Paper Citation Record · LEDGER

ESIGMAHM: An Eccentric, Spinning inspiral-merger-ringdown waveform model with Higher Modes for the detection and characterization of binary black holes

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 14 inbound Pith citation observations for arXiv:2409.13866.

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

pith.paper-citation-record.v1
2409.13866 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 14 of 14 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00

measured 14 of 14 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-09T11:24:09.518780Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T11:48:04.580847Z

Reference resolution

0 of 0 outbound references displayed

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verified fuzzy0
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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 54bf2b5e-a638-428b-bba1-36b6c8f59f3e · inbound

Post-Newtonian theory-inspired framework for characterizing eccentricity in gravitational waveforms cites this paper.

Post-Newtonian theory-inspired framework for characterizing eccentricity in gravitational waveforms ESIGMAHM: An Eccentric, Spinning inspiral-merger-ringdown waveform model with Higher Modes for the detection and characterization of binary black holes

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-09T11:24:09.518780Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 53398e7b-2e09-4157-b83d-9ceb687dc646 · inbound

Improved post-Newtonian waveform model for inspiralling precessing-eccentric compact binaries cites this paper.

Improved post-Newtonian waveform model for inspiralling precessing-eccentric compact binaries ESIGMAHM: An Eccentric, Spinning inspiral-merger-ringdown waveform model with Higher Modes for the detection and characterization of binary black holes

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-09T00:23:46.805139Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation deadf782-4b85-4c28-868a-9dba0f3c985f · inbound

Probing the existence of a minimal length through compact binary inspiral cites this paper.

Probing the existence of a minimal length through compact binary inspiral ESIGMAHM: An Eccentric, Spinning inspiral-merger-ringdown waveform model with Higher Modes for the detection and characterization of binary black holes

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-07T13:07:34.445880Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2b412195-5c1c-438a-9164-4ad28d3b6431 · inbound

Early Warning From Eccentric Compact Binaries: Template Initialization And Sub-dominant Mode Effects cites this paper.

Early Warning From Eccentric Compact Binaries: Template Initialization And Sub-dominant Mode Effects ESIGMAHM: An Eccentric, Spinning inspiral-merger-ringdown waveform model with Higher Modes for the detection and characterization of binary black holes

Reference 99

Resolution: unresolved; no resolver link, observed 2026-08-06T18:55:59.195649Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f1d83efb-efd1-4533-95da-3c820767fda9 · inbound

Testing the nature of GW200105 by probing the frequency evolution of eccentricity cites this paper.

Testing the nature of GW200105 by probing the frequency evolution of eccentricity ESIGMAHM: An Eccentric, Spinning inspiral-merger-ringdown waveform model with Higher Modes for the detection and characterization of binary black holes

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-04T13:37:59.294017Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a4fb8941-cb4e-42ba-92ca-4cd08d5db78d · 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 ESIGMAHM: An Eccentric, Spinning inspiral-merger-ringdown waveform model with Higher Modes for the detection and characterization of binary black holes

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:56.963720Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4b8c51fe-c52c-402d-9f81-59457cdace00 · inbound

Biased parameter inference of eccentric, spin-precessing binary black holes cites this paper.

Biased parameter inference of eccentric, spin-precessing binary black holes ESIGMAHM: An Eccentric, Spinning inspiral-merger-ringdown waveform model with Higher Modes for the detection and characterization of binary black holes

Reference 133

Resolution: verified exact; arxiv_id, observed 2026-05-18T09:51:12.777991Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 734d9e9d-42e8-4541-a067-d2835ddd6bbc · inbound

Post-Newtonian inspiral waveform model for eccentric precessing binaries with higher-order modes and matter effects cites this paper.

Post-Newtonian inspiral waveform model for eccentric precessing binaries with higher-order modes and matter effects ESIGMAHM: An Eccentric, Spinning inspiral-merger-ringdown waveform model with Higher Modes for the detection and characterization of binary black holes

Reference 52

Resolution: verified exact; arxiv_id, observed 2026-05-10T15:00:31.134947Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 5203bb93-d931-4b54-a28e-7a7d30044cdd · inbound

Including higher-order modes in a quadrupolar eccentric numerical relativity surrogate using universal eccentric modulation functions cites this paper.

Including higher-order modes in a quadrupolar eccentric numerical relativity surrogate using universal eccentric modulation functions ESIGMAHM: An Eccentric, Spinning inspiral-merger-ringdown waveform model with Higher Modes for the detection and characterization of binary black holes

Reference 72

Resolution: verified exact; arxiv_id, observed 2026-05-10T12:10:22.535094Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 61234c8f-f323-4b92-957c-e7aa58156414 · inbound

A universal framework to identify eccentric binary mergers: GW200105 case study cites this paper.

A universal framework to identify eccentric binary mergers: GW200105 case study ESIGMAHM: An Eccentric, Spinning inspiral-merger-ringdown waveform model with Higher Modes for the detection and characterization of binary black holes

Reference 34

Resolution: verified exact; arxiv_id, observed 2026-05-20T08:53:09.967716Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 7a36fad1-df45-4145-82b9-a7d73f9b76c0 · 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 ESIGMAHM: An Eccentric, Spinning inspiral-merger-ringdown waveform model with Higher Modes for the detection and characterization of binary black holes

Reference 189

Resolution: verified exact; arxiv_id, observed 2026-06-29T11:03:19.449405Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 1a02688b-7962-4e5f-9173-6e1913005570 · inbound

Eccentric and unbound compact binaries in the LIGO-Virgo-KAGRA catalog: parameter estimation and waveform systematics with SEOBNRv6EHM cites this paper.

Eccentric and unbound compact binaries in the LIGO-Virgo-KAGRA catalog: parameter estimation and waveform systematics with SEOBNRv6EHM ESIGMAHM: An Eccentric, Spinning inspiral-merger-ringdown waveform model with Higher Modes for the detection and characterization of binary black holes

Reference 56

Resolution: verified exact; arxiv_id, observed 2026-06-29T13:13:28.327301Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 6b7d7318-5b51-4caa-874e-9b06c91ddf06 · inbound

Horizon absorption in eccentric precessing binary black hole inspirals and its importance for gravitational wave data analysis cites this paper.

Horizon absorption in eccentric precessing binary black hole inspirals and its importance for gravitational wave data analysis ESIGMAHM: An Eccentric, Spinning inspiral-merger-ringdown waveform model with Higher Modes for the detection and characterization of binary black holes

Reference 94

Resolution: verified exact; arxiv_id, observed 2026-07-03T11:48:04.582330Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 3d078492-93c3-4dc6-acfa-6f9dc00ee4f4 · 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 ESIGMAHM: An Eccentric, Spinning inspiral-merger-ringdown waveform model with Higher Modes for the detection and characterization of binary black holes

Reference 42

Resolution: verified exact; arxiv_id, observed 2026-06-30T16:24:59.205311Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.