TY - JOUR
T1 - Performance of 8 × 8 pixel LaBr3
T2 - Ce and Gd 2SiO5: Ce scintillator arrays coupled to a 64-channel multi-anode PMT
AU - Kurosawa, Shunsuke
AU - Kubo, Hidetoshi
AU - Hattori, Kaori
AU - Ida, Chihiro
AU - Iwaki, Satoru
AU - Kabuki, Shigeto
AU - Miuchi, Kentaro
AU - Nishimura, Hironobu
AU - Okada, Yoko
AU - Parker, Joseph D.
AU - Takada, Atsushi
AU - Takahashi, Michiaki
AU - Tanimori, Toru
AU - Ueno, Kazuki
AU - Yanagida, Yoshio
N1 - Funding Information:
Manuscript received February 01, 2009; revised August 10, 2009. Current version published December 09, 2009. This work is supported by the Global COE “Next Generation Physics, Spun from Universality and Emergence”; a Grant-in-Aid in Scientific Research of the Japan Ministry of Education, Culture, Science, Sports, Technology; “SENTAN”, JST.
PY - 2009/12
Y1 - 2009/12
N2 - We have developed a LaBr3 :Ce scintillator array consisting of 8 × 8 pixels with a size of 5.8 mm × 5.8 mm × 15.0 mm, which serves as an absorber of scattered gamma rays with energies from 0.1 to 1 MeV in a Compton camera. The pixels were cut from two pieces of LaBr3 :Ce crystal with a diameter of 38 mm and a length of 38 mm with full width at half-maximum (FWHM) energy resolutions of 4.1 ± 0.1 % and 3.0 ± 0.1 % at 356 and 662 keV, respectively, measured with a single anode photomultiplier tube (PMT). The crystal had the following volumetric uniformities: light outputs with a difference of 0.5% (standard deviation: SD) and energy resolutions with that of 2% (SD) at 356 keV. In contrast, for each pixel in the array, the average and SD FWHM energy resolutions over 64 pixels, measured with a single-anode PMT and a collimator, were 5.8 ± 0.9% at 356 keV. The array was then coupled to a 64-channel multi-anode PMT (Hamamatsu H8500), the anode pitch of which was the same as the LaBr :Ce pixel pitch of 6.1 mm. When the 64 anodes were read out from four channels in a resistor chain by the charge division method, the FWHM energy resolution of all 64 pixels was 7.0 ± 0.5 % at 662 keV, whereas that of the inner6 × 6 pixels was 5.8±0.4% at 662 keV. In addition, we measured a Gd2SiO 5 :Ce (GSO:Ce) scintillator array consisting of 8×8 pixels with a size of 5.9 mm × 5.9 mm × 13.0 mm to compare its performance with that of the LaBr3 :Ce array. The FWHM energy resolution of all 64 GSO:Ce pixels was 10.8 ± 0.3% at 662 keV. With these energy resolutions, FWHM angular resolutions of the Compton camera using the LaBr3 :Ce and GSO:Ce arrays are expected to be 4.6° and 5.3°, respectively, at 662 keV.
AB - We have developed a LaBr3 :Ce scintillator array consisting of 8 × 8 pixels with a size of 5.8 mm × 5.8 mm × 15.0 mm, which serves as an absorber of scattered gamma rays with energies from 0.1 to 1 MeV in a Compton camera. The pixels were cut from two pieces of LaBr3 :Ce crystal with a diameter of 38 mm and a length of 38 mm with full width at half-maximum (FWHM) energy resolutions of 4.1 ± 0.1 % and 3.0 ± 0.1 % at 356 and 662 keV, respectively, measured with a single anode photomultiplier tube (PMT). The crystal had the following volumetric uniformities: light outputs with a difference of 0.5% (standard deviation: SD) and energy resolutions with that of 2% (SD) at 356 keV. In contrast, for each pixel in the array, the average and SD FWHM energy resolutions over 64 pixels, measured with a single-anode PMT and a collimator, were 5.8 ± 0.9% at 356 keV. The array was then coupled to a 64-channel multi-anode PMT (Hamamatsu H8500), the anode pitch of which was the same as the LaBr :Ce pixel pitch of 6.1 mm. When the 64 anodes were read out from four channels in a resistor chain by the charge division method, the FWHM energy resolution of all 64 pixels was 7.0 ± 0.5 % at 662 keV, whereas that of the inner6 × 6 pixels was 5.8±0.4% at 662 keV. In addition, we measured a Gd2SiO 5 :Ce (GSO:Ce) scintillator array consisting of 8×8 pixels with a size of 5.9 mm × 5.9 mm × 13.0 mm to compare its performance with that of the LaBr3 :Ce array. The FWHM energy resolution of all 64 GSO:Ce pixels was 10.8 ± 0.3% at 662 keV. With these energy resolutions, FWHM angular resolutions of the Compton camera using the LaBr3 :Ce and GSO:Ce arrays are expected to be 4.6° and 5.3°, respectively, at 662 keV.
KW - Array camera
KW - Compton camera
KW - GSO:Ce
KW - LaBr:Ce
KW - Scintillation detectors
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U2 - 10.1109/TNS.2009.2034657
DO - 10.1109/TNS.2009.2034657
M3 - Article
AN - SCOPUS:72349086609
SN - 0018-9499
VL - 56
SP - 3779
EP - 3788
JO - IEEE Transactions on Nuclear Science
JF - IEEE Transactions on Nuclear Science
IS - 6
M1 - 5341429
ER -