Gamma-ray Large Area Gamma-ray Large Area Space TelescopeSpace Telescope
AssociatingAssociatingCalMip and Track CalMip and Track
VariablesVariables
Stefano GermaniMonica Pepe
INFN Perugia
Instrument Analysis MeetingDecember 16, 2005
SVAC Instrument Analysis Meeting, December 16, 2005
Stefano Germani & Monica Pepe 2
Outlook Outlook
• The second part of the study concerns Mip reconstructed directions
– consistency check
– correlation with the Mip segment length
– comparison to the Track directions
All plots refer to following cuts» TkrNumTracks = 1» CalMipNum > 0
SVAC Instrument Analysis Meeting, December 16, 2005
Stefano Germani & Monica Pepe 3
CalMip PositionCalMip Position
CalMip1Pos(X)C
alM
ip1P
os(
Y)
CalMip1Pos(X)
Cal
Mip
1Po
s(Y
)
All 1 Track EventsOn Axis Events VtxZDir<-0.9 (25.8 deg)
On Axis events have more homogeneous CalMip1Pos distribution
TkrNumTracks=1CalMipNum > 0
SVAC Instrument Analysis Meeting, December 16, 2005
Stefano Germani & Monica Pepe 4
Mip direction and segment lengthMip direction and segment length
CalMip1Dir(Z)
CalMip1ArcLen
mm
CAL thickness
Cal thickness ~160 mm(8×1Layer = 8×20 mm)
Try to understand the meaning of second peak in the next slides
At least 3 layers
TkrNumTracks=1CalMipNum > 0
SVAC Instrument Analysis Meeting, December 16, 2005
Stefano Germani & Monica Pepe 5
CalMip1Dir(Z) vs CalMip1ArcLen (I)
CalMip1ArcLen (mm)
Cal
Mip
1Dir
(Z)
Mip Finder requires:• XtalEnergy > 8 MeV• NLayers >= 3
The plot structure reflects the number of CAL layers crossed by the MIP(see next slide)
TkrNumTracks=1CalMipNum > 0
SVAC Instrument Analysis Meeting, December 16, 2005
Stefano Germani & Monica Pepe 6
CalMip1Dir(Z) vs CalMip1ArcLen (II)
Energy deposition > 8 MeV in 8 Layers
Energy deposition > 8 MeV in only 6 Layers
mm
mm
MIP
MIP
Mip Finder requires:• XtalEnergy > 8 MeV• NLayers >= 3
TkrNumTracks=1CalMipNum > 0
SVAC Instrument Analysis Meeting, December 16, 2005
Stefano Germani & Monica Pepe 7
Investigating long Mip segments
Energy deposition > 8 MeV in Layers 07
All Events
SelectedRegion
CalMip1Dir(z)
CalMip1ArcLen (mm)
All Events
CalMip1Dir(z) > -.78
-.88 <CalMip1Dir/z) <- .7828° 39°C
alM
ip1
Dir
(z)
CalMip1ArcLen (mm)
We understand correlation between Mip direction and arc length but
Why so many “green” MIPs?
0°28°
39°
TkrNumTracks=1CalMipNum > 0
SVAC Instrument Analysis Meeting, December 16, 2005
Stefano Germani & Monica Pepe 8
Look at MIP segment directionLook at MIP segment direction
CalMip1Dir(X)
CalMip1Dir(Y)
CalMip1Dir(Y) vs CalMip1Dir(X)
Fred please Fred please
cross check!cross check!
On Axis Tracks
CalMip1Dir(Z) second peak
TkrNumTracks=1CalMipNum > 0
SVAC Instrument Analysis Meeting, December 16, 2005
Stefano Germani & Monica Pepe 9
Correlating CAL and TrackCorrelating CAL and Track
X Dir
Y Dir
Z Dir
CA
L
CA
L
CA
L
Track
Track
Track
CAL: CalMip1Dir(X,Y,Z)
Track: Vtx(X,Y,Z)Dir
MIP finder well correlated to reconstructed track
but……….
TkrNumTracks=1CalMipNum > 0
SVAC Instrument Analysis Meeting, December 16, 2005
Stefano Germani & Monica Pepe 10
CalMip1Dir vs Tkr1EndDirCalMip1Dir vs Tkr1EndDir
X Dir
Z Dir
VtxZDir
Tkr1EndDir(2)
CAL: CalMip1Dir(X,Y,Z)
Track: Tkr1EndDir(X,Y,Z)
CA
LC
AL
Track
Track
Beware of different orientation for initial (Vtx) and final (Tkr) Track direction
SVAC Instrument Analysis Meeting, December 16, 2005
Stefano Germani & Monica Pepe 11
ConclusionsConclusions
• Mip direction is well correlated to Track direction as expected
• We have still to understand better the peaks in the Mip Direction distributions (X,Y,Z)– maybe they reflect the Cal Layer geometry ?
SVAC Instrument Analysis Meeting, December 16, 2005
Stefano Germani & Monica Pepe 12
Summary of CalMip SVAC variablesSummary of CalMip SVAC variables
• Analyzed– CalMipNum– CalMipnPos(3) n=1,2– CalMipnDir(3)– CalMipnChi2 – CalMipnArcLen– CalMipnEcor– CalMipnErm
• Not yet checked– CalMipnD2edge– CalMipnEcorRms
Thanks Frederic for useful explanations !!
We are waiting for real data!!
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