Paper Citation Record · LEDGER

Coma cluster $\gamma$-ray and radio emission is consistent with a secondary electron origin for the radio halo

As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2404.13111.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2404.13111 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-20T06:33:59.587034+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T21:06:46.241239Z

measured 1 of 1 external citation measurements

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

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

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
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External citation measurements

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

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 93781f9d-7b79-42d6-a103-751643ce6a17 · inbound

Relativistic ions with power-law spectra explain radio phoenixes cites this paper.

Relativistic ions with power-law spectra explain radio phoenixes Coma cluster $\gamma$-ray and radio emission is consistent with a secondary electron origin for the radio halo

Reference 15

Resolution: verified exact; arxiv_id, observed 2026-05-23T00:15:14.550577Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation bba6b6cc-4803-4cc6-a4dd-d29247aff790 · inbound

Primordial Black Holes as Coma Cluster Dark Matter and the Unresolved {\gamma}-Ray Background cites this paper.

Primordial Black Holes as Coma Cluster Dark Matter and the Unresolved {\gamma}-Ray Background Coma cluster $\gamma$-ray and radio emission is consistent with a secondary electron origin for the radio halo

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-06T21:06:46.241239Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0202baef-801b-4dc0-a5f7-182b78571b95 · inbound

High-energy Multi-messenger Emission from Galaxy Clusters in the Local Universe cites this paper.

High-energy Multi-messenger Emission from Galaxy Clusters in the Local Universe Coma cluster $\gamma$-ray and radio emission is consistent with a secondary electron origin for the radio halo

Reference 56

Resolution: verified exact; arxiv_id, observed 2026-05-13T05:07:17.566526Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 36c06bb5-c9be-42fe-968a-cd5f87a5cf9f · inbound

Galaxy-cluster-stacked Fermi-LAT, part IV: $\sim70$ GeV WIMP annihilation lines cites this paper.

Galaxy-cluster-stacked Fermi-LAT, part IV: $\sim70$ GeV WIMP annihilation lines Coma cluster $\gamma$-ray and radio emission is consistent with a secondary electron origin for the radio halo

Reference 98

Resolution: verified exact; arxiv_id, observed 2026-07-03T18:08:46.724622Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation c06b7cac-26c8-42c8-b366-1e1b0709786e · inbound

Galaxy-cluster-stacked Fermi-LAT, part IV: $\sim70$ GeV WIMP annihilation lines cites this paper.

Galaxy-cluster-stacked Fermi-LAT, part IV: $\sim70$ GeV WIMP annihilation lines Coma cluster $\gamma$-ray and radio emission is consistent with a secondary electron origin for the radio halo

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-04T04:46:36.731390Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a19a6ffe-80a4-4f3b-826f-585415bee493 · inbound

CRESCENDO II: Spectral cosmic rays with improved energy losses and realistic supernova seeding cites this paper.

CRESCENDO II: Spectral cosmic rays with improved energy losses and realistic supernova seeding Coma cluster $\gamma$-ray and radio emission is consistent with a secondary electron origin for the radio halo

Reference 196

Resolution: unresolved; no resolver link, observed 2026-08-02T02:26:53.168581Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.