Andy Blake Cambridge University Wednesday June 13 th 2007
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Transcript of Andy Blake Cambridge University Wednesday June 13 th 2007
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Andy BlakeCambridge University
Wednesday June 13th 2007
Combined Atmospheric Analysis:Study of 6 Month’s Data.
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Overview
Andy Blake, Cambridge University Combined Analysis, slide 2
• Developing a combined atmospheric neutrino analysis:
– Contained vertex muon neutrinos (John Chapman).
– Upward-going muons (Brian Rebel, John Chapman).
– Contained vertex electron neutrinos (Ben Speakman).
• Currently developing event selection code:
– All track and shower selection variables now calculated in AtNuOutput classes and stored in AtNuEvent classes.
– Event selection implemented in AtNuAna package.
– Analysis variables written to short AtNuAna Ntuples.
• Have now completed study using six month data sample.
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Event Selection
Andy Blake, Cambridge University Combined Analysis, slide 3
DATA / MC
DATA QUALITY CHECKS
GOOD TRACKS GOOD SHOWERS
GOOD EVENTS
UPWARD-GOINGMUONS
CONTAINEDVERTEX
ELECTRONNEUTRINOS
Outline ofevent selection:
John and Brian’strack selection
Ben’sshower selection
Data: HV, coil, GPS, LI, bad chips etc. MC: large scatters.
LI rejection,clean planes,
“fiducial” event
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Event Types
Andy Blake, Cambridge University Combined Analysis, slide 4
typedef enum EEventType { kNothing = 0x00, kGoodSlice = 0x01, kGoodEvent = 0x02, kGoodTrack = 0x04, kGoodShower = 0x08, kCV = 0x10, kCE = 0x20, kUP = 0x40, kFC = 0x80, kPC = 0x100, kPCDN = 0x200, kPCUP = 0x400, kUPMU = 0x800, kCosmic = 0x1000, kStoppingMuon = 0x2000, kThroughGoingMuon = 0x4000, kMultipleMuon = 0x8000, kVeto = 0x10000, kSpill = 0x20000, kBeamSpill = 0x40000, kFakeSpill = 0x80000, kGoodDirection = 0x100000, kGoodCharge = 0x200000, kPositiveCharge = 0x400000, kNegativeCharge = 0x800000, kAtmosNumu = 0x1000000, kAtmosNumuCV = 0x2000000, kAtmosNumuUP = 0x4000000, kAtmosNue = 0x8000000, kLIevent = 0x10000000, kMCscatter = 0x20000000 } EventType_t;
typedef enum EAtmosEventType { kNothing = 0x00, kGoodEvent = 0x01, kSpill = 0x02, kBeamSpill = 0x04, kVeto = 0x08, kCV = 0x10, kUP = 0x20, kGoodTrack = 0x40, kGoodShower = 0x80, kAtmosNumu = 0x100, kAtmosNumuCV = 0x200, kAtmosNumuUP = 0x400, kAtmosNue = 0x800, kAtmosNumuCVcut1 = 0x1000, kAtmosNumuCVcut2 = 0x2000, kAtmosNumuCVcut3 = 0x4000, kAtmosNumuCVcut4 = 0x8000, kAtmosNumuUPcut1 = 0x10000, kAtmosNumuUPcut2 = 0x20000, kAtmosNumuUPcut3 = 0x40000, kAtmosNumuUPcut4 = 0x80000, kAtmosNueCVcut1 = 0x100000, kAtmosNueCVcut2 = 0x200000, kAtmosNueCVcut3 = 0x400000, kAtmosNueCVcut4 = 0x800000 } AtmosEventType_t;
Eve
nt
Typ
es
containment
cosmics
veto shield,beam spills
good direction,good charge
light injectionMC scatter
Atm
osp
her
ic N
eutr
ino
Eve
nt
Typ
es
containment cuts
upward goingcuts
electron neutrinocuts
Above event types defined by methods in AtNuAna class.
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6 Month Study
Andy Blake, Cambridge University Combined Analysis, slide 5
• Data. – runs 31812/0-33480/6. (Jun 1st 2005 - Dec 31st 2005). – 206 days live time.
• Atmospheric Neutrino MC. – runs 233-242 (Cambridge). – 10x 178.3 kT-Yrs.
• Upward Muon MC. – runs 900-999 (Brian). – 100x 2 yrs .
• Cosmic Muon MC. – runs 651-750 (Cambridge). – 100x 17 hrs (70 days) .
