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\subsubsection{Reconstruction of Z$\rightarrow e^+e^-$ events}
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acosta |
1.3 |
This exercise has multiple goals: one is the selection of
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Z$\rightarrow e^{+} e^{-}$ out of the ``Electroweak Soup'' (EWK) and their
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use to evaluate the performance of the electron reconstruction;
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and another one is the demonstration of the workflow for running offline
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ECAL calibration at a remote Tier-2 centre, starting from an AlcaReco
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stream produced at the Tier-1 centre.
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meridian |
1.1 |
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For this reason a special skim filter job has been designed, producing as output two streams for the same events: one is the standard electron AlcaReco stream, as described in section \ref{calibtool}, the other one is the standard RECOSIM output.
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acosta |
1.3 |
The events are selected on the basis of Monte Carlo generator
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information, requiring only Drell-Yan $e^+e^-$ events in a mass
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range from 50 to 130 GeV/c$^2$. The electrons are also required to
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have $p_T$ greater than 5 GeV/c and $|\eta|<2.7$.
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This selection has an efficiency over the Electroweak Soup of 3.7$\%$.
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Skim jobs were processed at the CNAF Tier-1, starting from less than 3
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million EWK soup events (not the full EWK dataset have been processed
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using the CMSSW\_1\_0\_5 release). Out of these events, a sample of
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76494 events have been selected and the two created streams were
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transferred to the Rome Tier-2. The total amount of data amounts to
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about 33.5GB, of which around 500MB are occupied by the AlcaReco
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electron stream.
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acosta |
1.2 |
Analysis jobs are sent to the Rome Tier-2 using CRAB\_1\_3\_0 and CMSSW\_1\_0\_5 on both the RECOSIM and the AlcaReco stream.
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meridian |
1.1 |
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acosta |
1.3 |
The main purpose is to validate the electron reconstruction, evaluating the electron reconstruction performance.
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meridian |
1.1 |
The electron reconstruction efficiency both versus $p_T$ and $\eta$ is shown in Fig.~\ref{fig:zee-eleeff}.
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\begin{figure}[!hbtp]
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\centering
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{\includegraphics[width=0.49\textwidth]{figs/zee-eleeffpt.pdf}}
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{\includegraphics[width=0.49\textwidth]{figs/zee-eleeffeta.pdf}}
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\caption{ (left) Electron reconstruction efficiency as a function of $p_T$ and (right) $\eta$.\label{fig:zee-eleeff} }
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\end{figure}
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acosta |
1.3 |
The two main ingredients for the electron reconstruction, the
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supercluster and the electron track, are then evaluated separately.
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The ratio of reconstructed supercluster energy over the true energy as
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a function of $\eta$ is visible in Fig.~\ref{fig:zee-erecetrue},
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showing a well-known problem in the CMSSW\_1\_0\_5 release for what
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concerns the endcap supercluster reconstruction. The projected
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distribution for the barrel is presented in the right plot of
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Fig.~\ref{fig:zee-erecetrue}.
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meridian |
1.1 |
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\begin{figure}[!hbtp]
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\centering
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{\includegraphics[width=0.49\textwidth]{figs/zee-erecetrueeta.pdf}}
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{\includegraphics[width=0.49\textwidth]{figs/zee-erecetruebarrel.pdf}}
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\caption{ (left) Distribution of the electron reconstructed supercluster energy over the true energy as a function of $\eta$ and (right) the corresponding distribution in the ECAL barrel acceptance. \label{fig:zee-erecetrue} }
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\end{figure}
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The quality of the track reconstruction is evaluated looking at the E/p distribution, using the track parameters both at the vertex and at the outermost state, as it can be seen in Fig.~\ref{fig:zee-eoverp}.
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\begin{figure}[!hbtp]
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\centering
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{\includegraphics[width=0.49\textwidth]{figs/zee-eoverpvertex.pdf}}
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{\includegraphics[width=0.49\textwidth]{figs/zee-eoverpoutermost.pdf}}
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\caption{Distribution of the E/p variable using track parameters at the (left) vertex (right) outermost state. \label{fig:zee-eoverp} }
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\end{figure}
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acosta |
1.3 |
At the time of the CMSSW\_1\_0\_5, the reconstructed electron track
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was not the track after the smoothing step, and for this reason the
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quality of the E/p distribution with the track parameters at the
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vertex is rather poor. A refitting of the electron track has been
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tried in the offline analysis, improving the quality of the E/p
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matching, as it visible in Fig.~\ref{fig:zee-refittedeoverp}.
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meridian |
1.1 |
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\begin{figure}[htbp]
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\centering
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\includegraphics[width=0.6\textwidth]{figs/zee-refittedeoverp.pdf}
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\caption{Distribution of the E/p variable using refitted track parameters at the vertex. \label{fig:zee-refittedeoverp} }
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\end{figure}
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acosta |
1.3 |
The invariant mass computed from the electron pair nearest two the nominal Z mass is presented in Fig.~\ref{fig:zee-invariantmass}.
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meridian |
1.1 |
\begin{figure}[h]
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\centering
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\includegraphics[width=0.6\textwidth]{figs/zee-invariantmass.pdf}
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\caption{Electron pair invariant mass in Z$\rightarrow e^{+} e^{-}$ events. \label{fig:zee-invariantmass}}
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\end{figure}
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acosta |
1.3 |
The distribution of the difference between the reconstructed mass and
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the generated mass is shown in
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Fig.~\ref{fig:zee-relativemassdifference}, where the right plot
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displays the difference as a fuction of $\eta$. The distribution shows
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the expected
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behaviour due to the effect of the increasing tracker material towards
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$\eta$ over the electron reconstruction.
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meridian |
1.1 |
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\begin{figure}[!hbtp]
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\centering
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{\includegraphics[width=0.49\textwidth]{figs/zee-relativemassdifference.pdf}}
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{\includegraphics[width=0.49\textwidth]{figs/zee-relativemassdifferenceeta.pdf}}
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\caption{ (left) Relative difference between the reconstructed and the generated mass in Z$\rightarrow e^{+} e^{-}$ events and (right) its bahaviour as a function of $\eta$. \label{fig:zee-relativemassdifference} }
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\end{figure}
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acosta |
1.2 |
%It can be argued that
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Using the corrections present in CMSSW\_1\_0\_5, the invariant mass peak is about 1.4$\%$ off, while the Z invariant mass resolution is about 1.8$\%$,
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meridian |
1.1 |
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