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claudioc |
1.1 |
\section{Data Driven Background Estimation Methods}
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\label{sec:datadriven}
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We have developed two data-driven methods to
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estimate the background in the signal region.
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benhoob |
1.10 |
The first one exploits the fact that
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benhoob |
1.22 |
SumJetPt and \met$/\sqrt{\rm SumJetPt}$ are nearly
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claudioc |
1.1 |
uncorrelated for the $t\bar{t}$ background
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(Section~\ref{sec:abcd}); the second one
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is based on the fact that in $t\bar{t}$ the
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$P_T$ of the dilepton pair is on average
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nearly the same as the $P_T$ of the pair of neutrinos
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from $W$-decays, which is reconstructed as \met in the
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detector.
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benhoob |
1.15 |
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claudioc |
1.6 |
%{\color{red} I took these
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%numbers from the twiki, rescaling from 11.06 to 30/pb.
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%They seem too large...are they really right?}
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claudioc |
1.1 |
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\subsection{ABCD method}
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\label{sec:abcd}
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benhoob |
1.22 |
We find that in $t\bar{t}$ events SumJetPt and
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benhoob |
1.16 |
\met$/\sqrt{\rm SumJetPt}$ are nearly uncorrelated,
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benhoob |
1.31 |
as demonstrated in Fig.~\ref{fig:uncor}.
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claudioc |
1.1 |
Thus, we can use an ABCD method in the \met$/\sqrt{\rm SumJetPt}$ vs
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sumJetPt plane to estimate the background in a data driven way.
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benhoob |
1.24 |
%\begin{figure}[bht]
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%\begin{center}
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%\includegraphics[width=0.75\linewidth]{uncorrelated.pdf}
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%\caption{\label{fig:uncor}\protect Distributions of SumJetPt
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%in MC $t\bar{t}$ events for different intervals of
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%MET$/\sqrt{\rm SumJetPt}$.}
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%\end{center}
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%\end{figure}
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claudioc |
1.21 |
\begin{figure}[bht]
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claudioc |
1.1 |
\begin{center}
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benhoob |
1.24 |
\includegraphics[width=0.75\linewidth]{uncor.png}
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claudioc |
1.1 |
\caption{\label{fig:uncor}\protect Distributions of SumJetPt
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in MC $t\bar{t}$ events for different intervals of
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benhoob |
1.24 |
MET$/\sqrt{\rm SumJetPt}$. h1, h2, and h3 refer to the MET$/\sqrt{\rm SumJetPt}$
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intervals 4.5-6.5, 6.5-8.5 and $>$8.5, respectively.}
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claudioc |
1.1 |
\end{center}
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\end{figure}
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claudioc |
1.21 |
\begin{figure}[tb]
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claudioc |
1.1 |
\begin{center}
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benhoob |
1.31 |
\includegraphics[width=0.75\linewidth]{ttdil_uncor_38X.png}
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benhoob |
1.22 |
\caption{\label{fig:abcdMC}\protect Distributions of MET$/\sqrt{\rm SumJetPt}$ vs.
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benhoob |
1.31 |
SumJetPt for SM Monte Carlo. Here we also show our choice of ABCD regions. The correlation coefficient
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${\rm corr_{XY}}$ is computed for events falling in the ABCD regions.}
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claudioc |
1.1 |
\end{center}
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\end{figure}
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Our choice of ABCD regions is shown in Figure~\ref{fig:abcdMC}.
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The signal region is region D. The expected number of events
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benhoob |
1.29 |
in the four regions for the SM Monte Carlo, as well as the background
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prediction A $\times$ C / B are given in Table~\ref{tab:abcdMC} for an integrated
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benhoob |
1.33 |
luminosity of 35 pb$^{-1}$. In Table~\ref{tab:abcdsyst}, we test the stability of
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observed/predicted with respect to variations in the ABCD boundaries.
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Based on the results in Tables~\ref{tab:abcdMC} and~\ref{tab:abcdsyst}, we assess
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a systematic uncertainty of 20\% on the prediction of the ABCD method.
