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Open access Nov 2026

Imaging exoplanets below the telescope stability limit

Exoplanet imaging is the main method for detailed characterization of planets orbiting beyond 1 au (ref. 1) but it requires suppressing the bright glare of the star to see the faint planet light. As well as sophisticated instrumentation2,3, effective image processing is necessary for starlight suppression, which contin...

Rodrigo Ferrer-Chávez, Jason J. Wang, K. Bouman et al. · 0 citations
Open access Aug 2026

Video reconstruction of variable VLBI observations with neural fields

Supermassive black hole accretion and the ejection of collimated, relativistic jets of plasma are intrinsically dynamic processes shaped by large-scale magnetic fields1, 2, 3–4. Various algorithms have been developed to image these objects at different scales using radio interferometric observations5, 6, 7–8. However,...

M. Foschi, Brandon Zhao, A. Fuentes et al. · 1 citation

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