Paper Citation Record · LEDGER

A higher-multipole gravitational waveform model for an eccentric binary black holes based on the effective-one-body-numerical-relativity formalism

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 11 inbound Pith citation observations for arXiv:2102.08614.

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

pith.paper-citation-record.v1
2102.08614 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 11 of 11 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-16T06:30:59.297886+00:00

measured 11 of 11 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T19:45:10.261693Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-06-30T16:24:59.091894Z

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 a47f46ff-14e7-453d-a2f7-56f08159906e · inbound

A geometric template bank for the detection of spinning low-mass compact binaries with moderate orbital eccentricity cites this paper.

A geometric template bank for the detection of spinning low-mass compact binaries with moderate orbital eccentricity A higher-multipole gravitational waveform model for an eccentric binary black holes based on the effective-one-body-numerical-relativity formalism

Reference 142

Resolution: unresolved; no resolver link, observed 2026-08-11T19:45:10.261693Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 876da49b-8fa2-4392-8dad-7f35da12c449 · inbound

Inferring additional physics through unmodelled signal reconstructions cites this paper.

Inferring additional physics through unmodelled signal reconstructions A higher-multipole gravitational waveform model for an eccentric binary black holes based on the effective-one-body-numerical-relativity formalism

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-11T14:41:19.134577Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 17ad9037-fb9b-47df-b631-28d6223842c4 · inbound

Accurate waveforms for eccentric, aligned-spin binary black holes: The multipolar effective-one-body model SEOBNRv5EHM cites this paper.

Accurate waveforms for eccentric, aligned-spin binary black holes: The multipolar effective-one-body model SEOBNRv5EHM A higher-multipole gravitational waveform model for an eccentric binary black holes based on the effective-one-body-numerical-relativity formalism

Reference 235

Resolution: unresolved; no resolver link, observed 2026-08-11T13:49:13.587875Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 551ff33c-a083-446b-a756-e1301bbfeb98 · inbound

Third post-Newtonian dynamics for eccentric orbits and aligned spins in the effective-one-body waveform model SEOBNRv5EHM cites this paper.

Third post-Newtonian dynamics for eccentric orbits and aligned spins in the effective-one-body waveform model SEOBNRv5EHM A higher-multipole gravitational waveform model for an eccentric binary black holes based on the effective-one-body-numerical-relativity formalism

Reference 207

Resolution: unresolved; no resolver link, observed 2026-08-11T13:46:55.204742Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 83bf8c0d-dc6c-4ac2-af08-cce94b37168f · inbound

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides cites this paper.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides A higher-multipole gravitational waveform model for an eccentric binary black holes based on the effective-one-body-numerical-relativity formalism

Reference 126

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:20.378674Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5d241fd1-55d7-4cb2-bd0d-3e806a0c6735 · inbound

Residual Test for the Third Gravitational-Wave Transient Catalog cites this paper.

Residual Test for the Third Gravitational-Wave Transient Catalog A higher-multipole gravitational waveform model for an eccentric binary black holes based on the effective-one-body-numerical-relativity formalism

Reference 20

Resolution: verified exact; arxiv_id, observed 2026-05-18T16:11:35.426357Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 33e2ef81-47c2-4f12-ac37-9f22e1bb5ad6 · inbound

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates cites this paper.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates A higher-multipole gravitational waveform model for an eccentric binary black holes based on the effective-one-body-numerical-relativity formalism

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.403224Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 82d41ae9-5878-470c-9950-f83df212dd6e · 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 A higher-multipole gravitational waveform model for an eccentric binary black holes based on the effective-one-body-numerical-relativity formalism

Reference 102

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 41482b5b-57e7-4d4e-840e-f57c75ec8ceb · inbound

Highly eccentric non-spinning binary black hole mergers: quadrupolar post-merger waveforms cites this paper.

Highly eccentric non-spinning binary black hole mergers: quadrupolar post-merger waveforms A higher-multipole gravitational waveform model for an eccentric binary black holes based on the effective-one-body-numerical-relativity formalism

Reference 144

Resolution: verified exact; arxiv_id, observed 2026-05-10T10:19:21.158994Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 76a1f310-5290-4e37-aad9-f30a209e56fc · inbound

Accurate waveforms for generic planar-orbit binary black holes: The multipolar effective-one-body model SEOBNRv6EHM cites this paper.

Accurate waveforms for generic planar-orbit binary black holes: The multipolar effective-one-body model SEOBNRv6EHM A higher-multipole gravitational waveform model for an eccentric binary black holes based on the effective-one-body-numerical-relativity formalism

Reference 269

Resolution: verified exact; arxiv_id, observed 2026-06-29T11:03:19.431657Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 544ce692-33d9-4df5-a106-7f6856d17379 · inbound

Efficient Eccentric Effective-One-Body Dynamics via Near-Identity Averaging Transformations cites this paper.

Efficient Eccentric Effective-One-Body Dynamics via Near-Identity Averaging Transformations A higher-multipole gravitational waveform model for an eccentric binary black holes based on the effective-one-body-numerical-relativity formalism

Reference 101

Resolution: verified exact; arxiv_id, observed 2026-06-30T16:24:59.099432Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.