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Development of the Large Aperture EBCCD A. Suzuki, S. AokiKobe Univ.J. HabaKEK) M. SakudaOkayama Univ.M. SuyamaHamamatsu Photonics

Development of the Large Aperture EBCCDndip.in2p3.fr › ndip08 › Presentations › 3Tuesday › Matin › 230-Suzuki.pdfthe K2K SciFi detector [K2K Collab., A.Suzuki, et al., NIM

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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