SKA-VLBI can deliver high-sensitivity milliarcsecond imaging and polarimetry of faint blazars to constrain models of high-energy photon and neutrino emission in AGN jets.
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4 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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2026 4verdicts
UNVERDICTED 4representative citing papers
SKAMPI prototype achieves first S-band VLBI fringes with EVN, LBA, and VLBA while evaluating integration and imaging performance.
Reports 550 radio sources in one neutrino field and outlines a future SKA-Mid plus VLBI census strategy to find potential neutrino-emitting sources.
Outlines science opportunities for space VLBI using SKA-Mid as ground anchor to study AGN jets, high-redshift sources, interstellar scattering, and precise astrometry.
citing papers explorer
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VLBI with SKAMPI, the SKA-Mid MPIfR dish demonstrator
SKAMPI prototype achieves first S-band VLBI fringes with EVN, LBA, and VLBA while evaluating integration and imaging performance.