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to predict the number of background events with |
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$\HT > 300\GeV$ and $\MET > 275\GeV$ ($\HT > 600\GeV$ and $\MET > 200\GeV$). |
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In practice, we apply two corrections to this prediction, following the same procedure as in Ref.~\cite{ref:ospaper}. |
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The first correction is $K_{50}=1.5 \pm 0.3$ ($1.3 \pm 0.2$) for the high \MET\ (high \Ht) signal region. |
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The second correction factor is $K_C = 1.5 \pm 0.5$ ($1.3 \pm 0.4$) for the |
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The first correction accounts for the fact that we require \met\ $>$ 50\GeV in the preselection |
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but there is no corresponding requirement on \ptll; this correction |
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is $K_{50}=1.5 \pm 0.3$ ($1.3 \pm 0.2$) for the high \MET\ (high \Ht) signal region. |
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The second correction factor accounts for the $W$ polarization in \ttbar\ events, as well |
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as detector effects such as hadronic energy scale; this correction is $K_C = 1.5 \pm 0.5$ ($1.3 \pm 0.4$) for the |
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high \MET (high \Ht) signal region. |
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|
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Our third background estimation method is based on the fact that many models of new physics |
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produce an excess of SF with respect to OF lepton pairs, while for the \ttbar\ background the |
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rates of SF and OF lepton pairs are the same. Hence we make use of the OF subtraction technique |
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discussed in Sec.~\ref{sec:fit} in which we performed a shape analysis of the dilepton mass distribution. |
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rates of SF and OF lepton pairs are the same, as discussed in Sec.~\ref{sec:fit}. |
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Here we perform a counting experiment, by quantifying the excess of SF vs. OF pairs using the |
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quantity |
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|