Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Gravitational waves from inspiralling compact binaries: Angular momentum flux, evolution of the orbital elements and the wave form to the second post-Newtonian order
As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:gr-qc/9710075.
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 2026-08-12T06:34:41.77262+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-06T17:18:50.024838Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-13T11:11:56.900000Z
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 e201ae0b-ab45-4b12-a88d-b19cc1673944 · inbound
The Confrontation between General Relativity and Experiment cites this paper.
The Confrontation between General Relativity and Experiment Gravitational waves from inspiralling compact binaries: Angular momentum flux, evolution of the orbital elements and the wave form to the second post-Newtonian order
Reference 160
- Resolution
- verified exact
- arxiv_id, observed 2026-07-04T19:09:20.449550Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 8613f1d5-696b-4c27-8e6f-0d3adc98507d · inbound
The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster cites this paper.
The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Gravitational waves from inspiralling compact binaries: Angular momentum flux, evolution of the orbital elements and the wave form to the second post-Newtonian order
Reference 65
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T17:18:50.024838Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8eac0b46-ac30-41e7-aff4-67b2a8c0e331 · inbound
Including higher-order modes in a quadrupolar eccentric numerical relativity surrogate using universal eccentric modulation functions cites this paper.
Including higher-order modes in a quadrupolar eccentric numerical relativity surrogate using universal eccentric modulation functions Gravitational waves from inspiralling compact binaries: Angular momentum flux, evolution of the orbital elements and the wave form to the second post-Newtonian order
Reference 90
- Resolution
- verified exact
- arxiv_id, observed 2026-07-04T19:09:20.449550Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.