everything on Run1 S21 ntuples:

\begin{center}
\includegraphics[width=0.49\textwidth]{images/S_factor_2GeV_Run1.png}
\includegraphics[width=0.49\textwidth]{images/OLD.pdf}\\
\end{center}
\ARROW Quite compatible ;)
\end{frame}












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\end{document}