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Paper Citation Record · LEDGER

Accurate black hole evolutions by fourth-order numerical relativity

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:gr-qc/0505055.

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

pith.paper-citation-record.v1
gr-qc/0505055 v2

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 2026-08-22T06:32:14.747728+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T05:57:54.360797Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-05-19T02:51:59.881647Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
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  • 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 10264178-90cb-493e-81cf-f801e852b006 · inbound

AthenaK simulations of the binary black hole merger GW150914 cites this paper.

AthenaK simulations of the binary black hole merger GW150914 Accurate black hole evolutions by fourth-order numerical relativity

Reference 81

Resolution
unresolved
no resolver link, observed 2026-08-07T05:57:54.360797Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T05:57:54.360797Z digest=sha256:2707e8c78f56342b7c0cd3f97bbde03595b433f37011d4d6a34cffcc9b3c8087

Observation f3a93fea-b61b-415b-a72c-67f08bff0486 · inbound

Parameter Estimation with Targeted Eccentric Numerical-Relativity Simulations for GW200208_22 and GW190620 cites this paper.

Parameter Estimation with Targeted Eccentric Numerical-Relativity Simulations for GW200208_22 and GW190620 Accurate black hole evolutions by fourth-order numerical relativity

Reference 62

Resolution
verified exact
local_arxiv, observed 2026-05-19T02:51:59.883893Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=pdf_text observed=2026-05-19T02:51:11.710911Z digest=sha256:18a14133cf1dc8f4d8bb4e57b3f89ca28f5f87088ca9b48222995db278b7e582