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The Panoramic SETI (Search for Extraterrestrial Intelligence) experiment(PANOSETI) aims to detect and quantify optical transients from nanosecond tosecond precision over a large field-of-view ($\sim$4,450 square-degrees). Tomeet these challenging timing and wide-field requirements, the PANOSETIexperiment will use two assemblies of $\sim$45 telescopes to reject spurioussignals by coincidence detection, each one comprising custom-made fastphoton-counting hardware combined with ($f/1.32$) focusing optics. Preliminaryon-sky results from pairs of PANOSETI prototype telescopes (100 sq.deg.) arepresented in terms of instrument performance and false alarm rates. We foundthat a separation of $>$1 km between telescopes surveying the samefield-of-view significantly reduces the number of false positives due to nearbysources (e.g., Cherenkov showers) in comparison to a side-by-side configurationof telescopes. Design considerations on the all-sky PANOSETI instrument andexpected field-of-views are reported.

Panoramic SETI: on-sky results from prototype telescopes and instrumental design