This project aims to provide a low resolution and multiple-passband full-sky survey with an imaging cadence of a few
minutes. Based on our earlier tests, we found that a novel type of astronomical telescope mount on a hexapod platform can
provide the accuracy of sidereal tracking needed by our instrumentation. The fully configured Fly's Eye device contains 19
wide-field cameras equipped with fast focal ratio optics which are arranged in a mosaic form and have an effective
resolution of 20 arcseconds per pixel. The scientific goal of this project is to continuously monitor stellar brightness
variations in the full Sloan photometric system down to the magnitude of r=15 or the limit of apparent stellar confusion.
The data acquisition will then cover roughly 6 magnitudes of the time domain, from the scales of minutes up to the several
years of planned operations. Fly's Eye data yield is complementary to that of the Large Synoptic Survey Telescope since the
saturation magnitude of LSST is close to the faint limit of the Fly's Eye setup.
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