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benhoob |
1.29 |
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%As shown in Table~\ref{tab:abcdsyst}, we assess systematic uncertainties
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%by varying the boundaries by an amount consistent with the hadronic energy scale uncertainty,
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%which we take as $\pm$5\% for SumJetPt and $\pm$2.5\% for MET/$\sqrt{\rm SumJetPt}$, since the
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%uncertainty on this quantity partially cancels due to the fact that it is a ratio of correlated
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%quantities. Based on these studies we assess a correction factor $k_{ABCD} = 1.2 \pm 0.2$ to the
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%predicted yield using the ABCD method.
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benhoob |
1.24 |
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claudioc |
1.9 |
%{\color{red} Avi wants some statement about stability
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%wrt changes in regions. I am not sure that we have done it and
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%I am not sure it is necessary (Claudio).}
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claudioc |
1.1 |
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claudioc |
1.21 |
\begin{table}[ht]
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claudioc |
1.1 |
\begin{center}
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\caption{\label{tab:abcdMC} Expected SM Monte Carlo yields for
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benhoob |
1.13 |
35 pb$^{-1}$ in the ABCD regions, as well as the predicted yield in
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benhoob |
1.16 |
the signal region given by A $\times$ C / B. Here `SM other' is the sum
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benhoob |
1.13 |
of non-dileptonic $t\bar{t}$ decays, $W^{\pm}$+jets, $W^+W^-$,
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$W^{\pm}Z^0$, $Z^0Z^0$ and single top.}
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benhoob |
1.16 |
\begin{tabular}{lccccc}
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benhoob |
1.13 |
\hline
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benhoob |
1.27 |
sample & A & B & C & D & A $\times$ C / B \\
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benhoob |
1.13 |
\hline
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benhoob |
1.27 |
$t\bar{t}\rightarrow \ell^{+}\ell^{-}$ & 8.27 $\pm$ 0.18 & 32.16 $\pm$ 0.35 & 4.69 $\pm$ 0.13 & 1.05 $\pm$ 0.06 & 1.21 $\pm$ 0.04 \\
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$Z^0 \rightarrow \ell^{+}\ell^{-}$ & 0.22 $\pm$ 0.11 & 1.54 $\pm$ 0.29 & 0.05 $\pm$ 0.05 & 0.16 $\pm$ 0.09 & 0.01 $\pm$ 0.01 \\
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SM other & 0.54 $\pm$ 0.03 & 2.28 $\pm$ 0.12 & 0.23 $\pm$ 0.03 & 0.07 $\pm$ 0.01 & 0.05 $\pm$ 0.01 \\
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benhoob |
1.25 |
\hline
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benhoob |
1.27 |
total SM MC & 9.03 $\pm$ 0.21 & 35.97 $\pm$ 0.46 & 4.97 $\pm$ 0.15 & 1.29 $\pm$ 0.11 & 1.25 $\pm$ 0.05 \\
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claudioc |
1.1 |
\hline
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\end{tabular}
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\end{center}
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\end{table}
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benhoob |
1.24 |
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\begin{table}[ht]
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\begin{center}
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benhoob |
1.27 |
\caption{\label{tab:abcdsyst}
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Results of the systematic study of the ABCD method by varying the boundaries
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benhoob |
1.24 |
between the ABCD regions shown in Fig.~\ref{fig:abcdMC}. Here $x_1$ is the lower SumJetPt boundary and
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$x_2$ is the boundary separating regions A and B from C and D, their nominal values are 125 and 300~GeV,
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respectively. $y_1$ is the lower MET/$\sqrt{\rm SumJetPt}$ boundary and
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$y_2$ is the boundary separating regions B and C from A and D, their nominal values are 4.5 and 8.5~GeV$^{1/2}$,
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respectively.}
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\begin{tabular}{cccc|c}
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\hline
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$x_1$ & $x_2$ & $y_1$ & $y_2$ & Observed/Predicted \\
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\hline
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benhoob |
1.33 |
nominal & nominal & nominal & nominal & $1.03 \pm 0.10$ \\
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+5\% & +5\% & +2.5\% & +2.5\% & $1.13 \pm 0.13$ \\
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+5\% & +5\% & nominal & nominal & $1.08 \pm 0.12$ \\
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nominal & nominal & +2.5\% & +2.5\% & $1.07 \pm 0.11$ \\
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nominal & +5\% & nominal & +2.5\% & $1.09 \pm 0.12$ \\
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nominal & -5\% & nominal & -2.5\% & $0.98 \pm 0.08$ \\
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-5\% & -5\% & +2.5\% & +2.5\% & $1.03 \pm 0.09$ \\
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+5\% & +5\% & -2.5\% & -2.5\% & $1.03 \pm 0.11$ \\
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benhoob |
1.24 |
\hline
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\end{tabular}
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\end{center}
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\end{table}
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claudioc |
1.2 |
\subsection{Dilepton $P_T$ method}
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\label{sec:victory}
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This method is based on a suggestion by V. Pavlunin\cite{ref:victory},
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and was investigated by our group in 2009\cite{ref:ourvictory}.
