Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-05-10T19:02:39.395408Z
Paper Citation Record · LEDGER
As of 10 August 2026, this Paper Citation Record lists 6 of 6 outbound references and 2 inbound Pith citation observations for arXiv:2604.06302.
A citation records a reference. It does not transfer a finding from one paper to another.
Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-05-10T19:02:39.395408Z
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-06-26T07:50:38.631331Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-05T02:28:24.338817Z
6 of 6 outbound references displayed
External citation measurements
0
pith, observed 2026-08-05T02:28:24.338817Z
Observation d56abaf9-21b0-404f-8c8f-b968133b02b1 · outbound
Zooming in on radio relics -- II. How relic morphology probes density fluctuations at the edge of galaxy clusters Anticipated Performance of the Square Kilometre Array -- Phase 1 (SKA1)
Reference 1
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 62f1822e-1a47-4d2d-8b49-bb47adf51e1c · outbound
Zooming in on radio relics -- II. How relic morphology probes density fluctuations at the edge of galaxy clusters At the edge of the main relic, there is a region of low-brightness (≈15μJy beam−1) emission, which bridges some of the gap
Reference 2
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation d4cacee5-5403-4e33-9aa3-53d22363524c · outbound
Zooming in on radio relics -- II. How relic morphology probes density fluctuations at the edge of galaxy clusters Unresolved cited work
Reference 3
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 865d8f4c-6d9a-44dd-9153-639d5b7be302 · outbound
Zooming in on radio relics -- II. How relic morphology probes density fluctuations at the edge of galaxy clusters Unresolved cited work
Reference 4
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 5672aafe-9524-42c5-94a9-0feb3b7861a9 · outbound
Zooming in on radio relics -- II. How relic morphology probes density fluctuations at the edge of galaxy clusters A major additional boost could be realised through Fermi-I re-acceleration
Reference 5
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 3fac7751-5234-47cc-b469-1adff4176f21 · outbound
Zooming in on radio relics -- II. How relic morphology probes density fluctuations at the edge of galaxy clusters 9, in particular)
Reference 6
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation ad150a87-ffa7-4abf-8064-603fb2d002e6 · inbound
Revisiting radio synchrotron diagnostics in star-forming galaxies Zooming in on radio relics -- II. How relic morphology probes density fluctuations at the edge of galaxy clusters
Reference 4
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 16ba9ca5-c1e6-4cec-9f1f-4420dddc6a0d · inbound
The PICO-Cluster Project: presenting the galaxy cluster sample and studying magnetic field growth, Faraday rotation and Braginskii heating Zooming in on radio relics -- II. How relic morphology probes density fluctuations at the edge of galaxy clusters
Reference 239
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.