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Paper Citation Record · LEDGER

Reducing orbital eccentricity in initial data of binary neutron stars

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1405.6207.

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

pith.paper-citation-record.v1
1405.6207 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T10:51:21.717233Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-07T11:41:20.432754Z

Reference resolution

0 of 0 outbound references displayed

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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 ab805dbc-7292-459f-8988-5ebea776571b · 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 Reducing orbital eccentricity in initial data of binary neutron stars

Reference 36

Resolution
unresolved
no resolver link, observed 2026-08-11T10:51:21.717233Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation b9e009e0-a0e2-4b4b-aa56-ee66bd630a39 · inbound

SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement cites this paper.

SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement Reducing orbital eccentricity in initial data of binary neutron stars

Reference 123

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unresolved
no resolver link, observed 2026-08-09T05:33:08.345805Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T05:33:08.345805Z digest=sha256:5e80d659306686b04353166d5e7799b5e105c8a4b9ccc78bece5824caeec6193

Observation ee17e05b-d5cc-434f-9031-847850fa977e · 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 Reducing orbital eccentricity in initial data of binary neutron stars

Reference 146

Resolution
verified exact
local_arxiv, observed 2026-08-07T11:41:20.447339Z

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.

source=pdf_text observed=2026-08-07T11:41:09.288566Z digest=sha256:f99e5d9154e9e561122c415310f1b9a341cd11651bcba7a7b14e02e371e6c3ca

Observation be0230b2-2884-4b7b-a14b-c62dafd3894e · inbound

Celephais: efficient spectral initial data code for precessing compact binaries cites this paper.

Celephais: efficient spectral initial data code for precessing compact binaries Reducing orbital eccentricity in initial data of binary neutron stars

Reference 79

Resolution
unresolved
no resolver link, observed 2026-08-11T00:32:37.340238Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T00:32:37.340238Z digest=sha256:36c8b9fe591386379c7300bce45d192139c97a4efc595410779ca3776754d20e