Online blind deconvolution for astronomical imaging

Atmospheric turbulences blur astronomical images taken by earth-based telescopes. Taking many short-time exposures in such a situation provides noisy images of the same object, where each noisy image has a different blur. Commonly astronomers apply a technique called "Luck Imaging" that selects a few of the recorded frames that ful-fill certain criteria, such as reaching a certain peak intensity ("Strehl ratio"). The selected frames are then averaged to obtain a better image. In this paper we introduce and analyze a new method that exploits all the frames and generates an improved image in an online fashion. Our initial experiments with controlled artificial data and real-world astronomical datasets yields promising results.