Paper Citation Record · LEDGER

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates

As of 21 August 2026, this Paper Citation Record lists 100 of 134 outbound references and 4 inbound Pith citation observations for arXiv:2510.00116.

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

pith.paper-citation-record.v1
2510.00116 v3

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measured 100 of 134 reference resolution

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Source: paper_references, paper_reference_links, observed 2026-08-04T13:34:57.568224Z

measured 104 of 104 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-21T06:32:19.484+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-06-30T04:42:30.728872Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-06-30T16:24:59.325333Z

Reference resolution

100 of 134 outbound references displayed

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Outbound references

Observation 5e74c1c8-44ab-4ff5-b8d9-cefa8cc32b8f · outbound

This paper cites GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:51.654169Z

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Observation 31c1747d-50a9-4011-82d3-321ac68bd7d5 · outbound

This paper cites GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:51.707550Z

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Observation 7e95d3e4-42c8-4dd0-82eb-5064c5a751ca · outbound

This paper cites GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:51.836437Z

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Observation 5fc56e35-dc18-42bd-91b7-a5dfe4417aa9 · outbound

This paper cites GWTC-4.0: Updating the Gravitational-Wave Transient Catalog with Observations from the First Part of the Fourth LIGO-Virgo-KAGRA Observing Run.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates GWTC-4.0: Updating the Gravitational-Wave Transient Catalog with Observations from the First Part of the Fourth LIGO-Virgo-KAGRA Observing Run

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:51.961186Z

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Observation 0849a58c-467a-48d2-8dec-7ed8916665ca · outbound

This paper cites Binary Black Hole Population Properties Inferred from the First and Second Observing Runs of Advanced LIGO and Advanced Virgo.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Binary Black Hole Population Properties Inferred from the First and Second Observing Runs of Advanced LIGO and Advanced Virgo

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:52.029456Z

Source-reported events for the cited work

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Observation ddca6b6a-a126-42ab-b52b-888a81179218 · outbound

This paper cites Population Properties of Compact Objects from the Second LIGO-Virgo Gravitational-Wave Transient Catalog.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Population Properties of Compact Objects from the Second LIGO-Virgo Gravitational-Wave Transient Catalog

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:52.103731Z

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Observation 66656eed-0b07-41ae-a490-492e9533eba7 · outbound

This paper cites The population of merging compact binaries inferred using gravitational waves through GWTC-3.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates The population of merging compact binaries inferred using gravitational waves through GWTC-3

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:52.185330Z

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Observation cf3d129a-8906-42d3-9ef8-d1a1279b6cbd · outbound

This paper cites GWTC-4.0: Population Properties of Merging Compact Binaries.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates GWTC-4.0: Population Properties of Merging Compact Binaries

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:52.240466Z

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Observation a1f04394-901e-4859-8615-310ac4ab17be · outbound

This paper cites The Evolution of Compact Binary Star Systems.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates The Evolution of Compact Binary Star Systems

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:52.292438Z

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Observation c8d5dd8d-a2fe-4121-8f87-3326ee28bab0 · outbound

This paper cites an unresolved cited work.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Unresolved cited work

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:52.358898Z

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Observation 77de7bec-38eb-4858-9486-22a56de7e177 · outbound

This paper cites Three-Body Dynamics with Gravitational Wave Emission.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Three-Body Dynamics with Gravitational Wave Emission

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:52.425354Z

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Observation 125d8f36-9fc7-4ff8-b6f5-67f6eb1156fa · outbound

This paper cites The Formation of Eccentric Compact Binary Inspirals and the Role of Gravitational Wave Emission in Binary-Single Stellar Encounters.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates The Formation of Eccentric Compact Binary Inspirals and the Role of Gravitational Wave Emission in Binary-Single Stellar Encounters

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:52.545391Z

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Observation fc77ab57-42cb-45fe-ae47-1e7d7628d5e6 · outbound

This paper cites Black hole mergers and blue stragglers from hierarchical triples formed in globular clusters.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Black hole mergers and blue stragglers from hierarchical triples formed in globular clusters

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:52.660508Z

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Observation bd652c7d-6d7e-47df-8819-def66df2e78f · outbound

This paper cites On the Assembly Rate of Highly Eccentric Binary Black Hole Mergers.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates On the Assembly Rate of Highly Eccentric Binary Black Hole Mergers

