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# Content
1 \clearpage
2 \section {Analysis Demonstrations}
3
4 A wide variety of physics analysis demonstrations were
5 prepared by the
6 physics groups for CSA06 in order to test the analysis workflow for
7 CSA06. The analyses conducted on the CSA-produced data
8 samples numbered approximately 30, with nearly 70
9 active participants.
10 These demonstrations proved to be useful training
11 exercises for collaborators in the new software and computing tools as well.
12 The list of specialized calibration and
13 alignment streams produced at the Tier-0 and analyzed is discussed in
14 Section~\ref{sec:offlineswalca}. The list of general physics analysis
15 skims produced at the Tier-1 centres is covered in
16 Table~\ref{tab:tier1skim}. Table~\ref{tab:analyses} lists the physics
17 analyses that were conducted as part of CSA06. Details on these
18 analyses are contained in the following subsections.
19 %Unless noted,
20 %CRAB was used to submit the analysis jobs.
21
22
23 \begin{table}[phtb]
24 \centering
25 \caption{List of CSA06 analyses.}
26 \vspace{3mm}
27 \label{tab:analyses}
28 \begin{tabular}{|l|l|l|l|}
29 \hline
30 Group & Analysis & People & Dataset \\ \hline
31 eg & ECAL isol. electron calib. & L.Agostino (CERN), P. Govoni (Milan), & AlCaReco \\
32 & & L.Malgeri (CERN), R.Ofierzynski (CERN) & \\
33 eg & ECAL Phi symmetry calib. & D.Futyan (IC) & minbias AlCaReco \\
34 eg & Z$\rightarrow ee$ reco. & P.Meridiani (Rome) & Zee AlCaReco \\
35 \hline
36 jm & HCAL Phi symmetry calib. & O.Kodolova (Moscow) & minbias AlCaReco \\
37 jm & HCAL isol. trk. calib. & M.Szleper (Northwestern), & minbias AlCaReco \\
38 & & S.Petrushanko (Moscow) & \\
39 jm & Jet calib. & R.Harris, M.Cardaci (FNAL) & Jets \\
40 \hline
41 tk & Partial Tracker alignment & L.Edera, F.Ronga, and
42 O.Buchmuller (CERN), & Zmumu AlcaReco \\
43 & & F.-P. Schilling (Karlsruhe), & \\
44 tk & Misalignments effects on track reco & M.Abbrescia, G.Cuscela,
45 N.De Filippis, & Zmumu skim \\
46 & & G.Donvito, G.Maggi, S.My (Bari) & \\
47 \hline
48 mu & Muon alignment & J.Fernandez, P.Martinez,
49 & Muon AlCaReco \\
50 & & F.Matorras (IFCA, Santander) & \\
51 mu & W$\rightarrow\mu\nu$ & M.Biasotto, U.Gasparini, M.Margoni, & EWK, Soft Muon skims \\
52 & & E.Torassa (Padova) & \\
53 mu & J/Psi and Z$\rightarrow\mu\mu$ & J.Alcaraz, J.Hernandez,
54 J.Caballero & EWK, Soft Muon skims \\
55 & & P.Garcia Abia (CIEMAT) & \\
56 mu & Z$\rightarrow\mu\mu$ and muon effic. & C.Liu and N.Neumeister (Purdue) & EWK skim \\
57 & & M.Schmitt (Northwestern) & \\
58 mu & Dimuon reconstruction & B.Kim (Florida) & SoftMuon, minbias \\
59 \hline
60 hg & Selection of Z$\rightarrow 2\tau$ &
61 K.Petridis (IC), A.Kalinowski (Warsaw) & EWK skims \\
62 hg & jet$\rightarrow \tau$ mis id &
63 F.Blekman (IC), C.Siamitros (Brunel) & Z+jet\\
64 hg & tau tagging efficiency from Z$\rightarrow 2\tau$ &
65 S.Gennai and G.Bagliesi (Pisa), & EWK skims \\
66 & & A.Goussiou and R.Vasques Sierra (FNAL) & \\
67 hg & tau HLT with pixel trigger using Z$\rightarrow 2\tau$ &
68 D.Kotlinski and P.Trueb (PSI) & EWK skims \\
69 hg & Background to H$\rightarrow WW\rightarrow \ell\ell$ &
70 F. Stoeckli (ETH) & TTbar \\
71 hg & Z+2Jet background to qqH, H$\rightarrow$inv &
72 J.Brooke and S.Metson (Bristol), & EWK skims \\
73 & & K. Mazumdar (TIFR), S.Bansal (Panjab) & \\
74 \hline
75 sm & underlying event/minbias & L.Fano and F.Ambroglini (Pisa) &
76 m.b., Jets, D-Y skims \\
77 & & P.Bartalini and R.Field (Florida) & \\
78 & & F.Bechtel (Hamburg) & \\
79 sm & T-Tbar dilepton selection & I.Gonzalez-Caballero (IFCA, Santander), & TTbar skim \\
