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ATLAS Offline Software
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#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"Go to the source code of this file.
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... | |
1.8.18