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\section{Data Sets, Cross-Sections, Luminosity}
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\label{sec:datasets}
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\subsection{Data sets}
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We use the following data sets:
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\begin{itemize}
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\item {\bf Dilepton data samples:} \\
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MinimumBias\_Commissioning10-May6thPDSkim2\_SD\_EG-v1 \\
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MinimumBias\_Commissioning10-SD\_EG-v9 \\
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EG\_Run2010A-PromptReco-v1 \\
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EG\_Run2010A-PromptReco-v2 \\
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MinimumBias\_Commissioning10-May6thPDSkim2\_SD\_Mu-v1 \\
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MinimumBias\_Commissioning10-SD\_Mu-v9 \\
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Mu\_Run2010A-PromptReco-v1 \\
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Mu\_Run2010A-PromptReco-v2
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\item {\bf QCD samples to measure the FR:} \\
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MinimumBias\_Commissioning10-May6thPDSkim2\_SD\_JetMETTau-v1 \\
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MinimumBias\_Commissioning10-SD\_JetMETTau-v9 \\
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JetMETTau\_Run2010A-PromptReco-v1 \\
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JetMETTau\_Run2010A-PromptReco-v2 \\
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MinimumBias\_Commissioning10-May6thPDSkim2\_SD\_JetMETTauMonitor-v1 \\
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MinimumBias\_Commissioning10-SD\_JetMETTauMonitor-v9 \\
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JetMETTauMonitor\_Run2010A-PromptReco-v1 \\
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JetMETTauMonitor\_Run2010A-PromptReco-v2
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\item {\bf Photon QCD MC samples:} \\
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QCD\_Pt15/Spring10-START3X\_V26\_S09-v1 \\
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QCD\_Pt30/Spring10-START3X\_V26\_S09-v1
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\item {\bf Pythia $\gamma~+$ jets MC sample:} \\
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PhotonJet\_Pt15/Spring10-START3X\_V26\_S09-v1
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\item {\bf Pythia Drell Yan MC samples:} \\
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Ztautau/Spring10-START3X\_V26\_S09-v1 \\
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Zmumu/Spring10-START3X\_V26\_S09-v1 \\
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Zee/Spring10-START3X\_V26\_S09-v1 \\
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DYee\_M10to20/Spring10-START3X\_V26\_S09-v1 \\
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DYmumu\_M10to20/Spring10-START3X\_V26\_S09-v1
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\end{itemize}
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\subsection{Cross-sections}
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All assumed Monte Carlo cross-sections are lowest order and are
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taken from the Monte Carlo production twiki~\cite{ref:xsec}.
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\subsection{Luminosity}
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\label{sec:lumi}
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The luminosity of the analyzed data is estimated to be 11.5 nb$^{-1}$
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for the OS analysis and slightly larger (14.1 nb$^{-1}$) for the SS
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analysis. The different integrated luminosities are due to
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technical reasons. This will fixed in the next update.
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