2008 IEEE Nuclear Science Symposium Conference Record 2008
DOI: 10.1109/nssmic.2008.4774554
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Silicon photo-multiplier readouts for scintillators in high-energy astronomy

Abstract: New scintillator materials have recently been shown to hold great potential for low-eost, reliable gamma-ray detectors in high-energy astronomy. New devices for the detection of scintillation light promise to make scintillator-based instruments even more attractive by reducing mass and power requirements. In particular, silicon photo-multipliers (SiPMs) are starting to become commercially available that otTer gains and quantum efficiencies similar to those of photo-multiplier tubes (PMTs), but with greatly red… Show more

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Cited by 5 publications
(10 citation statements)
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“…The energy resolution measured at 662 keV is 7.2 ± 0.1% (FWHM). This is a better value than achieved in previous work [8], but not as good as expected. The low energy threshold is ~10 keV using our simple level trigger.…”
Section: Spectral Data Analysiscontrasting
confidence: 46%
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“…The energy resolution measured at 662 keV is 7.2 ± 0.1% (FWHM). This is a better value than achieved in previous work [8], but not as good as expected. The low energy threshold is ~10 keV using our simple level trigger.…”
Section: Spectral Data Analysiscontrasting
confidence: 46%
“…In our previous work we required a coincidence between fast outputs in order to reduce the effects of uncorrelated dark counts and lower the trigger threshold [8]. Due to the improved light collection of the larger S10985, however, we did not find this to be necessary this time.…”
Section: Laboratory Test Proceduresmentioning
confidence: 97%
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“…For the past several years we have therefore been investigating the use of commercially available SiPMs in various scintillator readout configurations [9], [10]. In this paper we describe the successful balloon test flight of a small LaBr3/SiPM detector, and initial tests with larger devices.…”
Section: Introductionmentioning
confidence: 99%