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Updating the PATH framework with FRB host galaxy models

astro-ph.HE · 2026-06-09 · conditional · novelty 4.0

PATH is extended with three fitted P(m_r|z) prior models combined with P(z|DM), raising host-association confidence for ASKAP FRBs while showing fainter-than-expected host magnitude distribution.

The Cosmic Ray Life Cycle in Galaxy Clusters

astro-ph.CO · 2026-06-24 · unverdicted · novelty 2.0

Review of cosmic ray production and radio emission in galaxy clusters with recommendations for SKA observations of magnetic fields and low-energy particles.

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