Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-05-23T23:38:37.094812Z
Paper Citation Record · LEDGER
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity
As of 8 August 2026, this Paper Citation Record lists 100 of 121 outbound references and 13 inbound Pith citation observations for arXiv:2407.18319.
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 2026-08-07T06:34:17.273281+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-06T21:08:41.747895Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-03T02:57:35.585361Z
Reference resolution
100 of 121 outbound references displayed
- verified exact67
- verified fuzzy23
- unresolved7
- parse uncertain0
- malformed identifier0
- metadata mismatch3
External citation measurements
No source-named external measurement is stored.
Outbound references
Observation d0f21184-e3d9-4b07-8a25-79112761fa4a · outbound
This paper cites Advanced LIGO.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Advanced LIGO
Reference 1
- Resolution
- verified exact
- local_arxiv, observed 2026-05-23T23:43:38.511067Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 2269fccc-7a3b-4af8-8ed2-f01c2acde4ee · outbound
This paper cites Advanced Virgo: a 2nd generation interferometric gravitational wave detector.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Advanced Virgo: a 2nd generation interferometric gravitational wave detector
Reference 2
- Resolution
- verified exact
- local_arxiv, observed 2026-05-23T23:43:38.505566Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 4123c858-1899-4dff-a416-00184cb84e5c · outbound
This paper cites Akutsuet al.(KAGRA), PTEP2021, 05A101 (2021), arXiv:2005.05574 [physics.ins-det].
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Akutsuet al.(KAGRA), PTEP2021, 05A101 (2021), arXiv:2005.05574 [physics.ins-det]
Reference 3
- Resolution
- verified exact
- arxiv_id, observed 2026-05-23T23:43:38.598715Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 401e4fb6-030f-46db-80ef-1e1e75cd8242 · 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.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs
Reference 4
- Resolution
- verified exact
- local_arxiv, observed 2026-05-23T23:43:38.495159Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation bd780f6f-4310-45b6-ad8d-4e8d3c08a88b · outbound
This paper cites GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run
Reference 5
- Resolution
- verified exact
- local_arxiv, observed 2026-05-23T23:43:38.572892Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation f4bfdf1a-3f23-41f0-aa6f-a70e782cec8e · outbound
This paper cites GWTC-2.1: Deep Extended Catalog of Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity GWTC-2.1: Deep Extended Catalog of Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run
Reference 6
- Resolution
- verified exact
- local_arxiv, observed 2026-05-23T23:43:38.489586Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 18acc5bc-8c1d-471a-a708-b8c7f983ca7f · outbound
This paper cites GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run
Reference 7
- Resolution
- verified exact
- local_arxiv, observed 2026-05-23T23:43:38.539711Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 3ee8f590-45c5-4a20-b1e3-b3f166bd9227 · outbound
This paper cites Abbott et al.
Reference 8
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-23T23:43:39.365650Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation cbe5c1c5-9d94-461e-838e-e555a8a9a162 · outbound
This paper cites Waveform Modelling for the Laser Interferometer Space Antenna.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Waveform Modelling for the Laser Interferometer Space Antenna
Reference 9
- Resolution
- verified exact
- local_arxiv, observed 2026-05-23T23:43:38.521873Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 75579200-99a4-42cd-b6b9-e10c4040e59b · outbound
This paper cites Cosmic Explorer: The U.S. Contribution to Gravitational-Wave Astronomy beyond LIGO.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Cosmic Explorer: The U.S. Contribution to Gravitational-Wave Astronomy beyond LIGO
Reference 10
- Resolution
- verified exact
- local_arxiv, observed 2026-05-23T23:43:38.721944Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 8ef0681c-4519-4e3e-9422-5fa2e5cca6e1 · outbound
This paper cites Punturo et al.
Reference 11
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-23T23:43:39.362694Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 6d6fadf9-f84e-40a3-89fe-025daa20df8e · outbound
This paper cites Ready for what lies ahead? -- Gravitational waveform accuracy requirements for future ground based detectors.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Ready for what lies ahead? -- Gravitational waveform accuracy requirements for future ground based detectors
Reference 12
- Resolution
- verified exact
- arxiv_id, observed 2026-05-23T23:43:38.389506Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 414109d5-6f05-4eaa-a6db-afd3124237a2 · outbound
This paper cites Ferguson et al.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Ferguson et al
Reference 13
- Resolution
- verified exact
- doi, observed 2026-05-23T23:43:38.070969Z
Source-reported events for the cited work
correction dated 2021-08-17. Source: crossref record 10.1103/physrevd.104.044037->10.1103/physrevd.104.044037:correction, observed 2026-07-11T03:01:23.692413+00:00. This notice travels one citation hop only.
