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+%\section{Systematics Uncertainties on the Background Prediction}
+%\label{sec:systematics}
-+
+[DESCRIBE HERE ONE BY ONE THE UNCERTAINTIES THAT ARE PRESENT IN THE SPREADSHHET
-+
+FROM WHICH WE CALCULATE THE TOTAL UNCERTAINTY. WE KNOW HOW TO DO THIS
-+
+AND
-+
+WE HAVE THE TECHNOLOGY FROM THE 7 TEV ANALYSIS TO PROPAGATE ALL
-+
+UNCERTAINTIES
-+
+CORRECTLY THROUGH.  WE WILL DO IT ONCE WE HAVE SETTLED ON THE
-+
+INDIVIDUAL PIECES WHICH ARE STILL IN FLUX]
-+
-+
+In this Section we discuss the systematic uncertainty on the BG
-+
+prediction.  This prediction is assembled from the event
-+
+counts in the peak region of the transverse mass distribution as
-+
+well as Monte Carlo
-+
+with a number of correction factors, as described previously.
-+
+The
-+
+final uncertainty on the prediction is built up from the uncertainties in these
-+
+individual
-+
+components.
-+
+The calculation is done for each signal
-+
+region,
-+
+for electrons and muons separately.
-+
-+
+The choice to normalizing to the peak region of $M_T$ has the
-+
+advantage that some uncertainties, e.g., luminosity, cancel.
-+
+It does however introduce complications because it couples
-+
+some of the uncertainties in non-trivial ways.  For example,
-+
+the primary effect of an uncertainty on the rare MC cross-section
-+
+is to introduce an uncertainty in the rare MC background estimate
-+
+which comes entirely from MC.   But this uncertainty also affects,
-+
+for example,
-+
+the $t\bar{t} \to$ dilepton BG estimate because it changes the
-+
+$t\bar{t}$ normalization to the peak region (because some of the
-+
+events in the peak region are from rare processes).  These effects
-+
+are carefully accounted for.  The contribution to the overall
-+
+uncertainty from each BG source is tabulated in
-+
+Section~\ref{sec:bgunc-bottomline}.
-+
+First, however, we discuss the uncertainties one-by-one and we comment
-+
+on their impact on the overall result, at least to first order.
-+
+Second order effects, such as the one described, are also included.
-+
-+
+\subsection{Statistical uncertainties on the event counts in the $M_T$
-+
+peak regions}
-+
+These vary between XX and XX \%, depending on the signal region
-+
+(different
-+
+signal regions have different \met\ requirements, thus they also have
-+
+different $M_T$ regions used as control.
-+
+Since
-+
+the major BG, eg, $t\bar{t}$ are normalized to the peak regions, this
-+
+fractional uncertainty is pretty much carried through all the way to
-+
+the end.  There is also an uncertainty from the finite MC event counts
-+
+in the $M_T$ peak regions.  This is also included, but it is smaller.
-+
-+
+\subsection{Uncertainty from the choice of $M_T$ peak region}
-+
+IN 7 TEV DATA WE HAD SOME SHAPE DIFFERENCES IN THE MTRANS REGION THAT
-+
+LED US TO CONSERVATIVELY INCLUDE THIS UNCERTAINTY.  WE NEED TO LOOK
-+
+INTO THIS AGAIN
-+
-+
+\subsection{Uncertainty on the Wjets cross-section and the rare MC cross-sections}
-+
+These are taken as 50\%, uncorrelated.
-+
+The primary effect is to introduce a 50\%
-+
+uncertainty
-+
+on the $W +$ jets and rare BG
-+
+background predictions, respectively.  However they also
-+
+have an effect on the other BGs via the $M_T$ peak normalization
-+
+in a way that tends to reduce the uncertainty.  This is easy
-+
+to understand: if the $W$ cross-section is increased by 50\%, then
-+
+the $W$ background goes up.  But the number of $M_T$ peak events
-+
+attributed to $t\bar{t}$ goes down, and since the $t\bar{t}$ BG is
-+
+scaled to the number of $t\bar{t}$ events in the peak, the $t\bar{t}$
-+
+BG goes down.
