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Revision: 1.3
Committed: Sun Jan 28 19:14:17 2007 UTC (18 years, 3 months ago) by acosta
Content type: application/x-tex
Branch: MAIN
CVS Tags: HEAD
Changes since 1.2: +42 -11 lines
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major edits from DA

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# User Rev Content
1 meridian 1.1 \subsubsection{Reconstruction of Z$\rightarrow e^+e^-$ events}
2    
3 acosta 1.3 This exercise has multiple goals: one is the selection of
4     Z$\rightarrow e^{+} e^{-}$ out of the ``Electroweak Soup'' (EWK) and their
5     use to evaluate the performance of the electron reconstruction;
6     and another one is the demonstration of the workflow for running offline
7     ECAL calibration at a remote Tier-2 centre, starting from an AlcaReco
8     stream produced at the Tier-1 centre.
9 meridian 1.1
10     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.
11 acosta 1.3 The events are selected on the basis of Monte Carlo generator
12     information, requiring only Drell-Yan $e^+e^-$ events in a mass
13     range from 50 to 130 GeV/c$^2$. The electrons are also required to
14     have $p_T$ greater than 5 GeV/c and $|\eta|<2.7$.
15     This selection has an efficiency over the Electroweak Soup of 3.7$\%$.
16    
17     Skim jobs were processed at the CNAF Tier-1, starting from less than 3
18     million EWK soup events (not the full EWK dataset have been processed
19     using the CMSSW\_1\_0\_5 release). Out of these events, a sample of
20     76494 events have been selected and the two created streams were
21     transferred to the Rome Tier-2. The total amount of data amounts to
22     about 33.5GB, of which around 500MB are occupied by the AlcaReco
23     electron stream.
24 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.
25 meridian 1.1
26 acosta 1.3 The main purpose is to validate the electron reconstruction, evaluating the electron reconstruction performance.
27 meridian 1.1 The electron reconstruction efficiency both versus $p_T$ and $\eta$ is shown in Fig.~\ref{fig:zee-eleeff}.
28    
29     \begin{figure}[!hbtp]
30     \centering
31     {\includegraphics[width=0.49\textwidth]{figs/zee-eleeffpt.pdf}}
32     {\includegraphics[width=0.49\textwidth]{figs/zee-eleeffeta.pdf}}
33     \caption{ (left) Electron reconstruction efficiency as a function of $p_T$ and (right) $\eta$.\label{fig:zee-eleeff} }
34    
35     \end{figure}
36    
37 acosta 1.3 The two main ingredients for the electron reconstruction, the
38     supercluster and the electron track, are then evaluated separately.
39     The ratio of reconstructed supercluster energy over the true energy as
40     a function of $\eta$ is visible in Fig.~\ref{fig:zee-erecetrue},
41     showing a well-known problem in the CMSSW\_1\_0\_5 release for what
42     concerns the endcap supercluster reconstruction. The projected
43     distribution for the barrel is presented in the right plot of
44     Fig.~\ref{fig:zee-erecetrue}.
45 meridian 1.1
46     \begin{figure}[!hbtp]
47     \centering
48     {\includegraphics[width=0.49\textwidth]{figs/zee-erecetrueeta.pdf}}
49     {\includegraphics[width=0.49\textwidth]{figs/zee-erecetruebarrel.pdf}}
50     \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} }
51    
52     \end{figure}
53    
54     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}.
55    
56     \begin{figure}[!hbtp]
57     \centering
58     {\includegraphics[width=0.49\textwidth]{figs/zee-eoverpvertex.pdf}}
59     {\includegraphics[width=0.49\textwidth]{figs/zee-eoverpoutermost.pdf}}
60     \caption{Distribution of the E/p variable using track parameters at the (left) vertex (right) outermost state. \label{fig:zee-eoverp} }
61    
62     \end{figure}
63    
64 acosta 1.3 At the time of the CMSSW\_1\_0\_5, the reconstructed electron track
65     was not the track after the smoothing step, and for this reason the
66     quality of the E/p distribution with the track parameters at the
67     vertex is rather poor. A refitting of the electron track has been
68     tried in the offline analysis, improving the quality of the E/p
69     matching, as it visible in Fig.~\ref{fig:zee-refittedeoverp}.
70 meridian 1.1
71     \begin{figure}[htbp]
72     \centering
73     \includegraphics[width=0.6\textwidth]{figs/zee-refittedeoverp.pdf}
74     \caption{Distribution of the E/p variable using refitted track parameters at the vertex. \label{fig:zee-refittedeoverp} }
75    
76     \end{figure}
77    
78 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}.
79 meridian 1.1 \begin{figure}[h]
80     \centering
81     \includegraphics[width=0.6\textwidth]{figs/zee-invariantmass.pdf}
82     \caption{Electron pair invariant mass in Z$\rightarrow e^{+} e^{-}$ events. \label{fig:zee-invariantmass}}
83    
84     \end{figure}
85    
86 acosta 1.3 The distribution of the difference between the reconstructed mass and
87     the generated mass is shown in
88     Fig.~\ref{fig:zee-relativemassdifference}, where the right plot
89     displays the difference as a fuction of $\eta$. The distribution shows
90     the expected
91     behaviour due to the effect of the increasing tracker material towards
92     $\eta$ over the electron reconstruction.
93 meridian 1.1
94     \begin{figure}[!hbtp]
95     \centering
96     {\includegraphics[width=0.49\textwidth]{figs/zee-relativemassdifference.pdf}}
97     {\includegraphics[width=0.49\textwidth]{figs/zee-relativemassdifferenceeta.pdf}}
98     \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} }
99    
100     \end{figure}
101    
102 acosta 1.2 %It can be argued that
103     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$\%$,
104 meridian 1.1
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