Nuisances of SiPMs and how to deal with them in ... - KICP Workshops

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Optical Crosstalk Nepomuk Otte 24
Photon Emission during Breakdown Avalanches produce a lot of photons, emission processes are being debated Photons in a very narrow energy range propagate out of their originating cell and absorb in neighboring if Photon energy is between 1.1 eV and 1.4 eV Photon intensity: 3x10 -5 photons per avalanche electron -> Intensity is direct proportional to gain ANO NIM A (610) 2009, 105–109 Nepomuk Otte Picture by C. Merck 25
Page 1 and 2: Nuisances of SiPMs and how to deal
Page 3 and 4: CTA-US SC telescope Schwarzschild C
Page 5 and 6: Module Conceptional Design Cold fin
Page 7 and 8: Night Sky Background Light From sta
Page 9 and 10: Intensities are not to scale Nepomu
Page 11 and 12: P(n) = λ n /n! exp(-λ) Non-Poisso
Page 13 and 14: Operational Requirements Purpose of
Page 15 and 16: Output signals
Page 17 and 18: Faster output pulses by adding one
Page 19 and 20: Temperature Dependencies Critical E
Page 21 and 22: PDE Different effects contribute to
Page 23: Conceptual Design Primary goal for
Page 27 and 28: Non-Poisson tails due to optical cr
Page 29 and 30: Dependency of gain on NSB rate Larg

Nuisances of SiPMs and how to deal with them in ... - KICP Workshops

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