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:52.823482Z

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Observation 73ab0143-372f-4c2a-ace2-edbb71140c43 · outbound

This paper cites Post-Newtonian Dynamics in Dense Star Clusters: Highly-Eccentric, Highly-Spinning, and Repeated Binary Black Hole Mergers.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Post-Newtonian Dynamics in Dense Star Clusters: Highly-Eccentric, Highly-Spinning, and Repeated Binary Black Hole Mergers

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:52.937544Z

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Observation bd3a356a-e983-4607-9ea3-8b6bd0d04f55 · outbound

This paper cites Eccentric Black Hole Mergers in Dense Star Clusters: The Role of Binary-Binary Encounters.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Eccentric Black Hole Mergers in Dense Star Clusters: The Role of Binary-Binary Encounters

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:53.042973Z

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Observation bc5f2ffc-1f0c-466c-871f-ba6f761bc287 · outbound

This paper cites AGN as Potential Factories for Eccentric Black Hole Mergers.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates AGN as Potential Factories for Eccentric Black Hole Mergers

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:53.153641Z

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Observation 60cbd2c7-756f-49c2-aeb1-ea22c6445dcb · outbound

This paper cites Eccentric Mergers in AGN Discs: Influence of the Supermassive Black-Hole on Three-body Interactions.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Eccentric Mergers in AGN Discs: Influence of the Supermassive Black-Hole on Three-body Interactions

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:53.253721Z

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Observation d0835472-f2ca-4b99-8e47-dba2192288d5 · outbound

This paper cites Gravitational Wave Phase Shifts in Eccentric Black Hole Mergers as a Probe of Dynamical Formation Environments.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Gravitational Wave Phase Shifts in Eccentric Black Hole Mergers as a Probe of Dynamical Formation Environments

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:53.367189Z

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Observation d87bf0a6-4b69-4594-9f6e-7bebd5a5e1ef · outbound

This paper cites Kozai, Secular perturbations of asteroids with high inclination and eccentricity, Astron.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Kozai, Secular perturbations of asteroids with high inclination and eccentricity, Astron

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:53.467631Z

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Observation d642d4e0-da13-432d-b02a-64d6edcbfe2c · outbound

This paper cites an unresolved cited work.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Unresolved cited work

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:53.585187Z

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Observation c7d9869e-299d-4385-9c72-a8063037ad1a · outbound

This paper cites Implications of Eccentric Observations on Binary Black Hole Formation Channels.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Implications of Eccentric Observations on Binary Black Hole Formation Channels

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:53.725443Z

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Observation 71b36e39-9e1b-44a4-8388-92abda21ff91 · outbound

This paper cites Measuring eccentricity of binary black holes in GWTC-1 by using inspiral-only waveform.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Measuring eccentricity of binary black holes in GWTC-1 by using inspiral-only waveform

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:53.838034Z

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Observation 49b666a8-8d1a-481e-b449-7b892bc2d8d8 · outbound

This paper cites Signs of eccentricity in two gravitational-wave signals may indicate a sub-population of dynamically assembled binary black holes.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Signs of eccentricity in two gravitational-wave signals may indicate a sub-population of dynamically assembled binary black holes

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:53.933979Z

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Observation d33976c8-901b-4313-9a3f-6a38a2d92c2c · outbound

This paper cites Four eccentric mergers increase the evidence that LIGO--Virgo--KAGRA's binary black holes form dynamically.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Four eccentric mergers increase the evidence that LIGO--Virgo--KAGRA's binary black holes form dynamically

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:54.099807Z

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Observation 000559b6-59f4-413b-90f6-2c20fd79ce20 · outbound

This paper cites GW190521: orbital eccentricity and signatures of dynamical formation in a binary black hole merger signal.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates GW190521: orbital eccentricity and signatures of dynamical formation in a binary black hole merger signal

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:54.216236Z

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Observation 310833ca-4440-4d20-af85-d31627f19865 · outbound

This paper cites Eccentricity Estimate for Black Hole Mergers with Numerical Relativity Simulations.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Eccentricity Estimate for Black Hole Mergers with Numerical Relativity Simulations

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:54.269920Z

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Observation 1184af96-fe21-446f-86c7-b19638ead491 · outbound

This paper cites Evidence for eccentricity in the population of binary black holes observed by LIGO-Virgo-KAGRA.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Evidence for eccentricity in the population of binary black holes observed by LIGO-Virgo-KAGRA

