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Comparing UserCode/Vuko/Notes/WZCSA07/Response.tex (file contents):
Revision 1.1 by vuko, Wed Jul 16 08:26:57 2008 UTC vs.
Revision 1.4 by vuko, Wed Jul 16 13:48:18 2008 UTC

# Line 17 | Line 17 | 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 < them to the list of uncertainties affecting the cross section. They are however also relevant for the
21 < expected significance. The estimated significance depends on the number of expected
22 < signal events, which depend on the WZ cross section. Of course the significance we will one day
23 < estimate on real data does not depend on this. The PDF uncertainties on the cross section have been
24 < determined at the PTDR time by varying the PDF within the range allowed by the errors of the PDF
20 > 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   fit (to HERA data).
27  
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 < The response is complex: the signal simulated by Pythia do not include
33 < the gamma* but the k-factor which has been used to go from LO to
34 < NLO as been computed via MC@NLO including gamma* (NLO with gamma*/LO with gamma*).
32 > 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  
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).
# Line 42 | Line 42 | $https://hypernews.cern.ch/HyperNews/CMS
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 < $Zbbar{b}$ m(gamma*)$>$40 GeV. Please see the webpage:
45 > $Zb\bar{b}$ m(gamma*)$>$40 GeV. Please see the webpage:
46   $http://cmsdoc.cern.ch/\sim anikiten/cms\-higgs/sm\_cross\-sections.txt$ 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 < Yes the production has been done within: 40 GeV<M(z/gamma*)<200GeV
50 > Yes the production has been done within: 40 GeV$<$M(z/gamma*)$<$200GeV
51   please see the note:IN 2007/031.
52  
53 < \item \textbf{Can you improve signal over background by adding a cut on MET?}
53 > \item \textbf{Can you improve signal over background by adding a cut on MET?}\\
54   We have studied the possibility but we obtain a better significance by
55   applying a cut on transverse mass of W candidate ($>$50 GeV). In the
56   analysis we are now considering such cuts. The studies of the
57 < different angle proposed have been also performed but the transverse
58 < mass remain the best variable. DO YOU HAVE PLOTS?
57 > different angle proposed have been also performed, see figures~\ref{fig:metcos},
58 > \ref{fig:metsin} and \ref{fig:sig_metcos}, but the transverse
59 > mass remain the best variable.
60  
61 < \item \textbf{Produce Event yield table and mass plot with MET$>$20}
62 < We have update the note but with a transverse mass cut at 50 GeV.
61 > \begin{figure}[!bp]
62 >  \begin{center}
63 >  \scalebox{0.6}{\includegraphics{backupfigs/metcos.eps}}
64 >  \caption{
65 >    Longitudinal component of the MET vector with respect to the direction of the
66 >    lepton associated to the W-decay.
67 >  }
68 >  \label{fig:metcos}
69 >  \end{center}
70 > \end{figure}
71 >
72 > \begin{figure}[p]
73 >  \begin{center}
74 >  \scalebox{0.6}{\includegraphics{backupfigs/metsin.eps}}
75 >  \caption{
76 >    Transverse component of the MET vector with respect to the direction of the
77 >    lepton associated to the W-decay.
78 >  }
79 >  \label{fig:metcos}
80 >
81 >  \scalebox{0.6}{\includegraphics{backupfigs/sig_metsin.eps}}
82 >  \caption{
83 >    Signal significance as a function of a cut on the transverse component of the MET
84 >    vector with respect to the direction of the  lepton associated to the W-decay.
85 >  }
86 >  \label{fig:sig_metsin}
87 >  \end{center}
88 > \end{figure}
89 >
90 >
91 >
92 > \item \textbf{Produce Event yield table and mass plot with MET$>$20}\\
93 > We have updated the note but with a transverse mass cut at 50 GeV.
94  
95   \item \textbf{Redo all plots with 300pb$^{-1}$, produce event yields table with errors}\\
96   Done in the note
# Line 78 | Line 110 | Done please see below [M(W)$>$50 GeV has
110  
111  
112   \item \textbf{Please developp the way systematics will be evaluated}\\
113 < We have added:\\ {\it Trigger}: [...] From the current analysis of
114 < $Z\rightarrow l^+l^-$ in CMS~\ref{Zmumu}~\ref{Zee}, the number of Z
113 > We have added: (Bibliography is done in the note)\\
114 > \begin{itemize}
115 > \item {\it Trigger}: [...] From the current analysis of
116 > $Z\rightarrow l^+l^-$ in CMS~\cite{Zmumu}~\cite{Zee}, the number of Z
117   events is estimated of the order of 50k per 100pb$^{-1}$ of data
118   analysed. To determine the trigger efficiency ``tag-and-probe''
119 < method~\ref{TP} will be used.\\ {\it Reconstruction}: The
119 > method~\cite{TP} will be used.
120 > \item {\it Reconstruction}: The
121   mismeasurement of the charge is of the order of 2\% in CMSSW\_1\_6\_7
122   release for electron. The estimation of the fraction with data will be
123   done by looking at the Z peak without opposite charge
124   requirement. Then number of events within the Z mass windows asking
125   for two leptons of same sign will give us a estimate of the fraction
126 < of mismeasure sign leptons.\\ {\it Lepton identification}:The letpons
126 > of mismeasure sign leptons.
127 > \item {\it Lepton identification}:The leptons
128   scale will be established using the Z mass peak.  
129 <
129 > \item {\it PDF uncertainties}: see response about PDF's above
130 > \end{itemize}
131  
132   \item \textbf{Write a section on the pseudo-experiment and start the plot at 100pb$^-1$}\\
133   To estimate the amount of data necessary to claim an evidence or observation
134   of the WZ signal, we perform 200,000 pseudoexperiements for data for a given
135   value of data that is varied from 40 to 500 pb$^{-1}$. For each pseudoexperiment
136 < we use Poission statistics to estimate the expected number of events for
136 > we use Poisson statistics to estimate the expected number of events for
137   signal and for each background sources separately, for each signature channel.
138   The mean of the expected number of events is varied using Gaussian statistic
139   using systematic uncertainties given in Table~\ref{tab:FullSys}.  The significance of the
# Line 109 | Line 146 | where $N_S$ and $N_B$ are the expected n
146   events observed in the four signatures of the analysis, respectively. By summing
147   signal and background together, we assume no correlation between the signature
148   channels, which result in a conservative estimation of the sensitivity reach.
149 < Obtained $S_L$ distribution is fit with Gaussian function to obtain the mean
149 > The obtained $S_L$ distribution is fitted with Gaussian function to obtain the mean
150   and resolution width, which would correspond to the most probable value of $S_L$
151   and its uncertainty for a given value of integrated luminosity. The 68\% and 95\%
152   CL bands are $\pm 1\sigma$ and $\pm 1.96\sigma$ bands around the mean value

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