Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes | Paper Citation Record

Observation c19bb2d2-94b6-43b8-9368-1340f68e5dd0 · inbound

Computationally efficient models for the dominant and sub-dominant harmonic modes of precessing binary black holes cites this paper.

Computationally efficient models for the dominant and sub-dominant harmonic modes of precessing binary black holes Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 16

Resolution: verified exact; arxiv_id, observed 2026-05-13T21:55:09.201039Z

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 2011418f-3660-4fc3-9395-f89f4f3ec80c · inbound

Tests of General Relativity with Binary Black Holes from the second LIGO-Virgo Gravitational-Wave Transient Catalog cites this paper.

Tests of General Relativity with Binary Black Holes from the second LIGO-Virgo Gravitational-Wave Transient Catalog Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 113

Resolution: verified exact; arxiv_id, observed 2026-05-15T03:47:46.610957Z

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 b9bd80b7-0a6c-49f2-92ac-ec742373277d · inbound

GWTC-2.1: Deep Extended Catalog of Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run cites this paper.

GWTC-2.1: Deep Extended Catalog of Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 57

Resolution: metadata mismatch; arxiv_id, observed 2026-05-16T07:45:53.129259Z

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 fc51ec8c-c38a-4c0a-82f2-3d0ec71e04cf · inbound

Tests of General Relativity with GWTC-3 cites this paper.

Tests of General Relativity with GWTC-3 Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 111

Resolution: verified exact; arxiv_id, observed 2026-05-12T02:40:31.237554Z

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 1b438435-a515-47de-8f00-6d17be664ae1 · inbound

Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors cites this paper.

Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-09T04:46:13.451617Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8f2061d2-85aa-4247-8265-28e2054f8ea7 · 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 Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 153

Resolution: unresolved; no resolver link, observed 2026-08-09T00:23:47.119444Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9a593e32-62df-4b78-87b5-e5bfe0f4628f · inbound

The Long Road to Alignment: Measuring Black Hole Spin Orientation with Expanding Gravitational-Wave Datasets cites this paper.

The Long Road to Alignment: Measuring Black Hole Spin Orientation with Expanding Gravitational-Wave Datasets Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-07T15:36:26.588539Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 434b5903-2b8d-4220-940e-4178e1d0e3cb · inbound

Revisiting GW150914 with a non-planar, eccentric waveform model cites this paper.

Revisiting GW150914 with a non-planar, eccentric waveform model Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 227

Resolution: unresolved; no resolver link, observed 2026-08-07T13:33:33.078496Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 635b56ee-a3ae-4b1a-bece-4a3a7939a243 · inbound

AthenaK simulations of the binary black hole merger GW150914 cites this paper.

AthenaK simulations of the binary black hole merger GW150914 Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-07T05:57:54.249545Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d18ac479-48b0-4d75-aae6-4f8e27e78572 · inbound

Detectability and Parameter Estimation for Einstein Telescope Configurations with GWJulia cites this paper.

Detectability and Parameter Estimation for Einstein Telescope Configurations with GWJulia Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-06T22:29:59.351961Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 46876b2c-f36b-4777-96e2-c3bbe0c96591 · inbound

PhenomXPNR: An improved gravitational wave model linking precessing inspirals and NR-calibrated merger-ringdown cites this paper.

PhenomXPNR: An improved gravitational wave model linking precessing inspirals and NR-calibrated merger-ringdown Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-06T20:31:46.758851Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation de21a5cf-dcd4-4dc8-9bff-c9dcdc48ad44 · 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 Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-06T18:39:46.813290Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 46d9de99-5d61-4947-bfa4-8e291537f465 · inbound

Sampler-free gravitational wave inference using matrix multiplication cites this paper.

Sampler-free gravitational wave inference using matrix multiplication Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-06T15:27:56.750271Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ed1c2596-2466-47ac-afb2-b70ae9aa56a4 · inbound

Coincident morphological transitions in precessing black-hole binaries cites this paper.

Coincident morphological transitions in precessing black-hole binaries Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-05T15:37:37.803709Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ce42c0ba-aae2-4be8-8160-2ee1c25066de · 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 Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 176

Resolution: unresolved; no resolver link, observed 2026-08-05T14:59:58.273430Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7f7948a6-95d0-4280-81fe-c1b8406c5fd4 · inbound

Primordial black holes versus their impersonators at gravitational wave observatories cites this paper.

