Pith. sign in

Paper Citation Record · LEDGER

Efficient gravitational-wave model for fully-precessing and moderately-eccentric, compact binary inspirals

As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 11 inbound Pith citation observations for arXiv:2402.06804.

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

pith.paper-citation-record.v1
2402.06804 v2

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 2026-08-20T06:33:59.587034+00:00

measured 11 of 11 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T19:45:10.201291Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-02T23:57:28.414845Z

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 4066e381-1cf0-417c-974f-4fb58acb9462 · 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 Efficient gravitational-wave model for fully-precessing and moderately-eccentric, compact binary inspirals

Reference 136

Resolution
unresolved
no resolver link, observed 2026-08-11T19:45:10.201291Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T19:45:10.201291Z digest=sha256:6d54d1a13dbcaa9337abf15b1da2b506a130a5a311e83dcf935e4b63576b0ecf

Observation 457d44be-d724-41cb-bced-897b32f1a5ce · inbound

Enhancing Early Detection and Localization of Gravitational Waves via Eccentricity-Induced Higher Harmonic Modes with 2G Detector Networks cites this paper.

Enhancing Early Detection and Localization of Gravitational Waves via Eccentricity-Induced Higher Harmonic Modes with 2G Detector Networks Efficient gravitational-wave model for fully-precessing and moderately-eccentric, compact binary inspirals

Reference 36

Resolution
verified exact
arxiv_id, observed 2026-05-23T07:27:42.841043Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-23T07:26:44.341644Z digest=sha256:f317430548074cbc22e5a502a8fe7ca0e9bf20cac70b6aea9c6ba0500d661a81

Observation cae8e2ff-f1f7-443a-92b9-0c73ecb974ec · 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 Efficient gravitational-wave model for fully-precessing and moderately-eccentric, compact binary inspirals

Reference 80

Resolution
unresolved
no resolver link, observed 2026-08-09T00:23:46.833399Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T00:23:46.833399Z digest=sha256:db38d783d1b9196010bdbafb6f491ef389ba587ad1a6d487faff781cdc5c51a7

Observation d926805b-a214-4873-96a3-1ed076cad1ef · inbound

Toward claiming a detection of gravitational memory cites this paper.

Toward claiming a detection of gravitational memory Efficient gravitational-wave model for fully-precessing and moderately-eccentric, compact binary inspirals

Reference 180

Resolution
verified exact
arxiv_id, observed 2026-05-16T09:20:48.046603Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-16T09:18:23.702726Z digest=sha256:5d40e8062e087aa2544a565678fc7d4d0c6f15f94b8837f245bf9197ab4547dc

Observation 2a7b28b3-6a0c-4c0b-bf0a-633a776248f6 · 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 Efficient gravitational-wave model for fully-precessing and moderately-eccentric, compact binary inspirals

Reference 108

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:ffd903579d8acacb8433baa42a4d24e5d339787b877ac6477008a8f2b4cec710

Observation b29b47c6-4bf9-4da3-96ff-12da378a6c07 · inbound

Analytical Solution of Spinning, Eccentric Binary Black Hole Dynamics at the Second Post-Newtonian Order cites this paper.

Analytical Solution of Spinning, Eccentric Binary Black Hole Dynamics at the Second Post-Newtonian Order Efficient gravitational-wave model for fully-precessing and moderately-eccentric, compact binary inspirals

Reference 29

Resolution
verified exact
arxiv_id, observed 2026-05-15T08:25:18.887681Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-15T08:24:38.929005Z digest=sha256:ac895f72abaf5fc21dfba26a7dde4bfb1c536d5ac548f7ca5c4f24fd531e8413

Observation 99ee90b3-4304-4ec1-93cf-0f8f4a84a576 · 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 Efficient gravitational-wave model for fully-precessing and moderately-eccentric, compact binary inspirals

Reference 64

Resolution
verified exact
arxiv_id, observed 2026-05-10T15:00:31.464160Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-10T15:00:29.655032Z digest=sha256:13e7cfbc6db1df290328aaec00c893833f167d98ee2d1e0b706882db3a9c3ab7

Observation 263f7938-4dda-4f6d-8e5e-348d11a11791 · 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 Efficient gravitational-wave model for fully-precessing and moderately-eccentric, compact binary inspirals

Reference 181

Resolution
verified exact
arxiv_id, observed 2026-06-29T10:53:19.502867Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-06-29T10:39:57.468339Z digest=sha256:4660723714bf3612945cc04eb2c53fdf157defffa8968fab45f988d827b99cf7

Observation b04101ef-6dd5-4a1f-869d-b3d08b87b38d · inbound

Line-of-sight acceleration in compact binaries with higher harmonics and eccentricity cites this paper.

Line-of-sight acceleration in compact binaries with higher harmonics and eccentricity Efficient gravitational-wave model for fully-precessing and moderately-eccentric, compact binary inspirals

Reference 60

Resolution
verified exact
arxiv_id, observed 2026-07-02T23:57:28.416326Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-06-27T17:41:13.400252Z digest=sha256:c55b915a6e88df0e79f25deca332f15a56b2fa742f197377cd13bdc33cab08d5

Observation dabe452b-44c0-4691-83b8-fee295430579 · inbound

High-Post-Newtonian-Order Dynamics Induced by Tail-of-Tail Interactions: The Non-Geodesic Terms cites this paper.

High-Post-Newtonian-Order Dynamics Induced by Tail-of-Tail Interactions: The Non-Geodesic Terms Efficient gravitational-wave model for fully-precessing and moderately-eccentric, compact binary inspirals

Reference 55

Resolution
unresolved
no resolver link, observed 2026-08-04T21:28:07.466892Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T21:28:07.466892Z digest=sha256:d793f4548a3a20217791467a6d1a2fd36213cb5d901adf2cfe93782163d451dd

Observation a06ae77a-6bb6-4966-98f2-5d4138740c6c · inbound

High-Post-Newtonian-Order Dynamics Induced by Tail-of-Tail Interactions: The Non-Geodesic Terms cites this paper.

High-Post-Newtonian-Order Dynamics Induced by Tail-of-Tail Interactions: The Non-Geodesic Terms Efficient gravitational-wave model for fully-precessing and moderately-eccentric, compact binary inspirals

Reference 55

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:14.138069Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T00:15:14.138069Z digest=sha256:9ef50973e24bbdf3c1a4c13674472bf6325f0871605a2067ae0c1950b79ee296