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NELIOTA (NEO Lunar Impacts and Optical TrAnsients) is an ESA-funded lunarmonitoring project, which aims to determine the size-frequency distribution ofsmall Near-Earth Objects (NEOs) via detection of impact flashes on the surfaceof the Moon. A prime focus, high-speed, twin-camera system providingsimultaneous observations in two photometric bands at a rate of 30frames-per-second on the 1.2 m Kryoneri telescope of the National Observatoryof Athens was commissioned for this purpose. A dedicated software processes theimages and automatically detects candidate lunar impact flashes, which are thenvalidated by an expert user. The four year observing campaign began in February2017 and has so far detected more than 40 lunar impact events. The softwareroutinely detects satellites, which typically appear as streaks or dotscrossing the lunar disk. To avoid confusing these events with real flashes, wecheck different available catalogs with spacecraft orbital information andexclude spacecraft identifications.

NELIOTA Lunar Impact Flash Detection and Event Validation