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:54.349877Z

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Observation b7504361-30ee-4904-9c0c-de50ff705914 · outbound

This paper cites an unresolved cited work.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Unresolved cited work

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:54.428691Z

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Observation 57f54bd9-9635-4533-8c94-2365d4a1c118 · outbound

This paper cites Morras, G.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Morras, G

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:54.512855Z

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Observation 3eb6921d-8e93-4e01-b081-ba7cd6af352e · outbound

This paper cites an unresolved cited work.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Unresolved cited work

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:54.585358Z

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Observation 7df5dd3a-7940-40fd-bced-a7b68c4afbf4 · outbound

This paper cites Kacanja, K.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Kacanja, K

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:54.669716Z

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Observation 40d19669-3183-4b62-94cf-de7aecdf852a · outbound

This paper cites Jan, B.-J.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Jan, B.-J

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:54.724581Z

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Observation ca25899e-53b9-4aba-b2bb-658fd789c713 · outbound

This paper cites Laser Interferometer Space Antenna.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Laser Interferometer Space Antenna

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:54.800348Z

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Observation 4cc75258-78d9-4698-a138-0b8717cef0b2 · outbound

This paper cites Punturoet al., The Einstein Telescope: A third-generation gravitational wave observatory, Class.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Punturoet al., The Einstein Telescope: A third-generation gravitational wave observatory, Class

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:54.876846Z

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Observation 11b80703-4ecb-45c6-84dc-475415c1e629 · outbound

This paper cites Beyond the Second Generation of Laser-Interferometric Gravitational Wave Observatories.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Beyond the Second Generation of Laser-Interferometric Gravitational Wave Observatories

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:54.934013Z

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Observation d38c53ea-c509-47ec-873b-bf7862e93de1 · outbound

This paper cites Cosmic Explorer: The U.S. Contribution to Gravitational-Wave Astronomy beyond LIGO.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Cosmic Explorer: The U.S. Contribution to Gravitational-Wave Astronomy beyond LIGO

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:54.987019Z

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Observation 0ea5f647-aad8-4e10-bb20-269b47b3d4e1 · outbound

This paper cites Exploring the Sensitivity of Next Generation Gravitational Wave Detectors.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Exploring the Sensitivity of Next Generation Gravitational Wave Detectors

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:55.060728Z

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Observation 894e9cd3-f94a-4ed2-9186-9b6959b53fc9 · outbound

This paper cites Resolving the eccentricity of stellar mass binary black holes with next generation ground-based gravitational wave detectors.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Resolving the eccentricity of stellar mass binary black holes with next generation ground-based gravitational wave detectors

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:55.111152Z

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Observation 0d852f7e-454d-41a7-90b1-1cb699566e20 · outbound

This paper cites Post-Circular Expansion of Eccentric Binary Inspirals: Fourier-Domain Waveforms in the Stationary Phase Approximation.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Post-Circular Expansion of Eccentric Binary Inspirals: Fourier-Domain Waveforms in the Stationary Phase Approximation

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:55.182245Z

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Observation abbe9006-874b-4587-bbf8-3802699873a2 · outbound

This paper cites Computing waveforms for spinning compact binaries in quasi-eccentric orbits.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Computing waveforms for spinning compact binaries in quasi-eccentric orbits

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:55.239192Z

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Observation 8966296d-bcd7-4cc0-a9e7-8349574c35d9 · outbound

This paper cites Characterizing Spinning Black Hole Binaries in Eccentric Orbits with LISA.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Characterizing Spinning Black Hole Binaries in Eccentric Orbits with LISA

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:55.308151Z

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Observation b8a89484-5fbe-4570-b933-1d5a698ac470 · outbound

This paper cites Accurate and efficient waveforms for compact binaries on eccentric orbits.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Accurate and efficient waveforms for compact binaries on eccentric orbits

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:55.362067Z

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Observation 9a5152cf-9bfa-4c57-aa01-635c1fe8d3ef · outbound

This paper cites Frequency and time domain inspiral templates for comparable mass compact binaries in eccentric orbits.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Frequency and time domain inspiral templates for comparable mass compact binaries in eccentric orbits

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:55.435489Z

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Observation 455e2181-ffbf-4e75-b348-99e6595bd569 · outbound

This paper cites Eccentric Gravitational Wave Bursts in the Post-Newtonian Formalism.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Eccentric Gravitational Wave Bursts in the Post-Newtonian Formalism

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:55.525089Z

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Unavailable: canonical work link unavailable.

