Variables | |
tuple | doPixels = cms.bool(True) |
tuple | doStrips = cms.bool(True) |
tuple | fileName = cms.untracked.string('myOutputFile.root') |
tuple | fileNames |
tuple | pixelClusters = cms.InputTag("siPixelClusters") |
tuple | pixelModule = cms.string('BPIX,FPIX,PIXEL') |
tuple | pixelVariables = cms.string('pHits,pSize,pCharge') |
tuple | process = cms.Process("ClusterSummaryProducer") |
tuple | stripClusters = cms.InputTag("siStripClusters") |
tuple | stripModule = cms.string('TOB,TIB,TID,TEC,TRACKER') |
tuple | stripVariables = cms.string('cHits,cSize,cCharge') |
tuple | verbose = cms.bool(False) |
For running on pre 3.6 files the current needed to determine the magnetic field is taken from Conditions DB. More... | |
tuple clustersummaryproducer_cfg.doPixels = cms.bool(True) |
Definition at line 34 of file clustersummaryproducer_cfg.py.
Referenced by ClusterAnalyzer.analyze().
tuple clustersummaryproducer_cfg.doStrips = cms.bool(True) |
Definition at line 33 of file clustersummaryproducer_cfg.py.
Referenced by ClusterAnalyzer.analyze().
tuple clustersummaryproducer_cfg.fileName = cms.untracked.string('myOutputFile.root') |
Definition at line 39 of file clustersummaryproducer_cfg.py.
tuple clustersummaryproducer_cfg.fileNames |
Definition at line 10 of file clustersummaryproducer_cfg.py.
tuple clustersummaryproducer_cfg.pixelClusters = cms.InputTag("siPixelClusters") |
Definition at line 19 of file clustersummaryproducer_cfg.py.
Referenced by HLTTrack.analyze(), HLTTrackClusterRemover.produce(), TrackClusterRemover.produce(), SeedClusterRemover.produce(), FastPrimaryVertexProducer.produce(), ClusterSummaryProducer.produce(), and MeasurementTrackerImpl.updatePixels().
tuple clustersummaryproducer_cfg.pixelModule = cms.string('BPIX,FPIX,PIXEL') |
Definition at line 27 of file clustersummaryproducer_cfg.py.
tuple clustersummaryproducer_cfg.pixelVariables = cms.string('pHits,pSize,pCharge') |
Definition at line 30 of file clustersummaryproducer_cfg.py.
tuple clustersummaryproducer_cfg.process = cms.Process("ClusterSummaryProducer") |
Definition at line 3 of file clustersummaryproducer_cfg.py.
tuple clustersummaryproducer_cfg.stripClusters = cms.InputTag("siStripClusters") |
Definition at line 18 of file clustersummaryproducer_cfg.py.
Referenced by HLTTrackClusterRemover.produce(), TrackClusterRemover.produce(), SeedClusterRemover.produce(), and ClusterSummaryProducer.produce().
tuple clustersummaryproducer_cfg.stripModule = cms.string('TOB,TIB,TID,TEC,TRACKER') |
Definition at line 22 of file clustersummaryproducer_cfg.py.
tuple clustersummaryproducer_cfg.stripVariables = cms.string('cHits,cSize,cCharge') |
Definition at line 25 of file clustersummaryproducer_cfg.py.
tuple clustersummaryproducer_cfg.verbose = cms.bool(False) |
For running on pre 3.6 files the current needed to determine the magnetic field is taken from Conditions DB.
process.load("Configuration.StandardSequences.FrontierConditions_GlobalTag_cff") specify tag: process.GlobalTag.globaltag = 'START36_V10::All' or use auto-cond: from Configuration.AlCa.autoCond import autoCond process.GlobalTag.globaltag = autoCond['mc'] Request EveService Extractor of geometry needed to display it in Eve. Required for "DummyEvelyser".
For running on pre 3.6 files the current needed to determine the magnetic field is taken from Conditions DB.
Required for "DummyEvelyser".
Definition at line 35 of file clustersummaryproducer_cfg.py.