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Paper Citation Record · LEDGER

Simulations of inspiraling and merging double neutron stars using the Spectral Einstein Code

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1604.00782.

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

pith.paper-citation-record.v1
1604.00782 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 2026-08-14T15:45:09.713251Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-14T13:24:33.093925Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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  • malformed identifier0
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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 f938be85-ab66-46a3-829a-63ee4830d391 · inbound

Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission cites this paper.

Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission Simulations of inspiraling and merging double neutron stars using the Spectral Einstein Code

Reference 56

Resolution
unresolved
no resolver link, observed 2026-08-14T15:45:09.713251Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T15:45:09.713251Z digest=sha256:3ed4c8cfd8bf496a90c3c5c8142ba460e25e6efebfc61e9c6dfede700daf2cc5

Observation 2b80a6c2-ed5b-422b-b4a8-86b0b66003c6 · inbound

Smooth equations of state for high-accuracy simulations of neutron star binaries cites this paper.

Smooth equations of state for high-accuracy simulations of neutron star binaries Simulations of inspiraling and merging double neutron stars using the Spectral Einstein Code

Reference 29

Resolution
verified exact
local_arxiv, observed 2026-08-14T13:24:33.105158Z

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=2026-08-14T13:24:32.336686Z digest=sha256:17e1bb1cf7f4dbfaaf22ae2b78f4c01f16bade3ee3d1458d7047d9dd19e6080a