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1 fisk 1.1 \section {Analysis Demonstrations}
2    
3 acosta 1.15 A wide variety of physics analysis demonstrations were prepared by the
4     physics groups for CSA06 in order to test the analysis workflow for
5     CSA06. These demonstrations also proved to be useful training
6     exercises for collaborators in the new software and computing tools.
7     The list of specialized calibration and
8     alignment streams produced at the Tier-0 and analyzed is discussed in
9     Section~\ref{sec:offlineswalca}. The list of general physics analysis
10     skims produced at the Tier-1 centres is covered in
11     Table~\ref{tab:tier1skim}. Table~\ref{tab:analyses} lists the physics
12     analyses that were conducted as part of CSA06. Details on these
13     analyses are contained in the following subsections. Unless noted,
14     CRAB was used to submit the analysis jobs.
15    
16    
17     \begin{table}[phtb]
18     \centering
19     \caption{List of CSA06 analyses.}
20     \label{tab:analyses}
21     \begin{tabular}{|l|l|l|l|l|}
22     \hline
23     Group & Analysis & People & Dataset & Comments \\ \hline
24     hg & Selection of Z$\rightarrow 2\tau$ &
25     K.Petridis (IC), A.Kalinowski (Warsaw) & EWK skims & \\
26     hg & jet$\rightarrow \tau$ mis id &
27     F.Blekman (IC), C.Siamitros (Brunel) & Z+jet& \\
28     hg & tau tagging efficiency from Z$\rightarrow 2\tau$ &
29     S.Gennai and G.Bagliesi (Pisa), & EWK skims & \\
30     & & A.Goussiou and R.Vasques Sierra (FNAL) & & \\
31     hg & tau HLT with pixel trigger using Z$\rightarrow 2\tau$ &
32     D.Kotlinski and P.Trueb (PSI) & EWK skims & \\
33     hg & H$\rightarrow WW\rightarrow \ell\ell$ &
34     F. Stoeckli (ETH) & EWK & CERN batch\\
35     hg & Z+2Jet background to qqH, H$\rightarrow$inv &
36     J.Brooke and S.Metson (Bristol), & EWK skims & \\
37     & & K. Mazumdar, S.Bansal (TIFR) & & \\
38     \hline
39     \end{tabular}
40     \end{table}
41    
42    
43 ndefilip 1.3
44 fisk 1.1 \subsection {Calibration}
45    
46 acosta 1.14 \label{sec:calib}
47    
48 malgeri 1.6 \input{calib_ana.tex}
49    
50 fpschill 1.5 %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
51    
52     \subsection {Alignment}
53    
54 acosta 1.14 \label{sec:align}
55    
56 fpschill 1.5 A tracker alignment CSA06 exercise was carried out with the goal to
57     demonstrate the full work- and dataflow of the alignment process.
58     The exercise followed closely the ideas and concepts
59     developed during the T0-RTAG~\cite{tier0rtag}.
60     The exercise comprised the following steps:
61     \begin{itemize}
62     \item Reading of alignment constants from the offline database during prompt
63     reconstruction;
64     \item Writing dedicated AlCaReco streams for alignment;
65     \item Defining a misalignment scenario and insertion of the corresponding
66     object into the offline database;
67     \item Running an alignment algorithm at the Tier-0;
68     \item Inserting the resulting alignment corrections into the database;
69     \item Running re-reconstruction at a Tier-1 centre reading this alignment
70     object;
71     \item Running analysis jobs in which ideal, misaligned
72     and aligned distributions are compared.
73     \end{itemize}
74    
75     The steps regarding production of the dedicated AlCaReco streams
76     as well as enabling the prompt reconstruction to read alignment
77     constants from the offline database were already described in
78     section~\ref{sec:offlineswalca}. In the following, a short
79     summary of the exercise is given. For more details,
80     see~\cite{alcacsa06note}.
81    
82     The following misalignment scenario was defined for this exercise: The
83     sensors of the Tracker Inner Barrel TIB as well as the Rods of the
84     Tracker Outer Barrel TOB were misaligned. Random shifts drawing from
85     a flat distribution in the range $\pm 100 \rm\ \mu m$ were applied in
86     $u$, $v$, $w$ (local coordinate system) for layers built from double
87     sided modules, and in $u$ (precise coordinate) only for layers built
88     from single sided modules. In addition, random rotations around all
89     three local coordinate axes of size $\pm 10 \rm\ mrad$ were applied to
90     the modules/rods of both single and double sided TIB and TOB layers.
91     The pixel detector was kept fixed
92     in order to define a reference system. In addition, the outermost TOB
93     layer was also kept fixed in order to improve the convergence. This
94     misalignment scenario was inserted as an alignment object into the
95     offline database. In addition, another object corresponding to the
96     ideal tracker geometry was inserted, to be used during prompt
97     reconstruction.
