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

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