-+
-+
+\subsection{Scale factors for the tail-to-peak ratios for lepton +
-+
+  jets top and W events}
-+
+These tail-to-peak ratios are described in Section~\ref{sec:ttp}.
-+
+They are studied in CR1 and CR2.  The studies are described
-+
+in Sections~\ref{sec:cr1} and~\ref{sec:cr2}), respectively, where
-+
+we also give the uncertainty on the scale factors.
-+
-+
+\subsection{Uncertainty on extra jet radiation for dilepton
-+
+  background}
-+
+As discussed in Section~\ref{sec:jetmultiplicity}, the
-+
+jet distribution in
-+
+$t\bar{t} \to$
-+
+dilepton MC is rescaled by the factors $K_3$ and $K_4$ to make
-+
+it agree with the data.  The XX\% uncertainties on $K_3$ and $K_4$
-+
+comes from data/MC statistics.  This
-+
+result directly in a XX\% uncertainty on the dilepton BG, which is by far
-+
+the most important one.
-+
-+
+\subsection{Uncertainty on the \ttll\ Acceptance}
+The \ttbar\ background prediction is obtained from MC, with corrections
+  Pythia (LO). It may also be noted that MC@NLO uses Herwig6 for the
+  hadronisation, while POWHEG uses Pythia6.
+\item Modeling of taus: The alternative sample does not include
-<
+  Tauola and is otherwise identical to the Powheg sample.
->
+  Tauola and is otherwise identical to the Powheg sample.
->
+  This effect was studied earlier using 7~TeV samples and found to be negligible.
+\item The PDF uncertainty is estimated following the PDF4LHC
+  recommendations[CITE]. The events are reweighted using alternative
+  PDF sets for CT10 and MSTW2008 and the uncertainties for each are derived using the
+  addition, the NNPDF2.1 set with 100 replicas. The central value is
+  determined from the mean and the uncertainty is derived from the
+  $1\sigma$ range. The overall uncertainty is derived from the envelope of the
-<
+  alternative predictions and their uncertainties.
-<
+\end{itemize}
->
+  alternative predictions and their uncertainties.
->
+  This effect was studied earlier using 7~TeV samples and found to be negligible.
->
+  \end{itemize}
+\begin{figure}[hbt]
+          alternative sample predictions are indicated by the
+          datapoints. The uncertainties on the alternative predictions
+          correspond to the uncorrelated statistical uncertainty from
-<
+          the size of the alternative sample only.}
->
+          the size of the alternative sample only.
->
+        [TO BE UPDATED WITH THE LATEST SELECTION AND SFS]}
+      \end{center}
+    \end{figure}
-<
->
+\clearpage
+%\end{tabular}
+%\end{center}
+%\end{table}
-+
-+
+\subsection{Uncertainty from the isolated track veto}
-+
+This is the uncertainty associated with how well the isolated track
-+
+veto performance is modeled by the Monte Carlo.  This uncertainty
-+
+only applies to the fraction of dilepton BG events that have
-+
+a second e/$\mu$ or a one prong $\tau \to h$, with
-+
+$P_T > 10$ GeV in $|\eta| < 2.4$.  This fraction is 1/3 (THIS WAS THE
-+
+TEV NUMBER, CHECK).  The uncertainty for these events
-+
+is XX\% and is obtained from Tag and Probe studies of Section~\ref{sec:trkveto}
-+
-+
+\subsubsection{Isolated Track Veto: Tag and Probe Studies}
-+
+\label{sec:trkveto}
-+
-+
+[EVERYTHING IS 7TEV HERE, UPDATE WITH NEW RESULTS \\
-+
+ADD TABLE WITH FRACTION OF EVENTS THAT HAVE A TRUE ISOLATED TRACK]
-+
-+
+In this section we compare the performance of the isolated track veto in data and MC using tag-and-probe studies
-+
+with samples of Z$\to$ee and Z$\to\mu\mu$. The purpose of these studies is to demonstrate that the efficiency
-+
+to satisfy the isolated track veto requirements is well-reproduced in the MC, since if this were not the case
-+
+we would need to apply a data-to-MC scale factor in order to correctly predict the \ttll\ background. This study
-+
+addresses possible data vs. MC discrepancies for the {\bf efficiency} to identify (and reject) events with a
-+
+second {\bf genuine} lepton (e, $\mu$, or $\tau\to$1-prong). It does not address possible data vs. MC discrepancies
-+
+in the fake rate for rejecting events without a second genuine lepton; this is handled separately in the top normalization
-+
+procedure by scaling the \ttlj\ contribution to match the data in the \mt\ peak after applying the isolated track veto.
