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Paper Citation Record · LEDGER

Simulations of pulsar wind formation

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0201360.

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

pith.paper-citation-record.v1
astro-ph/0201360 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 2026-08-18T06:34:40.430872+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-05T16:38:03.591606Z

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

0 of 0 outbound references displayed

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

External citation measurements

3
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 1e839d57-4058-4029-8227-7e6e81698171 · inbound

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years cites this paper.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years Simulations of pulsar wind formation

Reference 56

Resolution
unresolved
no resolver link, observed 2026-08-05T16:38:03.591606Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-05T16:38:03.591606Z digest=sha256:a6e7a7effac114021c8c696754b7cf71c146fed4d755227f950a4f8daa633317

Observation ded9e4a6-eee6-4814-875a-b0bddc5389c5 · inbound

Diocotron Modes in Pulsar Magnetospheres: Charge Diffusion and Implications for Radio Emission Variability cites this paper.

Diocotron Modes in Pulsar Magnetospheres: Charge Diffusion and Implications for Radio Emission Variability Simulations of pulsar wind formation

Reference 43

Resolution
metadata mismatch
local_arxiv, observed 2026-06-28T08:51:48.408019Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-06-28T08:47:47.631802Z digest=sha256:7ec3a51c40e1e2dba0ea1328c116d8d5906d208f3400ce7e89b2baa237b6e136