Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Phenomenological model of gravitational self-force enhanced tides in inspiralling binary neutron stars
As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2407.08538.
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 2026-08-11T06:34:44.6726+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-10T19:21:20.693015Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-06-30T09:04:32.354196Z
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 e4ef9577-82cc-4ca5-8adc-d8b5ab2fded7 · inbound
Data-driven approach for extracting tidal information from neutron star binary mergers observed with the Einstein Telescope cites this paper.
Data-driven approach for extracting tidal information from neutron star binary mergers observed with the Einstein Telescope Phenomenological model of gravitational self-force enhanced tides in inspiralling binary neutron stars
Reference 50
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:21:20.693015Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation df321d5a-a754-4987-81a0-2b8d58fbbade · 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 Phenomenological model of gravitational self-force enhanced tides in inspiralling binary neutron stars
Reference 49
- Resolution
- verified exact
- arxiv_id, observed 2026-06-30T09:04:32.355484Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.