Observation 7e66b1a9-587b-412a-8b77-fe61011582a4 · outbound
This paper cites Second MAYA Catalog of Binary Black Hole Numerical Relativity Waveforms.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Second MAYA Catalog of Binary Black Hole Numerical Relativity Waveforms
Reference 14
- Resolution
- verified exact
- arxiv_id, observed 2026-05-23T23:43:38.382873Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation a45082c1-48f5-40f4-a833-70efc220048b · outbound
This paper cites A catalog of 174 binary black-hole simulations for gravitational-wave astronomy.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity A catalog of 174 binary black-hole simulations for gravitational-wave astronomy
Reference 15
- Resolution
- verified exact
- local_arxiv, observed 2026-05-23T23:43:38.398307Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation dd9c888d-9d5e-485c-bba6-42df17020a3b · outbound
This paper cites Boyle et al.
Reference 16
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-23T23:43:39.353833Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation a188ed57-45cb-469b-ba6b-880e73cdd36b · outbound
This paper cites L¨ offleret al.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity L¨ offleret al
Reference 17
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-23T23:43:39.349032Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 0ee4d5b8-a100-494e-8340-9433d2c025fe · outbound
This paper cites Georgia Tech Catalog of Gravitational Waveforms.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Georgia Tech Catalog of Gravitational Waveforms
Reference 18
- Resolution
- verified exact
- local_arxiv, observed 2026-05-23T23:43:38.477962Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation a5eb41d3-2840-4dac-a0aa-51b69249daac · outbound
This paper cites The RIT binary black hole simulations catalog.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity The RIT binary black hole simulations catalog
Reference 19
- Resolution
- verified exact
- local_arxiv, observed 2026-05-23T23:43:38.727549Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 73e39ff1-176c-4ca7-9c67-b34fbd2883cc · outbound
This paper cites The second RIT binary black hole simulations catalog and its application to gravitational waves parameter estimation.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity The second RIT binary black hole simulations catalog and its application to gravitational waves parameter estimation
Reference 20
- Resolution
- verified exact
- local_arxiv, observed 2026-05-23T23:43:38.484219Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation fd26cf4c-50be-4499-9994-1c1e88468c65 · outbound
This paper cites The Third RIT binary black hole simulations catalog.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity The Third RIT binary black hole simulations catalog
Reference 21
- Resolution
- verified exact
- arxiv_id, observed 2026-05-23T23:43:38.464269Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 4656c164-9bfb-4c67-b605-29ca359064a8 · outbound
This paper cites The Fourth RIT binary black hole simulations catalog: Extension to Eccentric Orbits.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity The Fourth RIT binary black hole simulations catalog: Extension to Eccentric Orbits
Reference 22
- Resolution
- verified exact
- arxiv_id, observed 2026-05-23T23:43:38.458950Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation dc67ddee-94b0-492d-8a18-0b57fb1fa7fa · outbound
This paper cites Neilsen et al., Bulletin of the American Physical So- ciety (2022).
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Neilsen et al., Bulletin of the American Physical So- ciety (2022)
Reference 23
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-23T23:43:39.345002Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation d1f63413-0da2-4977-89c8-5887b651b84f · outbound
This paper cites Targeted large mass ratio numerical relativity surrogate waveform model for GW190814.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Targeted large mass ratio numerical relativity surrogate waveform model for GW190814
Reference 24
- Resolution
- verified exact
- arxiv_id, observed 2026-05-23T23:43:38.445437Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 2eb04624-0563-45f5-81cc-a7277f506b98 · outbound
This paper cites Nu- merical simulations of extreme mass ratio binary black holes.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Nu- merical simulations of extreme mass ratio binary black holes
Reference 25
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-23T23:43:39.341729Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 69f98a3f-5a8f-48f1-8d9f-845f10d3f081 · outbound
This paper cites Exploring the small mass ratio binary black hole merger via Zeno's dichotomy approach.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Exploring the small mass ratio binary black hole merger via Zeno's dichotomy approach
Reference 26
- Resolution
- verified exact
- arxiv_id, observed 2026-05-23T23:43:38.822716Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 49722328-1b0f-48ce-8520-8369aa12d993 · outbound
This paper cites Exploring intermediate and massive black-hole binaries with the Einstein Telescope.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Exploring intermediate and massive black-hole binaries with the Einstein Telescope
Reference 27
- Resolution
- verified exact
- local_arxiv, observed 2026-05-23T23:43:38.499970Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 464966c0-6d3e-4f82-bf80-ec853f598d8b · outbound
This paper cites Where are the Intermediate Mass Black Holes?.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Where are the Intermediate Mass Black Holes?
