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

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SiPMs the (almost) perfect Photon Detector for Cherenkov Telescopes Potential for very high PDE in the blue Robust Reliable Cheap .... SiPMs begin to outperform classical PMTs in astroparticle applications Biggest nuisances these days: Slow signals Temperature dependence of gain, PDE, ... Optical Crosstalk All these nuisances can be eliminated at device level but for the time being we have to deal with them Nepomuk Otte MEPhI/Pulsar SiPM 14
Output signals
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: Operational Requirements Purpose of
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 and 24: Conceptual Design Primary goal for
Page 25 and 26: Photon Emission during Breakdown Av
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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