A morphology-plus-color pipeline decomposes and removes Galactic cirrus from deep wide-field images, improving low surface brightness galaxy detection and yielding optical DGL measurements.
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Fuzzy Galaxies or Cirrus? Decomposition of Galactic Cirrus in Deep Wide-Field Images
A morphology-plus-color pipeline decomposes and removes Galactic cirrus from deep wide-field images, improving low surface brightness galaxy detection and yielding optical DGL measurements.