Reference 28
- Resolution
- verified exact
- local_arxiv, observed 2026-05-23T23:43:38.550585Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 3b34be29-ab2b-4f36-bf48-8bba86ee0909 · outbound
This paper cites Intermediate and Extreme Mass-Ratio Inspirals -- Astrophysics, Science Applications and Detection using LISA.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Intermediate and Extreme Mass-Ratio Inspirals -- Astrophysics, Science Applications and Detection using LISA
Reference 29
- Resolution
- verified exact
- local_arxiv, observed 2026-05-23T23:43:38.528148Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 8b404882-d720-49c7-af6e-e0fc890f46ac · outbound
This paper cites an unresolved cited work.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Unresolved cited work
Reference 30
- Resolution
- unresolved
- raw_fallback, observed 2026-05-23T23:43:39.335669Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation e60b5ad1-4c0f-4346-bdec-d8de06b117ee · outbound
This paper cites an unresolved cited work.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Unresolved cited work
Reference 31
- Resolution
- unresolved
- raw_fallback, observed 2026-05-23T23:43:39.374217Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 782ef277-905d-4a13-908d-b4a834f7f74c · outbound
This paper cites Monte-Carlo simulations of black hole mergers in AGN disks: Low $\chi_{\rm eff}$ mergers and predictions for LIGO.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Monte-Carlo simulations of black hole mergers in AGN disks: Low $\chi_{\rm eff}$ mergers and predictions for LIGO
Reference 32
- Resolution
- verified exact
- arxiv_id, observed 2026-05-23T23:43:38.567890Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation e6bde245-dd0e-496d-87f1-a2e4fb4d31f6 · outbound
This paper cites The motion of a system of bodies under the influence of their mutual attraction, according to einstein’s theory.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity The motion of a system of bodies under the influence of their mutual attraction, according to einstein’s theory
Reference 33
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-23T23:43:39.329117Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation f890c9b2-1c8b-4500-9dd0-1239cc942245 · outbound
This paper cites Post-Newtonian Theory for Gravitational Waves.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Post-Newtonian Theory for Gravitational Waves
Reference 34
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-05-23T23:43:38.577981Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 108d4225-c234-47bf-a5c6-bffad5aa51af · outbound
This paper cites an unresolved cited work.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Unresolved cited work
Reference 35
- Resolution
- unresolved
- raw_fallback, observed 2026-05-23T23:43:39.325837Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation f765fd10-4447-4c62-a636-a7b7d0012fc8 · outbound
This paper cites Buonanno and T.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Buonanno and T
Reference 36
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-23T23:43:39.409263Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation e173d10a-09b1-4db6-89d6-6ab4b05520aa · outbound
This paper cites An improved effective-one-body model of spinning, nonprecessing binary black holes for the era of gravitational-wave astrophysics with advanced detectors.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity An improved effective-one-body model of spinning, nonprecessing binary black holes for the era of gravitational-wave astrophysics with advanced detectors
Reference 37
- Resolution
- verified exact
- local_arxiv, observed 2026-05-23T23:43:38.413200Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation e8b80d5a-c26a-4a77-a854-2f7197327e10 · outbound
This paper cites Enriching the Symphony of Gravitational Waves from Binary Black Holes by Tuning Higher Harmonics.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Enriching the Symphony of Gravitational Waves from Binary Black Holes by Tuning Higher Harmonics
Reference 38
- Resolution
- verified exact
- arxiv_id, observed 2026-05-23T23:43:38.630711Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation e453fd3c-0892-459d-a53b-8d89bcae8f56 · outbound
This paper cites Frequency domain reduced order model of aligned-spin effective-one-body waveforms with higher-order modes.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Frequency domain reduced order model of aligned-spin effective-one-body waveforms with higher-order modes
Reference 39
- Resolution
- verified exact
- arxiv_id, observed 2026-05-23T23:43:38.407552Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 8223bb87-ebd3-4bf8-9391-7e90e2b26cf1 · outbound
This paper cites Inspiral-merger-ringdown waveforms of spinning, precessing black-hole binaries in the effective-one-body formalism.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Inspiral-merger-ringdown waveforms of spinning, precessing black-hole binaries in the effective-one-body formalism
Reference 40
- Resolution
- verified exact
