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appendix B

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# User Rev Content
1 claudioc 1.1 \section{Example BG prediction calculation}
2     \label{BGexample}
3    
4     The calculation of the background prediction is a bit complicated.
5     Here we walk the reader through a concrete example.
6    
7     {\bf NB: the numbers
8     in this section corresponded to the numbers in V2 of the analysis note.
9     They will not be updated, because this is meant as an illustration only.}.
10    
11     The main background is $t\bar{t}$
12     The main idea is to normalize to the $M_T$ peak region ($50 < M_T < 80$ GeV).
13     This eliminates dependence on \ttbar\ cross-section, luminosity,
14     trigger efficiency, JES, lepton ID, etc. This gets a bit complicated because
15     the $M_T$ peak region, while dominantly \ttbar\ lepton $+$ jets,
16     also includes some \wjets, \ttdl, rare processes, etc. Also, we want
17     to minimize our need to understand the effect of the isolated
18     track veto on \ttsl. As a result we actually define two $M_T$ peak
19     regions: one before and one after applying the isolated track veto.
20     Then the \ttdl\ background is normalized the the ``before veto'' region,
21     and the \ttsl\ and \wjets\ background are normalized to the ``post veto''
22     region.
23    
24     This complex procedure is important for the high statistics signal regions
25     with relatively low \met\ requirements, eg, SRA. For these SRs we want to keep the
26     systematics low in order to be sensistive to low mass stop; for the signal regions
27     with hard cuts on \met\, this is less important. However, we apply the same
28     procedure to all SRs.
29    
30     For concreteness, we show the calculation for SRA, electron channel. The MC and data
31     event counts used in the background calculation are collected in Table~\ref{tab:bgexample}.
32     Note that the background uncertainties have already been described
33     in Section~\ref{sec:systematics}. The one tricky point to keep in mind is that
34     when the \wjets\ and rare cross-sections are changed by their assumed uncertainties
35     (50\% each), the whole calculation describe below is repeated in order to take care
36     of all the correlations properly.
37    
38    
39     \begin{table}[!h]
40     \begin{center}
41     \begin{tabular}{l||c|c|c|}
42     \hline
43     Sample & $M_T$ peak, before trk veto & $M_T$ peak, after trk veto & Signal Region A \\
44     \hline
45     \ttdl\ & $290 \pm 6$ & $116 \pm 4$ & $261 \pm 6$ \\
46     \ttsl\ (1\Lep) & $2899 \pm 19$ & $2595 \pm 18$ & not used \\
47     \wjets\ & $252 \pm 28$ & $236 \pm 28$ & not used \\
48     Rare & $89 \pm 5$ & $62 \pm 4$ & $26 \pm 2$ \\
49     \hline
50     Total & $3530 \pm 35$ & $3009 \pm 34$ & not used \\
51     \hline
52     Data & 3358 & 2787 & not used \\
53     \hline
54     \end{tabular}
55     \caption{ Data and MC event counts used to predict the background in SRA, for electron events.
56     Uncertainties are statistical only. The trigger efficiency has been applied to the MC samples. In the
57     case of \ttdl\, the $K_3$ and $K_4$ factors of Section~\ref{sec:jetmultiplicity} have also been applied.
58     \label{tab:bgexample}}
59     \end{center}
60     \end{table}
61    
62    
63     \subsection{Central value of dilepton background}
64     A ``before veto'' scale factor is defined from the second column in Table~\ref{tab:bgexample} as the factor by which
65     all MC except the ``rare'' need to be scaled up in order to have data/MC agreement. This is
66    
67     \noindent $SF_{pre} = (3358 - 89)/(2899 + 252 + 290) = 0.950$.
68    
69     Then the \ttdl\ background prediction is the number of events predicted by the MC in SRA (261 from the
70     last column of SRA), rescaled by $SF_{pre}$. The result for the central value is 248 events.
71    
72     \subsection{Central value of the \ttsl\ background}
73     \label{sec:cenvttlj}
74     A ``post veto'' scale factor is defined from the third column in Table~\ref{tab:bgexample} as the factor by which
75     the \ttsl\ and the \wjets\ backgrounds need to be scaled to have data/MC agreement.
76    
77     \noindent $SF_{post} = (2787 - 62 - SF_{pre} \cdot 116) / (2595 + 236) = 0.924$.
78    
79     Then the \ttsl\ background is obtained as the product of the following four factors
80    
81     \begin{itemize}
82     \item $SF_{post} = 0.924$ as obtained above
83     \item 2595, from the third column of Table~\ref{tab:bgexample}
84     \item The tail-to-peak ratio $R_{top} = 0.015$ from Table~\ref{tab:ttp} (we use the average of electrons
85     and muons)
86     \item The tail-to-peak ratio scale factod $SFR_{top} = 1.89 \pm 0.56$ from Table~\ref{tab:cr2yields}.
87     \end{itemize}
88    
89     The result for the central value is 68 events.
90    
91     \subsection{Central value for the \wjets\ background}
92    
93     It is calculated as the product of
94     \begin{itemize}
95     \item $SF_{post} = 0.924$ from Section~\ref{sec:cenvttlj}
96     \item 236, from the third column of Table~\ref{tab:bgexample}
97     \item The tail-to-peak ratio $R_{wjet} = 0.04$ from Table~\ref{tab:ttp} (we use the average of electrons and muons)
98     \item The tail-to-peak ratio scale factod $SFR_{wjet} = 1.64 \pm 0.38$ from Table~\ref{tab:cr1yields}.
99     \end{itemize}
100    
101     The result for the central value is 14.3 events.
102    
103     \subsection{Central value for the rare backgrounds}
104    
105     This is 26 events from Table~\ref{tab:bgexample}
106