98    
99     \begin{figure}
100     \centering
101 malgeri 1.6 \includegraphics[angle=270,width=0.8\linewidth]{figs/csa06_convergence}
102 fpschill 1.5 \caption{Alignment exercise: The convergence of the alignment
103     algorithm in $\Delta u, \Delta v, \Delta w$ is shown for double sided
104     TIB modules as a function of the iteration number (left), as well as
105     projected for initial misalignment (labeled ``after 0 Iterations'')
106     and after 4, 7 and 10 iterations (right). }
107     \label{fig:alignment_convergence}
108     \end{figure}
109    
110     The alignment was performed running the HIP alignment
111     algorithm~\cite{hipnote} as implemented in CMSSW\_1\_0\_6 over approx.
112     $1 \rm\ M$ AlCaReco $Z^0\rightarrow\mu^+\mu^-$ events produced during
113     prompt reconstruction at the Tier-0, reading the above mentioned
114     misalignment object from the offline database. The algorithm was run
115     on 20 dedicated CPUs in parallel at CERN, iterating 10 times over the
116     data sample. The result of the alignment was obtained in less than $5
117     \rm\ h$, and the corresponding tracker alignment object
118     was inserted into the database. Figure~\ref{fig:alignment_convergence}
119     illustrates the convergence of the alignment for the double sided TIB
120     sensors.
121    
122     \begin{figure}
123     \centering
124 malgeri 1.6 \includegraphics[angle=270,width=0.8\linewidth]{figs/csa06_aliexercise}
125 fpschill 1.5 \caption{Invariant mass distribution from $Z^0\to \mu^+ \mu^-$ events,
126     obtained from events produced by the prompt reconstruction at
127     the Tier-0 (``ideal''), from events processed with misalignment
128     as used as input for the alignment algorithm (``misaligned'') and
129     from events re-reconstructed at a Tier-1 centre (PIC) using the alignment
130     constants derived from the alignment algorithm (``realigned'').
131     }
132     \label{fig:aliexercise}
133     \end{figure}
134    
135     Once the alignment and calibration constants were inserted in the
136     database, they were deployed to the Tier-1/2 centres via Frontier.
137     Subsequently, re-reconstruction of some of the CSA06 datasets was
138     launched at various Tier-1 centres. For instance, the
139     $Z^0\rightarrow\mu^+\mu^-$ data set was re-reconstructed at PIC
140     (Barcelona) using the new alignment object. In order to demonstrate
141     the final missing piece of the workflow, grid analysis jobs were
142     submitted to PIC to process these re-reconstructed
143     $Z^0\rightarrow\mu^+\mu^-$ events. The reconstructed invariant di-muon
144     mass is presented in Figure~\ref{fig:aliexercise} for three cases:
145     \begin{itemize}
146     \item Using the ideal geometry, reading the RECO produced during prompt
147     reconstruction;
148     \item Using the misaligned geometry, reading the AlCaReco and the misalignment
149     scenario database object;
150     \item Using the realigned geometry, reading the events re-reconstructed
151     with the alignment database object.
152     \end{itemize}
153     As can be seen, the invariant mass resolution is degraded in the case
154     of misalignment. After the alignment algorithm has corrected the
155     tracker geometry, the resolution is recovered close to the original
156     value. This demonstrates that the work- and dataflow of the full
157     alignment was successfully carried out.
158    
159    
160 acosta 1.16 \input{muonalignment.tex}
161    
162 fpschill 1.5 %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
163 fisk 1.1
164     \subsection {Physics Analysis Exercises}
165    
166 ndefilip 1.2 \subsubsection {Effect of tracker misalignment on track reconstruction performances}
167    
168 ndefilip 1.3 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.
169     The analysis exercise performed by the team at Bari during the CSA06 had the purpose of study the effect of the CMS tracker misalignment on the performances of the track reconstruction \cite{misalignment}. Realistic estimates for the expected displacements of the tracking systems were supplied in different scenarios as specified in the following:
170    
171     \begin{itemize}
172     \item the ideal scenario with a perfect tracker geometry;
173     \item the short term misalignment scenario supposed to reproduce the mis-alignment conditions during the first
174     data taking when the uncertainties on the position of the sub-structures of the CMS
175     tracker will be between $10 \, \mu$ for pixel detectors and $400 \, \mu$ for microstrip silicon detectors in
176     the endcaps. Detector position and errors are read
177     from the offline database at CERN by caching the needed information locally via frontier/squid
178 ndefilip 1.7 software.
179 ndefilip 1.3
180     \item the long term scenario when the alignment uncertainties are supposed to be a factor 10 smaller because of the
181     improvement obtained by using aligmnent algorithms with a high statistics of tracks.
182    
183     \item the CSA06 aligned scenario by using the tracker module position and errors as obtained by the output of the
184     alignment procedure that was run at CERN Tier-0 to verify the efficiency of the alignment procedure on the track
185     reconstruction. The refit of tracks is performed also in this case.
186    
187     \end{itemize}
188    
189 ndefilip 1.4 Track reconstruction is based on the Kalman Filter formalism \cite{Kalman} for trajectory building, cleaning and
190     smoothing steps and uses hits from pixel detector as seeds to provide initial trajectory candidates.
