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The data yields and corresponding MC predictions after this event preselection |
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are given in Table~\ref{tab:yields}. The MC yields are normalized to~\lumifinal\ using |
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next-to-leading order (NLO) cross sections. At the current LHC luminosity, the mean |
7 |
< |
number of expected pile-up interactions is approximately 5. In the MC, pile-up interactions |
7 |
> |
number of interactions in a single beam crossing is approximately 5. In the MC, multiple interactions |
8 |
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are superimposed on the hard collision, and the MC is reweighted such that the distribution |
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of reconstructed primary vertices matches that in data. As expected, the MC predicts that the |
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sample passing the preselection is dominated by dilepton $t\bar{t}$. The data yield is in |
11 |
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reasonable agreement with the prediction. We also quote the yields for |
11 |
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reasonable agreement~\footnote{The luminosity is currently underestimated by approximately 10\%, |
12 |
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which explains the observed excess in data. The estimate will be updated before EPS.} |
13 |
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with the prediction. We also quote the yields for |
14 |
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the LM1 and LM3 benchmark scenarios. |
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|
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|
\begin{table}[htb] |
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The samples of MC $t\bar{t}$, $W^{\pm}$ + jets, and single-top events were |
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generated with \MADGRAPH. The Drell--Yan sample (which includes events with |
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invariant masses as low as 10\GeVcc) was generated using a mixture of \MADGRAPH\ and |
24 |
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\PYTHIA and contains decays to the $\tau^+\tau^-$ final state. All other samples were generated with \PYTHIA. |
25 |
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The LM0 and LM1 benchmark scenarios are defined in the text; the quoted $\sigma$ values refer to the total production |
24 |
> |
\PYTHIA and includes decays to the $\tau^+\tau^-$ final state. All other samples were generated with \PYTHIA. |
25 |
> |
The LM1 and LM3 benchmark scenarios are defined in the text; the quoted $\sigma$ values refer to the total production |
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cross section for SUSY particles in these scenarios. Uncertainties are statistical only. |
27 |
|
} |
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\vspace{2 mm} |
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\begin{tabular}{lr|cccc} |
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|
\hline |
31 |
< |
Sample & $\sigma$ & $ee$ & $\mu\mu$ & $e\mu$ & total \\ |
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Sample & $\sigma$ [pb] & $ee$ & $\mu\mu$ & $e\mu$ & total \\ |
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|
\hline |
33 |
< |
\ttll & 16.9 & 147.6 $\pm$ 3.2 &166.4 $\pm$ 3.2 &391.7 $\pm$ 5.1 &705.8 $\pm$ 6.8 \\ |
34 |
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\ttfake & 140.6 & 4.5 $\pm$ 0.6 & 1.3 $\pm$ 0.3 & 8.1 $\pm$ 0.7 & 13.9 $\pm$ 1.0 \\ |
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DY & 18417 & 6.6 $\pm$ 1.8 & 9.5 $\pm$ 2.1 & 13.4 $\pm$ 2.6 & 29.6 $\pm$ 3.8 \\ |
36 |
< |
\WW & 2.9 & 1.4 $\pm$ 0.2 & 1.5 $\pm$ 0.2 & 3.4 $\pm$ 0.2 & 6.3 $\pm$ 0.3 \\ |
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\WZ & 0.3 & 0.3 $\pm$ 0.0 & 0.4 $\pm$ 0.0 & 0.7 $\pm$ 0.1 & 1.3 $\pm$ 0.1 \\ |
38 |
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\ZZ & 4.3 & 0.1 $\pm$ 0.0 & 0.1 $\pm$ 0.0 & 0.2 $\pm$ 0.0 & 0.4 $\pm$ 0.0 \\ |
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single top & 33 & 4.5 $\pm$ 0.2 & 5.0 $\pm$ 0.2 & 11.9 $\pm$ 0.3 & 21.4 $\pm$ 0.5 \\ |
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< |
\wjets & 28049 & 4.5 $\pm$ 1.9 & 0.0 $\pm$ 0.0 & 2.8 $\pm$ 1.7 & 7.3 $\pm$ 2.6 \\ |
33 |
> |
\ttll & 17 & 147.6 $\pm$ 3.2 &166.4 $\pm$ 3.2 &391.7 $\pm$ 5.1 &705.8 $\pm$ 6.8 \\ |
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> |
\ttfake & 141 & 4.5 $\pm$ 0.6 & 1.3 $\pm$ 0.3 & 8.1 $\pm$ 0.7 & 13.9 $\pm$ 1.0 \\ |
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> |
DY$\to\ell^+\ell^-$ & 16677 & 6.6 $\pm$ 1.8 & 9.5 $\pm$ 2.1 & 13.4 $\pm$ 2.6 & 29.6 $\pm$ 3.8 \\ |
36 |
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\WW & 43 & 1.4 $\pm$ 0.2 & 1.5 $\pm$ 0.2 & 3.4 $\pm$ 0.2 & 6.3 $\pm$ 0.3 \\ |
37 |
> |
\WZ & 18 & 0.3 $\pm$ 0.0 & 0.4 $\pm$ 0.0 & 0.7 $\pm$ 0.1 & 1.3 $\pm$ 0.1 \\ |
38 |
> |
\ZZ & 5.9 & 0.1 $\pm$ 0.0 & 0.1 $\pm$ 0.0 & 0.2 $\pm$ 0.0 & 0.4 $\pm$ 0.0 \\ |
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> |
single top & 102 & 4.5 $\pm$ 0.2 & 5.0 $\pm$ 0.2 & 11.9 $\pm$ 0.3 & 21.4 $\pm$ 0.5 \\ |
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> |
\wjets & 96648 & 4.5 $\pm$ 1.9 & 0.0 $\pm$ 0.0 & 2.8 $\pm$ 1.7 & 7.3 $\pm$ 2.6 \\ |
41 |
|
\hline |
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total SM MC & & 169.7 $\pm$ 4.2 &184.3 $\pm$ 3.9 &432.2 $\pm$ 6.0 &786.1 $\pm$ 8.3 \\ |
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> |
total SM MC & & 169.7 $\pm$ 4.2 &184.3 $\pm$ 3.9 &432.2 $\pm$ 6.0 &786.1 $\pm$ 8.3 \\ |
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|
\hline |
44 |
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data & & 193 & 201 & 485 & 879 \\ |
44 |
> |
data & & 193 & 201 & 485 & 879 \\ |
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|
\hline |
46 |
< |
LM1 & 6.7 & 22.3 $\pm$ 0.6 & 24.8 $\pm$ 0.6 & 12.8 $\pm$ 0.4 & 59.9 $\pm$ 0.9 \\ |
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< |
LM3 & 5.3 & 7.9 $\pm$ 0.3 & 9.6 $\pm$ 0.3 & 14.2 $\pm$ 0.4 & 31.7 $\pm$ 0.6 \\ |
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> |
LM1 & 6.7 & 22.3 $\pm$ 0.6 & 24.8 $\pm$ 0.6 & 12.8 $\pm$ 0.4 & 59.9 $\pm$ 0.9 \\ |
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> |
LM3 & 5.3 & 7.9 $\pm$ 0.3 & 9.6 $\pm$ 0.3 & 14.2 $\pm$ 0.4 & 31.7 $\pm$ 0.6 \\ |
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|
\hline |
49 |
|
\end{tabular} |
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\end{center} |