Paper Citation Record · LEDGER

Simulation of astrophysical jet using the special relativistic hydrodynamics code

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:gr-qc/0602053.

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

pith.paper-citation-record.v1
gr-qc/0602053 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-03T03:12:37.454695Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-03T18:38:49.379846Z

Reference resolution

0 of 0 outbound references displayed

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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 f995f620-fd18-4c75-a17b-ceeae1de08bf · inbound

Dynamics, Ringdown, and Accretion-Driven Multiple Quasi-Periodic Oscillations of Kerr-Bertotti-Robinson Black Holes cites this paper.

Dynamics, Ringdown, and Accretion-Driven Multiple Quasi-Periodic Oscillations of Kerr-Bertotti-Robinson Black Holes Simulation of astrophysical jet using the special relativistic hydrodynamics code

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-03T03:12:37.454695Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fc0b91b7-0a0b-4a8a-a5f0-cffc561588b8 · inbound

Disformal Kerr Imprints on BHL Accretion: Shock Morphology, PSD Signatures, and Observational QPO Counterparts cites this paper.

Disformal Kerr Imprints on BHL Accretion: Shock Morphology, PSD Signatures, and Observational QPO Counterparts Simulation of astrophysical jet using the special relativistic hydrodynamics code

Reference 56

Resolution: verified exact; local_arxiv, observed 2026-05-20T17:28:48.071986Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation fa37770c-7b28-4ce7-a45e-7044d7092d12 · inbound

Disformal Kerr Imprints on BHL Accretion: Shock Morphology, PSD Signatures, and Observational QPO Counterparts cites this paper.

Disformal Kerr Imprints on BHL Accretion: Shock Morphology, PSD Signatures, and Observational QPO Counterparts Simulation of astrophysical jet using the special relativistic hydrodynamics code

Reference 56

Resolution: verified exact; local_arxiv, observed 2026-06-30T19:55:01.768367Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 0102f059-739a-471d-a456-e4d0fa5fbf47 · inbound

QPO-like Signatures and Hydrodynamical Variability in Accretion around a JNW-type Compact Spacetime in Freund-Nambu Scalar-Tensor Gravity cites this paper.

QPO-like Signatures and Hydrodynamical Variability in Accretion around a JNW-type Compact Spacetime in Freund-Nambu Scalar-Tensor Gravity Simulation of astrophysical jet using the special relativistic hydrodynamics code

Reference 48

Resolution: verified exact; local_arxiv, observed 2026-07-03T18:38:49.381129Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.