Avalanche diodes as photon-counting detectors in astronomical photometry

Dainis Dravins; Daniel Faria; Bo Nilsson

doi:10.1117/12.395485

16 August 2000 Avalanche diodes as photon-counting detectors in astronomical photometry

Dainis Dravins, Daniel Faria, Bo Nilsson

Proceedings Volume 4008, Optical and IR Telescope Instrumentation and Detectors; (2000) https://doi.org/10.1117/12.395485
Event: Astronomical Telescopes and Instrumentation, 2000, Munich, Germany

Abstract

Photon-counting silicon avalanche photo-diodes (APDs) offer very high quantum efficiency, and might eventually replace photocathode detectors in high-speed photometry of astronomical objects. Laboratory studies have been performed on both passively and actively quenched APDs. Peculiarities of APDs include that the dark signal may exhibit bistability, with the count rate jumping between discrete levels. Following any photon detection, the detector itself emits some light, which might be confusing under certain conditions. Deadtimes and after pulsing properties appear favorable, but the small physical size of APDs causes challenges in optically matching them to the entrance pupils of large telescopes.

Citation Download Citation

Dainis Dravins, Daniel Faria, and Bo Nilsson "Avalanche diodes as photon-counting detectors in astronomical photometry", Proc. SPIE 4008, Optical and IR Telescope Instrumentation and Detectors, (16 August 2000); https://doi.org/10.1117/12.395485

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