80 & & J.Cuevas Maestro (Oviedo) & \\
81 sm & T-Tbar inclusive & I.Gonzalez-Caballero (IFCA, Santander), & TTbar skims \\
82 & & J.Vizan (Oviedo) & \\
83 & & J.Heynick (Brussels) & \\
84 & & J.Vizan (Oviedo) & \\
85 sm & W mass & M.Malberti (Milan) & EWK skim \\
86 \hline
87 su & LM1 Jets + MET & M.Tytgat, M.Spiropulu (CERN) & Exotic, TTbar skims \\
88 su & Di-tau + MET & L.Houchu, D.J.Mangeol (Strasbourg) & Exotic \\
89 su & LM1 electron cleanup & F.Moortgat, L.Pape & Exotic \\
90 su & LM1 b-tagging & R.Stringer (Riverside) & Exotic \\
91 su & Dijet mass & R.Harris, M.Cardaci (FNAL) & QCD, Exotic skims\\
92 su & High energy $e^+e^-$ & P.Vanlaer (Brussels),
93 D.Evans (Bristol), & Exotic, EWK skims \\
94 & & C.Shepherd-Themistocleous (RAL) & \\
95 su & Z$'\rightarrow \mu^+\mu^-$ & M.Tytgat, M.Spiropulu (CERN) & Exotic \\
96 su & Z$'\rightarrow \mu^+\mu^-$ & A.Lanyov, S.Shmatov (Dubna) & Exotic \\
97 \hline
98 \end{tabular}
99 \end{table}
100
101
102
103 \subsection {Calibration}
104
105 \label{sec:calib}
106
107 \input{calib_ana.tex}
108
109 %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
110
111 \subsection {Alignment}
112
113 \label{sec:align}
114
115 \subsubsection{Tracker Alignment}
116
117 A tracker alignment CSA06 exercise was carried out with the goal to
118 demonstrate the full work- and dataflow of the alignment process.
119 The exercise followed closely the ideas and concepts
120 developed during the T0-RTAG~\cite{tier0rtag}.
121 The exercise comprised the following steps:
122 \begin{itemize}
123 \item Reading of alignment constants from the offline database during prompt
124 reconstruction;
125 \item Writing dedicated AlCaReco streams for alignment;
126 \item Defining a misalignment scenario and insertion of the corresponding
127 object into the offline database;
128 \item Running an alignment algorithm at the Tier-0;
129 \item Inserting the resulting alignment corrections into the database;
130 \item Running re-reconstruction at a Tier-1 centre reading this alignment
131 object;
132 \item Running analysis jobs in which ideal, misaligned
133 and aligned distributions are compared.
134 \end{itemize}
135
136 The steps regarding production of the dedicated AlCaReco streams
137 as well as enabling the prompt reconstruction to read alignment
138 constants from the offline database were already described in
139 section~\ref{sec:offlineswalca}. In the following, a short
140 summary of the exercise is given. For more details,
141 see~\cite{alcacsa06note}.
142
143 The following misalignment scenario was defined for this exercise: The
144 sensors of the Tracker Inner Barrel TIB as well as the Rods of the
145 Tracker Outer Barrel TOB were misaligned. Random shifts drawing from
146 a flat distribution in the range $\pm 100 \rm\ \mu m$ were applied in
147 $u$, $v$, $w$ (local coordinate system) for layers built from double
148 sided modules, and in $u$ (precise coordinate) only for layers built
149 from single sided modules. In addition, random rotations around all
150 three local coordinate axes of size $\pm 10 \rm\ mrad$ were applied to
151 the modules/rods of both single and double sided TIB and TOB layers.
152 The pixel detector was kept fixed
153 in order to define a reference system. In addition, the outermost TOB
154 layer was also kept fixed in order to improve the convergence. This
155 misalignment scenario was inserted as an alignment object into the
156 offline database. In addition, another object corresponding to the
157 ideal tracker geometry was inserted, to be used during prompt
158 reconstruction.
