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19 April 2024 |
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Article overview
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Background Measurements from Balloon-Borne CZT Detectors | | Johnathan A Jenkins
; Tomohiko Narita
; Jonathan E. Grindlay
; Peter F. Bloser
; Carl Stahle
; Brad Parker
; Scott Barthelmy
; | | Date: |
25 Nov 2002 | | Subject: | astro-ph | | Affiliation: | Harvard), Tomohiko Narita (Holy Cross), Jonathan E. Grindlay (Harvard), Peter F. Bloser (GSFC), Carl Stahle (GSFC), Brad Parker (GSFC), and Scott Barthelmy (GSFC | | Abstract: | We report detector characteristics and background measurements from two prototype imaging CZT detectors flown on a scientific balloon payload in May 2001. The detectors are both platinum-contact 10mm x 10mm x 5mm CZT crystals, each with a 4 $ imes$ 4 array of pixels tiling the anode. One is made from IMARAD horizontal Bridgman CZT, the other from eV Products high-pressure Bridgman material. Both detectors were mounted side-by-side in a flip-chip configuration and read out by a 32-channel IDE VA/TA ASIC preamp/shaper. We enclosed the detectors in the same 40deg field-of-view collimator (comprisinga graded passive shield and plastic scintillator) used in our previously-reported September 2000 flight. I-V curves for the detectors are diode-like, and we find that the platinum contacts adhere significantly better to the CZT surfaces than gold to previous detectors. The detectors and instrumentation performed well in a 20-hour balloon flight on 23/24 May 2001. Although we discovered a significant instrumental background component in flight, it was possible to measure and subtract this component from the spectra. The resulting IMARAD detector background spectrum (from 30 keV to ~450 keV) reaches ~5 x 10^{-3}$ counts/cm^2 -sec-keV at 100 keV and has a power-law index of ~2 at high energies. The eV Products detector has a similar spectrum, although there is more uncertainty in the energy scale because of calibration complications. | | Source: | arXiv, astro-ph/0211529 | | Services: | Forum | Review | PDF | Favorites | |
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