-+
+Furthermore, we test the data and MC
-+
+isolated track veto efficiencies for electrons and muons since we are using a Z tag-and-probe technique, but we do not
-+
+directly test the performance for hadronic tracks from $\tau$ decays. The performance for hadronic $\tau$ decay products
-+
+may differ from that of electrons and muons for two reasons. First, the $\tau$ may decay to a hadronic track plus one
-+
+or two $\pi^0$'s, which may decay to $\gamma\gamma$ followed by a photon conversion. As shown in Figure~\ref{fig:absiso},
-+
+the isolation distribution for charged tracks from $\tau$ decays that are not produced in association with $\pi^0$s are
-+
+consistent with that from $\E$s and $\M$s. Since events from single prong $\tau$ decays produced in association with
-+
+$\pi^0$s comprise a small fraction of the total sample, and since the kinematics of $\tau$, $\pi^0$ and $\gamma\to e^+e^-$
-+
+decays are well-understood, we currently demonstrate that the isolation is well-reproduced for electrons and muons only.
-+
+Second, hadronic tracks may undergo nuclear interactions and hence their tracks may not be reconstructed.
-+
+As discussed above, independent studies show that the MC reproduces the hadronic tracking efficiency within 4\%,
-+
+leading to a total background uncertainty of less than 0.5\% (after taking into account the fraction of the total background
-+
+due to hadronic $\tau$ decays with \pt\ $>$ 10 GeV tracks), and we hence regard this effect as neglgigible.
-+
-+
+The tag-and-probe studies are performed in the full 2011 data sample, and compared with the DYJets madgraph sample.
-+
+All events must contain a tag-probe pair (details below) with opposite-sign and satisfying the Z mass requirement 76--106 GeV.
-+
+We compare the distributions of absolute track isolation for probe electrons/muons in data vs. MC. The contributions to
-+
+this isolation sum are from ambient energy in the event from underlying event, pile-up and jet activitiy, and hence do
-+
+not depend on the \pt\ of the probe lepton. We therefore restrict the probe \pt\ to be $>$ 30 GeV in order to suppress
-+
+fake backgrounds with steeply-falling \pt\ spectra. To suppress non-Z backgrounds (in particular \ttbar) we require
-+
+\met\ $<$ 30 GeV and 0 b-tagged events.
-+
+The specific criteria for tags and probes for electrons and muons are:
-+
-+
+%We study the isolated track veto efficiency in bins of \njets.
-+
+%We are interested in events with at least 4 jets to emulate the hadronic activity in our signal sample. However since
-+
+%there are limited statistics for Z + $\geq$4 jet events, we study the isolated track performance in events with
-+
-+
-+
+\begin{itemize}
-+
+  \item{Electrons}
-+
-+
+    \begin{itemize}
-+
+    \item{Tag criteria}
-+
-+
+      \begin{itemize}
-+
+      \item Electron passes full analysis ID/iso selection
-+
+      \item \pt\ $>$ 30 GeV, $|\eta|<2.5$
-+
-+
+      \item Matched to 1 of the 2 electron tag-and-probe triggers
-+
+        \begin{itemize}
-+
+        \item \verb=HLT_Ele17_CaloIdVT_CaloIsoVT_TrkIdT_TrkIsoVT_SC8_Mass30_v*=
