CMS 3D CMS Logo

 All Classes Namespaces Files Functions Variables Typedefs Enumerations Enumerator Properties Friends Macros Pages
Variables
TtSemiLepJetCombWMassDeltaTopMass_cfi Namespace Reference

Variables

tuple findTtSemiLepJetCombWMassDeltaTopMass
 

Variable Documentation

tuple TtSemiLepJetCombWMassDeltaTopMass_cfi.findTtSemiLepJetCombWMassDeltaTopMass
Initial value:
1 = cms.EDProducer("TtSemiLepJetCombWMassDeltaTopMass",
2  ## jet input
3  jets = cms.InputTag("selectedPatJets"),
4  ## lepton input
5  leps = cms.InputTag("selectedPatMuons"),
6  ## met input
7  mets = cms.InputTag("patMETs"),
8  maxNJets = cms.int32(4),
9  ## nominal WMass parameter (in GeV)
10  wMass = cms.double(80.4),
11  ## use b-tagging two distinguish between light and b jets
12  useBTagging = cms.bool(False),
13  ## choose algorithm for b-tagging
14  bTagAlgorithm = cms.string("trackCountingHighEffBJetTags"),
15  ## minimum b discriminator value required for b jets and
16  ## maximum b discriminator value allowed for non-b jets
17  minBDiscBJets = cms.double(1.0),
18  maxBDiscLightJets = cms.double(3.0),
19  ## different ways to calculate a neutrino pz:
20  ## -1 : take MET as neutrino directly, i.e. pz = 0
21  ## or use mW = 80.4 GeV to solve the quadratic equation for the neutrino pz;
22  ## if two real solutions...
23  ## 0 : take the one closer to the lepton pz if neutrino pz < 300 GeV,
24  ## otherwise the more central one
25  ## 1 : always take the one closer to the lepton pz
26  ## 2 : always take the more central one, i.e. minimize neutrino pz
27  ## 3 : maximize the cosine of the angle between lepton and reconstructed W
28  ## in all these cases (0, 1, 2, 3), only the real part is used if solutions are complex
29  neutrinoSolutionType = cms.int32(-1)
30 )

Definition at line 6 of file TtSemiLepJetCombWMassDeltaTopMass_cfi.py.