ViewVC Help
View File | Revision Log | Show Annotations | Root Listing
root/cvsroot/UserCode/benhoob/cmsnotes/ZMet2012/bkg.tex
(Generate patch)

Comparing UserCode/benhoob/cmsnotes/ZMet2012/bkg.tex (file contents):
Revision 1.2 by benhoob, Wed Jun 27 16:38:31 2012 UTC vs.
Revision 1.3 by benhoob, Wed Jun 27 20:41:25 2012 UTC

# Line 20 | Line 20 | This background is estimated from MC as
20   \subsection{Estimating the \zjets\ Background with \MET\ Templates}
21   \label{sec:bkg_zjets}
22  
23 < The premise of this data driven technique is that \MET in \zjets\ events
23 > The premise of this data driven technique is that \MET\ in \zjets\ events
24   is produced by the hadronic recoil system and {\it not} by the leptons making up the Z.
25   Therefore, the basic idea of the \MET\ template method is to measure the \MET\ distribution in
26   a control sample which has no true MET and the same general attributes regarding
# Line 39 | Line 39 | to match the distribution of reconstruct
39  
40   To account for kinematic differences between the hadronic systems in the control vs. signal
41   samples, we measure the \MET\ distributions in the \gjets\ sample in bins of the number of jets
42 < and the scalar sum of jet transverse energies (\Ht). These \MET distributions are normalized to unit area to form ``MET templates''.
43 < The prediction of the MET in each \Z event is the template which corresponds to the \njets\ and
44 < \Ht in the \zjets\ event. The prediction for the \Z sample is simply the sum of all such templates.
45 < These templates are displayed in App.~\ref{app:templates}.
42 > and the scalar sum of jet transverse energies (\Ht). These \MET\ templates are extracted separately from the 5 single photon
43 > triggers with thresholds 22, 36, 50, 75, and 90 GeV, so that the templates are effectively binned in photon \pt.
44 > All \MET distributions are normalized to unit area to form ``MET templates''.
45 > The prediction of the MET in each \Z event is the template which corresponds to the \njets,
46 > \Ht, and Z \pt in the \zjets\ event. The prediction for the \Z sample is simply the sum of all such templates.
47 > All templates are displayed in App.~\ref{app:templates}.
48  
49   While there is in principle a small contribution from backgrounds other than \zjets\ in the preselection regions,
50   this contribution is only $\approx$3\% ($\approx$2\%) of the total sample in the inclusive search (targeted search),
51 < as shown in Table~\ref{table:zyields_2j} (Table~\ref{table:zyields_2j_targeted}, and is therefore negligible compared to the total
51 > as shown in Table~\ref{table:zyields_2j} (Table~\ref{table:zyields_2j_targeted}), and is therefore negligible compared to the total
52   background uncertainty.
53  
54   \subsection{Estimating the Flavor-Symmetric Background with e$\mu$ Events}
# Line 69 | Line 71 | Hence we define:
71   \item $N_{e\mu}^{\rm{trig}} = \epsilon_{e\mu}^{\rm{trig}}N_{e\mu}^{\rm{offline}}$.
72   \end{itemize}
73  
74 < Here $N_{\ell\ell}^{\rm{trig}}$ denotes the number of selected events in the $\ell\ell$ channel passing the offline and trigger selection
75 < (in other words, the number of recorded events), $\epsilon_{\ell\ell}^{\rm{trig}}$ is the trigger efficiency, and
76 < $N_{e\mu}^{\rm{offline}}$ is the number of events that would have passed the offline selection if the trigger had an efficiency of 100\%.
74 > Here $N_{\ell\ell}^{\rm{trig}}$ denotes the number of selected Z events in the $\ell\ell$ channel passing the offline and trigger selection
75 > (in other words, the number of recorded and selected events), $\epsilon_{\ell\ell}^{\rm{trig}}$ is the trigger efficiency, and
76 > $N_{\ell\ell}^{\rm{offline}}$ is the number of events that would have passed the offline selection if the trigger had an efficiency of 100\%.
