Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
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 20 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.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-20T06:33:59.587034+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-11T19:45:10.261693Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-06-30T16:24:59.091894Z
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 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 2026-08-20T06:33:59.587034+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 2026-08-20T06:33:59.587034+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 2026-08-20T06:33:59.587034+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 2026-08-20T06:33:59.587034+00:00.