159
160 \begin{figure}
161 \centering
162 \includegraphics[width=0.8\linewidth]{figs/csa06_convergence}
163 \caption{Alignment exercise: The convergence of the alignment
164 algorithm in $\Delta u, \Delta v, \Delta w$ is shown for double sided
165 TIB modules as a function of the iteration number (left), as well as
166 projected for initial misalignment (labeled ``after 0 Iterations'')
167 and after 4, 7 and 10 iterations (right). }
168 \label{fig:alignment_convergence}
169 \end{figure}
170
171 The alignment was performed running the HIP alignment
172 algorithm~\cite{hipnote} as implemented in CMSSW\_1\_0\_6 over approximately
173 $1 \rm\ M$ AlCaReco $Z^0\rightarrow\mu^+\mu^-$ events produced during
174 prompt reconstruction at the Tier-0, reading the above mentioned
175 misalignment object from the offline database. The algorithm was run
176 on 20 dedicated CPUs in parallel at CERN, iterating 10 times over the
177 data sample. The result of the alignment was obtained in less than $5
178 \rm\ h$, and the corresponding tracker alignment object
179 was inserted into the database. Figure~\ref{fig:alignment_convergence}
180 illustrates the convergence of the alignment for the double sided TIB
181 sensors.
182
183 \begin{figure}
184 \centering
185 \includegraphics[width=0.8\linewidth]{figs/csa06_aliexercise}
186 \caption{Invariant mass distribution from $Z^0\to \mu^+ \mu^-$ events,
187 obtained from events produced by the prompt reconstruction at
188 the Tier-0 (``ideal''), from events processed with misalignment
189 as used as input for the alignment algorithm (``misaligned'') and
190 from events re-reconstructed at a Tier-1 centre (PIC) using the alignment
191 constants derived from the alignment algorithm (``realigned'').
192 }
193 \label{fig:aliexercise}
194 \end{figure}
195
196 Once the alignment and calibration constants were inserted in the
197 database, they were deployed to the Tier-1/2 centres via Frontier.
198 Subsequently, re-reconstruction of some of the CSA06 datasets was
199 launched at various Tier-1 centres as described in Section~\ref{sec:rereco}. For instance, the
200 $Z^0\rightarrow\mu^+\mu^-$ data set was re-reconstructed at PIC
201 (Barcelona) using the new alignment object. In order to demonstrate
202 the final missing piece of the workflow, grid analysis jobs were
203 submitted to PIC to process these re-reconstructed
204 $Z^0\rightarrow\mu^+\mu^-$ events. The reconstructed invariant dimuon
205 mass is presented in Figure~\ref{fig:aliexercise} for three cases:
206 \begin{itemize}
207 \item Using the ideal geometry, reading the RECO produced during prompt
208 reconstruction;
209 \item Using the misaligned geometry, reading the AlCaReco and the misalignment
210 scenario database object;
211 \item Using the realigned geometry, reading the events re-reconstructed
212 with the alignment database object.
213 \end{itemize}
214 As can be seen, the invariant mass resolution is degraded in the case
215 of misalignment. After the alignment algorithm has corrected the
216 tracker geometry, the resolution is recovered close to the original
217 value. This demonstrates that the work- and dataflow of the full
218 alignment was successfully carried out.
219
220
221 \input{muonalignment.tex}
222
223 %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
224
225 \subsection {Physics Analysis Exercises}
226
227 \subsubsection {Effect of tracker misalignment on track reconstruction performances}
228
229 The alignment uncertainties of the CMS Tracker detector, made of a huge amount of independent silicon sensors with an excellent position resolution, affect the performances of the track reconstruction and track parameters measurement.
230 The purpose of the analysis exercise performed by the team at Bari
231 during the CSA06 was to study the effect of the CMS tracker misalignment on
232 the performance of the track reconstruction
233 \cite{misalignment}. Realistic estimates for the expected
234 displacements of the tracking systems were supplied in different
235 scenarios as specified in the following:
236
237 \begin{itemize}
238 \item the ideal scenario with a perfect tracker geometry;
239 \item the short term misalignment scenario representing the
240 typical mis-alignment conditions during the first
241 data-taking when the uncertainties on the position of the sub-structures of the CMS
242 tracker will be between $10 \, \mu$m for pixel detectors and $400 \, \mu$m for microstrip silicon detectors in
243 the endcaps. Detector position and errors are read
244 from the offline database at CERN by caching the needed information locally via frontier/squid
245 software.
246
247 \item the long term scenario when the alignment uncertainties are expected to be a factor 10 smaller because of the
248 improvement obtained by using alignment algorithms with a high statistics of tracks.
249
250 \item the CSA06 aligned scenario by using the tracker module position and errors as obtained by the output of the
251 alignment procedure (Section~\ref{sec:align}) that was run at the
252 CERN Tier-0 to verify the efficiency of the alignment procedure on
253 the track
254 reconstruction. The refit of tracks is performed also in this case.
255
256 \end{itemize}
257
258 Track reconstruction is based on the Kalman Filter formalism \cite{Kalman} for trajectory building, cleaning and
259 smoothing steps and uses hits from pixel detector as seeds to provide initial trajectory candidates.