- local_arxiv, observed 2026-05-23T23:43:38.614935Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation acce6ff6-6fb1-4c51-a8f4-32ec770c18db · outbound
This paper cites Validating the effective-one-body model of spinning, precessing binary black holes against numerical relativity.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Validating the effective-one-body model of spinning, precessing binary black holes against numerical relativity
Reference 41
- Resolution
- verified exact
- local_arxiv, observed 2026-05-23T23:43:38.758665Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation fd894376-e9bd-4aef-9a3b-99f563123713 · outbound
This paper cites Multipolar Effective-One-Body Waveforms for Precessing Binary Black Holes: Construction and Validation.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Multipolar Effective-One-Body Waveforms for Precessing Binary Black Holes: Construction and Validation
Reference 42
- Resolution
- verified exact
- arxiv_id, observed 2026-05-23T23:43:38.625413Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 70b8acaf-fd45-433f-a82f-cca641316c99 · outbound
This paper cites A new effective-one-body description of coalescing nonprecessing spinning black-hole binaries.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity A new effective-one-body description of coalescing nonprecessing spinning black-hole binaries
Reference 43
- Resolution
- verified exact
- local_arxiv, observed 2026-05-23T23:43:38.620088Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 8afd5876-d6a2-444b-bbb4-d3541925dbd9 · outbound
This paper cites A Multipolar Effective One Body Model for Non-Spinning Black Hole Binaries.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity A Multipolar Effective One Body Model for Non-Spinning Black Hole Binaries
Reference 44
- Resolution
- verified exact
- arxiv_id, observed 2026-05-23T23:43:38.663701Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation a65df25f-5b2f-4401-b8b3-a8e617cf1556 · outbound
This paper cites A multipolar effective one body waveform model for spin-aligned black hole binaries.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity A multipolar effective one body waveform model for spin-aligned black hole binaries
Reference 45
- Resolution
- verified exact
- arxiv_id, observed 2026-05-23T23:43:38.790164Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 61e0eee6-ea6d-495e-a190-416f4eb638f5 · outbound
This paper cites TEOBResumS: assessment of consistent next-to-quasicircular corrections and post-adiabatic approximation in multipolar binary black holes waveforms.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity TEOBResumS: assessment of consistent next-to-quasicircular corrections and post-adiabatic approximation in multipolar binary black holes waveforms
Reference 46
- Resolution
- verified exact
- arxiv_id, observed 2026-05-23T23:43:38.698277Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 43bc0def-91b0-4e50-966b-c6e6bb3175c9 · outbound
This paper cites Theoretical groundwork supporting the precessing-spin two-body dynamics of the effective-one-body waveform models SEOBNRv5.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Theoretical groundwork supporting the precessing-spin two-body dynamics of the effective-one-body waveform models SEOBNRv5
Reference 47
- Resolution
- verified exact
- arxiv_id, observed 2026-05-23T23:43:38.783581Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 4145a95a-2b0a-4035-a803-39a57ca393cf · outbound
This paper cites Laying the foundation of the effective-one-body waveform models SEOBNRv5: improved accuracy and efficiency for spinning non-precessing binary black holes.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Laying the foundation of the effective-one-body waveform models SEOBNRv5: improved accuracy and efficiency for spinning non-precessing binary black holes
Reference 48
- Resolution
- verified exact
- arxiv_id, observed 2026-05-23T23:43:38.745921Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 6a237207-433a-492c-a3cc-258b48f88031 · outbound
This paper cites SEOBNRv5PHM: Next generation of accurate and efficient multipolar precessing-spin effective-one-body waveforms for binary black holes.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity SEOBNRv5PHM: Next generation of accurate and efficient multipolar precessing-spin effective-one-body waveforms for binary black holes
Reference 49
- Resolution
- verified exact
- arxiv_id, observed 2026-05-23T23:43:38.376893Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 17d99ddc-0075-4e5b-9701-a3239f39970b · outbound
This paper cites Enhancing the SEOBNRv5 effective-one-body waveform model with second-order gravitational self-force fluxes.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Enhancing the SEOBNRv5 effective-one-body waveform model with second-order gravitational self-force fluxes
Reference 50
- Resolution
- verified exact
- arxiv_id, observed 2026-07-17T01:20:32.101006Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 4ffae508-3e49-4793-ac50-58a590bde90a · outbound
This paper cites Ajith et al., Classical and Quantum Gravity 24, S689 (2007).
