A Radio U-Net pipeline produces pixel-level segmentation maps and probability scores for diffuse radio emission in 3822 galaxy clusters from LoTSS-DR3, yielding a high-confidence sample of 357 and confirming trends with mass and redshift.
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CTAO simulations show it can constrain IGMF strengths up to 10^{-15} G for GRB-like sources, with LST-1 observations of GRB 221009A favoring 3×10^{-17} G.
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Galaxy clusters in the LoTSS-DR3: Catalogues and detection pipeline for diffuse radio emission
A Radio U-Net pipeline produces pixel-level segmentation maps and probability scores for diffuse radio emission in 3822 galaxy clusters from LoTSS-DR3, yielding a high-confidence sample of 357 and confirming trends with mass and redshift.
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Intergalactic Magnetic Field constraints from detected very high-energy Gamma-Ray Bursts using the Cherenkov Telescope Array Observatory
CTAO simulations show it can constrain IGMF strengths up to 10^{-15} G for GRB-like sources, with LST-1 observations of GRB 221009A favoring 3×10^{-17} G.