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Revision 1.7 by claudioc, Thu Oct 11 07:33:42 2012 UTC vs.
Revision 1.12 by linacre, Thu Oct 18 21:21:58 2012 UTC

# Line 11 | Line 11 | mass ($M_T$), since except for resolutio
11   initial analysis is simply a counting experiment in the tail of the $M_T$ distribution.  
12  
13   The event selection is one-and-only-one high \pt\ isolated lepton, four or more jets, and
14 < an \met\ cut.  At least one of the jets has to be btagged to reduce $W+$ jets.
14 > an \met\ cut.  At least one of the jets has to be b tagged to reduce $W+$ jets.
15   The event sample is then dominated by $t\bar{t}$, but there are also contributions from $W+$ jets,
16   single top, dibosons, as well as rare SM processes such as $ttW$.
17  
# Line 19 | Line 19 | single top, dibosons, as well as rare SM
19   % tail has to be controlled at the level of 10\% or better. So this is (almost) a precision measurement.
20  
21   The $t\bar{t}$ events in the $M_T$ tail can be broken up into two categories:
22 < (i) $t\bar{t} \to \ell $+ jets and (ii) $t\bar{t} \to \ell^+ \ell^-$ where one of the two
22 > (i) $t\bar{t} \to \ell $+ jets, and (ii) $t\bar{t} \to \ell^+ \ell^-$ where one of the two
23   leptons is not found by the second-lepton-veto (here the second lepton can be a hadronically
24   decaying $\tau$).
25 < For a reasonable $M_T$ cut, say $M_T >$ 150 GeV, the dilepton background is of order 80\% of
25 > For a reasonable $M_T$ cut, say $M_T >$ 150 GeV, the dilepton background is approximately 70\% of
26   the total.  This is because in dileptons there are two neutrinos from $W$ decay, thus $M_T$
27   is not bounded by $M_W$.  This is a very important point: while it is true that we are looking in
28   the tail of $M_T$, the bulk of the background events end up there not because of some exotic
# Line 46 | Line 46 | final background prediction is assembled
46   % Sophisticated fully ``data driven'' techniques are not really needed.
47  
48   One general point is that in order to minimize systematic uncertainties, the MC background
49 < predictions are whenever possible normalized to the bulk of the $t\bar{t}$ data, ie, events passing all of the
49 > predictions are whenever possible normalized to the bulk of the $t\bar{t}$ data, i.e., events passing all of the
50   requirements but with $M_T \approx 80$ GeV.
51   This (mostly) removes uncertainties
52   due to $\sigma(t\bar{t})$, lepton ID, trigger efficiency, luminosity, etc.  
# Line 65 | Line 65 | from a study of CRs, as outlined below.
65   Note that the ratio described above is actually different for
66   $t\bar{t}$/single top and $W +$ jets.  This is because in $W$ events
67   there is a significant contribution to the $M_T$ tail from very off-shell
68 < $W$.
68 > $W$s.
69   This contribution is much smaller in top events because $M(\ell \nu)$
70 < cannot excees $M_{top}-M_b$.
70 > cannot exceed $M_{top}-M_b$. Therefore the large \mt\ tail in
71 > $t\bar{t}$/single top is dominated by jet resolution effects,
72 > while for \wjets\ events the large \mt\ tail is dominated by off-shell W production.
73 >
74 >
75  
76   For $W +$ jets the ability of the Monte Carlo to model this ratio
77 < ($R_{wjet}$) is tested in a sample of $\ell +$ jets enriched in
77 > ($R_{wjet}$) is validated in a sample of $\ell +$ jets enriched in
78   $W +$ jets by the application of a b-veto.
79 < The equivalent ratio for top events ($R_{top}$) is validated in a sample of well
79 > The equivalent ratio for top events ($R_{top}$) is tested in a sample of well
80   identified $Z \to \ell \ell$ with one lepton added to the \met\
81   calculation.
82   This sample is well suited to testing the resolution effects on
# Line 83 | Line 87 | Note that the fact that the ratios are d
87   $t\bar{t}$/single top and $W +$ jets introduces a systematic
88   uncertainty in the background calculation because one needs
89   to know the relative fractions of these two components in
90 < $M_T \approx 80$ GeV lepton $+$ jets sample.
90 > the $M_T \approx 80$ GeV lepton $+$ jets sample.
91  
92  
93   \subsection{Dilepton background}
94   \label{sec:dil-general}
95  
96 < To suppress dilepton backgrounds, we veto events with an isolated track of \pt $>$ 10 GeV.
96 > To suppress dilepton backgrounds, we veto events with an isolated track of \pt\ $>$ 10 GeV (see Sec.~\ref{sec:tkveto} for details).
97   Being the common feature for electron, muon, and one-prong
98   tau decays, this veto is highly efficient for rejecting
99   $t\bar{t}$ to dilepton events. The remaining dilepton background can be classified into the following categories:
# Line 101 | Line 105 | $t\bar{t}$ to dilepton events. The remai
105   %\item 1-prong hadronic tau decay
106   %\item $e$ or $\mu$ possibly from $\tau$ decay
107   %\end{itemize}
108 < %We have currently no veto against 3-prong taus.  For the other two categories, we explicitely
108 > %We have currently no veto against 3-prong taus.  For the other two categories, we explicitly
109   %veto events %with additional electrons and muons above 10 GeV , and we veto events
110   %with an isolated track of \pt\ $>$ 10 GeV.  This rejects electrons and muons (either from $W\to e/\mu$ or
111   %$W\to \tau\to e/\mu$) and 1-prong tau decays.
