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Comparing UserCode/benhoob/cmsnotes/OSPAS2011/yields.tex (file contents):
Revision 1.1 by benhoob, Mon Jun 13 12:37:14 2011 UTC vs.
Revision 1.2 by benhoob, Wed Jun 15 08:26:17 2011 UTC

# Line 15 | Line 15 | the LM1 and LM3 benchmark scenarios.
15   \begin{center}
16   \caption{\label{tab:yields} Data yields and MC predictions after preselection, using the quoted NLO production cross sections $\sigma$.
17   The \ttll\ corrresponds  to dilepton $t\bar{t}$, including
18 $t \to W \to \ell$; \tttau\ corresponds to dilepton $t\bar{t}$ in which at least 1 $W$ decays via
18   $t \to W \to \tau \to \ell$; \ttfake\ includes all other $t\bar{t}$ decay modes.
19   The samples of MC $t\bar{t}$, $W^{\pm}$ + jets, and single-top events were
20   generated with \MADGRAPH. The Drell--Yan sample (which includes events with
# Line 29 | Line 28 | cross section for SUSY particles in thes
28   \hline
29           Sample   & $\sigma$  &            $ee$   &       $\mu\mu$   &         $e\mu$   &       total  \\
30   \hline
31 <          \ttll   &      X & 120.1 $\pm$ 2.9   &133.1 $\pm$ 2.9   &320.3 $\pm$ 4.6   &573.5 $\pm$ 6.1  \\
33 <         \tttau   &      X &  27.5 $\pm$ 1.4   & 33.3 $\pm$ 1.4   & 71.5 $\pm$ 2.2   &132.3 $\pm$ 3.0  \\
31 >          \ttll   &   16.9 & 147.6 $\pm$ 3.2   &166.4 $\pm$ 3.2   &391.7 $\pm$ 5.1   &705.8 $\pm$ 6.8  \\
32          \ttfake   &  140.6 &   4.5 $\pm$ 0.6   &  1.3 $\pm$ 0.3   &  8.1 $\pm$ 0.7   & 13.9 $\pm$ 1.0  \\
33               DY   &  18417 &   6.6 $\pm$ 1.8   &  9.5 $\pm$ 2.1   & 13.4 $\pm$ 2.6   & 29.6 $\pm$ 3.8  \\
34              \WW   &    2.9 &   1.4 $\pm$ 0.2   &  1.5 $\pm$ 0.2   &  3.4 $\pm$ 0.2   &  6.3 $\pm$ 0.3  \\
# Line 44 | Line 42 | cross section for SUSY particles in thes
42             data   &        &             193   &            201   &            485   &            879  \\
43   \hline
44              LM1   &    6.7 &  22.3 $\pm$ 0.6   & 24.8 $\pm$ 0.6   & 12.8 $\pm$ 0.4   & 59.9 $\pm$ 0.9  \\
45 <            LM3   &      X &   5.2 $\pm$ 0.2   &  6.3 $\pm$ 0.2   &  9.0 $\pm$ 0.2   & 20.4 $\pm$ 0.4  \\
45 >            LM3   &    5.3 &   7.9 $\pm$ 0.3   &  9.6 $\pm$ 0.3   & 14.2 $\pm$ 0.4   & 31.7 $\pm$ 0.6  \\
46   \hline
47   \end{tabular}
48   \end{center}

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