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The idea is that in dilepton $t\bar{t}$ events the lepton and neutrinos
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from $W$ decays have the same $P_T$ spectrum (modulo $W$ polarization
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effects). One can then use the observed
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$P_T(\ell\ell)$ distribution to model the sum of neutrino $P_T$'s which
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is identified with the \met.
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Then, in order to predict the $t\bar{t} \to$ dilepton contribution to a
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selection with \met$+$X, one applies a cut on $P_T(\ell\ell)+$X instead.
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In practice one has to rescale the result of the $P_T(\ell\ell)+$X selection
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to account for the fact that any dilepton selection must include a
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moderate \met cut in order to reduce Drell Yan backgrounds. This
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is discussed in Section 5.3 of Reference~\cite{ref:ourvictory}; for a \met
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benhoob |
1.16 |
cut of 50 GeV, the rescaling factor is obtained from the MC as
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claudioc |
1.2 |
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\newcommand{\ptll} {\ensuremath{P_T(\ell\ell)}}
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\begin{center}
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benhoob |
1.31 |
$ K = \frac{\int_0^{\infty} {\cal N}(\ptll)~~d\ptll~}{\int_{50}^{\infty} {\cal N}(\ptll)~~d\ptll~} = 1.52$
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claudioc |
1.2 |
\end{center}
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benhoob |
1.10 |
%%%TO BE REPLACED
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%Given the integrated luminosity of the
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%present dataset, the determination of $K$ in data is severely statistics
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%limited. Thus, we take $K$ from $t\bar{t}$ Monte Carlo as
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%\begin{center}
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%$ K_{MC} = \frac{\int_0^{\infty} {\cal N}(\met)~~d\met~}{\int_{50}^{\infty} {\cal N}(\met)~~d\met~}$
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%\end{center}
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claudioc |
1.9 |
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benhoob |
1.10 |
%\noindent {\color{red} For the 11 pb result we have used $K$ from data.}
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claudioc |
1.2 |
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There are several effects that spoil the correspondance between \met and
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$P_T(\ell\ell)$:
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\begin{itemize}
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\item $Ws$ in top events are polarized. Neutrinos are emitted preferentially
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benhoob |
1.22 |
parallel to the $W$ velocity while charged leptons are emitted prefertially
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anti-parallel. Thus the $P_T(\nu\nu)$ distribution is harder
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claudioc |
1.2 |
than the $P_T(\ell\ell)$ distribution for top dilepton events.
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\item The lepton selections results in $P_T$ and $\eta$ cuts on the individual
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leptons that have no simple correspondance to the neutrino requirements.
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\item Similarly, the \met$>$50 GeV cut introduces an asymmetry between leptons and
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neutrinos which is only partially compensated by the $K$ factor above.
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\item The \met resolution is much worse than the dilepton $P_T$ resolution.
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benhoob |
1.16 |
When convoluted with a falling spectrum in the tails of \met, this results
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claudioc |
1.2 |
in a harder spectrum for \met than the original $P_T(\nu\nu)$.
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\item The \met response in CMS is not exactly 1. This causes a distortion
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in the \met distribution that is not present in the $P_T(\ell\ell)$ distribution.
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\item The $t\bar{t} \to$ dilepton signal includes contributions from
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$W \to \tau \to \ell$. For these events the arguments about the equivalence
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of $P_T(\ell\ell)$ and $P_T(\nu\nu)$ do not apply.
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\item A dilepton selection will include SM events from non $t\bar{t}$
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sources. These events can affect the background prediction. Particularly
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dangerous are high $P_T$ Drell Yan events that barely pass the \met$>$ 50
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GeV selection. They will tend to push the data-driven background prediction up.
