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1 < In this section, we will assign systematics errors to this
2 < analysis. The assignement of systematics is expected to be
3 < conservatives.
4 <
5 < \subsection{Experimental Systematics}
6 <
7 < The experimental systematics errors expected that will affect the
8 < signal and standard model background are:
1 > In this section, we estimate systematics uncertainties of the methods
2 > used in this analysis. We follow the rule of making conservative estimates
3 > throughout this section.
4 >
5 > \subsection{Modeling systematics}
6 >
7 > The sources of systematic uncertainties due to modeling of trigger,
8 > reconstruction, PDF, and luminosity are described below
9 >
10   \begin{itemize}
11 < \item For trigger selection, a systematics of 1\% is assigned. Even
12 < though the efficiency of the signal is greater than 99\%, the trigger
13 < path used for both muons and electron expect the leptons to be
14 < isolated. As the isolation depends on the occupancy of the events,
15 < the alignment of the tracker (when considering tracker isolation
16 < variables) and noise in the calorimeters (when considering a
17 < calorimetric isolation), this value is expected to be conservative.
18 <
19 < \item 3\% error is assigned on electron/muons reconstruction. Both of
20 < them are link to alignment of the track in order to reconstruct the
21 < leptons. A systematics of 2\% is assigned for the determination of
22 < the charge of the electron candidate while 1\% for the muon as the
23 < electron problem is coming from the high probability of emission of
24 < photons.
25 <
26 < \item A systematics of 1\% will be assigned for the measurement of
27 < the lepton energy.
11 > \item {\it Trigger}: the trigger path used to select four categories require
12 > leptons to be isolated. Though, the isolation criteria depends on the
13 > occupancy of the sub-detectors, the alignment of the tracker (when
14 > considering tracker isolation variables), and noise in the calorimeters (when
15 > considering a calorimetric isolation), the trigger efficiency is
16 > expected to be around 99\%, and therefore, a systematic uncertainty
17 > is conservatively estimated as 1\%.
18 >
19 > \item {\it Reconstruction}: we assign 2\% systematic uncertainty per lepton
20 > due to initial tracker alignment which is of paramount importance to
21 > reconstruct leptons, 2\% and 1\% is assigned for the determination
22 > of the charge of the electron and muon candidates, respectively. We assigned
23 > a larger electron charge identification uncertainty due to much stronger
24 > Bremsstrahlung energy loss which makes the charge identification more
25 > difficult.
26 >  
27 > \item {\it Lepton identification}: we assign 4\% of systematic uncertainty
28 > due to efficiency measurement from early data using ``tag-and-probe''
29 > method and 2\% for that for a muon. Additionally we assign a systematic
30 > uncertainty on lepton energy scale of 2\% per lepton.
31 >
32 > \item {\it PDF uncertainties}: we estimate PDF uncertainties following prescription
33 > described in~\cite{OldNote}. The uncertainty is found to be
34 > $$ \Delta \sigma_+ ^{tot} = 3.9\% \hspace{0.9cm} \Delta \sigma_- ^{tot} = 3.5\% $$.
35  
36 < \item 4\% of systematics are considered for the electron
29 < identification, 2\% for the muon case.
36 > \item {\it Luminosity}: we estimate luminosity uncertainty of 10\%.
37   \end{itemize}
38  
39 < The PDF uncertainties on the signal has been determined in~\cite{OldNote}.
33 < The uncertainty was found to be:
34 < \begin{equation}
35 < \Delta \sigma_+ ^{tot} = 3.9\% \hspace{0.9cm} \Delta \sigma_- ^{tot} = 3.5\%
36 < \end{equation}
39 > The systematic uncertainties are summarized in Table~\ref{tab:sys}.
40  
41 < The luminosity error is expected to be 10\%.
39 <
40 < The table~\ref{tab:sys} resume all systematics considered.
41 <
42 < \begin{table}[!]
41 > \begin{table}[!tb]
42   \begin{center}
43   \begin{tabular}{|l|c|c|} \hline
44 < Systematics Source (in \%)   &   Cross Section     & Signficance \\ \hline
44 >                &   \multicolumn{2}{c|}{Systematic uncertainty} \\
45 > Source   &   on the cross section,\%     &  on the signficance,\% \\ \hline
46   Luminosity  &   10.0   &  -         \\
47   Trigger & 1.0 & 1.0\\
48 < Lepton Reconstruction & 3.0 & 3.0\\
49 < Electron Charge Determination &2.0& 2.0\\
50 < Muon Charge Determination &1.0& 1.0\\
51 < Lepton Energy Scale& 1.0& 1.0\\
52 < Electron Identification& 4.0 &4.0\\
53 < Muon Identification& 2.0 &2.0\\
54 < PDF Uncertainties& - & + 3.9\\
48 > Lepton reconstruction & 2.0 & 2.0\\
49 > Electron charge determination &2.0& 2.0\\
50 > Muon charge determination &1.0& 1.0\\
51 > Lepton energy scale& 1.0& 1.0\\
52 > Electron identification& 4.0 &4.0\\
53 > Muon identification& 2.0 &2.0\\
54 > PDF uncertainties& - & + 3.9\\
55   &  & - 3.5 \\ \hline
56   \end{tabular}
57  
58   \end{center}
59 < \caption{Systematics in percent for $pp\rightarrow WZ$ cross section measurement and significance estimation for 1 fb$^-1$ of integrated luminosity.}
59 > \caption{Systematic uncertainties for $pp\rightarrow \WZ$ cross section measurement
60 > and significance estimation for 1 fb$^-1$ of integrated luminosity.}
61   \label{tab:sys}
62   \end{table}
63  
64  
65 < \subsection{Background Substraction Systematics}
65 > \subsection{Systematic uncertainties due to background estimation method}
66 >
67 > In the following we estimate a systematic uncertainty due to estimation
68 > of background using the matrix method described in Section~\ref{sec:D0Matrix} above.
