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Committed: Thu Nov 11 16:22:13 2010 UTC (14 years, 6 months ago) by claudioc
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# Content
1 \section{Event Preselection}
2 \label{sec:eventSel}
3 The purpose of the preselection is to define a data sample rich
4 in $t\bar{t} \to$ dileptons. We compare the kinematical
5 properties of this sample with expectations from $t\bar{t}$
6 Monte Carlo.
7
8 The preselection is based on the
9 $t\bar{t}$ analysis~\cite{ref:top}.
10 We select events with two opposite sign isolated
11 leptons ($ee$, $e\mu$, or $\mu\mu$); one of the leptons must
12 have $P_T > 20$ GeV,
13 the other one must have $P_T > 10$ GeV. Events consistent with $Z$ are rejected.
14 In case of events with
15 more than two such leptons, we select the pair that maximizes the scalar
16 sum of lepton $P_T$'s.
17 There must be two JPT
18 jets of $P_T > 30$ GeV and $|\eta| < 2.5$; the scalar sum of the
19 $P_T$ of all such jets must exceed 100 GeV; jets must pass
20 {\tt caloJetId} and be separated by $\Delta R >$ 0.4 from any
21 lepton passing the selection.
22 Finally $\met > 50$ GeV (we use tcMet). More details are given in the subsections below.
23
24 \subsection{Event Cleanup}
25 \label{sec:cleanup}
26 \begin{itemize}
27 \item Scraping cut: if there are $\geq$ 10 tracks, require at
28 least 25\% of them to be high purity.
29 \item Require at least one good vertex:
30 \begin{itemize}
31 \item not fake
32 \item ndof $>$ 4
33 \item $|\rho| < 2$ cm
34 \item $|z| < 24$ cm.
35 \end{itemize}
36 \end{itemize}
37
38
39 \subsection{Muon Selection}
40 \label{sec:muon}
41
42 Muon candidates are RECO muon objects passing the following
43 requirements:
44 \begin{itemize}
45
46 \item $|\eta| < 2.4$.
47
48 \item Global Muon and Tracker Muon.
49
50 \item $\chi^2$/ndof of global fit $<$ 10.
51
52 \item At least 11 hits in the tracker fit.
53
54 \item Transverse impact parameter with respect to the beamspot $<$ 200 $\mu$m.
55
56 \item $Iso \equiv $ $E_T^{\rm iso}$/Max(20 GeV, $P_T$) $<$ 0.15.
57 $E_T^{\rm iso}$
58 is defined as the sum of transverse energy/momentum deposits in ecal,
59 hcal, and tracker, in a cone of 0.3.
60
61 \item At least one of the hits from the
62 standalone muon must be used in the global fit.
63
64 \item Require tracker $\Delta P_T/P_T < 0.1$. This cut was not in the original top analysis.
65 It is motivated by the observation of
66 poorly measured muons in data with large
67 relative $P_T$ uncertainty, giving significant contributions to the \met.
68 %{\color{red} This is not applied to the 11 pb iteration.}
69
70
71 \end{itemize}
72
73
74
75 \subsection{Electron Selection}
76 \label{sec:electron}
77
78 Electron candidates are RECO GSF electrons passing the following
79 requirements:
80
81 \begin{itemize}
82
83 % \item $P_T > 10$ GeV. (The $t\bar{t}$ analysis uses 20 GeV but for
84 % completeness we calculate FR down to 10 GeV).
85
86 \item $|\eta| < 2.5$.
87
88 \item SuperCluster $E_T > 10$ GeV.
89
90 \item The electron must be ecal seeded.
91
92 \item VBTF90 identification\cite{ref:vbtf}.
93
94 \item Transverse impact parameter with respect to the beamspot $<$ 400 $\mu$m.
95
96 \item $Iso \equiv $ $E_T^{\rm iso}$/Max(20 GeV, $P_T$) $<$ 0.15.
97 $E_T^{\rm iso}$
98 is defined as the sum of transverse energy/momentum deposits in ecal,
99 hcal, and tracker, in a
100 cone of 0.3. A 1 GeV pedestal is subtracted from the ecal energy
101 deposition in the EB, however the ecal energy is never allowed to
102 go negative.
103
104 \item Electrons with a tracker or global muon within $\Delta R$ of
105 0.1 are vetoed.
106
107 \item The number of missing expected inner hits must be less than
108 two\cite{ref:conv}.
109
110 \item Conversion removal via partner track finding: any electron
111 where an additional GeneralTrack is found with $Dist < 0.02$ cm
112 and $\Delta \cot \theta < 0.02$ is vetoed\cite{ref:conv}.
113
114 \item Cleaning for ECAL spike (aka Swiss-Cross cleaning) has been applied
115 at the reconstruction level (CMSSW 38x).
116
117 \end{itemize}
118
119 \subsection{Invariant mass requirement}
120 \label{sec:zveto}
121
122 We remove $e^+e^-$ and $\mu^+ \mu^-$ events with invariant
123 mass between 76 and 106 GeV. We also remove events
124 with invariant mass $<$ 10 GeV, since this kinematical region is
125 not well reprodced in CMS Monte Carlos.