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benhoob |
1.16 |
Therefore we estimate the number of DY events entering the background prediction
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using the $R_{out/in}$ method as described in Sec.~\ref{sec:othBG}.
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claudioc |
1.2 |
\end{itemize}
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We have studied these effects in SM Monte Carlo, using a mixture of generator and
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reconstruction level studies, putting the various effects in one at a time.
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For each configuration, we apply the data-driven method and report as figure
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of merit the ratio of observed and predicted events in the signal region.
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The results are summarized in Table~\ref{tab:victorybad}.
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\begin{table}[htb]
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\begin{center}
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benhoob |
1.27 |
\caption{\label{tab:victorybad}
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Test of the data driven method in Monte Carlo
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benhoob |
1.35 |
under different assumptions, evaluated using 36X MC. See text for details.}
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claudioc |
1.6 |
\begin{tabular}{|l|c|c|c|c|c|c|c|c|}
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claudioc |
1.2 |
\hline
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claudioc |
1.6 |
& True $t\bar{t}$ dilepton & $t\to W\to\tau$& other SM & GEN or & Lepton $P_T$ & Z veto & \met $>$ 50& obs/pred \\
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benhoob |
1.28 |
& included & included & included & RECOSIM & and $\eta$ cuts & & & \\ \hline
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claudioc |
1.6 |
1&Y & N & N & GEN & N & N & N & 1.90 \\
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2&Y & N & N & GEN & Y & N & N & 1.64 \\
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3&Y & N & N & GEN & Y & Y & N & 1.59 \\
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4&Y & N & N & GEN & Y & Y & Y & 1.55 \\
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5&Y & N & N & RECOSIM & Y & Y & Y & 1.51 \\
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6&Y & Y & N & RECOSIM & Y & Y & Y & 1.58 \\
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benhoob |
1.17 |
7&Y & Y & Y & RECOSIM & Y & Y & Y & 1.38 \\
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claudioc |
1.2 |
\hline
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\end{tabular}
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\end{center}
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\end{table}
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benhoob |
1.28 |
\begin{table}[htb]
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\begin{center}
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\caption{\label{tab:victorysyst}
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benhoob |
1.35 |
Summary of variations in $K_C$ due to the MET scale and resolution uncertainty, and to backgrounds other than $t\bar{t} \to$~dilepton.
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benhoob |
1.28 |
In the first table, `up' and `down' refer to shifting the hadronic energy scale up and down by 5\%. In the second table, the quoted value
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refers to the amount of additional smearing of the MET, as discussed in the text. In the third table, the normalization of all backgrounds
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benhoob |
1.36 |
other than $t\bar{t} \to$~dilepton is varied.}
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benhoob |
1.28 |
\begin{tabular}{ lcccc }
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\hline
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MET scale & Predicted & Observed & Obs/pred \\
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\hline
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nominal & 0.92 $ \pm $ 0.11 & 1.29 $ \pm $ 0.11 & 1.40 $ \pm $ 0.20 \\
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up & 0.92 $ \pm $ 0.11 & 1.53 $ \pm $ 0.12 & 1.66 $ \pm $ 0.23 \\
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down & 0.81 $ \pm $ 0.07 & 1.08 $ \pm $ 0.11 & 1.32 $ \pm $ 0.17 \\
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\hline
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MET smearing & Predicted & Observed & Obs/pred \\
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\hline
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nominal & 0.92 $ \pm $ 0.11 & 1.29 $ \pm $ 0.11 & 1.40 $ \pm $ 0.20 \\
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10\% & 0.90 $ \pm $ 0.11 & 1.30 $ \pm $ 0.11 & 1.44 $ \pm $ 0.21 \\
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20\% & 0.84 $ \pm $ 0.07 & 1.36 $ \pm $ 0.11 & 1.61 $ \pm $ 0.19 \\
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30\% & 1.05 $ \pm $ 0.18 & 1.32 $ \pm $ 0.11 & 1.27 $ \pm $ 0.24 \\
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40\% & 0.85 $ \pm $ 0.07 & 1.37 $ \pm $ 0.11 & 1.61 $ \pm $ 0.19 \\
