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Published December 13, 2020 | Published
Book Section - Chapter Open

Panoramic SETI: overall focal plane electronics and timing and network protocols

Abstract

The PANOSETI experiment is an all-sky, all-the-time visible search for nanosecond to millisecond time-scale transients. The experiment will deploy observatory domes at several sites, each dome containing ~45 telescopes and covering ~4,440 square degrees. Here we describe the focal-plane electronics for the visible wavelength telescopes, each of which contains a Mother Board and four Quadrant Boards. On each quadrant board, 256 silicon photomultiplier (SiPM) photon detectors are arranged to measure pulse heights to search for nanosecond time-scale pulses. To simultaneously examine pulse widths over a large range of time scales (nanoseconds to milliseconds), the instrument implements both a Continuous Imaging Mode (CI-Mode) and a Pulse Height Mode (PH-Mode). Precise timing is implemented in the gateware with the White Rabbit protocol.

Additional Information

© 2020 Society of Photo-Optical Instrumentation Engineers (SPIE). The PANOSETI research and instrumentation program is made possible by the enthusiastic support and interest of Franklin Antonio. We thank the Bloomfield Family Foundation for supporting SETI research at UC San Diego in the CASS Optical and Infrared Laboratory. Harvard SETI was supported by The Bosack/Kruger Charitable Foundation and The Planetary Society. UC Berkeley's SETI efforts involved with PANOSETI are supported by NSF grant 1407804, the Breakthrough Prize Foundation, and the Marilyn and Watson Alberts SETI Chair fund. We would like to thank the staff at Mt. Laguna and Lick Observatory for their help with equipment testing. The following vendors have been most gracious with their answers to our frequent technical questions: Hamamatsu, Weeroc, CAEN Technologies, and Amplification Technologies.

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Published - SPIE-AS20-508d3c72-1005-ea11-813d-005056be4d05.pdf

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