Observation ad47d3e5-25de-45ad-9d2e-ae514b490165 · outbound

This paper cites Ready-to-use Fourier domain templates for compact binaries inspiraling along moderately eccentric orbits.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Ready-to-use Fourier domain templates for compact binaries inspiraling along moderately eccentric orbits

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:55.527770Z

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Observation 11c404e2-7983-4f14-87e3-801bb48ac738 · outbound

This paper cites Combining Post-Circular and Pad\'e approximations to compute Fourier domain templates for eccentric inspirals.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Combining Post-Circular and Pad\'e approximations to compute Fourier domain templates for eccentric inspirals

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:55.612071Z

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Observation 59af31c0-7c7a-46e3-989a-a2c7efc439fa · outbound

This paper cites A Fourier Domain Waveform for Non-Spinning Binaries with Arbitrary Eccentricity.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates A Fourier Domain Waveform for Non-Spinning Binaries with Arbitrary Eccentricity

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:55.759969Z

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Observation b7bb8774-c292-4ce7-8d9e-34715a4d60f5 · outbound

This paper cites A 3PN Fourier Domain Waveform for Non-Spinning Binaries with Moderate Eccentricity.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates A 3PN Fourier Domain Waveform for Non-Spinning Binaries with Moderate Eccentricity

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:55.871988Z

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Observation f4258e99-c46d-47b7-9541-4f955638294a · outbound

This paper cites Spin effects in the phasing formula of eccentric compact binary inspirals up to the third post-Newtonian order.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Spin effects in the phasing formula of eccentric compact binary inspirals up to the third post-Newtonian order

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:56.019522Z

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Observation e58be8c1-7794-4424-a64a-97acf27e8fcc · outbound

This paper cites Fourier domain gravitational waveforms for precessing eccentric binaries.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Fourier domain gravitational waveforms for precessing eccentric binaries

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:56.092402Z

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Observation c5eef553-fe55-4d9d-8f35-0e061e86e890 · outbound

This paper cites EFPE: Efficient fully precessing eccentric gravitational waveforms for binaries with long inspirals.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates EFPE: Efficient fully precessing eccentric gravitational waveforms for binaries with long inspirals

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:56.201175Z

Source-reported events for the cited work

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Observation d62630ab-af13-407c-8ef5-8a5eb652fc5e · outbound

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

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Improved post-Newtonian waveform model for inspiralling precessing-eccentric compact binaries

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:56.306053Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9bbf15a0-6aaa-46d8-956a-a3a29e88c59c · outbound

This paper cites Complete waveform model for compact binaries on eccentric orbits.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Complete waveform model for compact binaries on eccentric orbits

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:56.467871Z

Source-reported events for the cited work

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Observation c56e071c-d060-4577-a510-cfc3ec4d5c8b · outbound

This paper cites Eccentric, nonspinning, inspiral, Gaussian-process merger approximant for the detection and characterization of eccentric binary black hole mergers.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Eccentric, nonspinning, inspiral, Gaussian-process merger approximant for the detection and characterization of eccentric binary black hole mergers

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:56.632022Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 689f4a2f-fe05-4ad6-a0dc-f4d1411d2112 · outbound

This paper cites Observation of eccentric binary black hole mergers with second and third generation gravitational wave detector networks.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Observation of eccentric binary black hole mergers with second and third generation gravitational wave detector networks

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:56.795778Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a4fb8941-cb4e-42ba-92ca-4cd08d5db78d · outbound

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

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 59147f90-f21e-4993-b3e5-cc3fae853169 · outbound

This paper cites An eccentric binary black hole inspiral-merger-ringdown gravitational waveform model from numerical relativity and post-Newtonian theory.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates An eccentric binary black hole inspiral-merger-ringdown gravitational waveform model from numerical relativity and post-Newtonian theory

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.071601Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a1973d9e-7e83-432d-8ad5-e6bd4b5b3ad4 · outbound

This paper cites High accuracy post-Newtonian and numerical relativity comparisons involving higher modes for eccentric binary black holes and a dominant mode eccentric inspiral-merger-ringdown model.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates High accuracy post-Newtonian and numerical relativity comparisons involving higher modes for eccentric binary black holes and a dominant mode eccentric inspiral-merger-ringdown model

