Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Complete gravitational-waveform amplitude modes for quasi-circular compact binaries to the 3.5PN order
As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2210.15602.
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 2026-08-17T06:30:58.91139+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-11T13:46:55.426134Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-02T09:26:51.186244Z
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 ed9b06db-e196-4d25-a529-85a6558890de · inbound
Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries cites this paper.
Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries Complete gravitational-waveform amplitude modes for quasi-circular compact binaries to the 3.5PN order
Reference 36
- Resolution
- verified exact
- arxiv_id, observed 2026-05-23T23:18:36.012403Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.
Observation e9a96909-e0e0-4547-9f87-e1158f4a8952 · inbound
Third post-Newtonian dynamics for eccentric orbits and aligned spins in the effective-one-body waveform model SEOBNRv5EHM cites this paper.
Third post-Newtonian dynamics for eccentric orbits and aligned spins in the effective-one-body waveform model SEOBNRv5EHM Complete gravitational-waveform amplitude modes for quasi-circular compact binaries to the 3.5PN order
Reference 265
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T13:46:55.426134Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 5b98a9a6-8f5d-45b2-8d71-279de9b0874e · inbound
Tidal contributions to the full gravitational waveform to the second-and-a-half post-Newtonian order cites this paper.
Tidal contributions to the full gravitational waveform to the second-and-a-half post-Newtonian order Complete gravitational-waveform amplitude modes for quasi-circular compact binaries to the 3.5PN order
Reference 45
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T12:28:43.872255Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e9835067-2fcd-4c55-8b21-1e62e875b286 · inbound
Fast gravitational waveform models for quasi-circular coalescences of neutron star--black hole binaries cites this paper.
Fast gravitational waveform models for quasi-circular coalescences of neutron star--black hole binaries Complete gravitational-waveform amplitude modes for quasi-circular compact binaries to the 3.5PN order
Reference 115
- Resolution
- verified exact
- arxiv_id, observed 2026-07-02T09:26:51.187443Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.
Observation b61bfdb5-aede-4490-ba02-389a9b918d96 · inbound
Fast gravitational waveform models for quasi-circular coalescences of neutron star--black hole binaries cites this paper.
Fast gravitational waveform models for quasi-circular coalescences of neutron star--black hole binaries Complete gravitational-waveform amplitude modes for quasi-circular compact binaries to the 3.5PN order
Reference 115
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T02:15:40.276761Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.