Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Next-to-leading tail-induced spin-orbit effects in the gravitational radiation flux of compact binaries
As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:1307.6793.
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 2026-08-04T06:34:03.388597+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-04T13:28:19.625180Z
A source-named dated measurement, never combined with another source.
Source: cited_works
Reference resolution
0 of 0 outbound references displayed
- verified exact0
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- 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 b1fdb1d7-e533-4b76-98d5-444c7ea6bd04 · 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 Next-to-leading tail-induced spin-orbit effects in the gravitational radiation flux of compact binaries
Reference 52
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T13:28:19.625180Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.