Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Efficient fully precessing gravitational waveforms for binaries with neutron stars
As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2212.04657.
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 2026-08-21T06:32:19.484+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-10T16:33:20.295774Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-05T15:37:38.130923Z
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 a57c3ccc-e1d7-4275-a9db-9922194ee812 · inbound
Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides cites this paper.
Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Efficient fully precessing gravitational waveforms for binaries with neutron stars
Reference 115
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T16:33:20.295774Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation bd608cbf-b263-46e1-88d4-3790d5153753 · inbound
Improved post-Newtonian waveform model for inspiralling precessing-eccentric compact binaries cites this paper.
Improved post-Newtonian waveform model for inspiralling precessing-eccentric compact binaries Efficient fully precessing gravitational waveforms for binaries with neutron stars
Reference 191
- Resolution
- unresolved
- no resolver link, observed 2026-08-09T00:23:47.267454Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 5a2e6aef-62f6-4c73-be4e-a7950601f8c8 · inbound
Coincident morphological transitions in precessing black-hole binaries cites this paper.
Coincident morphological transitions in precessing black-hole binaries Efficient fully precessing gravitational waveforms for binaries with neutron stars
Reference 33
- Resolution
- verified exact
- local_arxiv, observed 2026-08-05T15:37:38.135274Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.