77   Thus we calculate the quantity:
78  
79   \begin{equation}
# Line 85 | Line 87 | The predicted yields in the ee and $\mu\
87  
88   \begin{itemize}
89   \item $N_{ee}^{\rm{predicted}}    = \frac {N_{e\mu}^{\rm{trig}}} {\epsilon_{e\mu}^{\rm{trig}}} \frac {\epsilon_{ee}^{\rm{trig}}} {2 R_{\mu e}}
90 < = \frac{N_{e\mu}^{\rm{trig}}}{0.92}\frac{0.95}{2\times1.26} = (0.41\pm0.04) \times N_{e\mu}^{\rm{trig}}$ ,
90 > = \frac{N_{e\mu}^{\rm{trig}}}{0.92}\frac{0.95}{2\times1.26} = (0.41\pm0.05) \times N_{e\mu}^{\rm{trig}}$ ,
91   \item $N_{\mu\mu}^{\rm{predicted}} = \frac {N_{e\mu}^{\rm{trig}}} {\epsilon_{e\mu}^{\rm{trig}}} \frac {\epsilon_{\mu\mu}^{\rm{trig}} R_{\mu e}}  {2}
92 < = \frac {N_{e\mu}^{\rm{trig}}} {0.95} \frac {0.88 \times 1.26}{2} = (0.58\pm0.06) \times N_{e\mu}^{\rm{trig}}$,
92 > = \frac {N_{e\mu}^{\rm{trig}}} {0.95} \frac {0.88 \times 1.26}{2} = (0.58\pm0.07) \times N_{e\mu}^{\rm{trig}}$,
93   \end{itemize}
94  
95   and the predicted yield in the combined ee and $\mu\mu$ channel is simply the sum of these two predictions:
# Line 96 | Line 98 | and the predicted yield in the combined
98   \item $N_{ee+\mu\mu}^{\rm{predicted}} = (0.99\pm0.06)\times N_{e\mu}^{\rm{trig}}$.
99   \end{itemize}
100  
101 < Note that the relative uncertainty in the combined ee and $\mu\mu$ prediction is smaller than the those for the individual ee and $\mu\mu$ predictions
101 > Note that the relative uncertainty in the combined ee and $\mu\mu$ prediction is smaller than those for the individual ee and $\mu\mu$ predictions
102   because the uncertainty in $R_{\mu e}$ cancels when summing the ee and $\mu\mu$ predictions. {\bf N.B. these uncertainties are preliminary}.
103  
104   To improve the statistical precision of the FS background estimate, we remove the requirement that the e$\mu$ lepton pair falls in the Z mass window.
# Line 179 | Line 181 | values in WZ and ZZ events arise from hi
181   and we therefore check that the MC does a reasonable job of reproducing the \pt distributions of the
182   leptonically decaying \Z. While the inclusive WZ yields are in reasonable agreement, we observe
183   an excess in data in events with at least 2 jets, corresponding to the jet multiplicity requirement
184 < in our preselection. We observe 60 events in data while the MC predicts $34\pm5.2$~(stat)), representing an excess of 78\%,
185 < as indicated in Table~\ref{tab:wz2j}.
184 < We note some possible causes for this discrepancy:
184 > in our preselection. We observe 60 events in data while the MC predicts $34\pm5.2$~(stat), representing an excess of 78\%,
185 > as indicated in Table~\ref{tab:wz2j}. We note some possible contributions to this discrepancy:
186  
187   \begin{itemize}
188  
# Line 196 | Line 197 | rate is typically under-estimated in the
197   on the \ttbar\ yield, if the \ttbar\ yield is doubled then the excess is reduced from 78\% to 57\%.
198  
199   \item Currently no attempt is made to reject jets from pile-up interactions, which may be responsible
200 < for some of this excess. To check this, we increase the jet \pt requirement to 40 GeV which
201 < helps to suppress PU jets and observe 39 events in data vs. an MC prediction of $25\pm5.2$~(stat),
200 > for some of the excess at large \njets. To check this, we increase the jet \pt threhsold to 40 GeV, which
201 > helps to suppress PU jets, and observe 39 events in data vs. an MC prediction of $25\pm5.2$~(stat),
202   decreasing the excess from 78\% to 58\%. In the future this may be improved by explicitly
203   requiring the jets to be consistent with originating from the signal primary vertex.