-+
+        \item \verb=HLT_Ele17_CaloIdVT_CaloIsoVT_TrkIdT_TrkIsoVT_Ele8_Mass30_v*=
-+
+        \end{itemize}
-+
+      \end{itemize}
-+
-+
+    \item{Probe criteria}
-+
+      \begin{itemize}
-+
+      \item Electron passes full analysis ID selection
-+
+      \item \pt\ $>$ 30 GeV
-+
+      \end{itemize}
-+
+      \end{itemize}
-+
+  \item{Muons}
-+
+    \begin{itemize}
-+
+    \item{Tag criteria}
-+
+      \begin{itemize}
-+
+      \item Muon passes full analysis ID/iso selection
-+
+      \item \pt\ $>$ 30 GeV, $|\eta|<2.1$
-+
+      \item Matched to 1 of the 2 electron tag-and-probe triggers
-+
+        \begin{itemize}
-+
+        \item \verb=HLT_IsoMu30_v*=
-+
+        \item \verb=HLT_IsoMu30_eta2p1_v*=
-+
+        \end{itemize}
-+
+      \end{itemize}
-+
+    \item{Probe criteria}
-+
+      \begin{itemize}
-+
+      \item Muon passes full analysis ID selection
-+
+      \item \pt\ $>$ 30 GeV
-+
+      \end{itemize}
-+
+    \end{itemize}
-+
+\end{itemize}
-+
-+
+The absolute track isolation distributions for passing probes are displayed in Fig.~\ref{fig:tnp}. In general we observe
-+
+good agreement between data and MC. To be more quantitative, we compare the data vs. MC efficiencies to satisfy
-+
+absolute track isolation requirements varying from $>$ 1 GeV to $>$ 5 GeV, as summarized in Table~\ref{tab:isotrk}.
-+
+In the $\geq$0 and $\geq$1 jet bins where the efficiencies can be tested with statistical precision, the data and MC
-+
+efficiencies agree within 7\%, and we apply this as a systematic uncertainty on the isolated track veto efficiency.
-+
+For the higher jet multiplicity bins the statistical precision decreases, but we do not observe any evidence for
-+
+a data vs. MC discrepancy in the isolated track veto efficiency.
-+
-+
-+
+%This is because our analysis requirement is relative track isolation $<$ 0.1, and m
-+
+%This requirement is chosen because most of the tracks rejected by the isolated
-+
+%track veto have a \pt\ near the 10 GeV threshold, and our analysis requirement is relative track isolation $<$ 1 GeV.
-+
-+
+\begin{figure}[hbt]
-+
+  \begin{center}
-+
+        %\includegraphics[width=0.3\linewidth]{plots/el_tkiso_0j.pdf}%
-+
+        %\includegraphics[width=0.3\linewidth]{plots/mu_tkiso_0j.pdf}
-+
+        %\includegraphics[width=0.3\linewidth]{plots/el_tkiso_1j.pdf}%
-+
+        %\includegraphics[width=0.3\linewidth]{plots/mu_tkiso_1j.pdf}
-+
+        %\includegraphics[width=0.3\linewidth]{plots/el_tkiso_2j.pdf}%
-+
+        %\includegraphics[width=0.3\linewidth]{plots/mu_tkiso_2j.pdf}
-+
+        %\includegraphics[width=0.3\linewidth]{plots/el_tkiso_3j.pdf}%
-+
+        %\includegraphics[width=0.3\linewidth]{plots/mu_tkiso_3j.pdf}
-+
+        %\includegraphics[width=0.3\linewidth]{plots/el_tkiso_4j.pdf}%
-+
+        %\includegraphics[width=0.3\linewidth]{plots/mu_tkiso_4j.pdf}
-+
+        \caption{
-+
+          \label{fig:tnp} Comparison of the absolute track isolation in data vs. MC for electrons (left) and muons (right)
-+
+for events with the \njets\ requirement varied from \njets\ $\geq$ 0 to \njets\ $\geq$ 4.
