Pith. sign in

Paper Citation Record · LEDGER

Utilizing cosmic-ray positron and electron observations to probe the averaged properties of Milky Way pulsars

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2111.05864.

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

pith.paper-citation-record.v1
2111.05864 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 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 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T19:15:10.776130Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-10T21:10:14.044495Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

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 0adf0aec-b5ea-4d50-ba6b-715d8f06f065 · inbound

SECRET: Stochasticity Emulator for Cosmic Ray Electrons cites this paper.

SECRET: Stochasticity Emulator for Cosmic Ray Electrons Utilizing cosmic-ray positron and electron observations to probe the averaged properties of Milky Way pulsars

Reference 37

Resolution
verified exact
local_arxiv, observed 2026-08-10T21:10:14.048894Z

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=2026-08-10T21:10:13.775531Z digest=sha256:018626ed1ec137c573c1f08c36c133bb5f08a4e54f4a5962c6af9af47692ef86

Observation 5813c0f2-91b3-4f9d-8e7f-9faa84c6ba73 · 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 Utilizing cosmic-ray positron and electron observations to probe the averaged properties of Milky Way pulsars

Reference 40

Resolution
unresolved
no resolver link, observed 2026-08-11T19:15:10.776130Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T19:15:10.776130Z digest=sha256:4059edba941c76028cb43b4355e62ef5eb7056ce25f9d5e80a338a23d9704019