Sub-arcsecond LOFAR imaging at 145 MHz resolves the acceleration site and downstream structure of a high-redshift radio relic, confirming its diffuse nature, showing log-normal magnetic field profiles, and providing hints of redshift evolution in the radio power versus cluster mass correlation.
Title resolution pending
3 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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2026 3representative citing papers
High-resolution spectral analysis of the double radio relics reveals flat integrated indices around -0.9, positive curvature inconsistent with ageing models, and Mach numbers of ~3.1-3.2, suggesting multiple shocks or re-acceleration shape the NE relic.
FRIIs show lower cluster association rates than FRIs (30.6% vs 48.6% volume-limited; 32.6% vs 45.6% paired), with the gap widening at high luminosity, yet similar environments once inside clusters.
citing papers explorer
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The LOFAR sub-arcsecond view of the high-redshift radio relic in PSZ2G091.83+26.11
Sub-arcsecond LOFAR imaging at 145 MHz resolves the acceleration site and downstream structure of a high-redshift radio relic, confirming its diffuse nature, showing log-normal magnetic field profiles, and providing hints of redshift evolution in the radio power versus cluster mass correlation.
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A high-resolution study of the double radio relic system in MACS J1752.0+4440
High-resolution spectral analysis of the double radio relics reveals flat integrated indices around -0.9, positive curvature inconsistent with ageing models, and Mach numbers of ~3.1-3.2, suggesting multiple shocks or re-acceleration shape the NE relic.
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Probing the environments of FRI and FRII radio galaxies in LoTSS DR2 with galaxy clusters
FRIIs show lower cluster association rates than FRIs (30.6% vs 48.6% volume-limited; 32.6% vs 45.6% paired), with the gap widening at high luminosity, yet similar environments once inside clusters.