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Paper Citation Record · LEDGER

Pulsars Do Not Produce Sharp Features in the Cosmic-Ray Electron and Positron Spectra

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2206.04699.

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

pith.paper-citation-record.v1
2206.04699 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-12T06:34:41.77262+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T19:15:10.793108Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-23T00:02:17.567764Z

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 3cb8e9ce-cc33-4854-bc29-a7e918ff6d3c · inbound

Discrete treatment of inverse Compton scattering: implications on parameter estimation in gamma-ray astronomy cites this paper.

Discrete treatment of inverse Compton scattering: implications on parameter estimation in gamma-ray astronomy Pulsars Do Not Produce Sharp Features in the Cosmic-Ray Electron and Positron Spectra

Reference 2

Resolution
verified exact
arxiv_id, observed 2026-05-23T00:02:17.570207Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-05-22T23:59:06.367210Z digest=sha256:0c166b0692d66771659ec94b3ee8a98b236d07bb6fe64cd80b959fa5cec4547d

Observation 27f713a3-1c4f-42ec-9168-b79786c221dc · inbound

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

PHECT: A lightweight computation tool for pulsar halo emission Pulsars Do Not Produce Sharp Features in the Cosmic-Ray Electron and Positron Spectra

Reference 78

Resolution
verified exact
arxiv_id, observed 2026-05-18T23:02:52.559562Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-05-18T23:02:15.483780Z digest=sha256:6c23f1160efaa79a7b5331970e8ba972551f02fc8cff8362140b14fef91bc9a2

Observation 5d80cdce-1167-4544-a853-c138a5dad45f · inbound

Astrophysical origins of TeV features in the cosmic-ray lepton spectrum cites this paper.

Astrophysical origins of TeV features in the cosmic-ray lepton spectrum Pulsars Do Not Produce Sharp Features in the Cosmic-Ray Electron and Positron Spectra

Reference 46

Resolution
unresolved
no resolver link, observed 2026-08-11T19:15:10.793108Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T19:15:10.793108Z digest=sha256:6fafbbee427241f4e681265e321954d95c1f191a48c0d261e8e197f0be395551