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Paper Citation Record · LEDGER

Data formats for numerical relativity waves

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:0709.0093.

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

pith.paper-citation-record.v1
0709.0093 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 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 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T13:13:32.841945Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-13T21:55:09.186489Z

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 4dc17b69-52c5-4470-a9ab-6f6996d521d3 · inbound

Two-harmonic approximation for gravitational waveforms from precessing binaries cites this paper.

Two-harmonic approximation for gravitational waveforms from precessing binaries Data formats for numerical relativity waves

Reference 92

Resolution
unresolved
no resolver link, observed 2026-08-14T13:13:32.841945Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T13:13:32.841945Z digest=sha256:07b3f33610d0a875a46d8bf5652dcdaa6b43488364cafce9542aaf378ba22390

Observation d014aefa-5ede-4dd1-ae9e-7e0114278ef8 · inbound

Computationally efficient models for the dominant and sub-dominant harmonic modes of precessing binary black holes cites this paper.

Computationally efficient models for the dominant and sub-dominant harmonic modes of precessing binary black holes Data formats for numerical relativity waves

Reference 120

Resolution
verified exact
arxiv_id, observed 2026-07-04T17:43:33.591217Z

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=2026-05-13T21:55:09.043540Z digest=sha256:0292c7c7656c909943cd24851d965cda7ae02fbb14fd1fe7196bf91b7616a6fe

Observation 1ba80ef6-5c45-4d1c-9899-699edfb619da · inbound

A comprehensive look into the accuracy of SpEC binary black hole waveforms cites this paper.

A comprehensive look into the accuracy of SpEC binary black hole waveforms Data formats for numerical relativity waves

Reference 87

Resolution
unresolved
no resolver link, observed 2026-08-04T11:14:45.659628Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T11:14:45.659628Z digest=sha256:e938d8f51f2afd1f319ec9ca82e530792f3a14a260140702dc165563ea478447