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1 < \section{Overview and Analysis Strategy}
1 > \section{Overview and Strategy for Background Determination}
2   \label{sec:overview}
3  
4 + [THIS SECTION IS NOW MORE OR LESS OK.  NEED TO FIX THE ``XX'' IN
5 + FORWARD SECTION REFERENCES]
6 +
7   We are searching for a $t\bar{t}\chi^0\chi^0$ or $W b W \bar{b} \chi^0 \chi^0$ final state
8   (after top decay in the first mode, the final states are actually the same).  So to first order
9   this is ``$t\bar{t} +$ extra \met''.  
# Line 13 | Line 16 | initial analysis is simply a counting ex
16   The event selection is one-and-only-one high \pt\ isolated lepton, four or more jets, and
17   some moderate \met\ cut.  At least one of the jets has to be btagged to reduce $W+$ jets.
18   The event sample is then dominated by $t\bar{t}$, but there are also contributions from $W+$ jets,
19 < single top, dibosons, etc.
19 > single top, dibosons, as well as rare SM processes such as $ttW$.
20  
21 < In order to be sensitive to $\widetilde{t}\widetilde{t}$ production, the background in the $M_T$
22 < tail has to be controlled at the level of 10\% or better. So this is (almost) a precision measurement.
21 > % In order to be sensitive to $\widetilde{t}\widetilde{t}$ production, the background in the $M_T$
22 > % tail has to be controlled at the level of 10\% or better. So this is (almost) a precision measurement.
23  
24   The $t\bar{t}$ events in the $M_T$ tail can be broken up into two categories:
25   (i) $t\bar{t} \to \ell $+ jets and (ii) $t\bar{t} \to \ell^+ \ell^-$ where one of the two
# Line 27 | Line 30 | the total.  This is because in dileptons
30   is not bounded by $M_W$.  This is a very important point: while it is true that we are looking in
31   the tail of $M_T$, the bulk of the background events end up there not because of some exotic
32   \met\ reconstruction failure, but because of well understood physics processes.  This means that
33 < the background estimate can be taken from Monte Carlo (MC), after carefully accounting for possible
34 < data/MC differences.  Sophisticated fully ``data driven'' techniques are not really needed.
33 > the background estimate can be taken from Monte Carlo (MC)
34 > after carefully accounting for possible
35 > data/MC differences.  
36 >
37 > In Section XX we will describe the analysis of various Control Regions
38 > (CRs)  that are used to test the Monte Carlo model and, if necessary,
39 > to extract data/MC scale factors.  In this section we give a
40 > general description of the procedure.  The details of how the
41 > final background prediction is assembled are given in Section XX.
42 >
43 > The search is performed in a number of signal regions defined
44 > by minimum requirements on \met\  and $M_T$.  These signal
45 > regions are defined in Section XX.
46 >
47 > % Sophisticated fully ``data driven'' techniques are not really needed.
48  
49 < Another important point is that in order to minimize systematic uncertainties, the MC background
50 < predictions are always normalized to the bulk of the $t\bar{t}$ data, ie, events passing all of the
49 > One general point is that in order to minimize systematic uncertainties, the MC background
50 > predictions are whenever possible normalized to the bulk of the $t\bar{t}$ data, ie, events passing all of the
51   requirements but with $M_T \approx 80$ GeV.
52 < This removes uncertainties
52 > This (mostly) removes uncertainties
53   due to $\sigma(t\bar{t})$, lepton ID, trigger efficiency, luminosity, etc.  
54  
55 < The $\ell +$ jets background, which is dominated by
56 < $t\bar{t} \to \ell $+ jets, but also includes some $W +$ jets as well as single top,
57 < is estimated as follows:
58 < \begin{enumerate}
59 < \item We select a control sample of events passing all cuts, but anti-btagged, i.e. b-vetoed.  This
60 < sample is now dominated by $W +$ jets.  The sample is used to understand the
61 < $M_T$ tail in $\ell +$ jets processes.
62 < \item In MC we measure the ratio of the number of $\ell +$ jets events in the $M_T$ tail to
63 < the number of events with $M_T \approx$ 80 GeV.  This ratio turns out to be pretty much the
64 < same for all sources of $\ell +$ jets.
65 < \item In data we measure the same ratio but after correcting for the $t\bar{t} \to$ dilepton
66 < contribution, as well as dibosons etc.  The dilepton contribution is taken from MC after
67 < the correction described below.  
68 < \item We compare the two ratios, as well as the shapes of the data and MC $M_T$ distributions.
69 < If they do not agree, we try to figure out why and fix it.  If they agree well enough, we define a
70 < data-to-MC scale factor (SF) which is the ratio of the  ratios defined in step 2 and 3, keeping track of the
71 < uncertainty.  
