Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Spin-orbit precession for eccentric black hole binaries at first order in the mass ratio
As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1608.04811.
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 2026-08-07T00:15:14.642544Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-04T21:28:09.103023Z
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 4b82d1be-ebf7-4fb4-98b5-c9923a073ed6 · inbound
Metric reconstruction and the Hamiltonian for eccentric, precessing binaries in the small-mass-ratio limit cites this paper.
Metric reconstruction and the Hamiltonian for eccentric, precessing binaries in the small-mass-ratio limit Spin-orbit precession for eccentric black hole binaries at first order in the mass ratio
Reference 45
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T18:38:44.083404Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation fa0ad137-4aa7-4355-b050-6db281eeeff2 · inbound
High-Post-Newtonian-Order Dynamics Induced by Tail-of-Tail Interactions: The Non-Geodesic Terms cites this paper.
High-Post-Newtonian-Order Dynamics Induced by Tail-of-Tail Interactions: The Non-Geodesic Terms Spin-orbit precession for eccentric black hole binaries at first order in the mass ratio
Reference 153
- Resolution
- verified exact
- local_arxiv, observed 2026-08-04T21:28:09.209451Z
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.
Observation 978b5999-a930-4002-89be-aee94d9d86fd · inbound
High-Post-Newtonian-Order Dynamics Induced by Tail-of-Tail Interactions: The Non-Geodesic Terms cites this paper.
High-Post-Newtonian-Order Dynamics Induced by Tail-of-Tail Interactions: The Non-Geodesic Terms Spin-orbit precession for eccentric black hole binaries at first order in the mass ratio
Reference 153
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T00:15:14.642544Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.