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Ajith et al., Classical and Quantum Gravity 24, S689 (2007)
Reference 51
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-23T23:43:39.437861Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation a15de15e-78bb-4e37-beb0-06cfd6f02cbd · outbound
This paper cites Frequency-domain gravitational waves from non-precessing black-hole binaries. I. New numerical waveforms and anatomy of the signal.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Frequency-domain gravitational waves from non-precessing black-hole binaries. I. New numerical waveforms and anatomy of the signal
Reference 52
- Resolution
- verified exact
- local_arxiv, observed 2026-05-23T23:43:38.776416Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 9053a9cd-0309-4e71-8b1a-e6a68df66d52 · outbound
This paper cites Frequency-domain gravitational waves from non-precessing black-hole binaries. II. A phenomenological model for the advanced detector era.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Frequency-domain gravitational waves from non-precessing black-hole binaries. II. A phenomenological model for the advanced detector era
Reference 53
- Resolution
- verified exact
- local_arxiv, observed 2026-05-23T23:43:38.808889Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 2cf75e5d-77e4-44d3-b257-ef44d07f9608 · outbound
This paper cites First higher-multipole model of gravitational waves from spinning and coalescing black-hole binaries.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity First higher-multipole model of gravitational waves from spinning and coalescing black-hole binaries
Reference 54
- Resolution
- verified exact
- local_arxiv, observed 2026-05-23T23:43:38.692916Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation fef92d8a-1a59-4c5f-b322-a515faf3f7fc · outbound
This paper cites Phenomenological model for the gravitational-wave signal from precessing binary black holes with two-spin effects.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Phenomenological model for the gravitational-wave signal from precessing binary black holes with two-spin effects
Reference 55
- Resolution
- verified exact
- arxiv_id, observed 2026-05-23T23:43:38.713673Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 6c54680a-c8e7-433c-904d-5e9de154649b · outbound
This paper cites A simple model of complete precessing black-hole-binary gravitational waveforms.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity A simple model of complete precessing black-hole-binary gravitational waveforms
Reference 56
- Resolution
- verified exact
- local_arxiv, observed 2026-05-23T23:43:38.688080Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 3620a596-5c45-4f7b-a18a-c9e8fe9dc85f · outbound
This paper cites Including higher order multipoles in gravitational-wave models for precessing binary black holes.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Including higher order multipoles in gravitational-wave models for precessing binary black holes
Reference 57
- Resolution
- verified exact
- arxiv_id, observed 2026-05-23T23:43:38.678532Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation bb41324f-d61f-4799-8c56-ae8743a27e8e · outbound
This paper cites Computationally efficient models for the dominant and sub-dominant harmonic modes of precessing binary black holes.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Computationally efficient models for the dominant and sub-dominant harmonic modes of precessing binary black holes
Reference 58
- Resolution
- verified exact
- local_arxiv, observed 2026-05-23T23:43:38.683532Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation e7f5fe97-0a7b-4831-9fc3-7fad1a0f0efd · outbound
This paper cites IMRPhenomTP: A phenomenological time domain model for dominant quadrupole gravitational wave signal of coalescing binary black holes.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity IMRPhenomTP: A phenomenological time domain model for dominant quadrupole gravitational wave signal of coalescing binary black holes
Reference 59
- Resolution
- verified exact
- arxiv_id, observed 2026-05-23T23:43:38.708410Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 21d371cd-fcea-4f6d-bb96-99e356100977 · outbound
This paper cites Time domain phenomenological model of gravitational wave subdominant harmonics for quasi-circular non-precessing binary black hole coalescences.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Time domain phenomenological model of gravitational wave subdominant harmonics for quasi-circular non-precessing binary black hole coalescences
Reference 60
- Resolution
- verified exact
- arxiv_id, observed 2026-05-23T23:43:38.827694Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation bba1e20e-3d13-4d97-88d8-e5cdfb5734b3 · outbound
This paper cites New twists in compact binary waveform modelling: a fast time domain model for precession.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity New twists in compact binary waveform modelling: a fast time domain model for precession
Reference 61
- Resolution
- verified exact
- arxiv_id, observed 2026-05-23T23:43:38.658227Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 39c5ffac-21dd-445a-b6f6-9f143149ba20 · outbound
This paper cites The final twist: A model of gravitational waves from precessing black-hole binaries through merger and ringdown.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity The final twist: A model of gravitational waves from precessing black-hole binaries through merger and ringdown
Reference 62
- Resolution
- verified exact
- arxiv_id, observed 2026-05-23T23:43:38.557901Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 57e33b9e-1ada-4f02-9454-feecf529993e · outbound
