A grid of 434 Faraday rotation measures from MeerKAT polarimetry reveals enhanced RM scatter in the Abell 3391/95 clusters and suggests a relatively ordered magnetic field in the intercluster bridge on ~10 kpc scales.
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Fornax cluster magnetic field follows a power-law spectrum of slope ~2.7 with central strength ~5 μG scaling as n^1.6, consistent with recent central re-amplification and trends across 17 clusters.
Filament stacking outperforms pair stacking for HI detection in cosmic filaments, reaching column densities of 10^16-10^17 cm^-2 post-masking in simulations while pair stacking is heavily suppressed.
citing papers explorer
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Magnetic properties of the Abell 3391-3395 system revealed using wide-field MeerKAT polarimetry
A grid of 434 Faraday rotation measures from MeerKAT polarimetry reveals enhanced RM scatter in the Abell 3391/95 clusters and suggests a relatively ordered magnetic field in the intercluster bridge on ~10 kpc scales.
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The MeerKAT Fornax Survey VII. Characterisation of the Fornax cluster's magnetic field and new insights on magnetisation in large scale systems
Fornax cluster magnetic field follows a power-law spectrum of slope ~2.7 with central strength ~5 μG scaling as n^1.6, consistent with recent central re-amplification and trends across 17 clusters.
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Detection of HI filament: Pair Stacking vs. Filament Stacking
Filament stacking outperforms pair stacking for HI detection in cosmic filaments, reaching column densities of 10^16-10^17 cm^-2 post-masking in simulations while pair stacking is heavily suppressed.