Paper Citation Record · LEDGER

Improved Cauchy-characteristic evolution system for high-precision numerical relativity waveforms

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 10 inbound Pith citation observations for arXiv:2007.01339.

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

pith.paper-citation-record.v1
2007.01339 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 10 of 10 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00

measured 10 of 10 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T05:57:54.433639Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-06-29T15:33:32.903771Z

Reference resolution

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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 a96cbfdd-336e-4bba-a593-53fc8cc8703c · inbound

AthenaK simulations of the binary black hole merger GW150914 cites this paper.

AthenaK simulations of the binary black hole merger GW150914 Improved Cauchy-characteristic evolution system for high-precision numerical relativity waveforms

Reference 102

Resolution: unresolved; no resolver link, observed 2026-08-07T05:57:54.433639Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 92144a15-c10e-4f5c-b6a2-a60f20eae03d · 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 Improved Cauchy-characteristic evolution system for high-precision numerical relativity waveforms

Reference 97

Resolution: unresolved; no resolver link, observed 2026-08-06T21:32:50.640897Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9f8f1d87-381e-462d-9db4-e7ca1693bb10 · inbound

Quasinormal mode content of binary black hole ringdowns cites this paper.

Quasinormal mode content of binary black hole ringdowns Improved Cauchy-characteristic evolution system for high-precision numerical relativity waveforms

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-04T09:43:29.459571Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a7fa1eb2-dd5f-4d9f-9e85-6f64082ed659 · inbound

Twisting asymptotically-flat spacetimes cites this paper.

Twisting asymptotically-flat spacetimes Improved Cauchy-characteristic evolution system for high-precision numerical relativity waveforms

Reference 210

Resolution: unresolved; no resolver link, observed 2026-08-03T21:54:42.935468Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1234b565-8441-43ab-873e-3c2eccfecde5 · 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 Improved Cauchy-characteristic evolution system for high-precision numerical relativity waveforms

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-02T17:33:26.726137Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cf387ac9-db40-489c-8465-a13665459b0d · inbound

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

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-04T05:45:48.575474Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 405f99c4-40b7-422f-b01c-91cbac67167a · inbound

Merger remnant and eccentricity dynamics surrogates for eccentric nonspinning black hole binaries cites this paper.

Merger remnant and eccentricity dynamics surrogates for eccentric nonspinning black hole binaries Improved Cauchy-characteristic evolution system for high-precision numerical relativity waveforms

Reference 50

Resolution: verified exact; arxiv_id, observed 2026-05-11T15:01:09.083628Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation e91a8a1b-e59d-44fb-9221-f4b7b3fc5087 · inbound

Merger remnant and eccentricity dynamics surrogates for eccentric nonspinning black hole binaries cites this paper.

Merger remnant and eccentricity dynamics surrogates for eccentric nonspinning black hole binaries Improved Cauchy-characteristic evolution system for high-precision numerical relativity waveforms

Reference 50

Resolution: verified exact; arxiv_id, observed 2026-05-22T10:41:25.670925Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation d8b9e5c0-345d-458e-847e-c9da91af697e · inbound

Convergence of post-Newtonian for quasi-circular non-precessing comparable mass ratios BBHs cites this paper.

Convergence of post-Newtonian for quasi-circular non-precessing comparable mass ratios BBHs Improved Cauchy-characteristic evolution system for high-precision numerical relativity waveforms

Reference 25

Resolution: verified exact; arxiv_id, observed 2026-05-21T06:24:00.626686Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 6d6e5fb3-bb8a-4988-91b5-edbc5d2b16bf · inbound

Constraining Gravitational Wave Memory with Hierarchical Inference cites this paper.

Constraining Gravitational Wave Memory with Hierarchical Inference Improved Cauchy-characteristic evolution system for high-precision numerical relativity waveforms

Reference 72

Resolution: verified exact; arxiv_id, observed 2026-06-29T15:33:32.905197Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.