72 < \item We next perform the full selection in $t\bar{t} \to \ell +$ jets MC, and measure this ratio
73 < again (which should be the same as that in step 2).
74 < \item
75 < We perform the full selection in data. We count the number of events with $M_T \approx 80$ GeV, after subtracting off the dilepton contribution,
76 <  and multiply this count by the ratio from step 5 times the data/MC scale factor from step 4.
77 < %We count the events with $M_T \approx 80$ GeV, we
78 < %subtract off the dilepton contribution, we multiply the subtracted event count by the ratio from step 5 (or from
79 < %step 2), and also by the data/MC SF from step 4.  
80 < The result is the prediction for the $\ell +$ jets BG in the $M_T$ tail.
81 < \end{enumerate}
55 > \subsection{$\ell +$ jets background}
56 > \label{sec:ljbg-general}
57 >
58 > The $\ell +$ jets background is dominated by
59 > $t\bar{t} \to \ell $+ jets, but also includes some $W +$ jets as well as single top.
60 > The MC input used in the background estimation
61 > is the ratio of the number of events with $M_T$ in the signal region
62 > to the number of events with $M_T \approx 80$ GeV.
63 > This ratio is (possibly) corrected by a data/MC scale factor obtained
64 > from a study of CRs, as outlined below.
65 >
66 > Note that the ratio described above is actually different for
67 > $t\bar{t}$/single top and $W +$ jets.  This is because in $W$ events
68 > there is a significant contribution to the $M_T$ tail from very off-shell
69 > $W$.
70 > This contribution is much smaller in top events because $M(\ell \nu)$
71 > cannot excees $M_{top}-M_b$.
72 >
73 > For $W +$ jets the ability of the Monte Carlo to model this ratio
74 > ($R_{wjet}$) is tested in a sample of $\ell +$ jets enriched in
75 > $W +$ jets by the application of a b-veto.
76 > The equivalent ratio for top events ($R_{top}$) is validated in a sample of well
77 > identified $Z \to \ell \ell$ with one lepton added to the \met\
78 > calculation.
79 > This sample is well suited to testing the resolution effects on
80 > the $M_T$ tail, since off-shell effects are eliminated by the $Z$-mass
81 > requirement.
82 >
83 > Note that the fact that the ratios are different for
84 > $t\bar{t}$/single top and $W +$ jets introduces a systematic
85 > uncertainty in the background calculation because one needs
86 > to know the relative fractions of these two components in
87 > $M_T \approx 80$ GeV lepton $+$ jets sample.
88  
89 < Steps 1-4 above are all measurements on the b-vetoed samples in data and/or MC. Steps 5 and 6 are performed on the b-tagged sample.
89 >
90 > \subsection{Dilepton background}
91 > \label{sec:dil-general}
92  
93   To suppress dilepton backgrounds, we veto events with an isolated track of \pt $>$ 10 GeV.
94   Being the common feature for electron, muon, and one-prong
# Line 98 | Line 122 | Monte Carlo studies indicate that these
122   We note that at present we do not attempt to veto 3-prong tau decays as they are only 16\% of the total dilepton background according to the MC.
123  
124   The high $M_T$ dilepton backgrounds come from MC, but their rate is normalized to the
125 < $M_T \approx 80$ GeV peak.  In order to perform this normalization in data, the $W +$ jets
126 < events in the $M_T$ peak have to be subtracted off.  This introduces a systematic uncertainty.
125 > $M_T \approx 80$ GeV peak.  In order to perform this normalization in
126 > data, the non-$t\bar{t}$ (eg, $W +$ jets)
127 > events in the $M_T$ peak have to be subtracted off.  This also introduces a systematic uncertainty.
128  
129   There are two types of effects that can influence the MC dilepton prediction: physics effects
130   and instrumental effects.  We discuss these next, starting from physics.
# Line 139 | Line 164 | Note that JES uncertainties are effectiv
164   %The sample of events failing the last isolated track veto is an important control sample to
165   %check that we are doing the right thing.
166  
167 + \subsection{Other backgrounds}
168 + \label{sec:other-general}
169 + Other backgrounds are $tW$, $ttV$, dibosons, tribosons, Drell Yan.
170 + These  are small.  They are taken from MC with appropriate scale
171 + factors
172 + for trigger efficiency, etc.
173 +
174 +
175 + \subsection{Future improvements}
176 + \label{sec:improvements-general}
177   Finally, there are possible improvements to this basic analysis strategy that can be added in the future:
178   \begin{itemize}
179   \item Move from counting experiment to shape analysis.  But first, we need to get the counting

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