126
127 In addition, we remove $Z \to \mu\mu\gamma$
128 candidates with the $\gamma$ collinear with one of the muons. This is
129 done as follows:
130 if the ecal energy associated with one of the muons is greater than 6 GeV,
131 we add this energy to the momentum of the initial muon, and we recompute
132 the $\mu\mu$ mass. If this mass is between 76 and 106 GeV, the event is rejected.
133
134
135 \subsection{Trigger Selection}
136 \label{sec:trigSel}
137
138 Because most of the triggers implemented in the 2nd half of the
139 2010 run were not implemented in the Monte Carlo,
140 we do not make any requirements on HLT bits in the Monte Carlo.
141 Instead, as discussed in
142 Section~\ref{sec:trgEff}, a trigger efficiency weight is applied
143 to each event, based on the trigger efficiencies measured on data.
144 Trigger efficiency weights are very close to 1.
145
146 %For data, we require the logical OR of all (or most?) unprescaled
147 %single and double lepton triggers that were deployed during the 2010
148 %run. These are:
149 %{\color{red} Here we need to list the triggers, somehow.}
150
151 For data, we use a cocktail of unprescaled single
152 and double lepton triggers. An event
153 in the $ee$ final state is required to pass at least 1
154 single- or double-electron trigger, a
155 $\mu\mu$ event is required to pass at least 1 single
156 or double-muon trigger, while an $e\mu$ event
157 is required to pass at least 1 single-muon, single-electron,
158 or $e-\mu$ cross trigger.
159 % We currently
160 % do not require MC events to pass any triggers.
161
162
163
164
165
166
167
168
169
170 \begin{itemize}
171 \item single-muon triggers
172 \begin{itemize}
173 \item \verb=HLT_Mu5=
174 \item \verb=HLT_Mu7=
175 \item \verb=HLT_Mu9=
176 \item \verb=HLT_Mu11=
177 \item \verb=HLT_Mu13_v1=
178 \item \verb=HLT_Mu15_v1=
179 \item \verb=HLT_Mu17_v1=
180 \item \verb=HLT_Mu19_v1=
181 \end{itemize}
182 \item double-muon triggers
183 \begin{itemize}
184 \item \verb=HLT_DoubleMu3=
185 \item \verb=HLT_DoubleMu3_v2=
186 \item \verb=HLT_DoubleMu5_v1=
187 \end{itemize}
188 \item single-electron triggers
189 \begin{itemize}
190 \item \verb=HLT_Ele10_SW_EleId_L1R=
191 \item \verb=HLT_Ele10_LW_EleId_L1R=
192 \item \verb=HLT_Ele10_LW_L1R=
193 \item \verb=HLT_Ele10_SW_L1R=
194 \item \verb=HLT_Ele15_SW_CaloEleId_L1R=
195 \item \verb=HLT_Ele15_SW_EleId_L1R=
196 \item \verb=HLT_Ele15_SW_L1R=
197 \item \verb=HLT_Ele15_LW_L1R=
198 \item \verb=HLT_Ele17_SW_TightEleId_L1R=
199 \item \verb=HLT_Ele17_SW_TighterEleId_L1R_v1=
200 \item \verb=HLT_Ele17_SW_CaloEleId_L1R=
201 \item \verb=HLT_Ele17_SW_EleId_L1R=
202 \item \verb=HLT_Ele17_SW_LooseEleId_L1R=
203 \item \verb=HLT_Ele17_SW_TighterEleIdIsol_L1R_v2=
204 \item \verb=HLT_Ele20_SW_L1R=
205 \item \verb=HLT_Ele22_SW_TighterEleId_L1R_v2=
206 \item \verb=HLT_Ele32_SW_TightCaloEleIdTrack_L1R_v1=
207 \item \verb=HLT_Ele32_SW_TighterEleId_L1R_v2=
208 \item \verb=HLT_Ele27_SW_TightCaloEleIdTrack_L1R_v1=
209 \item \verb=HLT_Ele22_SW_TighterCaloIdIsol_L1R_v2=
210 \item \verb=HLT_Ele22_SW_TighterEleId_L1R_v3=
211 \item \verb=HLT_Ele22_SW_TighterCaloIdIsol_L1R_v2=
212 \end{itemize}
213 \item double-electron triggers
214 \begin{itemize}
215 \item \verb=HLT_DoubleEle15_SW_L1R_v1=
216 \item \verb=HLT_DoubleEle17_SW_L1R_v1=
217 \item \verb=HLT_Ele17_SW_TightCaloEleId_Ele8HE_L1R_v1=
218 \item \verb=HLT_Ele17_SW_TightCaloEleId_SC8HE_L1R_v1=
219 \item \verb=HLT_DoubleEle10_SW_L1R=
220 \item \verb=HLT_DoubleEle5_SW_L1R=
221 \end{itemize}
222 \item e-$\mu$ cross triggers
223 \begin{itemize}
224 \item \verb=HLT_Mu5_Ele5_v1=
225 \item \verb=HLT_Mu5_Ele9_v1=
226 \item \verb=HLT_Mu11_Ele8_v1=
227 \item \verb=HLT_Mu8_Ele8_v1=
228 \item \verb=HLT_Mu5_Ele13_v2=
229 \item \verb=HLT_Mu5_Ele17_v1=
230 \end{itemize}
231 \end{itemize}