-+
+}
-+
+      \end{center}
-+
+\end{figure}
-+
-+
+\clearpage
-+
-+
+\begin{table}[!ht]
-+
+\begin{center}
-+
+\caption{\label{tab:isotrk} Comparison of the data vs. MC efficiencies to satisfy the indicated requirements
-+
+on the absolute track isolation, and the ratio of these two efficiencies. Results are indicated separately for electrons and muons and for various
-+
+jet multiplicity requirements.}
-+
+\begin{tabular}{l|c|c|c|c|c}
-+
-+
+%Electrons:
-+
+%Total MC yields        : 323790
-+
+%Total DATA yields      : 2772586
-+
+%Muons:
-+
+%Total MC yields        : 456138
-+
+%Total DATA yields      : 4210022
-+
-+
+\hline
-+
+\hline
-+
+e + $\geq$0 jets   &           $>$ 1 GeV   &           $>$ 2 GeV   &           $>$ 3 GeV   &           $>$ 4 GeV   &           $>$ 5 GeV  \\
-+
+\hline
-+
+      data   &  0.097 $\pm$ 0.0002   &  0.035 $\pm$ 0.0001   &  0.016 $\pm$ 0.0001   &  0.009 $\pm$ 0.0001   &  0.005 $\pm$ 0.0000  \\
-+
+        mc   &  0.096 $\pm$ 0.0005   &  0.034 $\pm$ 0.0003   &  0.015 $\pm$ 0.0002   &  0.008 $\pm$ 0.0002   &  0.005 $\pm$ 0.0001  \\
-+
+   data/mc   &     1.01 $\pm$ 0.01   &     1.04 $\pm$ 0.01   &     1.06 $\pm$ 0.02   &     1.04 $\pm$ 0.02   &     1.01 $\pm$ 0.02  \\
-+
-+
+\hline
-+
+\hline
-+
+$\mu$ + $\geq$0 jets   &           $>$ 1 GeV   &           $>$ 2 GeV   &           $>$ 3 GeV   &           $>$ 4 GeV   &           $>$ 5 GeV  \\
-+
+\hline
-+
+      data   &  0.094 $\pm$ 0.0001   &  0.034 $\pm$ 0.0001   &  0.016 $\pm$ 0.0001   &  0.009 $\pm$ 0.0000   &  0.006 $\pm$ 0.0000  \\
-+
+        mc   &  0.093 $\pm$ 0.0004   &  0.033 $\pm$ 0.0003   &  0.015 $\pm$ 0.0002   &  0.008 $\pm$ 0.0001   &  0.005 $\pm$ 0.0001  \\
-+
+   data/mc   &     1.01 $\pm$ 0.00   &     1.04 $\pm$ 0.01   &     1.05 $\pm$ 0.01   &     1.06 $\pm$ 0.02   &     1.07 $\pm$ 0.02  \\
-+
-+
+\hline
-+
+\hline
-+
+e + $\geq$1 jets   &           $>$ 1 GeV   &           $>$ 2 GeV   &           $>$ 3 GeV   &           $>$ 4 GeV   &           $>$ 5 GeV  \\
-+
+\hline
-+
+      data   &  0.109 $\pm$ 0.0005   &  0.043 $\pm$ 0.0003   &  0.022 $\pm$ 0.0002   &  0.013 $\pm$ 0.0002   &  0.009 $\pm$ 0.0002  \\
-+
+        mc   &  0.109 $\pm$ 0.0014   &  0.042 $\pm$ 0.0009   &  0.020 $\pm$ 0.0006   &  0.012 $\pm$ 0.0005   &  0.008 $\pm$ 0.0004  \\
-+
+   data/mc   &     1.00 $\pm$ 0.01   &     1.04 $\pm$ 0.02   &     1.08 $\pm$ 0.04   &     1.13 $\pm$ 0.05   &     1.13 $\pm$ 0.06  \\
-+
-+
+\hline
-+
+\hline
-+
+$\mu$ + $\geq$1 jets   &           $>$ 1 GeV   &           $>$ 2 GeV   &           $>$ 3 GeV   &           $>$ 4 GeV   &           $>$ 5 GeV  \\
-+
+\hline
-+
+      data   &  0.106 $\pm$ 0.0004   &  0.043 $\pm$ 0.0003   &  0.023 $\pm$ 0.0002   &  0.014 $\pm$ 0.0002   &  0.010 $\pm$ 0.0001  \\
-+
+        mc   &  0.107 $\pm$ 0.0012   &  0.042 $\pm$ 0.0008   &  0.021 $\pm$ 0.0005   &  0.013 $\pm$ 0.0004   &  0.009 $\pm$ 0.0004  \\
-+
