Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Gravitational waveforms of binary neutron star inspirals using post-Newtonian tidal splicing
As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1911.10440.
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 2026-08-21T06:32:19.484+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-03T02:15:32.555287Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-02T09:26:51.428207Z
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 44ea3fc5-a706-4adf-b3eb-c1f81b917f68 · inbound
Toward claiming a detection of gravitational memory cites this paper.
Toward claiming a detection of gravitational memory Gravitational waveforms of binary neutron star inspirals using post-Newtonian tidal splicing
Reference 121
- Resolution
- verified exact
- arxiv_id, observed 2026-05-16T09:20:47.973495Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation 79a87ab6-d99d-498c-9530-404b6eb919aa · inbound
Fast gravitational waveform models for quasi-circular coalescences of neutron star--black hole binaries cites this paper.
Fast gravitational waveform models for quasi-circular coalescences of neutron star--black hole binaries Gravitational waveforms of binary neutron star inspirals using post-Newtonian tidal splicing
Reference 56
- Resolution
- verified exact
- arxiv_id, observed 2026-07-02T09:26:51.429562Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation ce799bed-e831-42d1-a63b-d71f38b7f926 · inbound
Fast gravitational waveform models for quasi-circular coalescences of neutron star--black hole binaries cites this paper.
Fast gravitational waveform models for quasi-circular coalescences of neutron star--black hole binaries Gravitational waveforms of binary neutron star inspirals using post-Newtonian tidal splicing
Reference 56
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T02:15:32.555287Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.