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Title resolution pending

3 Pith papers cite this work. Polarity classification is still indexing.

3 Pith papers citing it

years

2026 3

representative citing papers

The LOFAR sub-arcsecond view of the high-redshift radio relic in PSZ2G091.83+26.11

astro-ph.CO · 2026-02-26 · accept · novelty 7.0

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.

A high-resolution study of the double radio relic system in MACS J1752.0+4440

astro-ph.HE · 2026-04-02 · unverdicted · novelty 6.0

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.

citing papers explorer

Showing 3 of 3 citing papers.

  • The LOFAR sub-arcsecond view of the high-redshift radio relic in PSZ2G091.83+26.11 astro-ph.CO · 2026-02-26 · accept · none · ref 50

    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.

  • A high-resolution study of the double radio relic system in MACS J1752.0+4440 astro-ph.HE · 2026-04-02 · unverdicted · none · ref 44

    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.

  • Single- and double-headed odd radio circles in the LOFAR surveys astro-ph.GA · 2026-02-20 · unverdicted · none · ref 35

    The LOFAR DR3 survey yields 18 odd radio circles, confirming their rarity, heterogeneity, association with large ellipticals, and a relation where smaller ORCs avoid steep spectra.