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.228368Z

Source-reported events for the cited work

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Observation d704dd64-d2b4-46b2-a6e2-ff684e6fc72c · outbound

This paper cites Improved inspiral-merger-ringdown model for BBHs on elliptical orbits.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Improved inspiral-merger-ringdown model for BBHs on elliptical orbits

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.248869Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 279920c9-f550-4aff-8bb1-25d382ab5fe3 · outbound

This paper cites A waveform model for eccentric binary black hole based on effective-one-body-numerical-relativity (EOBNR) formalism.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates A waveform model for eccentric binary black hole based on effective-one-body-numerical-relativity (EOBNR) formalism

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.264394Z

Source-reported events for the cited work

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Observation 0a0309fd-35c9-4c2b-9d83-ba8c6555c7d8 · outbound

This paper cites Validating the Effective-One-Body Numerical-Relativity Waveform Models for Spin-aligned Binary Black Holes along Eccentric Orbits.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Validating the Effective-One-Body Numerical-Relativity Waveform Models for Spin-aligned Binary Black Holes along Eccentric Orbits

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.362549Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 33e2ef81-47c2-4f12-ac37-9f22e1bb5ad6 · outbound

This paper cites A higher-multipole gravitational waveform model for an eccentric binary black holes based on the effective-one-body-numerical-relativity formalism.

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

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Observation e7409c41-1138-4217-9668-2005d2c2721a · outbound

This paper cites Upgraded waveform model of eccentric binary black hole based on effective-one-body-numerical-relativity for spin-aligned binary black holes.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Upgraded waveform model of eccentric binary black hole based on effective-one-body-numerical-relativity for spin-aligned binary black holes

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.460266Z

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Observation 23e543e7-2ea7-491c-9f37-654a5dd6a97e · outbound

This paper cites A faithful analytical effective one body waveform model for spin-aligned, moderately eccentric, coalescing black hole binaries.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates A faithful analytical effective one body waveform model for spin-aligned, moderately eccentric, coalescing black hole binaries

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.471072Z

Source-reported events for the cited work

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Observation 0d7b3bef-79ca-430d-b5eb-f9982b2dcac9 · outbound

This paper cites Effective one body multipolar waveform model for spin-aligned, quasi-circular, eccentric, hyperbolic black hole binaries.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Effective one body multipolar waveform model for spin-aligned, quasi-circular, eccentric, hyperbolic black hole binaries

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.474025Z

Source-reported events for the cited work

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Observation 75159722-682a-45a4-a645-5540115cf620 · outbound

This paper cites Towards efficient Effective One Body models for generic, non-planar orbits.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Towards efficient Effective One Body models for generic, non-planar orbits

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.476725Z

Source-reported events for the cited work

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Observation 0cc6b648-e630-4602-96d8-729ad571b7e9 · outbound

This paper cites Effective-one-body waveform model for non-circularized, planar, coalescing black hole binaries: the importance of radiation reaction.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Effective-one-body waveform model for non-circularized, planar, coalescing black hole binaries: the importance of radiation reaction

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.479759Z

Source-reported events for the cited work

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Observation 4e6b2a5b-51c8-4d46-b63c-54a21654a30e · outbound

This paper cites Effective-one-body multipolar waveforms for eccentric binary black holes with non-precessing spins.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Effective-one-body multipolar waveforms for eccentric binary black holes with non-precessing spins

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.482596Z

Source-reported events for the cited work

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Observation 3fdf6fc4-c112-4dfb-9d14-d4c50d165675 · outbound

This paper cites Accurate waveforms for eccentric, aligned-spin binary black holes: The multipolar effective-one-body model SEOBNRv5EHM.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Accurate waveforms for eccentric, aligned-spin binary black holes: The multipolar effective-one-body model SEOBNRv5EHM

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.485879Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ae39407f-48cb-4535-8926-7c8070d4d5fe · outbound

This paper cites an unresolved cited work.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Unresolved cited work

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.488722Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 19e56e2b-27e7-4d11-a506-b549ab13994b · outbound

This paper cites Adding eccentricity to quasicircular binary-black-hole waveform models.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Adding eccentricity to quasicircular binary-black-hole waveform models

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.491129Z

Source-reported events for the cited work

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Observation 84c4281f-b251-4c48-9c60-049d692eb487 · outbound