69 >
70  
66 Two methods will be used to substract the different background. The
67 main background is the production $Z+jets$. Such background can be
68 estimated using data as presented in section~\ref{sec:SignalExt}. For
69 the $t\bar{t}$ background, we can use safely the side band around the
70 $Z$ mass in order to evaluate it.
71  
72 < If we consider an error of xx\% on the fake rate and an error of xx\%
72 > We present here, the result for the case where the $W$ is decaying via
73 > an electron.
74 >
75 > Two steps will be used to substract the different background: first,
76 > the non peaking background should be substracted, then the background
77 > $Z+jets$ will be determine using the method described
78 > in~\ref{sec:D0Matrix}.
79 >
80 > From the fit, we will consider a systematics error of 10\%.
81 >
82 > If we consider an error of 10\%
83 > on the fake rate and an error of 2\%
84   on the efficiency on signal to go from loose to tight criteria, we can
85   calculate the error on the estimated background as follow:
86   \begin{equation}
87 < \Delta N_j ^{t} = \frac{\sqrt{(p[N_{t} - p(N_{l}+N_{t})])^2 \times \Delta \epsilon^2
88 < +(\epsilon[\epsilon(N_{l}+N_{t})-N_{t}]^2 \times \Delta p^2
89 < + (p\epsilon)^2 \times N_{l} + [p(\epsilon -1 )]^2 \times N_{t}}}{\epsilon_{t} - p}
79 < %\Delta N_j ^{tight} = \frac{\sqrt{(p_{fake}[N_{tight} - p_{fake}(N_{loose}+N_{tight})])^2 \dot \Delta \epsilon^2
80 < %+(\epsilon[\epsilon(N_{loose}+N_{tight})-N_{tight}]^2 \dot \Delta p_{fake}^2
81 < %+ (p_{fake}\epsilon)^2 \dot N_{loose} + [p_{fake}(\epsilon -1 )]^2 \dot N_{tight}}}{\epsilon_{tight} - p_{fake}}
87 > \Delta N_j ^{t} = \sqrt{\left(\frac{p\left(N_t - pN_l\right)}{\left(\epsilon -p\right)^2}\right)^2 \times \Delta \epsilon^2
88 > +\left(\frac{\epsilon\left(\epsilon N_{l}-N_{t}\right)}{\left(\epsilon -p\right)^2}\right)^2 \times \Delta p^2
89 > + \frac{p^2\left(\epsilon^2\Delta N_{l}^2 -  \Delta N_{t}^2\left(2\epsilon -1\right)\right)}{\left(\epsilon -p\right)^2}}
90   \end{equation}
91 < where $N_{t}$ and $N_{l}$ represents respectivement the number of
92 < events in the tight sample and in the loose sample and if they are
93 < greater than 25.$\epsilon$ represent efficiency for a loose electron
94 < to pass the tight criteria, $\Delta \epsilon$ the error on this
95 < value.$p$ gives the probability for a fake loose electron to pass also
96 < the tight criteria and $\Delta p$ its error.
91 > where $N_{t}$,$\Delta N_{t}$ and $N_{l}$,$\Delta N_{l}$ represents
92 > respectivement the number of events in the tight sample and in the
93 > loose sample and their errors.$\epsilon$ represent efficiency for a
94 > loose electron to pass the tight criteria, $\Delta \epsilon$ the error
95 > on this value.$p$ gives the probability for a fake loose electron to
96 > pass also the tight criteria and $\Delta p$ its error.
97  
98 + The overall error from the background substraction is XXX %18\%.
99  
100 + \subsection{Summary of Systematics}
101  
102 < An example of the method is given on figure~\ref{fig:Fitbkg}. The
103 < number of estimated background compare to the true value is shown on
94 < table~\ref{tab:FitbkgSub}.
102 > In table~\ref{tab:FullSys}, the systematics errors are expressed for
103 > each channels.
104  
105 < We assign a systematics error of 20\%.
105 > \begin{table}[!tb]
106 > \begin{center}
107 > \begin{tabular}{|l|c|c|} \hline
108 > Channels   &   Cross Section     & Signficance \\ \hline
109 > 3e  &  8.4\% +10\% = 13.1\%  &  +9.3\% / - 9.2\%         \\
110 > 2e1$\mu$  & 7.7\% +10\% = 12.6\%  &  +8.7\% / - 8.5\%         \\
111 > 1e2$\mu$  &  6.5\% +10\% = 11.9\%  &  +7.6\% / - 7.4\%         \\
112 > 3$\mu$  &  5.5\% +10\% = 11.4\%  &  +6.7\% / - 6.5\%         \\\hline
113 > \end{tabular}
114  
115 + \end{center}
116 + \caption{Systematics per channels in percent for $pp\rightarrow WZ$ cross section measurement and significance estimation for 1 fb$^-1$ of integrated luminosity. These systematics do not include the background substraction.}
117 + \label{tab:FullSys}
118 + \end{table}
119  

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