Primordial black holes versus their impersonators at gravitational wave observatories Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 92

Resolution: verified exact; arxiv_id, observed 2026-05-21T22:15:42.008792Z

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 c8699fb8-bd80-495d-8aa4-14c1c4200d1a · inbound

Neural Post-Einsteinian Test of General Relativity with the Third Gravitational-Wave Transient Catalog cites this paper.

Neural Post-Einsteinian Test of General Relativity with the Third Gravitational-Wave Transient Catalog Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 75

Resolution: verified exact; arxiv_id, observed 2026-05-18T10:11:14.178373Z

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 a16c836e-34c7-4793-9e0b-e907ce7cc030 · inbound

Post-adiabatic self-force waveforms: slowly spinning primary and precessing secondary cites this paper.

Post-adiabatic self-force waveforms: slowly spinning primary and precessing secondary Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 164

Resolution: verified exact; arxiv_id, observed 2026-05-18T05:55:56.976207Z

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 2a8219ed-1f34-4470-be24-658be93784aa · inbound

Accelerated Sequential Posterior Inference via Reuse for Gravitational-Wave Analyses cites this paper.

Accelerated Sequential Posterior Inference via Reuse for Gravitational-Wave Analyses Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-03T23:47:06.014889Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation af9bb469-f4c7-4282-897d-4a809e30bfb1 · inbound

Learning Post-Newtonian Corrections from Numerical Relativity cites this paper.

Learning Post-Newtonian Corrections from Numerical Relativity Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 32

Resolution: verified exact; arxiv_id, observed 2026-05-17T22:35:25.404583Z

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 c7a46f98-1cfd-4781-aa57-7f3c54b168ce · inbound

Gravitational-wave parameter estimation to the Moon and back: massive binaries and the case of GW231123 cites this paper.

Gravitational-wave parameter estimation to the Moon and back: massive binaries and the case of GW231123 Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 63

Resolution: verified exact; arxiv_id, observed 2026-05-16T23:11:20.927957Z

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 182b1f76-e032-44b8-8369-f3b72193271c · inbound

Improved Identification of Strongly Lensed Gravitational Waves with Host Galaxy Locations cites this paper.

Improved Identification of Strongly Lensed Gravitational Waves with Host Galaxy Locations Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 49

Resolution: verified exact; arxiv_id, observed 2026-05-16T23:53:42.969170Z

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 992f7ba6-e7b7-463d-9656-df8d0a5b5063 · inbound

Search for Precessing Binary Black Holes in Advanced LIGO's Third Observing Run using Harmonic Decomposition cites this paper.

Search for Precessing Binary Black Holes in Advanced LIGO's Third Observing Run using Harmonic Decomposition Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 57

Resolution: metadata mismatch; arxiv_id, observed 2026-05-16T16:38:06.263087Z

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 c296eb1e-bbc4-4f23-91c2-8e1f26db0453 · inbound

Systematic biases in parameter estimation on LISA binaries. II. The effect of excluding higher harmonics for spin-aligned, high-mass binaries cites this paper.

Systematic biases in parameter estimation on LISA binaries. II. The effect of excluding higher harmonics for spin-aligned, high-mass binaries Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-03T03:09:41.260470Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a7745f14-5660-4431-9dbe-b895470043c7 · inbound

Extending Ground-Based Gravitational-Wave Sensitivity to 5 Hz cites this paper.

Extending Ground-Based Gravitational-Wave Sensitivity to 5 Hz Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-02T20:21:14.989322Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a77768df-aebc-4c97-92b9-44a719c4bc72 · inbound

Advancing the Effective-One-Body Framework in the Test-Mass Limit cites this paper.

Advancing the Effective-One-Body Framework in the Test-Mass Limit Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 48

Resolution: unresolved; no resolver link, observed 2026-07-15T14:26:35.666160Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9f037e46-026c-4d86-bb76-b79971174fc0 · 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 Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 118

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 358a9063-41d8-435e-9cf0-87bdcbce1f75 · inbound

Fixing the center-of-mass frame of numerical relativity waveforms using the post-Newtonian center-of-mass charge cites this paper.