+   data/mc   &     1.00 $\pm$ 0.01   &     1.03 $\pm$ 0.02   &     1.07 $\pm$ 0.03   &     1.12 $\pm$ 0.04   &     1.17 $\pm$ 0.05  \\
-+
-+
+\hline
-+
+\hline
-+
+e + $\geq$2 jets   &           $>$ 1 GeV   &           $>$ 2 GeV   &           $>$ 3 GeV   &           $>$ 4 GeV   &           $>$ 5 GeV  \\
-+
+\hline
-+
+      data   &  0.115 $\pm$ 0.0012   &  0.049 $\pm$ 0.0008   &  0.026 $\pm$ 0.0006   &  0.017 $\pm$ 0.0005   &  0.012 $\pm$ 0.0004  \\
-+
+        mc   &  0.114 $\pm$ 0.0032   &  0.046 $\pm$ 0.0021   &  0.023 $\pm$ 0.0015   &  0.015 $\pm$ 0.0012   &  0.010 $\pm$ 0.0010  \\
-+
+   data/mc   &     1.01 $\pm$ 0.03   &     1.09 $\pm$ 0.05   &     1.13 $\pm$ 0.08   &     1.09 $\pm$ 0.09   &     1.14 $\pm$ 0.12  \\
-+
-+
+\hline
-+
+\hline
-+
+$\mu$ + $\geq$2 jets   &           $>$ 1 GeV   &           $>$ 2 GeV   &           $>$ 3 GeV   &           $>$ 4 GeV   &           $>$ 5 GeV  \\
-+
+\hline
-+
+      data   &  0.111 $\pm$ 0.0010   &  0.048 $\pm$ 0.0007   &  0.026 $\pm$ 0.0005   &  0.018 $\pm$ 0.0004   &  0.013 $\pm$ 0.0004  \\
-+
+        mc   &  0.114 $\pm$ 0.0027   &  0.046 $\pm$ 0.0018   &  0.024 $\pm$ 0.0013   &  0.014 $\pm$ 0.0010   &  0.010 $\pm$ 0.0009  \\
-+
+   data/mc   &     0.98 $\pm$ 0.03   &     1.04 $\pm$ 0.04   &     1.12 $\pm$ 0.07   &     1.26 $\pm$ 0.10   &     1.30 $\pm$ 0.12  \\
-+
-+
+\hline
-+
+\hline
-+
+e + $\geq$3 jets   &           $>$ 1 GeV   &           $>$ 2 GeV   &           $>$ 3 GeV   &           $>$ 4 GeV   &           $>$ 5 GeV  \\
-+
+\hline
-+
+      data   &  0.122 $\pm$ 0.0030   &  0.058 $\pm$ 0.0022   &  0.034 $\pm$ 0.0017   &  0.023 $\pm$ 0.0014   &  0.017 $\pm$ 0.0012  \\
-+
+        mc   &  0.125 $\pm$ 0.0080   &  0.060 $\pm$ 0.0057   &  0.032 $\pm$ 0.0043   &  0.023 $\pm$ 0.0036   &  0.017 $\pm$ 0.0031  \\
-+
+   data/mc   &     0.98 $\pm$ 0.07   &     0.97 $\pm$ 0.10   &     1.06 $\pm$ 0.15   &     1.01 $\pm$ 0.17   &     1.01 $\pm$ 0.20  \\
-+
-+
+\hline
-+
+\hline
-+
+$\mu$ + $\geq$3 jets   &           $>$ 1 GeV   &           $>$ 2 GeV   &           $>$ 3 GeV   &           $>$ 4 GeV   &           $>$ 5 GeV  \\
-+
+\hline
-+
+      data   &  0.121 $\pm$ 0.0025   &  0.055 $\pm$ 0.0018   &  0.033 $\pm$ 0.0014   &  0.022 $\pm$ 0.0011   &  0.017 $\pm$ 0.0010  \\
-+
+        mc   &  0.125 $\pm$ 0.0070   &  0.053 $\pm$ 0.0047   &  0.027 $\pm$ 0.0035   &  0.018 $\pm$ 0.0028   &  0.013 $\pm$ 0.0024  \\
-+
+   data/mc   &     0.97 $\pm$ 0.06   &     1.05 $\pm$ 0.10   &     1.20 $\pm$ 0.16   &     1.19 $\pm$ 0.20   &     1.28 $\pm$ 0.25  \\
-+
-+
+\hline
-+
+\hline
-+
+e + $\geq$4 jets   &           $>$ 1 GeV   &           $>$ 2 GeV   &           $>$ 3 GeV   &           $>$ 4 GeV   &           $>$ 5 GeV  \\
-+
+\hline
-+
+      data   &  0.130 $\pm$ 0.0079   &  0.069 $\pm$ 0.0060   &  0.044 $\pm$ 0.0048   &  0.031 $\pm$ 0.0041   &  0.021 $\pm$ 0.0034  \\
-+