This paper cites Phenomenological relationship between eccentric and quasi-circular orbital binary black hole waveform.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Phenomenological relationship between eccentric and quasi-circular orbital binary black hole waveform

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.493637Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5543a8d2-73e1-48ff-809e-48e4aba7928c · outbound

This paper cites Study of eccentric binary black hole mergers using numerical relativity and an inspiral-merger-ringdown model.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Study of eccentric binary black hole mergers using numerical relativity and an inspiral-merger-ringdown model

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.496499Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e77ed226-5d9e-4533-b58d-4622e32600fa · outbound

This paper cites Universal phenomenological relations between spherical harmonic modes in non-precessing eccentric binary black hole merger waveforms.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Universal phenomenological relations between spherical harmonic modes in non-precessing eccentric binary black hole merger waveforms

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.499160Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4548bdb2-cd7a-4b09-9e5b-f5e739bc73bf · outbound

This paper cites Adding higher-order spherical harmonics in non-spinning eccentric binary black hole merger waveform models.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Adding higher-order spherical harmonics in non-spinning eccentric binary black hole merger waveform models

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.502089Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a2483f19-1a72-442f-953e-4effc9932955 · outbound

This paper cites an unresolved cited work.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Unresolved cited work

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.504739Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9eafcd80-399e-4545-8009-bfa7bc179494 · outbound

This paper cites Sacks, W.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Sacks, W

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.507799Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 87fa37fc-6139-409f-9c25-05e8f4bafc9d · outbound

This paper cites an unresolved cited work.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Unresolved cited work

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.510815Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8ff9aadc-1dde-4e3b-b364-ee5eb7d97ffd · outbound

This paper cites an unresolved cited work.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Unresolved cited work

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.513437Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6500c59f-bf4d-45d1-b1e2-50fd4b917e73 · outbound

This paper cites an unresolved cited work.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Unresolved cited work

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.515944Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fce0276f-6c56-41a2-b5e0-9c7489d3bd9a · outbound

This paper cites Fast prediction and evaluation of gravitational waveforms using surrogate models.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Fast prediction and evaluation of gravitational waveforms using surrogate models

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.518178Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 308b8c3c-8066-4212-980f-3ff3db2c9255 · outbound

This paper cites Frequency domain reduced order models for gravitational waves from aligned-spin compact binaries.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Frequency domain reduced order models for gravitational waves from aligned-spin compact binaries

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.520938Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5bc584b6-68cd-4da7-aed4-c6900e232f6f · outbound

This paper cites Frequency domain reduced order model of aligned-spin effective-one-body waveforms with generic mass-ratios and spins.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Frequency domain reduced order model of aligned-spin effective-one-body waveforms with generic mass-ratios and spins

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.523431Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 37082aac-a4ee-4625-811c-62dc59c8a7e1 · outbound

This paper cites Effective-one-body waveforms for binary neutron stars using surrogate models.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Effective-one-body waveforms for binary neutron stars using surrogate models

Reference 85

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.526031Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3b56e64f-1a27-4b20-8b96-fb502b34b758 · outbound

This paper cites Surrogate model for an aligned-spin effective one body waveform model of binary neutron star inspirals using Gaussian process regression.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Surrogate model for an aligned-spin effective one body waveform model of binary neutron star inspirals using Gaussian process regression

Reference 86

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.529170Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e545d1fd-91cd-4005-b414-c328ce317807 · outbound

This paper cites Frequency domain reduced order model of aligned-spin effective-one-body waveforms with higher-order modes.

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.531587Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c3b32d6c-8d6d-46ab-9b53-20b61913d060 · outbound

This paper cites Gravitational-wave surrogate models powered by artificial neural networks: The ANN-Sur for waveform generation.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Gravitational-wave surrogate models powered by artificial neural networks: The ANN-Sur for waveform generation

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.534228Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6e96b6f5-5934-4eb8-87b8-f3d0d7624033 · outbound

This paper cites Autoencoder-driven Spiral Representation Learning for Gravitational Wave Surrogate Modelling.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Autoencoder-driven Spiral Representation Learning for Gravitational Wave Surrogate Modelling

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.537206Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cec2478e-2828-4904-a0b3-2b830d4c499d · outbound

This paper cites A fully precessing higher-mode surrogate model of effective-one-body waveforms.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates A fully precessing higher-mode surrogate model of effective-one-body waveforms

