ATLAS Offline Software
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MuonNSWSegmentFinderTool.cxx File Reference
#include "MuonNSWSegmentFinderTool.h"
#include "EventPrimitives/EventPrimitivesHelpers.h"
#include "FourMomUtils/xAODP4Helpers.h"
#include "MuonPrepRawData/MMPrepData.h"
#include "MuonPrepRawData/MuonPrepDataCollection.h"
#include "MuonPrepRawData/sTgcPrepData.h"
#include "MuonReadoutGeometry/MuonPadDesign.h"
#include "MuonReadoutGeometry/MuonReadoutElement.h"
#include "MuonReadoutGeometry/sTgcReadoutElement.h"
#include "TrkEventPrimitives/FitQuality.h"
#include "TrkParameters/TrackParameters.h"
#include "TrkPseudoMeasurementOnTrack/PseudoMeasurementOnTrack.h"
#include "TrkTrack/Track.h"
#include "MuonDetDescrUtils/MuonSectorMapping.h"
#include "EventPrimitives/EventPrimitivesToStringConverter.h"
#include "CxxUtils/inline_hints.h"

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Namespaces

 Muon
 NRpcCablingAlg reads raw condition data and writes derived condition data to the condition store.
 

Typedefs

using Muon::MeasVec = NSWSeed::MeasVec
 Stereo seeds can be formed using hits from 4 independent layers by solving the following system of equations I: \vec{C}_{0} + \lambda \vec{e}_{0} = \vec{X}_{\mu} II: \vec{C}_{1} + \alpha \vec{e}_{1} = \vec{X}_{\mu} + A \vec{D}_{\mu} III: \vec{C}_{2} + \gamma \vec{e}_{2} = \vec{X}_{\mu} + G \vec{D}_{\mu} IV: \vec{C}_{3} + \kappa \vec{e}_{3} = \vec{X}_{\mu} + K \vec{D}_{\mu} where \vec{C}_{i} are the geometrical strip centres, \vec_{e}_{i} describe the orientations of each strip, X_{0} is the seed position and \vec{D}_{\mu} points along a straight line muon. More...