+        mc   &  0.136 $\pm$ 0.0219   &  0.045 $\pm$ 0.0134   &  0.027 $\pm$ 0.0108   &  0.022 $\pm$ 0.0093   &  0.016 $\pm$ 0.0084  \\
-+
+   data/mc   &     0.96 $\pm$ 0.17   &     1.55 $\pm$ 0.48   &     1.62 $\pm$ 0.67   &     1.41 $\pm$ 0.63   &     1.28 $\pm$ 0.68  \\
-+
-+
+\hline
-+
+\hline
-+
+$\mu$ + $\geq$4 jets   &           $>$ 1 GeV   &           $>$ 2 GeV   &           $>$ 3 GeV   &           $>$ 4 GeV   &           $>$ 5 GeV  \\
-+
+\hline
-+
+      data   &  0.136 $\pm$ 0.0067   &  0.064 $\pm$ 0.0048   &  0.041 $\pm$ 0.0039   &  0.029 $\pm$ 0.0033   &  0.024 $\pm$ 0.0030  \\
-+
+        mc   &  0.127 $\pm$ 0.0187   &  0.062 $\pm$ 0.0134   &  0.042 $\pm$ 0.0113   &  0.034 $\pm$ 0.0104   &  0.028 $\pm$ 0.0095  \\
-+
+   data/mc   &     1.07 $\pm$ 0.17   &     1.04 $\pm$ 0.24   &     0.98 $\pm$ 0.28   &     0.85 $\pm$ 0.28   &     0.87 $\pm$ 0.32  \\
-+
+\hline
-+
+\hline
-+
-+
+\end{tabular}
-+
+\end{center}
-+
+\end{table}
-+
-+
-+
-+
+%Figure.~\ref{fig:reliso} compares the relative track isolation
-+
+%for events with a track with $\pt > 10~\GeV$ in addition to a selected
-+
+%muon for $\Z+4$ jet events and various \ttll\ components. The
-+
+%isolation distributions show significant differences, particularly
-+
+%between the leptons from a \W\ or \Z\ decay and the tracks arising
-+
+%from $\tau$ decays. As can also be seen in the figure, the \pt\
-+
+%distribution for the various categories of tracks is different, where
-+
+%the decay products from $\tau$s are significantly softer. Since the
-+
+%\pt\ enters the denominator of the isolation definition and hence
-+
+%alters the isolation variable...
-+
-+
+%\begin{figure}[hbt]
-+
+%  \begin{center}
-+
+%       \includegraphics[width=0.5\linewidth]{plots/pfiso_njets4_log.png}%
-+
+%       \includegraphics[width=0.5\linewidth]{plots/pfpt_njets4.png}
-+
+%       \caption{
-+
+%         \label{fig:reliso}%\protect
-+
+%          Comparison of relative track isolation variable for PF cand probe in Z+jets and ttbar
-+
+%          Z+Jets and ttbar dilepton have similar isolation distributions
-+
+%          ttbar with leptonic and single prong taus tend to be less
-+
+%          isolated. The difference in the isolation can be attributed
-+
+%          to the different \pt\ distribution of the samples, since
-+
+%          $\tau$ decay products tend to be softer than leptons arising
-+
+%          from \W\ or \Z\ decays.}
-+
+%      \end{center}
-+
+%\end{figure}
-+
-+
+%       \includegraphics[width=0.5\linewidth]{plots/pfabsiso_njets4_log.png}
-+
-+
-+
+%BEGIN SECTION TO WRITE OUT
-+
+%In detail, the procedure to correct the dilepton background is:
-+
-+
+%\begin{itemize}
-+
+%\item Using tag-and-probe studies, we plot the distribution of {\bf absolute} track isolation for identified probe electrons
-+
+%and muons {\bf TODO: need to compare the e vs. $\mu$ track iso distributions, they might differ due to e$\to$e$\gamma$}.
