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claudioc |
1.1 |
\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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spadhi |
1.5 |
{\tt /MinimumBias/Commissioning10-May6thPDSkim2\_SD\_EG-v1/RECO } \\
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{\tt /MinimumBias/Commissioning10-SD\_EG-v9/RECO } \\
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{\tt /MinimumBias/Commissioning10-May6thPDSkim2\_SD\_Mu-v1/RECO } \\
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{\tt /MinimumBias/Commissioning10-SD\_Mu-v9/RECO } \\
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{\tt /EG/Run2010A-PromptReco-v1/RECO } \\
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{\tt /EG/Run2010A-PromptReco-v2/RECO } \\
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{\tt /Mu/Run2010A-PromptReco-v1/RECO } \\
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{\tt /Mu/Run2010A-PromptReco-v2/RECO }
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claudioc |
1.1 |
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\item {\bf QCD samples to measure the FR:} \\
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spadhi |
1.5 |
{\tt /MinimumBias/Commissioning10-May6thPDSkim2\_SD\_JetMETTau-v1/RECO } \\
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{\tt /MinimumBias/Commissioning10-May6thPDSkim2\_SD\_JetMETTauMonitor-v1/RECO } \\
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{\tt /MinimumBias/Commissioning10-SD\_JetMETTau-v9/RECO } \\
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{\tt /MinimumBias/Commissioning10-SD\_JetMETTauMonitor-v9/RECO } \\
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{\tt /JetMETTauMonitor/Run2010A-PromptReco-v1/RECO } \\
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{\tt /JetMETTauMonitor/Run2010A-PromptReco-v2/RECO } \\
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{\tt /JetMETTau/Run2010A-PromptReco-v1/RECO } \\
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{\tt /JetMETTau/Run2010A-PromptReco-v2/RECO }
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claudioc |
1.1 |
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claudioc |
1.4 |
\item {\bf QCD MC sample:} \\
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spadhi |
1.5 |
{\tt /QCD\_Pt15/Spring10-START3X\_V26\_S09-v1/GEN-SIM-RECO } \\
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{\tt /QCD\_Pt30/Spring10-START3X\_V26\_S09-v1/GEN-SIM-RECO }
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claudioc |
1.1 |
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\item {\bf Pythia $\gamma~+$ jets MC sample:} \\
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spadhi |
1.5 |
{\tt /PhotonJet\_Pt15/Spring10-START3X\_V26\_S09-v1/GEN-SIM-RECO }
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claudioc |
1.1 |
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\item {\bf Pythia Drell Yan MC samples:} \\
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spadhi |
1.5 |
{\tt /Ztautau/Spring10-START3X\_V26\_S09-v1/GEN-SIM-RECO } \\
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{\tt /Zmumu/Spring10-START3X\_V26\_S09-v1/GEN-SIM-RECO } \\
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{\tt /Zee/Spring10-START3X\_V26\_S09-v1/GEN-SIM-RECO } \\
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{\tt /DYee\_M10to20/Spring10-START3X\_V26\_S09-v1/GEN-SIM-RECO } \\
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{\tt /DYmumu\_M10to20/Spring10-START3X\_V26\_S09-v1/GEN-SIM-RECO }
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claudioc |
1.1 |
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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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claudioc |
1.2 |
for the OS analysis and slightly larger (12.5 nb$^{-1}$) for the SS
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claudioc |
1.1 |
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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