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Paper Citation Record · LEDGER

Scaling up global kinetic models of pulsar magnetospheres using a hybrid force-free-PIC numerical approach

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2406.14512.

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

pith.paper-citation-record.v1
2406.14512 v1

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 2026-08-19T06:32:44.657259+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T21:58:28.456187Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-10T05:30:23.456663Z

Reference resolution

0 of 0 outbound references displayed

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

External citation measurements

1
pith, observed 2026-08-10T05:30:23.456663Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 4b6e0292-39dc-4695-acb2-6c2567f22ecf · inbound

Modelling the multi-wavelength emission and polarisation signatures of the novel white-dwarf pulsar system AR Sco cites this paper.

Modelling the multi-wavelength emission and polarisation signatures of the novel white-dwarf pulsar system AR Sco Scaling up global kinetic models of pulsar magnetospheres using a hybrid force-free-PIC numerical approach

Reference 66

Resolution
unresolved
no resolver link, observed 2026-08-15T21:58:28.456187Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-15T21:58:28.456187Z digest=sha256:8c5c4157852180f507c4770147d917adca001efe4868e4d91ef5249cfa8b5b87

Observation 535c99b4-ef5f-4c54-81e3-ef9c2ab66f1a · inbound

Towards Modelling AR Sco: Calibration -- Reproducing High-Energy Pulsar Emission and Testing Convergence to Aristotelian Electrodynamics cites this paper.

Towards Modelling AR Sco: Calibration -- Reproducing High-Energy Pulsar Emission and Testing Convergence to Aristotelian Electrodynamics Scaling up global kinetic models of pulsar magnetospheres using a hybrid force-free-PIC numerical approach

Reference 51

Resolution
unresolved
no resolver link, observed 2026-08-07T04:31:50.330621Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T04:31:50.330621Z digest=sha256:ec06fd1bf0aef63b8b25dd814b941f4c8c7ae46e31f0c44b2196421c08ad4cff

Observation 8087e423-7a12-492e-bcf8-5257c93991d2 · 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 Scaling up global kinetic models of pulsar magnetospheres using a hybrid force-free-PIC numerical approach

Reference 54

Resolution
verified exact
local_arxiv, observed 2026-08-05T16:38:04.448047Z

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.

source=pdf_text observed=2026-08-05T16:38:03.412214Z digest=sha256:1c3d75747a121cc2a6d6569a3d13109e3df350851a0bfc1e1c95c60230364f76