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Revision: 1.3
Committed: Wed Jul 16 09:10:06 2008 UTC (16 years, 9 months ago) by beaucero
Content type: application/x-tex
Branch: MAIN
Changes since 1.2: +8 -8 lines
Log Message:
Steph Updates

File Contents

# User Rev Content
1 vuko 1.1 \documentclass[12pt,a4paper]{report}
2     \usepackage{graphicx}
3     \usepackage{textcomp}
4     \usepackage{amsmath,amssymb}
5     \usepackage{color,multirow,rotating}
6    
7     \begin{document}
8    
9     \begin{itemize}
10     \item \textbf{Do you understand the factor 2 increase in background Z+jets in 2e1mu channel compare to 3mu channel?}\\
11     We are trying to fully understand the behaviour (trying to obtain an
12     event display but as we have to dig the chowder soup [26 Millions of
13     events] this can take time), but by asking that the 3 letpons are
14     isolated to each others solve the issue. The fake muon is indeed
15     within DeltaR of 0.1 around one of the two electrons making the Z at
16     generator level.
17    
18     \item \textbf{Why the PDF systematics are only considered for significance (should be the opposite)?}\\
19     The PDF systematics should indeed also be considered for the cross section measurement and we added
20 vuko 1.2 them to the list of uncertainties affecting the cross section. It affects it through the signal acceptance
21     which may vary for different PDF assumptions. PDF uncertainties are not relevant for the signal significance
22     we will quote one day on real data, but they are however relevant for the expected significance we quote
23     in this analysis. The estimated significance depends on the number of expected
24     signal events, which depend on the WZ cross section. The PDF uncertainties on the cross section have
25     been determined at the PTDR time by varying the PDF within the range allowed by the errors of the PDF
26 vuko 1.1 fit (to HERA data).
27    
28     \item \textbf{What are the PDF systematics for ZZ background? [mainly for 3mu channel]}\\
29     We are using the systematics derived in note AN-2006/055 which are 6.4\%.
30    
31     \item \textbf{Does the cross section used for signal include the gamma*?}\\
32 vuko 1.2 The response is complex: the signal simulated by Pythia does not include
33     the $\gamma^*$ but the k-factor which has been used to go from LO to
34     NLO has been computed via MCFM including $\gamma^*$ (NLO with $\gamma^*$ / LO with $\gamma^*$).
35 vuko 1.1
36     \item \textbf{Does reconstruction efficiency (Z) depend on pt(Z) ?}\\
37     Indeed a bit, so we have applied a k-factor dependant on pt(Z).
38    
39     \item \textbf{Are you sure to not have a double counting between $Zb\bar{b}$ background and $Z+jets$?}\\
40     Yes, please see the hypernews message:\\
41     $https://hypernews.cern.ch/HyperNews/CMS/get/alpgen/83/1.html$
42    
43     \item \textbf{Can you confirm that gamma* is included in Zbb and ZZ Monte Carlo and that cross section are correctly calculated?}\\
44     For $ZZ$, the production as been done with a m(gamma*) $>$ 12 GeV and for
45 beaucero 1.3 $Zb\bar{b}$ m(gamma*)$>$40 GeV. Please see the webpage:
46 vuko 1.1 $http://cmsdoc.cern.ch/\sim anikiten/cms\-higgs/sm\_cross\-sections.txt$ for
47     $ZZ$ and the CMSNote AN 2008/020 for $Zb\bar{b}$ background.
48    
49     \item \textbf{Can you confirm that gamma* is included in $Z+jets$ samples?}\\
50 beaucero 1.3 Yes the production has been done within: 40 GeV$<$M(z/gamma*)$<$200GeV
51 vuko 1.1 please see the note:IN 2007/031.
52    
53 beaucero 1.3 \item \textbf{Can you improve signal over background by adding a cut on MET?}\\
54 vuko 1.1 We have studied the possibility but we obtain a better significance by
55     applying a cut on transverse mass of W candidate ($>$50 GeV). In the
56     analysis we are now considering such cuts. The studies of the
57     different angle proposed have been also performed but the transverse
58     mass remain the best variable. DO YOU HAVE PLOTS?
59    
60 beaucero 1.3 \item \textbf{Produce Event yield table and mass plot with MET$>$20}\\
61 vuko 1.2 We have updated the note but with a transverse mass cut at 50 GeV.
