Proposes applying sLDFC to the Roman Coronagraph to maintain darker, more stable dark holes and use bright-field signals to boost exoplanet detection limits.
The Direct Detectability of Giant Exoplanets in the Optical
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Demonstrating Improved Contrast on the Roman Coronagraph with Spatial Linear Dark Field Control
Proposes applying sLDFC to the Roman Coronagraph to maintain darker, more stable dark holes and use bright-field signals to boost exoplanet detection limits.