Paper Citation Record · LEDGER

Self-Generated Cosmic-Ray Turbulence Can Explain the Morphology of TeV Halos

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2111.01143.

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

pith.paper-citation-record.v1
2111.01143 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-19T06:32:44.657259+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T04:55:36.415525Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-24T06:49:01.965165Z

Reference resolution

0 of 0 outbound references displayed

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verified fuzzy0
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External citation measurements

No source-named external measurement is stored.

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 43cd75bd-ca18-427f-a792-d7227a302a1a · inbound

Constraining the slow-diffusion zone size and electron injection spectral index for the Geminga pulsar halo cites this paper.

Constraining the slow-diffusion zone size and electron injection spectral index for the Geminga pulsar halo Self-Generated Cosmic-Ray Turbulence Can Explain the Morphology of TeV Halos

Reference 27

Resolution: verified exact; arxiv_id, observed 2026-05-24T06:49:01.967493Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation d51190c1-f810-4073-9d48-a6890c8835e5 · inbound

Extended TeV Halos May Commonly Exist around Middle-Aged Pulsars cites this paper.

Extended TeV Halos May Commonly Exist around Middle-Aged Pulsars Self-Generated Cosmic-Ray Turbulence Can Explain the Morphology of TeV Halos

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-16T04:54:30.195910Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 65833b43-c3dd-4227-8b08-50651d22f2a7 · inbound

Absence of TeV halos around millisecond pulsars cites this paper.

Absence of TeV halos around millisecond pulsars Self-Generated Cosmic-Ray Turbulence Can Explain the Morphology of TeV Halos

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-16T04:55:36.415525Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 17266c2f-4eea-4676-b81a-654cfa87d5d3 · inbound

PHECT: A lightweight computation tool for pulsar halo emission cites this paper.

PHECT: A lightweight computation tool for pulsar halo emission Self-Generated Cosmic-Ray Turbulence Can Explain the Morphology of TeV Halos

Reference 34

Resolution: verified exact; arxiv_id, observed 2026-05-18T23:02:52.445060Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.