62 vuko 1.1
63     \item \textbf{Redo all plots with 300pb$^{-1}$, produce event yields table with errors}\\
64     Done in the note
65    
66     \item \textbf{Please check the quality of the fit of figure 11?}\\
67     Done please see below [M(W)$>$50 GeV has been applied]
68     \begin{figure}[!bp]
69     \begin{center}
70     \scalebox{0.4}{\includegraphics{FitTight3eErrors.eps}}
71     \caption{The invariant mass distribution of the $Z$ boson candidate that is fitted to a signal
72     parameterized as a Gaussian function convoluted with a Breit-Wigner function and
73     a background, parameterized as a straight line.}
74     \label{fig:ZFit}
75     \end{center}
76     \end{figure}
77    
78    
79    
80     \item \textbf{Please developp the way systematics will be evaluated}\\
81 beaucero 1.3 We have added: (Bibliography is done in the note)\\
82 vuko 1.2 \begin{itemize}
83     \item {\it Trigger}: [...] From the current analysis of
84 beaucero 1.3 $Z\rightarrow l^+l^-$ in CMS~\cite{Zmumu}~\cite{Zee}, the number of Z
85 vuko 1.1 events is estimated of the order of 50k per 100pb$^{-1}$ of data
86     analysed. To determine the trigger efficiency ``tag-and-probe''
87 beaucero 1.3 method~\cite{TP} will be used.
88 vuko 1.2 \item {\it Reconstruction}: The
89 vuko 1.1 mismeasurement of the charge is of the order of 2\% in CMSSW\_1\_6\_7
90     release for electron. The estimation of the fraction with data will be
91     done by looking at the Z peak without opposite charge
92     requirement. Then number of events within the Z mass windows asking
93     for two leptons of same sign will give us a estimate of the fraction
94 vuko 1.2 of mismeasure sign leptons.
95 beaucero 1.3 \item {\it Lepton identification}:The leptons
96 vuko 1.1 scale will be established using the Z mass peak.
97 vuko 1.2 \item {\it PDF uncertainties}: see response about PDF's above
98     \end{itemize}
99 vuko 1.1
100     \item \textbf{Write a section on the pseudo-experiment and start the plot at 100pb$^-1$}\\
101     To estimate the amount of data necessary to claim an evidence or observation
102     of the WZ signal, we perform 200,000 pseudoexperiements for data for a given
103     value of data that is varied from 40 to 500 pb$^{-1}$. For each pseudoexperiment
104 vuko 1.2 we use Poisson statistics to estimate the expected number of events for
105 vuko 1.1 signal and for each background sources separately, for each signature channel.
106     The mean of the expected number of events is varied using Gaussian statistic
107     using systematic uncertainties given in Table~\ref{tab:FullSys}. The significance of the
108     signal in each pseudo-experiment is calculated using the likelihood ratio
109     \begin{equation}
110     \label{eq:sl}
111     S_L=\sqrt{2\ln Q},\ Q=\biggl( 1+\frac{N_S}{N_B}\biggr)^{N_S+N_B}e^{-N_S},
112     \end{equation}
113     where $N_S$ and $N_B$ are the expected number of signal and background
114     events observed in the four signatures of the analysis, respectively. By summing
115     signal and background together, we assume no correlation between the signature
116     channels, which result in a conservative estimation of the sensitivity reach.
117 vuko 1.2 The obtained $S_L$ distribution is fitted with Gaussian function to obtain the mean
118 vuko 1.1 and resolution width, which would correspond to the most probable value of $S_L$
119     and its uncertainty for a given value of integrated luminosity. The 68\% and 95\%
120     CL bands are $\pm 1\sigma$ and $\pm 1.96\sigma$ bands around the mean value
121     of the $S_L$ respectively. To estimate the effect of the systematic uncertainty in
122     this estimation, we double all the systematic uncertainties and re-calculate the
123     68\% and 95\% CL bands. The results for the sensitivity of the analysis without
124     requirements on the $W$ boson transverse mass are given in Fig.~\ref{fig:sl_full}.
125     5$\sigma$ significance of the WZ signal can be established with data size between
126     50 and 300 pb$^{-1}$ of integrated luminosity at 95\% CL.
127    
128     \end{itemize}
129    
130     \end{document}