Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
An accurate analytical fit to the gravitational-wave inspiral duration for eccentric binaries
As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2110.09254.
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 2026-08-10T06:31:04.303077+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-10T13:27:10.573765Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-03T22:39:01.823443Z
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 aaf788b7-d6e1-4c61-9ffe-d3fa90a5f9ad · inbound
Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers cites this paper.
Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers An accurate analytical fit to the gravitational-wave inspiral duration for eccentric binaries
Reference 85
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T13:27:10.573765Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ad7f9c47-54c4-4866-bf16-d8f9743a9e43 · inbound
Stable mass transfer in massive binaries leading to merging black holes cites this paper.
Stable mass transfer in massive binaries leading to merging black holes An accurate analytical fit to the gravitational-wave inspiral duration for eccentric binaries
Reference 117
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T14:34:34.561929Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 5b20b6d6-cdc1-497c-bc2f-ce974fbb602a · inbound
Orbital evolution of asymmetric binaries within accreting environments cites this paper.
Orbital evolution of asymmetric binaries within accreting environments An accurate analytical fit to the gravitational-wave inspiral duration for eccentric binaries
Reference 51
- Resolution
- verified exact
- arxiv_id, observed 2026-07-03T22:39:01.824656Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.