This paper cites Fast prediction and evaluation of gravitational waveforms using surrogate models.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Fast prediction and evaluation of gravitational waveforms using surrogate models
Reference 63
- Resolution
- verified exact
- local_arxiv, observed 2026-05-23T23:43:38.544978Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 8baa90be-3615-483b-86c5-252df382b568 · outbound
This paper cites Fast and accurate prediction of numerical relativity waveforms from binary black hole coalescences using surrogate models.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Fast and accurate prediction of numerical relativity waveforms from binary black hole coalescences using surrogate models
Reference 64
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-05-23T23:43:38.673465Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation b7283d8d-f64a-4e10-b362-a414183aa243 · outbound
This paper cites A Surrogate Model of Gravitational Waveforms from Numerical Relativity Simulations of Precessing Binary Black Hole Mergers.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity A Surrogate Model of Gravitational Waveforms from Numerical Relativity Simulations of Precessing Binary Black Hole Mergers
Reference 65
- Resolution
- verified exact
- local_arxiv, observed 2026-05-23T23:43:38.643516Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 6caa09c0-b76d-4e6f-90ec-23d7ffa09e35 · outbound
This paper cites A Numerical Relativity Waveform Surrogate Model for Generically Precessing Binary Black Hole Mergers.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity A Numerical Relativity Waveform Surrogate Model for Generically Precessing Binary Black Hole Mergers
Reference 66
- Resolution
- verified exact
- local_arxiv, observed 2026-05-23T23:43:38.653044Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 158eee88-768b-4d80-a2b0-f82128c03713 · outbound
This paper cites Surrogate models for precessing binary black hole simulations with unequal masses.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Surrogate models for precessing binary black hole simulations with unequal masses
Reference 68
- Resolution
- verified exact
- local_arxiv, observed 2026-05-23T23:43:38.668816Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation fb2ce2dd-afc0-4ac2-b667-f90664c0a52b · outbound
This paper cites A Surrogate Model for Gravitational Wave Signals from Comparable- to Large- Mass-Ratio Black Hole Binaries.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity A Surrogate Model for Gravitational Wave Signals from Comparable- to Large- Mass-Ratio Black Hole Binaries
Reference 69
- Resolution
- verified exact
- arxiv_id, observed 2026-05-23T23:43:38.638427Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 21f5b9f9-d8dd-44a3-96f5-b3ed05fd3a57 · 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.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity 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 70
- Resolution
- verified exact
- arxiv_id, observed 2026-05-23T23:43:38.084465Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 58616ddd-a341-42cc-a9f7-02aeaeb11a08 · outbound
This paper cites an unresolved cited work.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Unresolved cited work
Reference 71
- Resolution
- unresolved
- raw_fallback, observed 2026-05-23T23:43:39.420667Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation e61f0a59-4e86-4c25-a8c0-9bed509fd71d · outbound
This paper cites an unresolved cited work.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Unresolved cited work
Reference 72
- Resolution
- unresolved
- raw_fallback, observed 2026-05-23T23:43:39.412072Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 5524e60a-28cb-4774-a256-52f2b13e664c · outbound
This paper cites an unresolved cited work.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Unresolved cited work
Reference 73
- Resolution
- unresolved
- raw_fallback, observed 2026-05-23T23:43:39.414791Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation f1954e46-b4d6-4c3f-b75d-e3bda9bf21e1 · outbound
This paper cites Zengino˘ glu and G.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Zengino˘ glu and G
Reference 74
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-23T23:43:39.423516Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation d6ca6338-b939-4412-9c08-207424998712 · outbound
This paper cites gwsurrogate.
Reference 76
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-23T23:43:39.426354Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 6c3128bd-6ed5-4245-a759-a0fc832e169e · outbound
This paper cites Ori and K.
Reference 77
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-23T23:43:39.440580Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 7c0bf89a-0904-41db-8986-a7018748a83d · outbound
This paper cites Learning about black hole binaries from their ringdown spectra.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Learning about black hole binaries from their ringdown spectra
Reference 78
- Resolution
- verified exact
- arxiv_id, observed 2026-05-23T23:43:38.593715Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 5173a771-8b48-4a0d-a09c-4e855e4554f4 · outbound
This paper cites Apte and S.
Reference 79
- Resolution
- verified exact
- doi, observed 2026-05-23T23:43:38.077872Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 4f8bbcd0-a9e3-46e7-a465-e869f8573b89 · outbound
This paper cites Fujita and H.
Reference 80
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-23T23:43:39.396403Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 8f724bea-5cc9-43ee-98be-a5927f398a43 · outbound
This paper cites Fujita and H.
