Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
A new numerical method to construct binary neutron star initial data
As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:0908.0620.
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 2026-08-11T10:51:21.703688Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-07T11:41:20.774922Z
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 7907a766-c921-476e-bec1-7bd085c843cf · inbound
Eccentricity reduction of binary neutron star initial data with the entropy based flux limiting scheme cites this paper.
Eccentricity reduction of binary neutron star initial data with the entropy based flux limiting scheme A new numerical method to construct binary neutron star initial data
Reference 33
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T10:51:21.703688Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4c7e5962-c4f8-4a31-b51f-4ac73e1d9db1 · 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 A new numerical method to construct binary neutron star initial data
Reference 137
- Resolution
- verified exact
- local_arxiv, observed 2026-08-07T11:41:20.779485Z
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.
Observation 3364d5d3-824c-4a37-97d0-3027bcc54182 · inbound
SPH methods in the modelling of compact objects cites this paper.
SPH methods in the modelling of compact objects A new numerical method to construct binary neutron star initial data
Reference 195
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T01:02:22.893841Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 31ef5422-8cd7-4c6d-82fe-b6c6a0300c0a · inbound
Celephais: efficient spectral initial data code for precessing compact binaries cites this paper.
Celephais: efficient spectral initial data code for precessing compact binaries A new numerical method to construct binary neutron star initial data
Reference 34
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T00:32:37.143207Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.