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50\% & 1.08 $ \pm $ 0.18 & 1.36 $ \pm $ 0.11 & 1.26 $ \pm $ 0.24 \\
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\hline
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non-$t\bar{t} \to$~dilepton scale factor & Predicted & Observed & Obs/pred \\
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\hline
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ttdil only & 0.77 $ \pm $ 0.07 & 1.05 $ \pm $ 0.06 & 1.36 $ \pm $ 0.14 \\
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nominal & 0.92 $ \pm $ 0.11 & 1.29 $ \pm $ 0.11 & 1.40 $ \pm $ 0.20 \\
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double non-ttdil yield & 1.06 $ \pm $ 0.18 & 1.52 $ \pm $ 0.20 & 1.43 $ \pm $ 0.30 \\
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\hline
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\end{tabular}
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\end{center}
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\end{table}
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| 252 |
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| 253 |
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| 254 |
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claudioc |
1.2 |
The largest discrepancy between prediction and observation occurs on the first
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| 256 |
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line of Table~\ref{tab:victorybad}, {\em i.e.}, at the generator level with no
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| 257 |
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cuts. We have verified that this effect is due to the polarization of
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| 258 |
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the $W$ (we remove the polarization by reweighting the events and we get
|
| 259 |
|
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good agreement between prediction and observation). The kinematical
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| 260 |
claudioc |
1.6 |
requirements (lines 2,3,4) compensate somewhat for the effect of W polarization.
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| 261 |
|
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Going from GEN to RECOSIM, the change in observed/predicted is small.
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% We have tracked this down to the fact that tcMET underestimates the true \met
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| 263 |
|
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% by $\approx 4\%$\footnote{We find that observed/predicted changes by roughly 0.1
|
| 264 |
|
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%for each 1.5\% change in \met response.}.
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| 265 |
|
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Finally, contamination from non $t\bar{t}$
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| 266 |
benhoob |
1.16 |
events can have a significant impact on the BG prediction.
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| 267 |
|
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%The changes between
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| 268 |
|
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%lines 6 and 7 of Table~\ref{tab:victorybad} is driven by 3
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| 269 |
|
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%Drell Yan events that pass the \met selection in Monte Carlo (thus the effect
|
| 270 |
|
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%is statistically not well quantified).
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| 271 |
claudioc |
1.2 |
|
| 272 |
|
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An additional source of concern is that the CMS Madgraph $t\bar{t}$ MC does
|
| 273 |
|
|
not include effects of spin correlations between the two top quarks.
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| 274 |
|
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We have studied this effect at the generator level using Alpgen. We find
|
| 275 |
claudioc |
1.7 |
that the bias is at the few percent level.
|
| 276 |
claudioc |
1.2 |
|
| 277 |
benhoob |
1.31 |
Based on the results of Table~\ref{tab:victorysyst}, we conclude that the
|
| 278 |
benhoob |
1.28 |
naive data-driven background estimate based on $P_T{(\ell\ell)}$ needs to
|
| 279 |
benhoob |
1.31 |
be corrected by a factor of $ K_C = 1.4 \pm 0.2({\rm stat})$.
|
| 280 |
claudioc |
1.2 |
|
| 281 |
benhoob |
1.31 |
The dominant sources of systematic uncertainty in $K_C$ are due to non-$t\bar{t} \to$~dilepton backgrounds,
|
| 282 |
|
|
and the MET scale and resolution uncertainties, as summarized in Table~\ref{tab:victorysyst}.
|
| 283 |
|
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The impact of non-$t\bar{t}$-dilepton background is assessed
|
| 284 |
|
|
by varying the yield of all backgrounds except for $t\bar{t} \to$~dilepton.
|
| 285 |
|
|
The uncertainty is assessed as the larger of the differences between the nominal $K_C$ value and the values
|
| 286 |
benhoob |
1.28 |
obtained using only $t\bar{t} \to$~dilepton MC and obtained by doubling the non $t\bar{t} \to$~dilepton component,
|
| 287 |
|
|
giving an uncertainty of $0.04$.
