Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Parameter estimation of inspiralling compact binaries using 3.5 post-Newtonian gravitational wave phasing: The non-spinning case
As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:gr-qc/0411146.
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 2026-08-16T06:30:59.297886+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T15:23:18.427404Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-05-24T08:54:15.796007Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- 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 f67129af-0475-4df4-90a0-9530c9c4d6b3 · inbound
Post-Newtonian Theory for Gravitational Waves cites this paper.
Post-Newtonian Theory for Gravitational Waves Parameter estimation of inspiralling compact binaries using 3.5 post-Newtonian gravitational wave phasing: The non-spinning case
Reference 13
- Resolution
- verified exact
- arxiv_id, observed 2026-05-13T00:25:44.240833Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 9772b8dc-012f-421e-a9d8-d5840a8de66c · inbound
Worldline effective field theory of inspiralling black hole binaries in presence of dark photon and axionic dark matter cites this paper.
Worldline effective field theory of inspiralling black hole binaries in presence of dark photon and axionic dark matter Parameter estimation of inspiralling compact binaries using 3.5 post-Newtonian gravitational wave phasing: The non-spinning case
Reference 26
- Resolution
- verified exact
- local_arxiv, observed 2026-05-24T08:54:15.798570Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 46440d12-e4f6-4d01-8019-9d5cb542f68a · inbound
Consistency of spin effects between numerical relativity and perturbation theory for inspiraling comparable-mass black hole binaries cites this paper.
Consistency of spin effects between numerical relativity and perturbation theory for inspiraling comparable-mass black hole binaries Parameter estimation of inspiralling compact binaries using 3.5 post-Newtonian gravitational wave phasing: The non-spinning case
Reference 45
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T13:28:19.090887Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 79e8b9ae-548e-4657-bf69-00b863c44cda · inbound
The Impact of Spin Priors on Parameterized Tests of General Relativity cites this paper.
The Impact of Spin Priors on Parameterized Tests of General Relativity Parameter estimation of inspiralling compact binaries using 3.5 post-Newtonian gravitational wave phasing: The non-spinning case
Reference 15
- Resolution
- verified exact
- arxiv_id, observed 2026-05-11T18:21:06.304413Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 96519c98-1db2-484f-90a8-2fea7b0a5154 · inbound
Classical Black Hole Scattering to Celestial Amplitudes in Effective Theories of Gravity cites this paper.
Classical Black Hole Scattering to Celestial Amplitudes in Effective Theories of Gravity Parameter estimation of inspiralling compact binaries using 3.5 post-Newtonian gravitational wave phasing: The non-spinning case
Reference 78
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T15:23:18.427404Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.