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Revision: 1.13
Committed: Mon Jul 14 17:32:45 2008 UTC (16 years, 9 months ago) by ymaravin
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Log Message:
Modifications from Yurii include WTM/MET studies
and new plots with 300 pb^{-1} together with modified
text on k-factor treatment.

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# Content
1
2 In this section, we estimate systematics uncertainties of the methods
3 used in this analysis. We follow the rule of making conservative estimates
4 throughout this section.
5
6 \subsection{Modeling systematics}
7
8
9 The sources of systematic uncertainties due to modeling of trigger,
10 reconstruction, PDF, and luminosity are described below
11
12 \begin{itemize}
13 \item {\it Trigger}: the trigger path used to select four categories
14 require leptons to be isolated. Though, the isolation criteria
15 depends on the occupancy of the sub-detectors, the alignment of the
16 tracker (when considering tracker isolation variables), and noise in
17 the calorimeters (when considering a calorimetric isolation), the
18 trigger efficiency is expected to be around 99\%, and therefore, a
19 systematic uncertainty is conservatively estimated as 1\%. From the
20 current analysis of $Z\rightarrow l^+l^-$ in
21 CMS~\ref{Zmumu}~\ref{Zee}, the number of \Z events is estimated of the
22 order of 50k per 100pb$^{-1}$ of data analysed. To determine the
23 trigger efficiency ``tag-and-probe'' method~\ref{TP} will be used.
24
25 \item {\it Reconstruction}: we assign 2\% systematic uncertainty per
26 lepton due to initial tracker alignment which is of paramount
27 importance to reconstruct leptons, 2\% and 1\% is assigned for the
28 determination of the charge of the electron and muon candidates,
29 respectively. We assigned a larger electron charge identification
30 uncertainty due to much stronger Bremsstrahlung energy loss which
31 makes the charge identification more difficult. The mismeasurement of
32 the charge is of the order of 2\% in CMSSW\_1\_6\_7 release for
33 electron. The estimation of the fraction with data will be done by
34 looking at the \Z peak without opposite charge requirement. Then
35 number of events within the \Z mass windows asking for two leptons of
36 same sign will give us a estimate of the fraction of mismeasure sign
37 leptons.
38
39 \item {\it Lepton identification}: we assign 4\% of systematic
40 uncertainty due to efficiency measurement from early data using
41 ``tag-and-probe'' method and 2\% for that for a muon. Additionally we
42 assign a systematic uncertainty on lepton energy scale of 2\% per
43 lepton. The letpons scale will be established using the \Z mass peak.
44
45 \item {\it PDF uncertainties}: we estimate PDF uncertainties following prescription
46 described in~\cite{OldNote}. The uncertainty is found to be
47 $$ \Delta \sigma_+ ^{tot} = 3.9\% \hspace{0.9cm} \Delta \sigma_- ^{tot} = 3.5\% $$.
48
49 \item {\it Luminosity}: we estimate luminosity uncertainty of 10\%.
50 \end{itemize}
51
52 The systematic uncertainties are summarized in Table~\ref{tab:sys}.
53
54 \begin{table}[!tb]
55 \begin{center}
56 \begin{tabular}{|l|c|c|} \hline
57 & \multicolumn{2}{c|}{Systematic uncertainty} \\
58 Source & on the cross section,\% & on the signficance,\% \\ \hline
59 Luminosity & 10.0 & - \\
60 Trigger & 1.0 & 1.0\\
61 Lepton reconstruction & 2.0 & 2.0\\
62 Electron charge determination &2.0& 2.0\\
63 Muon charge determination &1.0& 1.0\\
64 Lepton energy scale& 1.0& 1.0\\
65 Electron identification& 4.0 &4.0\\
66 Muon identification& 2.0 &2.0\\
67 PDF uncertainties& - & + 3.9\\
68 & & - 3.5 \\ \hline
69 \end{tabular}
70
71 \end{center}
72 \caption{Systematic uncertainties for $pp\rightarrow \WZ$ cross section measurement
73 and significance estimation for 300 \invpb of integrated luminosity.}
74 \label{tab:sys}
75 \end{table}
76
77
78 \subsection{Systematic uncertainties due to background estimation method}
79
80 In the following we estimate a systematic uncertainty due to estimation
81 of background using the matrix method described in Section~\ref{sec:D0Matrix} above.
82
83
84
85 We present here, the result for the case where the $W$ is decaying via
86 an electron.
87
88 Two steps will be used to substract the different background: first,
89 the non peaking background should be substracted, then the background
90 $Z+jets$ will be determine using the method described
91 in~\ref{sec:D0Matrix}.
92
93 From the fit, we will consider a systematics error of 10\%.
94
95 If we consider an error of 10\%
96 on the fake rate and an error of 2\%
97 on the efficiency on signal to go from loose to tight criteria, we can
98 calculate the error on the estimated background as follow:
99 \begin{equation}
100 \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
101 +\left(\frac{\epsilon\left(\epsilon N_{l}-N_{t}\right)}{\left(\epsilon -p\right)^2}\right)^2 \times \Delta p^2
102 + \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}}
103 \end{equation}
104 where $N_{t}$,$\Delta N_{t}$ and $N_{l}$,$\Delta N_{l}$ represents
105 respectivement the number of events in the tight sample and in the
106 loose sample and their errors.$\epsilon$ represent efficiency for a
107 loose electron to pass the tight criteria, $\Delta \epsilon$ the error
108 on this value.$p$ gives the probability for a fake loose electron to
109 pass also the tight criteria and $\Delta p$ its error.
110
111 The overall error from the background substraction is XXX %18\%.
112
113 \subsection{Summary of Systematics}
114
115 In table~\ref{tab:FullSys}, the systematics errors are expressed for
116 each channels.
117
118 \begin{table}[!tb]
119 \begin{center}
120 \begin{tabular}{|l|c|c|} \hline
121 Channels & Cross Section & Signficance \\ \hline
122 3e & 8.4\% +10\% = 13.1\% & +9.3\% / - 9.2\% \\
123 2e1$\mu$ & 7.7\% +10\% = 12.6\% & +8.7\% / - 8.5\% \\
124 1e2$\mu$ & 6.5\% +10\% = 11.9\% & +7.6\% / - 7.4\% \\
125 3$\mu$ & 5.5\% +10\% = 11.4\% & +6.7\% / - 6.5\% \\\hline
126 \end{tabular}
127
128 \end{center}
129 \caption{Systematics per channels in percent for $pp\rightarrow WZ$ cross section measurement and significance estimation for 300 \invpb of integrated luminosity. These systematics do not include the background substraction.}
130 \label{tab:FullSys}
131 \end{table}
132