191     Because of the misalignment the analysis requires to refit tracks with a misaligned tracker geometry.
192     Global efficiency of track recostruction and track parameter resolutions for muons were
193     compared in all the cases. The association between simulated track and reconstruted tracks is performed
194     by comparing the corresponding track parameters at the closest approach point and choosing the pair which gives
195     the minimum $\chi^2$ from the best fit procedure.
196 ndefilip 1.3
197 ndefilip 1.4 Events from CSA06 $Z\rightarrow \mu \mu $ sample were firstly skimmed by selecting events with
198     Hep MC muons from Z decay with pseudorapidity, $\eta$, in the tracker acceptance, $|\eta| < 2.55$,
199     with transverse momentum larger than $5 \, \mathrm{GeV}/c^2$ and di-muons invariant mass in the following
200     range aroung the Z peak: $50 < m_{\mu\mu}(\mathrm{GeV}/c^2) < 130$; the efficiency of the previous selection is
201     between 50 and 60 \% mainly due to the cut on the acceptance, for a final statistics of 1 million events.
202     The output files in RECOSIM format were needed for the subsequent analysis.
203 ndefilip 1.3
204    
205 ndefilip 1.4 Jobs executing the misalignment analysis were submitted at Bari with CRAB\_1\_4\_0 in the LCG infrastructure.
206     A total of about 2.5 thousands jobs (45 at most in parallel) ran with a grid efficiency of 90 \% and an
207     application efficiency of 80\%, by accessing detector position and errors from the offline database via
208     frontier.
209 ndefilip 1.3
210 ndefilip 1.4
211     Some results of the misalignment analysis were summarized below. The global efficiency of track reconstruction of muons coming from
212     Z decay is shown in Fig.~\ref{eff} as a function of the pseudorapidity, $\eta$, in the tracker acceptance.
213     In the case of a perfect geometry the global track reconstruction was not fully efficient over all the $\eta$
214 ndefilip 1.12 range because of the track associator algorithm itself which discards tracks with $\chi^2$ of the fit larger
215 ndefilip 1.4 than 25. The effect of misalignment is relevant in the short term scenario and causes a partial inefficiency of the
216     track reconstruction; that can be recovered if the intrinsic position resolution of the tracker
217     detector is combined with the alignment uncertainties to make larger the error on the position of the
218     reconstructed hit (called alignment position error, APE) so improving the track fit at the
219     expence of a larger rate of fake tracks.
220    
221    
222     The tranverse momentum resolution as a function of the transverse momentum is reported in Fig.~\ref{respt};
223     the degradation of the tranverse momentum resolution at large $p_{T}$ because of the misalignment is in a factor
224     between 2 and 3 with respect to the perfect geometry case. At low transverse momentum (less than few $\mathrm{GeV}/c$
225     the multiple scattering is the
226     most important contribution to the resolution so the effect of misalignment is overwhelmed at all.
227    
228     The residual of Z mass obtained as the invariant mass of muons coming from Z decay in the case of perfect
229     tracker geometry and in short-term and long term misalignment scenarios is shown in Fig.~\ref{mz}; the $\sigma$ of
230     the Gaussian fit of the residual ditribution can be quoted as the Z mass resolution which is degradated of a factor 2
231     because of the tracker misalignment in the short term scenario.
232    
233     \begin{2figures}{hbt}
234 malgeri 1.6 \resizebox{\linewidth}{!}{\includegraphics{figs/Eff_eta}} &
235     \resizebox{\linewidth}{!}{\includegraphics{figs/SigmapT_pT}} \\
236 ndefilip 1.3 \caption{Global track reconstrution efficiency vs pseudorapidity for muons coming from Z decay in the case of perfect
237     tracker geometry and in short-term and long term misalignment scenarios when the APE is not used.}
238     \label{eff} &
239 ndefilip 1.4 \caption{$P_{T}$ resolution vs $p_{T}$ in the case of perfect
240     tracker geometry and in short-term and long term misalignment scenarios.}
241     \label{respt} \\
242     \end{2figures}
243    
244    
245     \begin{figure}[htb]
246     \begin{center}
247 malgeri 1.6 \resizebox{0.7\linewidth}{!}{\includegraphics{figs/Residual_mZ_mu}}
248 ndefilip 1.4 \end{center}
249 ndefilip 1.3 \caption{Residual of Z mass obtained as the invariant mass of muons coming from Z decay in the case of perfect
250     tracker geometry and in short-term and long term misalignment scenarios.}
251 ndefilip 1.4 \label{mz}
252     \end{figure}
253    
254 acosta 1.10 % min bias studies
255     \input{mbue.tex}
256 acosta 1.8
257     % tau analyses:
258 ndefilip 1.4
259 acosta 1.8 \input{z_2tau.tex}
260    
261     \input{taumisid.tex}
262    
263     \input{tau_validation.tex}
264    
265 acosta 1.9 % muon analyses
266    
267     \input{wmunu.tex}
268    
269 acosta 1.13 \input{dimuon.tex}
270    
271 meridian 1.11 % electron analyses
272     \input{zee.tex}
273    
274 ndefilip 1.12 \input{wmass.tex}