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Paper Citation Record · LEDGER

Zooming in on radio relics -- II. How relic morphology probes density fluctuations at the edge of galaxy clusters

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.

pith.paper-citation-record.v1
2604.06302 v1

Coverage vector

measured 6 of 6 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-05-10T19:02:39.395408Z

measured 8 of 8 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-06-26T07:50:38.631331Z

measured 1 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

6 of 6 outbound references displayed

  • verified exact1
  • verified fuzzy3
  • unresolved2
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

0
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

Observation d56abaf9-21b0-404f-8c8f-b968133b02b1 · outbound

This paper cites Anticipated Performance of the Square Kilometre Array -- Phase 1 (SKA1).

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

Resolution
verified exact
arxiv_id, observed 2026-05-10T23:35:49.711560Z

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.

source=pdf_text observed=2026-05-10T19:02:39.395408Z digest=sha256:585c1d29fa88790198adc14fa991b900b402f0f295d505fa0d33a6b828e7fbfd

Observation 62f1822e-1a47-4d2d-8b49-bb47adf51e1c · outbound

This paper cites At the edge of the main relic, there is a region of low-brightness (≈15μJy beam−1) emission, which bridges some of the gap.

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

Resolution
verified fuzzy
raw_fallback, observed 2026-05-16T09:22:41.279632Z

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.

source=pdf_text observed=2026-05-10T19:02:39.395408Z digest=sha256:6e86953cf04f84fc7bff054ba3e4748342949db020345287765441eb5cdcb6f0

Observation d4cacee5-5403-4e33-9aa3-53d22363524c · outbound

This paper cites an unresolved cited work.

Zooming in on radio relics -- II. How relic morphology probes density fluctuations at the edge of galaxy clusters Unresolved cited work

Reference 3

Resolution
unresolved
raw_fallback, observed 2026-05-16T09:22:41.281619Z

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.

source=pdf_text observed=2026-05-10T19:02:39.395408Z digest=sha256:ec72409f2f34097dd4f441adc10fe2d91dc1e870b1664aa8a47da2aa1ed70691

Observation 865d8f4c-6d9a-44dd-9153-639d5b7be302 · outbound

This paper cites an unresolved cited work.

Zooming in on radio relics -- II. How relic morphology probes density fluctuations at the edge of galaxy clusters Unresolved cited work

Reference 4

Resolution
unresolved
raw_fallback, observed 2026-05-16T09:22:41.283503Z

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.

source=pdf_text observed=2026-05-10T19:02:39.395408Z digest=sha256:6f8134c63aa372a396605d2d83f9c74f213be30cec60f4b2c226b027ade918ce

Observation 5672aafe-9524-42c5-94a9-0feb3b7861a9 · outbound

This paper cites A major additional boost could be realised through Fermi-I re-acceleration.

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

Resolution
verified fuzzy
raw_fallback, observed 2026-05-16T09:22:41.286080Z

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.

source=pdf_text observed=2026-05-10T19:02:39.395408Z digest=sha256:ada72fb0362151c1750350b087441c3f15e61958e25157d00c2cd8aec0902c9c

Observation 3fac7751-5234-47cc-b469-1adff4176f21 · outbound

This paper cites 9, in particular).

Zooming in on radio relics -- II. How relic morphology probes density fluctuations at the edge of galaxy clusters 9, in particular)

Reference 6

Resolution
verified fuzzy
raw_fallback, observed 2026-05-16T09:22:41.288213Z

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.

source=pdf_text observed=2026-05-10T19:02:39.395408Z digest=sha256:ce9a4eee18a7bbaca565cc290edd5fafca354072b3590a98eec3af6682ce02d2

Pith citing papers

Observation ad150a87-ffa7-4abf-8064-603fb2d002e6 · inbound

Revisiting radio synchrotron diagnostics in star-forming galaxies cites this paper.

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

Resolution
verified exact
local_arxiv, observed 2026-05-09T23:49:45.326606Z

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.

source=arxiv_source observed=2026-05-09T23:45:31.311222Z digest=sha256:a415b215857d90dc16047c82c1ac8e493feffdd3d6c09868cb7e2805abdb7f07

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 cites this paper.

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

Resolution
verified exact
local_arxiv, observed 2026-06-26T09:09:16.694478Z

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.

source=arxiv_source observed=2026-06-26T07:50:38.631331Z digest=sha256:3ace668810e844970cae1e997ad2f22046b6657e6a2a91d6862e7fe4a5ff81ad