Pith. sign in

Paper Citation Record · LEDGER

Accuracy of numerical relativity waveforms from binary neutron star mergers and their comparison with post-Newtonian waveforms

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1109.3611.

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

pith.paper-citation-record.v1
1109.3611 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-08T06:32:00.761636+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T11:41:12.711161Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-06T21:32:51.575494Z

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 e6528b3e-9abc-43fb-97bc-07fdd3438533 · 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 Accuracy of numerical relativity waveforms from binary neutron star mergers and their comparison with post-Newtonian waveforms

Reference 168

Resolution
unresolved
no resolver link, observed 2026-08-07T11:41:12.711161Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T11:41:12.711161Z digest=sha256:22ec8e8d4e12ba98d3c7a8a2c386937e2ed3225510f8267d404a4e4f20598c88

Observation a7d7cbff-c6de-42e0-bab1-4182d086b757 · 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 Accuracy of numerical relativity waveforms from binary neutron star mergers and their comparison with post-Newtonian waveforms

Reference 54

Resolution
verified exact
local_arxiv, observed 2026-08-06T21:32:51.578262Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=pdf_text observed=2026-08-06T21:32:50.526435Z digest=sha256:3d32e8a6a81adfc7901c15ac2dcae388f95a9511f2706967bdeb5c3aef1325aa

Observation 7b8fc865-2ccc-4f60-88f2-da5f9b12c3af · inbound

Impact of numerical-relativity waveform calibration on parametrized post-Einsteinian tests cites this paper.

Impact of numerical-relativity waveform calibration on parametrized post-Einsteinian tests Accuracy of numerical relativity waveforms from binary neutron star mergers and their comparison with post-Newtonian waveforms

Reference 126

Resolution
unresolved
no resolver link, observed 2026-07-14T00:11:25.155489Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-14T00:11:25.155489Z digest=sha256:f3b0323b32b604f2e1faa1da6a327201d06852d6e02bec4a2028509258cdce15

Observation a044d849-471f-473d-b5f2-6e34da67dec6 · inbound

Fixing the center-of-mass frame of numerical relativity waveforms using the post-Newtonian center-of-mass charge cites this paper.

Fixing the center-of-mass frame of numerical relativity waveforms using the post-Newtonian center-of-mass charge Accuracy of numerical relativity waveforms from binary neutron star mergers and their comparison with post-Newtonian waveforms

Reference 10

Resolution
unresolved
no resolver link, observed 2026-08-02T17:33:24.616486Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T17:33:24.616486Z digest=sha256:bff1c7595ded5d676c1d554c5f28a6f53292bc8c05e103d6b163f290654000ea

Observation 5082c7fc-8708-4b48-8052-9e1a002195a7 · inbound

Fixing the center-of-mass frame of numerical relativity waveforms using the post-Newtonian center-of-mass charge cites this paper.

Fixing the center-of-mass frame of numerical relativity waveforms using the post-Newtonian center-of-mass charge Accuracy of numerical relativity waveforms from binary neutron star mergers and their comparison with post-Newtonian waveforms

Reference 10

Resolution
unresolved
no resolver link, observed 2026-08-04T05:45:47.307054Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T05:45:47.307054Z digest=sha256:70f7b07b50dc0e56d745fdeb5930153e443eaf4d8b670b9f47eacd91aeb11c3f