|
| 288 |
|
|
|
| 289 |
|
|
The uncertainty in $K_C$ due to the MET scale uncertainty is assessed by varying the hadronic energy scale using
|
| 290 |
benhoob |
1.32 |
the same method as in~\cite{ref:top}, giving an uncertainty of 0.3. We also assess the impact of the MET resolution
|
| 291 |
benhoob |
1.31 |
uncertainty on $K_C$ by applying a random smearing to the MET. For each event, we determine the expected MET resolution
|
| 292 |
|
|
based on the sumJetPt, and smear the MET to simulate an increase in the resolution of 10\%, 20\%, 30\%, 40\% and 50\%.
|
| 293 |
|
|
The results show that $K_C$ does not depend strongly on the MET resolution and we therefore do not assess any uncertainty.
|
| 294 |
claudioc |
1.2 |
|
| 295 |
benhoob |
1.28 |
Incorporating all the statistical and systematic uncertainties we find $K_C = 1.4 \pm 0.4$.
|
| 296 |
claudioc |
1.6 |
|
| 297 |
claudioc |
1.2 |
\subsection{Signal Contamination}
|
| 298 |
|
|
\label{sec:sigcont}
|
| 299 |
|
|
|
| 300 |
claudioc |
1.6 |
All data-driven methods are in principle subject to signal contaminations
|
| 301 |
claudioc |
1.2 |
in the control regions, and the methods described in
|
| 302 |
|
|
Sections~\ref{sec:abcd} and~\ref{sec:victory} are not exceptions.
|
| 303 |
|
|
Signal contamination tends to dilute the significance of a signal
|
| 304 |
|
|
present in the data by inflating the background prediction.
|
| 305 |
|
|
|
| 306 |
|
|
It is hard to quantify how important these effects are because we
|
| 307 |
|
|
do not know what signal may be hiding in the data. Having two
|
| 308 |
|
|
independent methods (in addition to Monte Carlo ``dead-reckoning'')
|
| 309 |
|
|
adds redundancy because signal contamination can have different effects
|
| 310 |
|
|
in the different control regions for the two methods.
|
| 311 |
|
|
For example, in the extreme case of a
|
| 312 |
|
|
new physics signal
|
| 313 |
claudioc |
1.6 |
with $P_T(\ell \ell) = \met$, an excess of events would be seen
|
| 314 |
claudioc |
1.2 |
in the ABCD method but not in the $P_T(\ell \ell)$ method.
|
| 315 |
|
|
|
| 316 |
claudioc |
1.4 |
|
| 317 |
claudioc |
1.2 |
The LM points are benchmarks for SUSY analyses at CMS. The effects
|
| 318 |
|
|
of signal contaminations for a couple such points are summarized
|
| 319 |
benhoob |
1.14 |
in Table~\ref{tab:sigcont}. Signal contamination is definitely an important
|
| 320 |
claudioc |
1.2 |
effect for these two LM points, but it does not totally hide the
|
| 321 |
|
|
presence of the signal.
|
| 322 |
claudioc |
1.1 |
|
| 323 |
|
|
|
| 324 |
claudioc |
1.2 |
\begin{table}[htb]
|
| 325 |
|
|
\begin{center}
|
| 326 |
benhoob |
1.14 |
\caption{\label{tab:sigcont} Effects of signal contamination
|
| 327 |
|
|
for the two data-driven background estimates. The three columns give
|
| 328 |
|
|
the expected yield in the signal region and the background estimates
|
| 329 |
benhoob |
1.20 |
using the ABCD and $P_T(\ell \ell)$ methods. Results are normalized to 35~pb$^{-1}$.}
|
| 330 |
benhoob |
1.14 |
\begin{tabular}{lccc}
|
| 331 |
claudioc |
1.2 |
\hline
|
| 332 |
benhoob |
1.14 |
& Yield & ABCD & $P_T(\ell \ell)$ \\
|
| 333 |
|
|
\hline
|
| 334 |
benhoob |
1.27 |
SM only & 1.29 & 1.25 & 0.92 \\
|
| 335 |
|
|
SM + LM0 & 7.57 & 4.44 & 1.96 \\
|
| 336 |
|
|
SM + LM1 & 3.85 & 1.60 & 1.43 \\
|
| 337 |
claudioc |
1.2 |
\hline
|
| 338 |
|
|
\end{tabular}
|
| 339 |
|
|
\end{center}
|
| 340 |
|
|
\end{table}
|
| 341 |
|
|
|
