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Paper Citation Record · LEDGER

Full-3D relativistic MHD simulations of Bow Shock Pulsar Wind Nebulae: dynamics

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1902.00442.

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

pith.paper-citation-record.v1
1902.00442 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 2026-08-15T06:32:42.880941+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T12:17:55.995277Z

measured 0 of 1 external citation measurements

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

Source: cited_works

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 14175c6b-c112-4ca6-8737-35629ab6d4b7 · inbound

Magnetic fields in heavy ion collisions: flow and charge transport cites this paper.

Magnetic fields in heavy ion collisions: flow and charge transport Full-3D relativistic MHD simulations of Bow Shock Pulsar Wind Nebulae: dynamics

Reference 13

Resolution
unresolved
no resolver link, observed 2026-08-14T12:17:55.995277Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T12:17:55.995277Z digest=sha256:ec32fdd3ae5385675ca8ea50e1acbdf4cb36b038248357950a8d043b9593cb0c

Observation 1df79978-5045-4c7e-a96b-516921d85633 · inbound

Self-confinement of relativistic pair beams in magnetized interstellar plasmas: the case of pulsar X-ray filaments cites this paper.

Self-confinement of relativistic pair beams in magnetized interstellar plasmas: the case of pulsar X-ray filaments Full-3D relativistic MHD simulations of Bow Shock Pulsar Wind Nebulae: dynamics

Reference 21

Resolution
unresolved
no resolver link, observed 2026-08-03T15:48:49.761468Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T15:48:49.761468Z digest=sha256:ed296f97b4062ed09e0ca3f73226dc8585bdc886880f54e4640d72c7b565748a