Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
New and Robust Gravitational-Waveform Model for High-Mass-Ratio Binary Neutron Star Systems with Dynamical Tidal Effects
As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 21 inbound Pith citation observations for arXiv:2311.07456.
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 2026-08-17T06:30:58.91139+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-16T05:25:17.590113Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-02T09:26:51.292902Z
Reference resolution
0 of 0 outbound references displayed
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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 62dee2c3-82d1-439c-a3c2-da171a4e8451 · inbound
Tidal contributions to the full gravitational waveform to the second-and-a-half post-Newtonian order cites this paper.
Tidal contributions to the full gravitational waveform to the second-and-a-half post-Newtonian order New and Robust Gravitational-Waveform Model for High-Mass-Ratio Binary Neutron Star Systems with Dynamical Tidal Effects
Reference 91
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T12:28:44.158285Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f9f7c941-33bc-468b-b4e1-6505822c7714 · inbound
Fast frequency-domain gravitational waveforms for precessing binaries with a new twist cites this paper.
Fast frequency-domain gravitational waveforms for precessing binaries with a new twist New and Robust Gravitational-Waveform Model for High-Mass-Ratio Binary Neutron Star Systems with Dynamical Tidal Effects
Reference 68
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T10:24:53.479104Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 2434fd75-f47c-4ce2-957b-bd009cceb80d · inbound
Data-driven approach for extracting tidal information from neutron star binary mergers observed with the Einstein Telescope cites this paper.
Data-driven approach for extracting tidal information from neutron star binary mergers observed with the Einstein Telescope New and Robust Gravitational-Waveform Model for High-Mass-Ratio Binary Neutron Star Systems with Dynamical Tidal Effects
Reference 48
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:21:20.681696Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e0e778f6-a096-4b87-a7b7-eb6f75620bce · 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 New and Robust Gravitational-Waveform Model for High-Mass-Ratio Binary Neutron Star Systems with Dynamical Tidal Effects
Reference 31
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T16:33:19.685904Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b04ec0a7-d1ee-461a-8c1b-1fbf410e1407 · inbound
Numerical Relativity Simulations of Dark Matter Admixed Binary Neutron Stars cites this paper.
Numerical Relativity Simulations of Dark Matter Admixed Binary Neutron Stars New and Robust Gravitational-Waveform Model for High-Mass-Ratio Binary Neutron Star Systems with Dynamical Tidal Effects
Reference 103
- Resolution
- unresolved
- no resolver link, observed 2026-08-16T05:25:17.590113Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d20d801a-1370-4468-ad4e-701757f9edd1 · inbound
The error budget of binary neutron star merger simulations for configurations with high spin cites this paper.
The error budget of binary neutron star merger simulations for configurations with high spin New and Robust Gravitational-Waveform Model for High-Mass-Ratio Binary Neutron Star Systems with Dynamical Tidal Effects
Reference 68
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T11:40:12.025820Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 347b953f-3fa9-429b-97d2-1104a0765768 · inbound
Detectability and Parameter Estimation for Einstein Telescope Configurations with GWJulia cites this paper.
Detectability and Parameter Estimation for Einstein Telescope Configurations with GWJulia New and Robust Gravitational-Waveform Model for High-Mass-Ratio Binary Neutron Star Systems with Dynamical Tidal Effects
Reference 101
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:30:00.423514Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ab01a202-f0a5-41b9-9833-700313b133b8 · inbound
Binary black holes in the heat of merger cites this paper.
Binary black holes in the heat of merger New and Robust Gravitational-Waveform Model for High-Mass-Ratio Binary Neutron Star Systems with Dynamical Tidal Effects
Reference 33
- Resolution
- verified exact
- arxiv_id, observed 2026-05-19T07:52:09.604698Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.
Observation 53200723-29b2-479d-9aeb-d1e037b78bb0 · inbound
A case study of GW190425 for classifying binary neutron star versus binary black hole mergers and constraining asymmetric dark matter with gravitational wave detectors cites this paper.
A case study of GW190425 for classifying binary neutron star versus binary black hole mergers and constraining asymmetric dark matter with gravitational wave detectors New and Robust Gravitational-Waveform Model for High-Mass-Ratio Binary Neutron Star Systems with Dynamical Tidal Effects
Reference 46
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T18:39:46.886105Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8feee1ee-0d7f-4300-be5c-321684d6515c · inbound
Upper Limits on the Isotropic Gravitational-Wave Background from the first part of LIGO, Virgo, and KAGRA's fourth Observing Run cites this paper.
Upper Limits on the Isotropic Gravitational-Wave Background from the first part of LIGO, Virgo, and KAGRA's fourth Observing Run New and Robust Gravitational-Waveform Model for High-Mass-Ratio Binary Neutron Star Systems with Dynamical Tidal Effects
Reference 178
- Resolution
- unresolved
- no resolver link, observed 2026-08-05T14:59:58.278166Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 1860b89d-b9b7-4b9a-899a-4b38971f169b · inbound
Inferring neutron-star Love-Q relations from gravitational waves in the hierarchical Bayesian framework cites this paper.
