Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Frequency domain model of $f$-mode dynamic tides in gravitational waveforms from compact binary inspirals
As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1905.00818.
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 2026-08-10T16:33:19.692608Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-02T00:36:25.212926Z
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 e1345b39-e17e-4c8e-a636-4df1acf7fc81 · inbound
Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides cites this paper.
Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Frequency domain model of $f$-mode dynamic tides in gravitational waveforms from compact binary inspirals
Reference 40
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T16:33:19.692608Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8fb2a6d2-a18a-4942-9b79-f7a96062d15c · inbound
Improved post-Newtonian waveform model for inspiralling precessing-eccentric compact binaries cites this paper.
Improved post-Newtonian waveform model for inspiralling precessing-eccentric compact binaries Frequency domain model of $f$-mode dynamic tides in gravitational waveforms from compact binary inspirals
Reference 190
- Resolution
- unresolved
- no resolver link, observed 2026-08-09T00:23:47.263682Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 0411edcc-6611-40fa-8f16-497db1d45a38 · inbound
The error budget of binary neutron star merger simulations for configurations with high spin cites this paper.
The error budget of binary neutron star merger simulations for configurations with high spin Frequency domain model of $f$-mode dynamic tides in gravitational waveforms from compact binary inspirals
Reference 96
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T11:40:55.869925Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 85c2b8ca-8494-4b84-8a38-cb3d5f4eec54 · inbound
Speed and accuracy for long signals: Frequency-domain effective-one-body waveforms for compact binary coalescences cites this paper.
Speed and accuracy for long signals: Frequency-domain effective-one-body waveforms for compact binary coalescences Frequency domain model of $f$-mode dynamic tides in gravitational waveforms from compact binary inspirals
Reference 44
- Resolution
- verified exact
- arxiv_id, observed 2026-07-02T00:36:25.214777Z
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.