Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Comparison of post-Newtonian mode amplitudes with numerical relativity simulations of binary black holes
As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1901.08516.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T22:32:29.165377Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-20T22:03:47.528881Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
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- parse uncertain0
- 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 1b33b3ca-b234-4ef4-862c-b305581a0ed9 · inbound
Persistence of post-Newtonian amplitude structure in binary black hole mergers cites this paper.
Persistence of post-Newtonian amplitude structure in binary black hole mergers Comparison of post-Newtonian mode amplitudes with numerical relativity simulations of binary black holes
Reference 25
- Resolution
- verified exact
- arxiv_id, observed 2026-05-18T20:12:50.386330Z
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.
Observation bef58dad-bf2a-41ae-83d1-da50874ff9b3 · inbound
Gravitational radiation from hyperbolic orbits: comparison between self-force, post-Minkowskian, post-Newtonian, and numerical relativity results cites this paper.
Gravitational radiation from hyperbolic orbits: comparison between self-force, post-Minkowskian, post-Newtonian, and numerical relativity results Comparison of post-Newtonian mode amplitudes with numerical relativity simulations of binary black holes
Reference 30
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T02:13:52.263039Z
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.
Observation 946054d6-4d14-428b-879e-4cd59264a193 · inbound
Cusp Formation in Merging Black Hole Horizons cites this paper.
Cusp Formation in Merging Black Hole Horizons Comparison of post-Newtonian mode amplitudes with numerical relativity simulations of binary black holes
Reference 74
- Resolution
- verified exact
- arxiv_id, observed 2026-05-12T06:46:52.966921Z
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.
Observation 87abd255-59f6-4d47-ae6e-c22401f7c0a7 · inbound
Cusp Formation in Merging Black Hole Horizons cites this paper.
Cusp Formation in Merging Black Hole Horizons Comparison of post-Newtonian mode amplitudes with numerical relativity simulations of binary black holes
Reference 75
- Resolution
- verified exact
- arxiv_id, observed 2026-05-20T22:03:47.531703Z
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.
Observation e85040d6-0196-4417-9866-02f5396cc83c · inbound
Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories cites this paper.
Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Comparison of post-Newtonian mode amplitudes with numerical relativity simulations of binary black holes
Reference 74
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T22:32:29.165377Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.