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.540118Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ad07fd22-a95c-480a-a035-64f7cf6348d3 · outbound

This paper cites Accelerating multimodal gravitational waveforms from precessing compact binaries with artificial neural networks.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Accelerating multimodal gravitational waveforms from precessing compact binaries with artificial neural networks

Reference 91

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.542705Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 05c7e2b7-bc27-43a1-ad09-921fedbd8871 · outbound

This paper cites Fast and accurate prediction of numerical relativity waveforms from binary black hole coalescences using surrogate models.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Fast and accurate prediction of numerical relativity waveforms from binary black hole coalescences using surrogate models

Reference 92

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.545346Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cbac5c4c-e11c-49ce-8975-e3b1e0ff8f40 · outbound

This paper cites A Surrogate Model of Gravitational Waveforms from Numerical Relativity Simulations of Precessing Binary Black Hole Mergers.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates A Surrogate Model of Gravitational Waveforms from Numerical Relativity Simulations of Precessing Binary Black Hole Mergers

Reference 93

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.548829Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 301a4990-073e-4367-acc4-76d91a006991 · outbound

This paper cites A Numerical Relativity Waveform Surrogate Model for Generically Precessing Binary Black Hole Mergers.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates A Numerical Relativity Waveform Surrogate Model for Generically Precessing Binary Black Hole Mergers

Reference 94

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.551566Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c16f49df-a699-4ba7-a26d-a357a43c5d0c · outbound

This paper cites Surrogate model of hybridized numerical relativity binary black hole waveforms.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Surrogate model of hybridized numerical relativity binary black hole waveforms

Reference 95

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.554357Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b5bd6ee0-9cc7-49ba-920a-f2568c7dcf39 · outbound

This paper cites Surrogate models for precessing binary black hole simulations with unequal masses.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Surrogate models for precessing binary black hole simulations with unequal masses

Reference 96

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.557263Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation af57ccaa-3ad0-48f3-ba7a-fc1eca069902 · outbound

This paper cites A Precessing Numerical Relativity Waveform Surrogate Model for Binary Black Holes: A Gaussian Process Regression Approach.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates A Precessing Numerical Relativity Waveform Surrogate Model for Binary Black Holes: A Gaussian Process Regression Approach

Reference 97

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.560308Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8b09b8ec-7d06-46d1-938c-5b95047612b6 · outbound

This paper cites Numerical relativity surrogate model with memory effects and post-Newtonian hybridization.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Numerical relativity surrogate model with memory effects and post-Newtonian hybridization

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.562781Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 49e143c5-a0ab-464f-9508-075c69c4b71e · outbound

This paper cites A Surrogate Model for Gravitational Wave Signals from Comparable- to Large- Mass-Ratio Black Hole Binaries.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates A Surrogate Model for Gravitational Wave Signals from Comparable- to Large- Mass-Ratio Black Hole Binaries

Reference 99

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.565404Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 68309292-7139-4105-9227-f4dff524b051 · outbound

This paper cites Surrogate model for gravitational wave signals from non-spinning, comparable- to large-mass-ratio black hole binaries built on black hole perturbation theory waveforms calibrated to numerical relativity.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Surrogate model for gravitational wave signals from non-spinning, comparable- to large-mass-ratio black hole binaries built on black hole perturbation theory waveforms calibrated to numerical relativity

Reference 100

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.568224Z

Source-reported events for the cited work

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Pith citing papers

Observation ead542ad-a262-42fe-8933-88d723133662 · inbound

Fast neural network surrogate for multimodal effective-one-body gravitational waveforms from generically precessing compact binaries cites this paper.

Fast neural network surrogate for multimodal effective-one-body gravitational waveforms from generically precessing compact binaries Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates

Reference 122

Resolution: verified exact; arxiv_id, observed 2026-07-23T01:23:29.198237Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 4b12adee-5319-4e78-87ff-99f975fd2da1 · 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 Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates

Reference 74

Resolution: metadata mismatch; arxiv_id, observed 2026-07-23T01:23:29.198237Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation dd715913-b222-4e8f-b61a-d7e5fac548e3 · 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 Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates

Reference 62

Resolution: verified exact; arxiv_id, observed 2026-07-23T01:23:29.198237Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation fd78e507-e2a1-42b4-831f-6a01bc8c4d75 · 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 Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates

Reference 45

Resolution: verified exact; arxiv_id, observed 2026-07-23T01:23:29.198237Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.