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Paper Citation Record · LEDGER

The last orbit of binary black holes

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:gr-qc/0601091.

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

pith.paper-citation-record.v1
gr-qc/0601091 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 2026-08-19T06:32:44.657259+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T13:07:16.921795Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-08T17:55:20.609674Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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  • malformed identifier0
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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 235218af-b725-48ce-8cfa-4ecccec9b1ad · inbound

Gravitational waves in massive gravity: Waveforms generated by a particle plunging into a black hole and the excitation of quasinormal modes and quasibound states cites this paper.

Gravitational waves in massive gravity: Waveforms generated by a particle plunging into a black hole and the excitation of quasinormal modes and quasibound states The last orbit of binary black holes

Reference 33

Resolution
unresolved
no resolver link, observed 2026-08-12T13:07:16.921795Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-12T13:07:16.921795Z digest=sha256:43bccd47d3c82fc1d7737b8ae63f3c4774e0a93efcf2a307e01e805c84632cd0

Observation 2f91e38d-a17e-4571-b1f7-6e76af75faa4 · inbound

A Possible Triple Formation Scenario of Binary Black Hole Merge With One In Pair-instability Supernova Mass Gap cites this paper.

A Possible Triple Formation Scenario of Binary Black Hole Merge With One In Pair-instability Supernova Mass Gap The last orbit of binary black holes

Reference 91

Resolution
verified exact
local_arxiv, observed 2026-07-08T17:55:20.610975Z

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=2026-07-08T17:53:06.845093Z digest=sha256:c20826f040f2396342a156f271b5a01a02d3a83e802f7bb13ed0bb26f47a8d8c