260 Because of the misalignment, the analysis requires to refit tracks with a misaligned tracker geometry.
261 Global efficiency of track reconstruction and track parameter resolutions for muons were
262 compared in all the cases. The association between simulated track and reconstructed tracks is performed
263 by comparing the corresponding track parameters at the closest approach point and choosing the pair which gives
264 the minimum $\chi^2$ from the best fit procedure.
265
266 Events from CSA06 $Z\rightarrow \mu \mu $ sample were firstly skimmed by selecting events with
267 Hep MC muons from Z decay with pseudorapidity, $\eta$, in the tracker acceptance, $|\eta| < 2.55$,
268 with a transverse momentum larger than $5 \, \mathrm{GeV}/c^2$ and a dimuon invariant mass in the following
269 range aroung the Z peak: $50 < m_{\mu\mu}(\mathrm{GeV}/c^2) < 130$. The efficiency of this selection is
270 between 50 and 60\% mainly due to the cut on the acceptance, for a
271 final sample of 1 million events.
272 The output files in RECOSIM format were needed for the subsequent analysis.
273
274
275 Jobs executing the misalignment analysis were submitted at Bari with CRAB\_1\_4\_0 in the LCG infrastructure.
276 A total of about 2.5 thousands jobs (45 at most in parallel) ran with a grid efficiency of 90\% and an
277 application efficiency of 80\%, by accessing detector position and errors from the offline database via
278 frontier.
279
280
281 Some results of the misalignment analysis are summarized below. The global efficiency of track reconstruction of muons coming from
282 Z decay is shown in Fig.~\ref{eff} as a function of the pseudorapidity, $\eta$, in the tracker acceptance.
283 In the case of a perfect geometry the global track reconstruction is not fully efficient over all the $\eta$
284 range because of the track associator algorithm itself, which discards tracks with $\chi^2$ of the fit larger
285 than 25. The effect of misalignment is relevant observed ib the short term scenario and causes a partial inefficiency of the
286 track reconstruction that can be recovered if the intrinsic position resolution of the tracker
287 detector is combined with the alignment uncertainties to make larger the error on the position of the
288 reconstructed hit (called the alignment position error, or APE) so improving the track fit at the
289 expense of a larger rate of fake tracks.
290
291
292 The transverse momentum resolution as a function of the transverse momentum is reported in Fig.~\ref{respt};
293 the degradation of the transverse momentum resolution at large $p_{T}$ because of the misalignment is in a factor
294 between 2 and 3 with respect to the perfect geometry case. At low transverse momentum (less than few $\mathrm{GeV}/c$
295 the multiple scattering is the
296 most important contribution to the resolution so the effect of
297 misalignment is negligible.
298
299 The residual of the Z mass obtained as the invariant mass of muons coming from Z decays for the case of perfect
300 tracker geometry and for the short-term and long term misalignment scenarios is shown in Fig.~\ref{mz}; the $\sigma$ of
301 the Gaussian fit of the residual distribution can be quoted as the Z mass resolution which is degraded by a factor 2
302 because of the tracker misalignment in the short term scenario.
303
304 \begin{2figures}{hbt}
305 \resizebox{\linewidth}{!}{\includegraphics{figs/Eff_eta}} &
306 \resizebox{\linewidth}{!}{\includegraphics{figs/SigmapT_pT}} \\
307 \caption{Global track reconstruction efficiency vs pseudorapidity for muons coming from Z decay in the case of perfect
308 tracker geometry and in short-term and long term misalignment scenarios when the APE is not used.}
309 \label{eff} &
310 \caption{$p_{T}$ resolution vs $p_{T}$ in the case of perfect
311 tracker geometry and in short-term and long term misalignment scenarios.}
312 \label{respt} \\
313 \end{2figures}
314
315
316 \begin{figure}[htb]
317 \begin{center}
318 \resizebox{0.7\linewidth}{!}{\includegraphics{figs/Residual_mZ_mu}}
319 \end{center}
320 \caption{Residual of Z mass obtained as the invariant mass of muons coming from Z decayd for the case of perfect
321 tracker geometry and for the short-term and long term misalignment scenarios.}
322 \label{mz}
323 \end{figure}
324
325 % muon analyses
326
327 \input{wmunu.tex}
328
329 \input{dimuon.tex}
330
331 % electron analyses
332 \input{zee.tex}
333
334 \input{wmass.tex}
335
336
337 % tau analyses:
338
339 \input{z_2tau.tex}
340
341 \input{taumisid.tex}
342
343 \input{tau_validation.tex}
344
345 % Higgs
346 \input{hww_2l.tex}
347
348 \input{qqh_inv_zbkg.tex}
349
350 % min bias studies
351 \input{mbue.tex}
352
353 \input{ttbar_ana.tex}
354
355 % SUSY
356 \input{susybsm.tex}
357
358 %BSM analyses
359 %input{heep-analysis.tex}