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Purpose
Investigations of critical problems in both atmospheric science and astronomy are limited by the most basic problem of optical calibration: the precision of measurements of the brightness of the light sources. Is it possible to greatly improve precision of measurements of the magnitude of stars supernovae, and other astronomical sources, so that we can understand and calibrate measurements of the accelerating expansion of the Universe, measure various properties of Earth's atmosphere better, and furthermore create a new type of miniature stratospheric hub for telecommunication?
University of Victoria|Université de Victoria × Unknown
23 grants totalling $4.3M
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