-+
+%\item We verify that the distribution of absolute track isolation does not depend on the \pt\ of the probe lepton.
-+
+%This is due to the fact that this isolation is from ambient PU and jet activity in the event, which is uncorrelated with
-+
+%the lepton \pt {\bf TODO: verify this in data and MC.}.
-+
+%\item Our requirement is {\bf relative} track isolation $<$ 0.1. For a given \ttll\ MC event, we determine the \pt of the 2nd
-+
+%lepton and translate this to find the corresponding requirement on the {\bf absolute} track isolation, which is simply $0.1\times$\pt.
-+
+%\item We measure the efficiency to satisfy this requirement in data and MC, and define a scale-factor $SF_{\epsilon(trk)}$ which
-+
+%is the ratio of the data-to-MC efficiencies. This scale-factor is applied to the \ttll\ MC event.
-+
+%\item {\bf THING 2 we are unsure about: we can measure this SF for electrons and for muons, but we can't measure it for hadronic
-+
+%tracks from $\tau$ decays. Verena has showed that the absolute track isolation distribution in hadronic $\tau$ tracks is harder due
-+
+%to $\pi^0\to\gamma\gamma$ with $\gamma\to e^+e^-$.}
-+
+%\end{itemize}
-+
+%END SECTION TO WRITE OUT
-+
-+
-+
+{\bf fix me: What you have written in the next paragraph does not explain how $\epsilon_{fake}$ is measured.
-+
+Why not measure $\epsilon_{fake}$ in the b-veto region?}
-+
-+
+%A measurement of the $\epsilon_{fake}$ in data is non-trivial. However, it is
-+
+%possible to correct for differences in the $\epsilon_{fake}$ between data and MC by
-+
+%applying an additional scale factor for the single lepton background
-+
+%alone, using the sample in the \mt\ peak region. This scale factor is determined after applying the isolated track
-+
+%veto and after subtracting the \ttll\ component, corrected for the
-+
+%isolation efficiency derived previously.
-+
+%As shown in Figure~\ref{fig:vetoeffcomp}, the efficiency for selecting an
-+
+%isolated track in single lepton events is independent of \mt\, so the use of
-+
+%an overall scale factor is justified to estimate the contribution in
-+
+%the \mt\ tail.
-+
+%
-+
+%\begin{figure}[hbt]
-+
+%  \begin{center}
-+
+%       \includegraphics[width=0.5\linewidth]{plots/vetoeff_comp.png}
-+
+%       \caption{
-+
+%         \label{fig:vetoeffcomp}%\protect
-+
+%          Efficiency for selecting an isolated track comparing
-+
+%          single lepton \ttlj\ and dilepton \ttll\ events in MC and
-+
+%          data as a function of \mt. The
-+
+%          efficiencies in \ttlj\ and \ttll\ exhibit no dependence on
-+
+%          \mt\, while the data ranges between the two. This behavior
-+
+%          is expected since the low \mt\ region is predominantly \ttlj, while the
-+
+%          high \mt\ region contains mostly \ttll\ events.}
-+
+%      \end{center}
-+
+%\end{figure}
-+
-+
+\subsection{Summary of uncertainties}
-+
+\label{sec:bgunc-bottomline}.
-+
-+
+THIS NEEDS TO BE WRITTEN

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Comparing UserCode/benhoob/cmsnotes/StopSearch/systematics.tex (file contents): Revision 1.3 by vimartin, Fri Jun 29 03:00:35 2012 UTC vs. Revision 1.11 by benhoob, Mon Oct 8 09:07:01 2012 UTC

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Comparing UserCode/benhoob/cmsnotes/StopSearch/systematics.tex (file contents):
Revision 1.3 by vimartin, Fri Jun 29 03:00:35 2012 UTC vs.
Revision 1.11 by benhoob, Mon Oct 8 09:07:01 2012 UTC