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Contribution Poster
THE FLIGHT ELECTRONICS SYSTEM FOR THE COSMIC RAY ELECTRON SYNCHROTRON TELESCOPE (CREST) EXPERIMENT
Speakers
- G. TARLE
Primary authors
- G. TARLE (University of Michigan)
Co-authors
- J. AMEEL (University of Michigan)
- R. BALL (University of Michigan)
- C. BOWER (Indiana University)
- S. COUTU (Pennsylvania State University)
- M. GEPHARD (Indiana University)
- D. MULLER (University of Chicago)
- J. MUSSER (Indiana University)
- S. NUTTER (Northern Kentucky University)
- M. SCHUBNELL (University of Michigan)
- C. SMITH (University of Chicago)
- S. WAKELY (University of Chicago)
- A. YAGI (University of Michigan)
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Abstract content
The balloon-borne Cosmic Ray Electron Synchrotron Telescope (CREST)
experiment will employ a novel distributed
electronics system to collect timing and pulse height information from 1024
BaF2 crystal detectors and 42 PMTs in
its anticoincidence shield. The timing of single photoelectron triggers from the
PMTs in the crystal array is recorded
to an accuracy of 1 ns least count. Wide dynamic range pulse height
information from two dynodes on each PMT is
recorded when two or more crystals receive single photoelectron triggers.
Timing and pulse height information from
the anticoincidence shield is recorded only when received within a preset time
window of crystal array triggers.
Integral Cockroft-Walton high voltage power supplies, potted within the PMTs
are individually set by a digitally
addressable control and monitoring system. Extensive use of FPGAs and CPLDs
enable high-speed synchronous
operation and low power consumption with a flexible distributed and modular
architecture.
If this papers is presented for a collaboration, please specify the collaboration
CREST
Reference
Proceedings of the 30th International Cosmic Ray Conference; Rogelio Caballero, Juan Carlos D'Olivo, Gustavo Medina-Tanco, Lukas Nellen, Federico A. Sánchez, José F. Valdés-Galicia (eds.); Universidad Nacional Autónoma de México, Mexico City, Mexico, 2008; Vol. 2 (OG part 1), pages 313-316