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Spada: An Array of Spad Detectors For Astrophysical Applications
Authors:Giovanni Bonanno  Massimiliano Belluso  Franco Zappa  Simone Tisa  Sergio Cova  Piera Maccagnani  Domenico Bonaccini Calia  Roberto Saletti  Roberto Roncella  Sergio Billotta
Institution:(1) INAF; Catania Astrophysical Observatory, Catania, Italy;(2) Dept. of Electronics, Politecnico di Milano, Milano, Italy;(3) LAMEL, IMM-CNR, Bologna, Italy;(4) European Southern Observatory, Garching, Germany;(5) Dept. of Information Engineering, University of Pisa, Pisa, Italy
Abstract:Astrophysical studies require accurate, sensitive and fast detectors to detect faint sources with high variability. Recently an array of Single Photon Avalanche Diodes (SPAD), SPADA, has been developed. This array is suitable for competitive adaptive optics operations and fast transient image acquisition at a fraction of the current cost of imaging arrays. The fabricated solid-state photon counters are rugged, easily integrated with the optics, free from readout noise, and have very fast frame rates (> 10 kHz, for visible corrections) with nanosecond electronic gating. In this paper, the following are described: the development of silicon monolithic arrays of 60 photon-counters, the detection electronics (based on integrated active quenching circuits for each pixel of the array), the real-time data-processing board implemented into FPGA and some aspects of the mechanical housing.
Keywords:adaptive optics  fast transient phenomena  photon counter  photodetector array  single photon avalanche photodiode
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