Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Periastron advance in spinning black hole binaries: comparing effective-one-body and Numerical Relativity
As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1309.0544.
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 2026-08-08T06:32:00.761636+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-04T05:45:47.405865Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-06-30T09:04:33.111696Z
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 cb3e7e79-835f-4dad-8f2d-927129d4c6e8 · inbound
Fixing the center-of-mass frame of numerical relativity waveforms using the post-Newtonian center-of-mass charge cites this paper.
Fixing the center-of-mass frame of numerical relativity waveforms using the post-Newtonian center-of-mass charge Periastron advance in spinning black hole binaries: comparing effective-one-body and Numerical Relativity
Reference 11
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T17:33:24.706600Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 948db92c-6008-4ec5-ae47-96810acad0f0 · inbound
Fixing the center-of-mass frame of numerical relativity waveforms using the post-Newtonian center-of-mass charge cites this paper.
Fixing the center-of-mass frame of numerical relativity waveforms using the post-Newtonian center-of-mass charge Periastron advance in spinning black hole binaries: comparing effective-one-body and Numerical Relativity
Reference 11
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T05:45:47.405865Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 0866a659-82a1-457f-9977-f21e4f05dd10 · inbound
Quadrupole and quadratic-in-spin effects in quasicircular, spinning, asymmetric binaries cites this paper.
Quadrupole and quadratic-in-spin effects in quasicircular, spinning, asymmetric binaries Periastron advance in spinning black hole binaries: comparing effective-one-body and Numerical Relativity
Reference 142
- Resolution
- verified exact
- local_arxiv, observed 2026-06-30T09:04:33.112899Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.