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Data Quality Checks
Andy Blake, Cambridge University Combined Analysis, slide 6
Good Data
Bad Data
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Data Quality Checks
Andy Blake, Cambridge University Combined Analysis, slide 7
BAD HV
BAD COIL
Integrated Live Time
100% line
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Data/MC Checks
Andy Blake, Cambridge University Combined Analysis, slide 8
Stopping Muons: Reconstructed Zenith Angle
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Data/MC Checks
Andy Blake, Cambridge University Combined Analysis, slide 9
Stopping Muons: RMS of Down-Going Timing Fit
Timing fitting codeunder further study
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Data/MC Checks
Andy Blake, Cambridge University Combined Analysis, slide 10
Stopping Muons: Track Fit Relative Error
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Reconstruction Checks
Andy Blake, Cambridge University Combined Analysis, slide 11
Selected Contained Atmospheric Muon Neutrinos:Reconstructed Muon Momentum From Range.
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Reconstruction Checks
Andy Blake, Cambridge University Combined Analysis, slide 12
Selected Contained Atmospheric Muon Neutrinos:Reconstructed Muon Momentum From Curvature.
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Reconstruction Checks
Andy Blake, Cambridge University Combined Analysis, slide 13
Selected Contained Atmospheric Muon Neutrinos:Reconstructed Hadronic Shower Energy.
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Contained Event Selection
Andy Blake, Cambridge University Combined Analysis, slide 14
• Good Event Selection
– Data Quality Cuts.
• Good Track Selection.
– Track Planes. – Track Like Planes. – Track Pulse Height Fraction. – “Fiducial” Track.
• Containment Cuts.
– Contained Vertex. – Trace Cut. – Topology Cuts (I). – Topology Cuts (II). – Veto Shield Cut.
John C’s Selection Cuts
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Trace Cut
Andy Blake, Cambridge University Combined Analysis, slide 15
Contained Event Selection: Trace cut
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Topology Cuts (I)
Andy Blake, Cambridge University Combined Analysis, slide 16
Contained Event Selection: Mean/RMS position of strips around vertex
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Topology Cuts (I)
Andy Blake, Cambridge University Combined Analysis, slide 17
Contained Event Selection: Maximum plane charge, Strip displacement at vertex
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Topology Cuts (II)
Andy Blake, Cambridge University Combined Analysis, slide 18
Contained Event Selection: Vertex Charge vs Track Direction
Region removed by selection cut
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Veto Shield Cut
Andy Blake, Cambridge University Combined Analysis, slide 19
Time of Closest Veto Shield Hit (Cut at ±50 ns)
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Results
Andy Blake, Cambridge University Combined Analysis, slide 20
Data cosmic Background
atmos (no oscillations)
upward (no oscillations)
Contained 33,540 30,410 ± 3,040 94 ± 14 2 ± 0
Trace 2,330 2,090 ± 210 88 ± 13 1 ± 0
Topology (I) 712 510 ± 50 83 ± 12 1 ± 0
Topology (II) 301 175 ± 20 81 ± 12 1 ± 0
Veto Shield 84 6 ± 1 79 ± 12 1 ± 0
expectation = 86 ± 12 events(no oscillations)
Contained Event Selection
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Up-Going Event Selection
Andy Blake, Cambridge University Combined Analysis, slide 21
• Good Event Selection.
– Data Quality Cuts.
• Good Track Selection.
– Track Planes. – Track Like Planes. – Track Pulse Height Fraction. – “Fiducial” Track.
• Up Going Cuts.
– Topology Cuts. – Timing Cuts (I). – Timing Cuts (II).
John C’sSelection Cuts
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Timing Cuts (I)
Andy Blake, Cambridge University Combined Analysis, slide 22
Upward Event Selection: RMS timing deviations (up going, down going timing fits)
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Timing Cuts (I)
Andy Blake, Cambridge University Combined Analysis, slide 23
Upward Event Selection: RMS(up) / Range cut
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Timing Cuts (I)
Andy Blake, Cambridge University Combined Analysis, slide 24
Upward Event Selection: time slope cut
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Timing Cuts (II)
Andy Blake, Cambridge University Combined Analysis, slide 25
Upward Event Selection: RMS(up)-RMS(down)
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Results
Andy Blake, Cambridge University Combined Analysis, slide 26
Data cosmic Background
atmos (no oscillations)
upward (no oscillations)
Topology 790 400 ± 50 43 ± 6 52 ± 8
Timing (I) 69 0 31 ± 5 44 ± 7
Timing (II) 55 0 26 ± 4 43 ± 6
expectation = 69 ± 10 events(no oscillations)
Upward Event Selection
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Electron Neutrino Selection
Andy Blake, Cambridge University Combined Analysis, slide 27
• Good Event Selection.
– Data Quality Cuts.
• Good Shower Selection.
– Clean Planes. – Shower Planes. – Shower Pulse Height Fraction. – “Fiducial” Shower.
• Up Going Cuts.
– Contained Vertex. – Shower Trace. – Mean/RMS strips/charge per plane. – Moment of Inertia Tensor.
