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

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Overview The Cherenkov imaging technique Photon detector requirements SiPM nuisances: Effects, Impacts, Workarounds Slow output signals Temperature dependencies Optical crosstalk Bias
CTA-US SC telescope Schwarzschild Couder Optics Large FoV of 8 degrees Small plate scale -> small photon sensors Camera layout About 12000 pixel Grouped in modules of 64 pixel Effective Mirror Area per Tel. Nepomuk Otte ~100 m 2 Field of View (FoV) 8 deg. Pixelation ~0.05 deg. Angular Resolution 0.02 – 0.05 deg. 3
Page 1: Nuisances of SiPMs and how to deal
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 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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