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.
T., Jagannathan, P., Mooley, K
5 Pith papers cite this work. Polarity classification is still indexing.
5
Pith papers citing it
representative citing papers
XRISM Resolve measures the lowest turbulent velocity yet in a cluster core, indicating Abell 496 is dynamically quiescent despite prior cold fronts and weak radio activity.
Symmetric kiloparsec-scale radio knots in NGC 7213 indicate a confined weak jet and recurrent nuclear activity in this low-luminosity AGN.
High-resolution radio imaging shows TGSSJ1530+1049 as a ~5.5 kpc medium-sized symmetric object whose lobes align with but do not reach the full extent of the ionized gas seen by JWST in a dense z=4 environment.
RACS re-characterization confirms 66 compact sources and 18 very steep-spectrum sources among 171 TGSS candidates previously missed or misclassified in NVSS.
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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The Quiescent Sloshing Core of Abell 496 with XRISM
XRISM Resolve measures the lowest turbulent velocity yet in a cluster core, indicating Abell 496 is dynamically quiescent despite prior cold fronts and weak radio activity.
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Symmetric kiloparsec-scale radio knots in NGC 7213: evidence for a confined weak jet and recurrent nuclear activity
Symmetric kiloparsec-scale radio knots in NGC 7213 indicate a confined weak jet and recurrent nuclear activity in this low-luminosity AGN.
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High-resolution radio imaging of TGSSJ1530+1049, a radio galaxy in a dense environment at z=4
High-resolution radio imaging shows TGSSJ1530+1049 as a ~5.5 kpc medium-sized symmetric object whose lobes align with but do not reach the full extent of the ionized gas seen by JWST in a dense z=4 environment.
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From NVSS to RACS: Identifying truly Compact and Steep spectrum Radio sources
RACS re-characterization confirms 66 compact sources and 18 very steep-spectrum sources among 171 TGSS candidates previously missed or misclassified in NVSS.