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.
E., Pacaud, F., Reiprich, T
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Stacking analysis yields L-M slope 1.56, slightly steeper than self-similar, with X-ray detected clusters showing more centrally concentrated profiles than undetected ones.
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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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The eROSITA Final Equatorial-Depth Survey (eFEDS): X-ray stacking analysis of Subaru's optically selected clusters spanning low richness regime
Stacking analysis yields L-M slope 1.56, slightly steeper than self-similar, with X-ray detected clusters showing more centrally concentrated profiles than undetected ones.