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Development of the Large Aperture EBCCD
○A. Suzuki, S. Aoki(Kobe Univ.)J. Haba(KEK)
M. Sakuda(Okayama Univ.)M. Suyama(Hamamatsu Photonics)
Contents
1. Motivation of development2. Specification of the EBCCD3. Basic performance
HV endurance & gainSpatial resolutionLinearity between input & outputCosmic ray detection
4. Summary
For example,the K2K SciFi detector[K2K Collab., A.Suzuki, et al., NIM A453(2000) 165-176]・ Many channel readout(11k fibers/IIT) ・1pe detection (high gain).
IIT
SciFi detector of K2K 24 IITs (φ10cm photocathode) and φ0.7mm fiber were used.
1. Motivation of developmentAs a same kind of photosensor as EBCCD, IIT has been used so far in particle physics experiments.
~
Electron multiplication is fluctuated at MCP and fluorescent plate.
Accelerated photoelectrons directly reach CCD and multiplied. → No fluctuation in
multiplication in principle
Good linearity between input and output is expected.
Photocathode
MCPFluorescent plate
CCD
EBCCD
IIT
high gain & large aperture EBCCD is desired!
If such one is used for readout of a scintillating fiber detector like the K2K SciFi detector,
・ good linearity in dE/dX measurement gives good PID.
・many channels can be read out at one time.
Therefore,
But EBCCD so far --- low gain & small aperture
2. Specification of the EBCCD
10cm
20cm
* Such a large aperture was realized by electron demagnificaton.
2. Specification of the EBCCDParameters Description / Value Unit
Spectral response 300 to 650 nmMaterial Bi-alkali --
Effective area
46×36 mm
Window material Fiber optic plate (FOP) --Magnification 1/5
Type FT-CCDEffectivearea 9.0 (H) × 6.7 (V) mm
# of pixels 640 (H) × 480 (V)Pixel size 14 × 14 μm
Target
Photo-cathode
3. Basic performance
HV endurance
Photocathode voltage (-kV)12
2400
Gai
n
1200
Good linearity !
Spatial resolution (1)Estimated from brightness distributions of ladder chart images
← Brightness distribution
X position [pixel]
Brig
htne
ss [a
rbitr
ary
unit]
Ladder chart image →
Brightness distributions0.25 lp/mm 0.5 lp/mm 0.625 lp/mm
1 lp/mm 1.67 lp/mm 2 lp/mm
We can see clear peaks and valleys up to 2 line pairs/mm (corresponds to 3.5 × CCD pixel size).
Spatial resolution (2)Estimated from an image of Cu foil pattern on a
fluorescent plate irradiated with X-rays (14 keV and 18 keV) and γ-ray (60 keV) form an Am source
2413cm
3mm50μm thick Cu foil pattern
Fluorescent plate(0.5mm thick)
Am
X-rayγ-ray
EBCCD
241
241
We could see gaps of ~0.25mm, corresponding to 2 lp/mm
Image of Cu foil pattern
Gaps between neighboring foils are ~0.25mm here
Linearity between output and input
• EBCCD output was measured as a function of input LED light.
• Input light intensity was monitored by PMT.• Same measurement was done for IIT to
compare.
Setup for the measurement
Blue LED(from the side of the fiber)
Scintillating fiber (φ0.7mm)
orIIT
EBCCDorIIT
Comparison of linearities
Light yield on PMT
EBC
CD
IIT
outp
ut (a
rb. U
nit)
EBCCD
IIT
Cosmic ray detectionby the scintillating fiber block
Cosmic ray
・Cross sectional view・φ0.7mm fiber
Effectivearea
46mm
36m
m
Cosmic ray track image
In spite of no gating, we can see a track!(1 frame image of several photoelectrons)
4. SummaryLarge aperture EBCCD was produced.
photocathode φ10cm. The 1st one with such a large aperture.
Some basic performances were measured.・HV endurance --- up to –12k
(Gain vs HV showed good linearity.)・spatial resolution --- better than 2 lp/mm ・good linearity between input and output
(better linearity than that of IIT) ・cosmic ray track detection --- OK!
• We are planning to develop an EBCCD with higher gain and gating function and use in particle physics experiment practically.
Image distortion
Image of 5mm spacing lattice Spacing on the CCD at various positions (unit in CCD pixel)
No significant position dependence of the spacingsSame result for 2mm spacing lattice→ Negligible distortion in the effective area (46mm(H)×36mm(V))
Brightness distributions for ladder charts(measured by IIT)
MTF vs spatial resolution
Spatial resolution [lp/mm]
MTF
EBCCD
IIT
MTF vs spatial resolution measured with Cu foil pattern
Development of the Large Aperture EBCCDContentsMotivation of development2. Specification of the EBCCD2. Specification of the EBCCD3. Basic performanceHV enduranceSpatial resolution (1)Brightness distributionsSpatial resolution (2)Linearity between output and inputComparison of linearitiesCosmic ray detection �by the scintillating fiber block Cosmic ray track image4. SummaryImage distortionBrightness distributions for ladder charts�(measured by IIT)MTF vs spatial resolution MTF vs spatial resolution measured with Cu foil pattern