Fixing the center-of-mass frame of numerical relativity waveforms using the post-Newtonian center-of-mass charge Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-02T17:33:24.545950Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b7ee2d12-ac8e-419f-b9f4-94ebab740645 · inbound

Fixing the center-of-mass frame of numerical relativity waveforms using the post-Newtonian center-of-mass charge cites this paper.

Fixing the center-of-mass frame of numerical relativity waveforms using the post-Newtonian center-of-mass charge Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-04T05:45:47.240257Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 42fdc5f0-ebba-4ec4-bbc4-209c0e5b5d34 · inbound

Secular evolution of orbital parameters for general bound orbits in Kerr spacetime cites this paper.

Secular evolution of orbital parameters for general bound orbits in Kerr spacetime Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-03T02:30:58.784881Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 40866a6d-c8b3-4d7b-ae53-478dd44526ba · inbound

Not too close! Evaluating the impact of the baseline on the localization of binary black holes by next-generation gravitational-wave detectors cites this paper.

Not too close! Evaluating the impact of the baseline on the localization of binary black holes by next-generation gravitational-wave detectors Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 98

Resolution: verified exact; arxiv_id, observed 2026-05-11T10:31:02.338221Z

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 5548f16e-cde5-437c-83c5-b5296ea45156 · 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 Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 124

Resolution: verified exact; arxiv_id, observed 2026-05-10T15:00:31.067162Z

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 8500bcae-1c9f-4390-a227-1004cd92c09a · inbound

Lessons from binary dynamics of inspiralling equal-mass boson-star mergers cites this paper.

Lessons from binary dynamics of inspiralling equal-mass boson-star mergers Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 83

Resolution: verified exact; arxiv_id, observed 2026-05-12T00:31:15.562000Z

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 e3e8b3eb-fb9b-4461-a41f-c299b1591cf7 · inbound

GW240925 and GW250207: Astrophysical Calibration of Gravitational-wave Detectors cites this paper.

GW240925 and GW250207: Astrophysical Calibration of Gravitational-wave Detectors Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 211

Resolution: verified exact; arxiv_id, observed 2026-05-13T05:32:19.858700Z

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 1a8686ec-276f-4b9c-bcf0-ee70d4ce262f · 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 Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 64

Resolution: verified exact; arxiv_id, observed 2026-07-02T09:26:51.264787Z

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 a62f41b2-c194-4967-9d48-68733dcfbc04 · 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 Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-03T02:15:33.497750Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 77e00a47-fdae-4bc0-af61-da16860acfd5 · 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 Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 145

Resolution: verified exact; arxiv_id, observed 2026-07-03T11:48:04.665320Z

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 2277b71b-436b-422a-8dac-8267386084e5 · inbound

Joint inference of line-of-sight acceleration and orbital eccentricity in neutron-star--black-hole binaries cites this paper.

Joint inference of line-of-sight acceleration and orbital eccentricity in neutron-star--black-hole binaries Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 117

Resolution: verified exact; arxiv_id, observed 2026-07-01T17:35:52.327080Z

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 1bf0bc03-27d6-4be3-8e39-1c04eed0823b · 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 Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 154

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 a675a45e-c32c-49c4-9fd2-125113b29f25 · 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 Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-01T07:26:22.934566Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2367315e-bacd-4caa-bb13-e4530a36e3e1 · inbound

Gravitational Wave Modeling of White-Dwarf--Compact-Object Binaries and Observational Outlook cites this paper.

Gravitational Wave Modeling of White-Dwarf--Compact-Object Binaries and Observational Outlook Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 173

Resolution: unresolved; no resolver link, observed 2026-07-31T05:12:17.525150Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation dbbd2065-e255-4c95-8045-a83bf381e6b4 · 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 Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 197

Resolution: unresolved; no resolver link, observed 2026-07-31T07:22:45.999957Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 85e13eed-2cd9-45ce-aa8b-334eaff9854c · 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 Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-04T21:28:07.543971Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cedbd7cc-4df8-4b7c-9a3b-e55d6e6bb8e2 · 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 Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-07T00:15:14.223991Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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