Ben’sSelection Cuts
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Shower Trace Cut
Andy Blake, Cambridge University Combined Analysis, slide 28
Electron Neutrino Selection: Shower Trace.
SHORT SHOWERS LONG SHOWERS
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Topology Cuts
Andy Blake, Cambridge University Combined Analysis, slide 29
Electron Neutrino Selection: RMS Strips Per Plane.
SHORT SHOWERS LONG SHOWERS
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MOI Cuts
Andy Blake, Cambridge University Combined Analysis, slide 30
Electron Neutrino Selection: Moment of Inertia Tensor.
SHORT SHOWERS LONG SHOWERS
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Veto Shield Cut
Andy Blake, Cambridge University Combined Analysis, slide 31
Time of Closest Veto Shield Hit (Cut at ±50 ns)
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Results
Andy Blake, Cambridge University Combined Analysis, slide 32
Data cosmic Background
atmos (no oscillations)
upward (no oscillations)
Contained 4250 2790 ± 280 55 ± 8 0 ± 0
Trace 1860 1100 ± 111 51 ± 8 0 ± 0
Topology 352 157 ± 17 42 ± 6 0 ± 0
MOI 187 61 ± 7 37 ± 6 0 ± 0
Veto Shield 37 4 ± 1 36 ± 5 0 ± 0
expectation = 40 ± 5 events(no oscillations)
Electron Neutrino Selection
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Summary
Andy Blake, Cambridge University Combined Analysis, slide 33
Data cosmic Background
atmos (no oscillations)
upward (no oscillations)
FC 69 5.2 ± 0.5 72.4 ± 10.9 1.7 ± 0.3
PCDN 17 0.8 ± 0.1 9.3 ± 1.4 0.1 ± 0.0
PCUP 2 0 10.2 ± 1.5 1.3 ± 0.2
UPMU 34 0 1.7 ± 0.2 40.1 ± 6.2
Muon Neutrino Selection
Data cosmic Background
atmos (no oscillations)
upward (no oscillations)
NUE 37 4.4 ± 0.4 36.0 ± 5.4 0 ± 0
Electron Neutrino Selection
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Selected FC/PC Events
Andy Blake, Cambridge University Combined Analysis, slide 34
Selected FC/PC Events: Vertex Distance from Edge of Detector
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Selected FC/PC Events
Andy Blake, Cambridge University Combined Analysis, slide 35
Selected FC/PC Events: Reconstructed Neutrino Energy
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Selected FC/PC Events
Andy Blake, Cambridge University Combined Analysis, slide 36
Selected FC/PC Events: Reconstructed L/E
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Vetoed FC/PC Events
Andy Blake, Cambridge University Combined Analysis, slide 37
Vetoed FC/PC Events: Vertex Distance from Edge of Detector
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Vetoed FC/PC Events
Andy Blake, Cambridge University Combined Analysis, slide 38
Vetoed FC/PC Events: Reconstructed Zenith Angle (from top of track)
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Vetoed FC/PC Events
Andy Blake, Cambridge University Combined Analysis, slide 39
Vetoed FC/PC Events: Track Planes.
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Selected UPMU Events
Andy Blake, Cambridge University Combined Analysis, slide 40
Selected UPMU Events: Reconstructed Muon Momentum
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Selected UPMU Events
Andy Blake, Cambridge University Combined Analysis, slide 41
Selected UPMU Events: Reconstructed Zenith Angle
Need to add thehorizontal events
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Selected NUE Events
Andy Blake, Cambridge University Combined Analysis, slide 42
Selected NUE Events: Vertex Distance from Edge of Detctor
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Selected NUE Events
Andy Blake, Cambridge University Combined Analysis, slide 43
Selected NUE Events: Shower Planes
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Selected NUE Events
Andy Blake, Cambridge University Combined Analysis, slide 44
Selected NUE Events: Reconstructed Shower Energy.
Reconstructed usinghadronic energy scale,
So needs re-tuning
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Vetoed NUE Events
Andy Blake, Cambridge University Combined Analysis, slide 45
Vetoed NUE Events: Vertex Distance from Edge of Detector
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Vetoed NUE Events
Andy Blake, Cambridge University Combined Analysis, slide 46
Vetoed NUE Events: Reconstructed Shower Energy
Large disagreementbetween data and MC
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Summary
Andy Blake, Cambridge University Combined Analysis, slide 47
• Much of Analysis Implemented. – Data Quality Checks. – Data/MC Comparisons. – MC Checks. – Event Selection.
• Some disagreements. – Timing Simulation.
– Shower Energy Reconstruction. – Electron Neutrino Background.
• Future Work. – Timing Calibration for Latest Data. – Study Veto Shield. – Bayesian L/E Resolution.