Inferring neutron-star Love-Q relations from gravitational waves in the hierarchical Bayesian framework New and Robust Gravitational-Waveform Model for High-Mass-Ratio Binary Neutron Star Systems with Dynamical Tidal Effects
Reference 18
- Resolution
- verified exact
- arxiv_id, observed 2026-05-18T05:05:55.480707Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.
Observation f4d15679-d12e-4794-a9c1-77c27ed13d3b · inbound
Auto-encoder model for faster generation of effective one-body gravitational waveform approximations cites this paper.
Auto-encoder model for faster generation of effective one-body gravitational waveform approximations New and Robust Gravitational-Waveform Model for High-Mass-Ratio Binary Neutron Star Systems with Dynamical Tidal Effects
Reference 24
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T22:10:22.920609Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.
Observation 5b784e87-49dc-41b0-b703-ffdd2111e364 · inbound
Toward a Unified Understanding of the Dense Matter Equation of State cites this paper.
Toward a Unified Understanding of the Dense Matter Equation of State New and Robust Gravitational-Waveform Model for High-Mass-Ratio Binary Neutron Star Systems with Dynamical Tidal Effects
Reference 258
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T20:20:20.130665Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9b67f5e5-16b0-4e90-be6c-4a50ee2f689e · inbound
Fast gravitational waveform models for quasi-circular coalescences of neutron star--black hole binaries cites this paper.
Fast gravitational waveform models for quasi-circular coalescences of neutron star--black hole binaries New and Robust Gravitational-Waveform Model for High-Mass-Ratio Binary Neutron Star Systems with Dynamical Tidal Effects
Reference 67
- Resolution
- verified exact
- arxiv_id, observed 2026-07-02T09:26:51.294375Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.
Observation 7f15a9d2-3726-45e1-8f8c-156d9befb39e · inbound
Fast gravitational waveform models for quasi-circular coalescences of neutron star--black hole binaries cites this paper.
Fast gravitational waveform models for quasi-circular coalescences of neutron star--black hole binaries New and Robust Gravitational-Waveform Model for High-Mass-Ratio Binary Neutron Star Systems with Dynamical Tidal Effects
Reference 67
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T02:15:33.894257Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f6db25d3-3a04-4c0c-8ef2-33d0f73c09e8 · inbound
Quadrupole and quadratic-in-spin effects in quasicircular, spinning, asymmetric binaries cites this paper.
Quadrupole and quadratic-in-spin effects in quasicircular, spinning, asymmetric binaries New and Robust Gravitational-Waveform Model for High-Mass-Ratio Binary Neutron Star Systems with Dynamical Tidal Effects
Reference 48
- Resolution
- verified exact
- arxiv_id, observed 2026-06-30T09:04:32.363986Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.
Observation f0a152e5-e776-4a56-a0a8-3462a57fdf1f · inbound
nmma: An extended Bayesian framework for Nuclear Multimessenger Astronomy in the Era of Next-Generation Detectors cites this paper.
nmma: An extended Bayesian framework for Nuclear Multimessenger Astronomy in the Era of Next-Generation Detectors New and Robust Gravitational-Waveform Model for High-Mass-Ratio Binary Neutron Star Systems with Dynamical Tidal Effects
Reference 3
- Resolution
- unresolved
- no resolver link, observed 2026-07-12T05:14:58.841553Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 46efc36c-e164-42ee-a071-6cb85b94d472 · inbound
A story about a tipsy kangaroo: Reversible jump MCMC for model selection in the analysis of gravitational-wave signals from the coalescence of compact objects cites this paper.
A story about a tipsy kangaroo: Reversible jump MCMC for model selection in the analysis of gravitational-wave signals from the coalescence of compact objects New and Robust Gravitational-Waveform Model for High-Mass-Ratio Binary Neutron Star Systems with Dynamical Tidal Effects
Reference 86
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T07:26:23.177261Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 898a80d6-ba72-4f16-8b12-b4d6c005a288 · inbound
Binary neutron stars in the next-generation era: Multi-messenger detection prospects and constraints on the equation of state, mass distribution, and cosmology cites this paper.
Binary neutron stars in the next-generation era: Multi-messenger detection prospects and constraints on the equation of state, mass distribution, and cosmology New and Robust Gravitational-Waveform Model for High-Mass-Ratio Binary Neutron Star Systems with Dynamical Tidal Effects
Reference 1
- Resolution
- unresolved
- no resolver link, observed 2026-07-31T07:22:45.390607Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation cee134bd-dabc-4ef9-8b87-eb2cbdadaaaf · inbound
From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State cites this paper.
From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State New and Robust Gravitational-Waveform Model for High-Mass-Ratio Binary Neutron Star Systems with Dynamical Tidal Effects
Reference 6
- Resolution
- malformed identifier
- no resolver link, observed 2026-08-08T00:43:18.938178Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ffcb4d6b-ef7b-4287-be25-610b89126557 · inbound
LIGO A$^\sharp$: Detector Design and Science Prospects Beyond A+ cites this paper.
LIGO A$^\sharp$: Detector Design and Science Prospects Beyond A+ New and Robust Gravitational-Waveform Model for High-Mass-Ratio Binary Neutron Star Systems with Dynamical Tidal Effects
Reference 206
- Resolution
- unresolved
- no resolver link, observed 2026-08-16T00:36:34.801259Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.