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EAS Reconstruction with Cerenkov photons
Ching-Cheng Hsu, Jan.29 2003
Ching-Cheng Hsu National Taiwan Univ. Dept of physics Feb. 13 2003
Shower Simulation
Reconstruction Algorithm
Toy MC Study
Summary
Ching-Cheng Hsu PSROC 2003, Feb. 13, 2003
CORSIKA-> ReconstructionCORSIKA-> Reconstruction
Air Shower
Č photons
CORSIKA
telesim
Read out Č photons and
simple detector simulation photon weighting,
detectors sampling
Reconstruction
E, shower axis
Input card
?
Ching-Cheng Hsu PSROC 2003, Feb. 13, 2003
Detector configurations Detector configurations
4 m
4 m
2m
2m20m
Corsika detector
Our detector
40 X 50 detectors in a 4.5 x 5.0 km2 area
20m
Ching-Cheng Hsu PSROC 2003, Feb. 13, 2003
Detection areaDetection area
Y
X10 km
5 km
4.5 km
10 km
North
West
Ching-Cheng Hsu PSROC 2003, Feb. 13, 2003
Detector Parameters Detector Parameters
Lens area : 4 m2 . Transmittance 0.95
Focal length : 43 cm
Pixel angular Span: 0.5 degree
PMT QE : 0.3
Spot size : 0.04 cm < pixel size 0.375 cm
We have 40x40 pixels of PMT in a 15 cm x15 cm area
Ching-Cheng Hsu PSROC 2003, Feb. 13, 2003
Č Production Height
Higher Energy
Closer to the Ground
31-34 Km
1014 eV1016 eV
1018 eV
Electron showers with new atmospheric model
Ching-Cheng Hsu PSROC 2003, Feb. 13, 2003
Photon density on the groundPhoton density on the ground
1018eV
1016eV
1014eV
Peak position 680 – 750 m
MINUIT: minimize χ2 to get x,y,θ,φ and E
(x2, y2 )N2. t2
N1, t1
(x1, y1)E, (x, y,θ,φ)
Reconstruction Illustration Reconstruction Illustration
Ching-Cheng Hsu PSROC 2003, Feb. 13, 2003
Ching-Cheng Hsu PSROC 2003, Feb. 13, 2003
Cerenkov photon Cerenkov photon densitydensity
Double Gaussian
+ exponential decayPh
oto
n d
ensi
ty
Electron shower 1014eV
We know N(E, )
2
Ching-Cheng Hsu PSROC 2003, Feb. 13, 2003
The AlgorithmThe Algorithm
Within a polar angle 12 region, randomly pick one detector and choose another detector separated by 200 m distances to minimize the following
2 = ( 1 - 0.13)2 / 0.152 + (2 -0.13)2
/ 0.152 + d12 / 302 + d2
2 /302 + [N1-N(E, 1 )]2 / N1 + [N2-N(E, 2 ] 2 / N2 + (l1/c - l2 /c+t2-t1)2/ 0.32
Ching-Cheng Hsu PSROC 2003, Feb. 13, 2003
Reconstruction CORSIKA Reconstruction CORSIKA data data
Δx Δt
Δθ Er / Et
1014eVDetectors distance 200m
Ching-Cheng Hsu PSROC 2003, Feb. 13, 2003
Reconstruction CORSIKA Reconstruction CORSIKA datadata
1016eVDetectors distance 200m
Δx Δt
Δθ Er / Et
Ching-Cheng Hsu PSROC 2003, Feb. 13, 2003
Study of Two Detector Study of Two Detector Performance with Toy MC Performance with Toy MC
1015eV electron shower
One p.e. threshold, no background
Shower starts 30 km height
Mirror area 1 m2
Field of view 12o
Pixel angular span 1o
Vary the distance between the detectors with 100 m step
Ching-Cheng Hsu PSROC 2003, Feb. 13, 2003
Efficiency Efficiency
Within 2km, efficiency is flat.
→
Ching-Cheng Hsu PSROC 2003, Feb. 13, 2003
OK, near 1
The Mean Reconstructed Energy Ratio
Ching-Cheng Hsu PSROC 2003, Feb. 13, 2003
Reconstructed Augular Reconstructed Augular Deviation Deviation
1o can be achieved
Ching-Cheng Hsu PSROC 2003, Feb. 13, 2003
Summary Summary
We can reconstruct EAS with We can reconstruct EAS with ČČ photons from photons from Corsika data by two detectors.Corsika data by two detectors.
The reconstruction method is simple and can be The reconstruction method is simple and can be improved. improved.
The study done by a Toy MC indicates the The study done by a Toy MC indicates the detector separation of 3detector separation of 3oo-4-4oo is optimal. is optimal.
Next Step: Next Step:
Put in background and use pixel information for Put in background and use pixel information for shower reconstruction. shower reconstruction.
Ching-Cheng Hsu PSROC 2003, Feb. 13, 2003
Reconstruction by Toy Reconstruction by Toy MC MC
1014eV
ΔθEr / Et
Δx Δt
Ching-Cheng Hsu PSROC 2003, Feb. 13, 2003
Absolute Time differenceAbsolute Time difference in in Two DetectorsTwo Detectors
CORSIKA data
200 ns for separation distance 2km
Hard for coincidence?
Ching-Cheng Hsu PSROC 2003, Feb. 12, 2003
Fit to 5 km Fit to 5 km
Similar PDF parameters
Ching-Cheng Hsu PSROC 2003, Feb. 13, 2003
Difficulties of Difficulties of Simulation Simulation
Ching-Cheng Hsu PSROC 2003, Feb. 12, 2003
Difficulties of Difficulties of Simulation Simulation
Ching-Cheng Hsu PSROC 2003, Feb. 13, 2003
Difficulties of Difficulties of Simulation Simulation
Ching-Cheng Hsu PSROC 2003, Feb. 13, 2003
Difficulties of Difficulties of Simulation Simulation
Ching-Cheng Hsu PSROC 2003, Feb. 12, 2003
Difficulties of Difficulties of Simulation Simulation
Ching-Cheng Hsu PSROC 2003, Feb. 12, 2003
Difficulties of Difficulties of Simulation Simulation
Ching-Cheng Hsu PSROC 2003, Feb. 12, 2003
Difficulties of Difficulties of Simulation Simulation
Ching-Cheng Hsu PSROC 2003, Feb. 12, 2003
Difficulties of Difficulties of Simulation Simulation