112   %(it turns out that the explicit $e$ or $\mu$ veto is redundant with the isolated track veto).
113   %Therefore the latter two categories can be broken into
114   \begin{itemize}
115 < \item lepton is out of acceptance $(|\eta| > 2.50)$
115 > \item lepton is out of acceptance $(|\eta| > 2.5)$
116   \item lepton has \pt\ $<$ 10 GeV, and is inside the acceptance
117   \item lepton has \pt\ $>$ 10 GeV, is inside the acceptance, but survives the additional isolated track veto
118   \end{itemize}
# Line 116 | Line 120 | $t\bar{t}$ to dilepton events. The remai
120   %Monte Carlo studies indicate that there is no dominant contribution: it is ``a little bit of this,
121   %and a little bit of that''.
122  
123 < The last category includes 3-prong tau decays as well as electrons and muons from W decay that fail the isolation requirement.
124 < Monte Carlo studies indicate that these three components populate the $M_T$ tail in the proportions of roughly  6\%, 47\%, 47\%.
125 < 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 > The last category includes 1-prong and 3-prong hadronic tau decays, as well as electrons and muons either from direct W decay or via W$\to\tau\to\ell$ decay
124 > that fail the isolation requirement.
125 > % HOOBERMAN: commenting out for now
126 > %Monte Carlo studies indicate that these three components populate the $M_T$ tail in the proportions of roughly  6\%, 47\%, 47\%.
127 > We note that at present we do not attempt to veto 3-prong tau decays as they are about 15\% of the total dilepton background according to the MC.
128  
129 < The high $M_T$ dilepton backgrounds come from MC, but their rate is normalized to the
129 > The high $M_T$ dilepton background predictions come from MC, but their rate is normalized to the
130   $M_T \approx 80$ GeV peak.  In order to perform this normalization in
131 < data, the non-$t\bar{t}$ (eg, $W +$ jets)
126 < events in the $M_T$ peak have to be subtracted off.  This also introduces a systematic uncertainty.
131 > data, the rare background events in the $M_T$ peak are subtracted off.  This also introduces a systematic uncertainty.
132  
133   There are two types of effects that can influence the MC dilepton prediction: physics effects
134   and instrumental effects.  We discuss these next, starting from physics.
135  
136 < First of all, many of our $t\bar{t}$ MC samples (eg: MadGraph) have
136 > First of all, many of our $t\bar{t}$ MC samples (e.g. MadGraph) have
137   BR$(W \to \ell \nu)=\frac{1}{9} = 0.1111$.
138   PDG says BR$(W \to \ell \nu) = 0.1080 \pm 0.0009$.  This difference matters, so the $t\bar{t}$ MC
139   must be corrected to account for this.
140  
141 < Second, our selection is $\ell +$ 4 or more jets.  A dilepton event passes the selection only if there are
141 > Second, our selection is $\ell +4$ or more jets.  A dilepton event passes the selection only if there are
142   two additional jets from ISR, or one jet from ISR and one jet which is reconstructed from the
143   unidentified lepton, {\it e.g.}, a three-prong tau.  Therefore, all MC dilepton $t\bar{t}$ samples used
144   in the analysis must have their jet multiplicity corrected (if necessary) to agree with what is
145   seen in $t\bar{t}$ data.  We use a data control sample of well identified dilepton events with
146 < \met\ and at least two jets as a template to ``adjust'' the $N_{jet}$ distribution of the $t\bar{t} \to$
146 > \met\ and at least one jet (including at least one b-tag) as a template to ``adjust'' the $N_{jet}$ distribution of the $t\bar{t} \to$
147   dileptons MC samples.
148  
149   The final physics effect has to do with the modeling of $t\bar{t}$ production and decay.  Different
# Line 149 | Line 154 | and $N_{jet}$ dependence, are compared t
154   uncertainty associated with the $t\bar{t}$ generator modeling.
155  
156   The main instrumental effect is associated with the efficiency of the isolated track veto.
157 < We use tag-and-probe to compare the isolated track veto performance in $Z + 4$ jet data and
158 < MC, and we extract corrections if necessary.  Note that the performance of the isolated track veto
157 > We use tag-and-probe to compare the isolated track veto performance in $Z + 4$ jets data and
158 > MC.  Note that the performance of the isolated track veto
159   is not exactly the same on $e/\mu$ and on one prong hadronic tau decays.  This is because
160   the pions from one-prong taus are often accompanied by $\pi^0$'s that can then result in extra
161 < tracks due to phton conversions.  We let the simulation take care of that.  
161 > tracks due to photon conversions.  We let the simulation take care of that.  
162   Note that JES uncertainties are effectively ``calibrated away'' by the $N_{jet}$ rescaling described above.  
163  
164   %Similarly, at the moment
# Line 165 | Line 170 | Note that JES uncertainties are effectiv
170  
171   \subsection{Other backgrounds}
172   \label{sec:other-general}
173 < Other backgrounds are $tW$, $ttV$, dibosons, tribosons, Drell Yan.
173 > Other backgrounds are $tW$, $ttV$, dibosons, tribosons, and Drell Yan.
174   These  are small.  They are taken from MC with appropriate scale
175 < factors
171 < for trigger efficiency, etc.
175 > factors for trigger efficiency, and reweighting to match the distribution of reconstructed primary vertices in data.
176  
177  
178   \subsection{Future improvements}

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