204  
# Line 210 | Line 211 | Based on these studies we currently asse
211   \caption{\label{tab:wz} Data and Monte Carlo yields passing the WZ preselection. }
212   \begin{tabular}{lccccc}
213   \hline
214 + \hline
215           Sample   &            ee    &        $\mu\mu$   &        e$\mu$   &          total  \\
216   \hline
217               WZ   & 58.9 $\pm$ 0.7   & 82.2 $\pm$ 0.8   &  4.0 $\pm$ 0.2   &145.1 $\pm$ 1.0  \\
# Line 233 | Line 235 | Based on these studies we currently asse
235   \caption{\label{tab:wz2j} Data and Monte Carlo yields passing the WZ preselection and \njets\ $>$ 2. }
236   \begin{tabular}{lccccc}
237   \hline
236         Sample   &            ee    &        $\mu\mu$   &        e$\mu$   &          total  \\
238   \hline
239 +         Sample   &            ee    &        $\mu\mu$   &        e$\mu$   &          total  \\
240   \hline
241               WZ   &  9.8 $\pm$ 0.3   & 13.3 $\pm$ 0.3   &  0.6 $\pm$ 0.1   & 23.6 $\pm$ 0.4  \\
242           \ttbar   &  0.2 $\pm$ 0.2   &  2.0 $\pm$ 0.9   &  2.2 $\pm$ 1.2   &  4.4 $\pm$ 1.5  \\
# Line 243 | Line 245 | Based on these studies we currently asse
245               WW   &  0.0 $\pm$ 0.0   &  0.0 $\pm$ 0.0   &  0.0 $\pm$ 0.0   &  0.1 $\pm$ 0.0  \\
246       single top   &  0.0 $\pm$ 0.0   &  0.0 $\pm$ 0.0   &  0.0 $\pm$ 0.0   &  0.0 $\pm$ 0.0  \\
247   \hline
248 <      tot SM MC   & 10.3 $\pm$ 0.3   & 20.8 $\pm$ 5.0   &  2.8 $\pm$ 1.2   & 33.8 $\pm$ 5.2  \\
247 < \hline
248 >    total SM MC   & 10.3 $\pm$ 0.3   & 20.8 $\pm$ 5.0   &  2.8 $\pm$ 1.2   & 33.8 $\pm$ 5.2  \\
249             data   &             23   &             32   &              5   &             60  \\
250   \hline
251   \hline
# Line 285 | Line 286 | Based on this we apply an uncertainty of
286   \caption{\label{tab:zz} Data and Monte Carlo yields for the ZZ preselection. }
287   \begin{tabular}{lccccc}
288   \hline
288         Sample   &             ee   &       $\mu\mu$   &         e$\mu$   &          total  \\
289   \hline
290 <
290 >         Sample   &             ee   &       $\mu\mu$   &         e$\mu$   &          total  \\
291   \hline
292               ZZ   &  6.6 $\pm$ 0.0   &  9.9 $\pm$ 0.0   &  0.4 $\pm$ 0.0   & 17.0 $\pm$ 0.1  \\
293               WZ   &  0.1 $\pm$ 0.0   &  0.2 $\pm$ 0.0   &  0.0 $\pm$ 0.0   &  0.3 $\pm$ 0.0  \\
# Line 297 | Line 297 | Based on this we apply an uncertainty of
297       single top   &  0.0 $\pm$ 0.0   &  0.0 $\pm$ 0.0   &  0.0 $\pm$ 0.0   &  0.0 $\pm$ 0.0  \\
298   \hline
299      total SM MC   &  6.7 $\pm$ 0.0   & 10.1 $\pm$ 0.1   &  0.5 $\pm$ 0.0   & 17.3 $\pm$ 0.1  \\
300 \hline
300             data   &             13   &             16   &              0   &             29  \\
301   \hline
303
302   \hline
303   \end{tabular}
304   \end{center}
# Line 310 | Line 308 | Based on this we apply an uncertainty of
308   \begin{center}
309   \includegraphics[width=1\linewidth]{plots/ZZ.pdf}
310   \caption{\label{fig:zz}\protect
311 < Data vs. MC comparisons for the $ZZ$ selection discussed in the text for \lumi.
312 < The number of jets, missing transverse energy, and $Z$ boson transverse momentum are displayed.
311 > Data vs. MC comparisons for the ZZ selection discussed in the text for \lumi.
312 > The number of jets, missing transverse energy, and Z boson transverse momentum are displayed.
313   }
314   \end{center}
315   \end{figure}
# Line 322 | Line 320 | The number of jets, missing transverse e
320   \subsection{Estimating the Rare SM Backgrounds with MC}
321   \label{sec:bkg_raresm}
322  
323 < {\bf TODO: list samples, yields in preselection region, and \MET distribution}
323 > {\bf TODO: list samples, yields in preselection region, and show \MET\ distribution}

Diff Legend

Removed lines
+ Added lines
< Changed lines
> Changed lines