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root/cvsroot/UserCode/Friis/TancNote/note/tau_id.tex
Revision: 1.2
Committed: Thu Apr 22 16:13:12 2010 UTC (15 years ago) by friis
Content type: application/x-tex
Branch: MAIN
Changes since 1.1: +14 -11 lines
Log Message:
Adding NN observables inputs and other miscellaneous stuff

File Contents

# User Rev Content
1 friis 1.1 The tau identification strategies used in previously published CMS analyses are
2 friis 1.2 fully described in~\cite{PFT08001}. A summary of the basic methods and
3 friis 1.1 strategies is given here. There are two primary methods for selecting objects
4     used to reconstruct tau leptons. The CaloTau algorithm uses tracks
5     reconstructed by the tracker and clusters of hits in the electromagnetic and
6     hadronic calorimeter. The other method (PFTau) uses objects reconstructed by
7 friis 1.2 the CMS particle flow algorithm, which is described in~\cite{PFT09}. The
8 friis 1.1 particle flow algorithm provides a global and unique description of every
9     particle (charged hadron, photon, electron, etc.) in the event; measurements
10     from subdetectors are combined according to their measured resolutions to
11     improve energy and angular resolution and reduce double counting. The
12     strategies described in this paper use the particle flow objects.
13    
14 friis 1.2 Both methods use an ``leading object'' and an isolation requirement to reject
15     quark and gluon jet background. Quark and gluon jets are less collimated and
16     have a higher constituent multiplicity and softer constituent $p_T$ spectrum
17     than a kinematically comparable hadronic tau decays. The ``leading track''
18     requirement is applied by requiring a realitively high momentum object near the
19     center of the jet; typically a charged track with transverse momentum greater
20     than 5 GeV/c within $\Delta R < 0.1$ about the center of the jet axis. The
21     Isolation requirement exploits the collimation of true taus by defining an
22     isolation annulus about the kinematic center of the jet and requiring no
23     detector activity about a threshold in that annulus. This approach rejects QCD
24     backgrounds by a factor of $\mathcal O(100)$ while a maintaing hadronic tau
25     identification of approximately 50\%.