Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Constructing quasi-equilibrium initial data for binary neutron stars with arbitrary spins
As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1209.5336.
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 2026-08-09T00:07:29.589936Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-06T21:32:51.418880Z
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 33d91875-a241-4414-ad04-a335aadcf09e · inbound
Axisymmetric stability of neutron stars as extreme rotators in massive scalar-tensor theory cites this paper.
Axisymmetric stability of neutron stars as extreme rotators in massive scalar-tensor theory Constructing quasi-equilibrium initial data for binary neutron stars with arbitrary spins
Reference 37
- Resolution
- unresolved
- no resolver link, observed 2026-08-09T00:07:29.589936Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d77a87d0-d9f4-4a1a-8a46-89f87c502255 · 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 Constructing quasi-equilibrium initial data for binary neutron stars with arbitrary spins
Reference 139
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T11:40:59.667468Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a8e1966c-db3c-4504-82f5-23cbb23a5350 · inbound
Black-hole - neutron-star mergers: new numerical-relativity simulations and multipolar effective-one-body model with spin precession and eccentricity cites this paper.
Black-hole - neutron-star mergers: new numerical-relativity simulations and multipolar effective-one-body model with spin precession and eccentricity Constructing quasi-equilibrium initial data for binary neutron stars with arbitrary spins
Reference 72
- Resolution
- verified exact
- local_arxiv, observed 2026-08-06T21:32:51.422165Z
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.