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Paper Citation Record · LEDGER

Inspiralling eccentric binary neutron stars: orbital motion and tidal resonance

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1904.11089.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
1904.11089 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-15T06:32:42.880941+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T05:05:21.469768Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: pith, observed 2026-08-10T16:33:20.726842Z

Reference resolution

0 of 0 outbound references displayed

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External citation measurements

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Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation a5e18cef-23a5-49be-86bc-0068a829a49e · inbound

Analytic Waveforms for Eccentric Gravitational Wave Bursts cites this paper.

Analytic Waveforms for Eccentric Gravitational Wave Bursts Inspiralling eccentric binary neutron stars: orbital motion and tidal resonance

Reference 33

Resolution
unresolved
no resolver link, observed 2026-08-14T05:05:21.469768Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T05:05:21.469768Z digest=sha256:497c7201f8037a5c5f48e498f313e9f8b4ccab900132807ac8fb535eebb61246

Observation ae40bee3-17c6-4eb7-98ec-a2e74789e2d1 · 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 Inspiralling eccentric binary neutron stars: orbital motion and tidal resonance

Reference 121

Resolution
verified exact
local_arxiv, observed 2026-08-10T16:33:20.733819Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-10T16:33:20.338908Z digest=sha256:6417258b89c58027e9866cac76fbc44c1a6f54e5123bd6d12d9903df93138a24