Large-Area Scintillator Hodoscope with 50 ps Timing Resolution Onboard BESS
arXiv:hep-ex/0002047 · doi:10.1016/S0168-9002(00)00571-4
Abstract
We describe the design and performance of a large-area scintillator hodoscope onboard the BESS rigidity spectrometer; an instrument with an acceptance of 0.3 m^{2}sr. The hodoscope is configured such that 10 and 12 counters are respectively situated in upper and lower layers. Each counter is viewed from its ends by 2.5 inch fine-mesh photomultiplier tubes placed in a stray magnetic field of 0.2 Tesla. Various beam-test data are presented. Use of cosmic-ray muons at ground-level confirmed 50 ps timing resolution for each layer, giving an overall time-of-flight resolution of 70 ps rms using a pure Gaussian resolution function. Comparison with previous measurements on a similar scintillator hodoscope indicates good agreement with the scaling law that timing resolution is proportional to 1/, where is the effective number of photoelectrons.
arXiv comment16 pages, 14 figures
References in corpus (7)
- Precision Measurement of Cosmic-Ray Antiproton Spectrum
- Local Flux of Low-Energy Antiprotons from Evaporating Primordial Black Holes
- Measurement of Low-Energy Cosmic-Ray Antiprotons at Solar Minimum
- Expected Enhancement of the Primary Antiproton Flux at the Solar Minimum
- Development of a Large-Area Aerogel Cherenkov Counter Onboard BESS
- Feasibility Study of Single-Photon Counting Using a Fine-mesh Phototube for an Aerogel Readout
- Monte-Carlo Simulation for an Aerogel Cherenkov Counter
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