ay 191 experiment development of hard x-ray imaging detectors j. hong and j. grindlay
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Ay 191 Experiment Development of Hard X-ray Imaging Detectors J. Hong and J. Grindlay Hard X-rays (~10-600 keV) are direct probes of black holes : GRBs, AGNs, Stellar BHs, etc. - PowerPoint PPT PresentationTRANSCRIPT
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Ay 191 Experiment Development of Hard X-ray Imaging Detectors
J. Hong and J. Grindlay
• Hard X-rays (~10-600 keV) are direct probes of black holes: GRBs, AGNs, Stellar BHs, etc.
• Direct imaging possible only for narrow FoV (<~0.1º) and only for low energies (<~100 keV) => coded-aperture telescope
• Harvard balloon-borne telescope (ProtoEXIST) is a coded-aperture telescope for wide-field (~20ºx20º) hard X-ray imaging and is a prototype platform for development of the
scanning telescope needed for a major NASA mission,
EXIST, to conduct a very sensitive all-sky survey for BHs
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Coded-Aperture Hard X-ray Imaging Telescope
Decoding Shadowgram allows wide-field imaging.
Position-sensitive hard X-raydetectors needed: Use Cd-Zn-Te (CZT) arrays.
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Cd-Zn-Te (CZT) Hard X-ray imaging detector
CZT Detectors 8 x 8 pixels on each 20 x 20mmCZT crystal (pixels on bottom)
Schematic CZT detector:
Electrons drift to anode
Under ~700V bias
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CZT detectors: prototype lab arrayCZT detectors: prototype lab array
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4cm x 8cm Detector Crystal Array (DCA)
ProtoEXIST detector array
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Energetic X-ray Imaging Telescope Experiment (ProtoEXIST)with 1000 cm2 CZT detectors
Balloon-borne ProtoEXIST Telescope
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• Learn about -Hard X-ray sources in the sky: Black holes … -Hard X-ray Imaging: Coded-aperture telescopes -Hard X-ray Detectors: CdZnTe detector
• Experiments to be conducted (at CfA ProtoEXIST lab, B-105):
-Calibrating new CZT imager with 60, 122, 356 keV sources
-Measuring spatial and spectral resolution over detector
-Sensitivity to multi-pixel (split) events-Cooling test (to -10°C) with CZT modules-Design considerations for ProtoEXIST balloon-
telescope
Ay191 experiments