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This document summarizes the results of a feasibility study conducted at the Astronomical Observatory of the Autonomous Region of Aosta Valley. The study demonstrated that the observatory is well-suited for detecting small, transiting exoplanets around nearby M dwarf stars. Researchers monitored three known transiting planet systems with a 25 cm telescope from May to August 2009, achieving photometric precision below 0.003 magnitudes for stars brighter than magnitude 13. They also outline plans to set up a

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