Reference 81
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-23T23:43:39.400061Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation df5586d7-4ecd-43a5-bf0e-91cae1d1a8d5 · outbound
This paper cites an unresolved cited work.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Unresolved cited work
Reference 82
- Resolution
- unresolved
- raw_fallback, observed 2026-05-23T23:43:39.403274Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 31164b83-37c0-4cc8-bfc0-7d8a70e6db1c · outbound
This paper cites Throwe, High precision calculation of generic ex- treme mass ratio inspirals , Ph.D.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Throwe, High precision calculation of generic ex- treme mass ratio inspirals , Ph.D
Reference 83
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-23T23:43:39.390275Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 1b450d6b-90f2-4cb7-9a82-a6116b299c3f · outbound
This paper cites Black Hole Perturbation Toolkit.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Black Hole Perturbation Toolkit
Reference 84
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-23T23:43:39.379940Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation acaef445-02c9-4d3f-8f8c-d55e7fb4fbdf · outbound
This paper cites Strong-field tidal distortions of rotating black holes: Formalism and results for circular, equatorial orbits.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Strong-field tidal distortions of rotating black holes: Formalism and results for circular, equatorial orbits
Reference 85
- Resolution
- verified exact
- local_arxiv, observed 2026-05-23T23:43:38.516677Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation f88bf821-ba76-44f9-b6c9-fb1277baa05f · outbound
This paper cites Drasco and S.
Reference 86
- Resolution
- verified exact
- doi, observed 2026-05-23T23:43:38.060173Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation a41040a3-4c7c-4564-bad8-5eeec61cf384 · outbound
This paper cites Hinderer and E.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Hinderer and E
Reference 87
- Resolution
- verified exact
- doi, observed 2026-05-23T23:43:38.063666Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 16f0842e-2450-4a20-a8e5-d9d97d2502ae · outbound
This paper cites an unresolved cited work.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Unresolved cited work
Reference 88
- Resolution
- verified exact
- doi, observed 2026-05-23T23:43:38.074530Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 64eefa81-b301-4361-8c51-cbb038f777d8 · outbound
This paper cites Pound, Physical Review Letters 109 (2012), 10.1103/physrevlett.109.051101.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Pound, Physical Review Letters 109 (2012), 10.1103/physrevlett.109.051101
Reference 89
- Resolution
- verified exact
- doi, observed 2026-05-23T23:43:38.067653Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 52012357-c66c-4a88-bbe5-43a7359202bd · outbound
This paper cites Second-order self-force calculation of the gravitational binding energy in compact binaries.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Second-order self-force calculation of the gravitational binding energy in compact binaries
Reference 90
- Resolution
- verified exact
- arxiv_id, observed 2026-05-23T23:43:38.739748Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation f4c41eb7-5d26-43f9-b0d1-e3f24d6bb696 · outbound
This paper cites Wardell et al., Physical Review Letters 130, 241402 (2023).
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Wardell et al., Physical Review Letters 130, 241402 (2023)
Reference 91
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-23T23:43:39.359884Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 49adfcd1-19b8-4d31-ab1e-95feff1c34a9 · outbound
This paper cites McKennon, G.
Reference 92
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-23T23:43:39.356793Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation e8ddef53-d826-4f35-a020-87913e8e73d4 · outbound
This paper cites Frequency domain reduced order models for gravitational waves from aligned-spin compact binaries.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Frequency domain reduced order models for gravitational waves from aligned-spin compact binaries
Reference 93
- Resolution
- verified exact
- local_arxiv, observed 2026-05-23T23:43:38.753324Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation c42de293-9581-4a10-8fc0-ab122081a71d · outbound
This paper cites Surrogate model of hybridized numerical relativity binary black hole waveforms.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Surrogate model of hybridized numerical relativity binary black hole waveforms
Reference 94
- Resolution
- verified exact
- local_arxiv, observed 2026-05-23T23:43:38.469629Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation e3794dfb-f272-4e96-9ff3-d5473964be55 · outbound
This paper cites High-accuracy mass, spin, and recoil predictions of generic black-hole merger remnants.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity High-accuracy mass, spin, and recoil predictions of generic black-hole merger remnants
Reference 95
- Resolution
- verified exact
- local_arxiv, observed 2026-05-23T23:43:38.437542Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation d9902e9e-c499-4987-9b44-ac4f9a9c5d6d · outbound
This paper cites A fully precessing higher-mode surrogate model of effective-one-body waveforms.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity A fully precessing higher-mode surrogate model of effective-one-body waveforms
Reference 96
- Resolution
- verified exact
- arxiv_id, observed 2026-05-23T23:43:38.451192Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation e2f91190-9e33-4272-bb07-84f8afa044f6 · outbound
This paper cites Smith et al., Physical Review D 94, 044031 (2016).
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Smith et al., Physical Review D 94, 044031 (2016)
Reference 97
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-23T23:43:39.322582Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 69a4dfa9-7376-42c8-a61c-eeafd69ca2de · outbound
This paper cites Taracchini et al.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Taracchini et al
Reference 98
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-23T23:43:39.316887Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 6256ad19-7a0c-43a4-8545-8dee4e99b2bc · outbound
This paper cites Lim et al., Physical Review D 100, 084032 (2019).
