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Paper Citation Record · LEDGER

A Numerical Method for General Relativistic Magnetohydrodynamics

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:astro-ph/0210518.

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

pith.paper-citation-record.v1
astro-ph/0210518 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 2026-08-14T06:32:32.682623+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T03:10:33.599966Z

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

179
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation fd4eda2b-7621-4b78-9bbb-1c593c8b0542 · inbound

Relative Magnification Factor of Point Sources on Accretion Disks cites this paper.

Relative Magnification Factor of Point Sources on Accretion Disks A Numerical Method for General Relativistic Magnetohydrodynamics

Reference 72

Resolution
verified exact
arxiv_id, observed 2026-05-11T06:46:44.047375Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-05-10T17:27:08.924918Z digest=sha256:5cec85a5b6f6dee71f720b76718f4e013df4375086b93c9c3673a26ee724f3de

Observation 3b8db4bb-fd01-46f4-9185-2eb2b25da4c5 · inbound

Simulation-Based Prediction of Black Hole Fe K$\alpha$ Line Profiles cites this paper.

Simulation-Based Prediction of Black Hole Fe K$\alpha$ Line Profiles A Numerical Method for General Relativistic Magnetohydrodynamics

Reference 95

Resolution
verified exact
local_arxiv, observed 2026-05-21T01:29:21.965351Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:5d3c267a40c56abcd0805dadc7972f421af0cefa8238dbb1021fa483c4006198

Observation 1a91520b-c543-445b-af37-0ffaadc5c3c1 · inbound

Dark matter environments and safeguards for spacetime inference from horizon scale interferometry cites this paper.

Dark matter environments and safeguards for spacetime inference from horizon scale interferometry A Numerical Method for General Relativistic Magnetohydrodynamics

Reference 46

Resolution
unresolved
no resolver link, observed 2026-08-02T03:10:33.599966Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T03:10:33.599966Z digest=sha256:4a29a4f294475e89b2217846b9ced348ce70e6d569e7b48e30fe70061f59a3ee