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Lim et al., Physical Review D 100, 084032 (2019)
Reference 99
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-23T23:43:39.319834Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 3b7ee59e-129f-4558-b437-21127c8ef6aa · outbound
This paper cites Maday et al., Communications on Pure and Applied Analysis 8, 383 (2009).
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Maday et al., Communications on Pure and Applied Analysis 8, 383 (2009)
Reference 100
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-23T23:43:39.332691Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 1e265422-ed30-46c5-a9a8-494a70add5fd · outbound
This paper cites Chaturantabut and D.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Chaturantabut and D
Reference 101
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-23T23:43:39.370955Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 95b9e4a7-8851-4e7e-827f-2e1df2248eb3 · outbound
This paper cites Accelerated gravitational-wave parameter estimation with reduced order modeling.
Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Accelerated gravitational-wave parameter estimation with reduced order modeling
Reference 102
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-05-23T23:43:38.604341Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Pith citing papers
Observation bbd011b8-74b6-4416-9b31-fa06361ffee7 · inbound
Searching for intermediate mass ratio binary black hole mergers in the third observing run of LIGO-Virgo-KAGRA cites this paper.
Searching for intermediate mass ratio binary black hole mergers in the third observing run of LIGO-Virgo-KAGRA Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity
Reference 76
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T21:08:41.747895Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ca382da5-1921-454e-962d-f66b8c487f0a · inbound
Primordial black holes versus their impersonators at gravitational wave observatories cites this paper.
Primordial black holes versus their impersonators at gravitational wave observatories Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity
Reference 102
- Resolution
- verified exact
- local_arxiv, observed 2026-05-21T22:15:42.023110Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 51a65085-f366-48f3-82bb-00a0491a1d19 · inbound
Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates cites this paper.
Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity
Reference 101
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T13:34:57.571275Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 72c7af3d-0dd6-4ad2-b2e7-cd2db6f85c78 · inbound
Consistency of spin effects between numerical relativity and perturbation theory for inspiraling comparable-mass black hole binaries cites this paper.
Consistency of spin effects between numerical relativity and perturbation theory for inspiraling comparable-mass black hole binaries Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity
Reference 30
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T13:28:17.274744Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3453b32a-37c1-42f5-aa13-e94c9a9b35ad · inbound
Accurate models for recoil velocity distribution in black hole mergers with comparable to extreme mass-ratios and their astrophysical implications cites this paper.
Accurate models for recoil velocity distribution in black hole mergers with comparable to extreme mass-ratios and their astrophysical implications Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity
Reference 80
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T22:13:55.308319Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c6a624b4-3ed3-4445-a364-9d326444651c · inbound
Analysis of late-time tails in spin-aligned eccentric binary black hole mergers cites this paper.
Analysis of late-time tails in spin-aligned eccentric binary black hole mergers Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity
Reference 78
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T20:00:56.462347Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b86a31a5-ab14-477e-a6f9-beab79553299 · 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 Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity
Reference 35
- 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 b81a0e39-8d75-4029-a1dd-ca242d28285d · inbound
Shaving off soft hairs and the black hole image memory effect cites this paper.
Shaving off soft hairs and the black hole image memory effect Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity
Reference 86
- Resolution
- verified exact
- arxiv_id, observed 2026-05-20T00:02:02.676713Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation d65815cb-296e-4cb5-9d12-6fad16576b8f · 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 Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity
Reference 47
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T02:30:56.949421Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9867a91d-013a-4c76-b1e0-29782161e8af · inbound
Radiation outer boundary conditions and near-to-far field signal transformations for the Bardeen-Press equation cites this paper.
Radiation outer boundary conditions and near-to-far field signal transformations for the Bardeen-Press equation Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity
Reference 47
- Resolution
- verified exact
- arxiv_id, observed 2026-05-20T00:02:02.676713Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 66139761-d155-4b69-8454-19b6f17214b1 · inbound
Modified Teukolsky Formalism for Extreme Mass-Ratio Inspirals in Higher-Derivative Gravity cites this paper.
Modified Teukolsky Formalism for Extreme Mass-Ratio Inspirals in Higher-Derivative Gravity Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity
Reference 26
- Resolution
- verified exact
- local_arxiv, observed 2026-07-03T02:57:35.586736Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation bccace35-e2c4-4551-bf52-8041a0dd764e · 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 Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity
Reference 60
- Resolution
- verified exact
- local_arxiv, observed 2026-06-30T08:54:29.882607Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 6bb2d649-199b-4040-b712-fdbf90ddac2d · inbound
Unified remnant models for aligned-spin, precessing, and eccentric binary black hole mergers cites this paper.
Unified remnant models for aligned-spin, precessing, and eccentric binary black hole mergers Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity
Reference 83
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T00:42:37.310119Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.