Paper Citation Record · LEDGER

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals

As of 18 August 2026, this Paper Citation Record lists 51 of 51 outbound references and 5 inbound Pith citation observations for arXiv:2411.09147.

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

pith.paper-citation-record.v1
2411.09147 v3

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measured 51 of 51 reference resolution

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Source: paper_references, paper_reference_links, observed 2026-08-12T21:08:18.352538Z

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-17T06:30:58.91139+00:00

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Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T20:28:15.018325Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-01T13:35:45.732062Z

Reference resolution

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Outbound references

Observation 1406b477-5fe6-404b-a3b2-f5f49ed97967 · outbound

This paper cites Laser Interferometer Space Antenna.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals Laser Interferometer Space Antenna

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-12T21:08:18.096167Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9e0d4f88-6a3d-4946-a5c3-3285ec3d924e · outbound

This paper cites TianQin: a space-borne gravitational wave detector.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals TianQin: a space-borne gravitational wave detector

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-12T21:08:18.101638Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9252e3ca-4380-42a9-baf2-149b9e3bf564 · outbound

This paper cites Taiji Program: Gravitational-Wave Sources.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals Taiji Program: Gravitational-Wave Sources

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-12T21:08:18.107349Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d33c4838-639d-412c-a3b2-1c9554cbba3d · outbound

This paper cites Gravitational Waves Notes, Issue #2 : "A probe of spacetime and astrophysics: EMRIs".

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals Gravitational Waves Notes, Issue #2 : "A probe of spacetime and astrophysics: EMRIs"

Reference 4

Resolution: verified exact; local_arxiv, observed 2026-08-12T21:08:19.038395Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 7bfdf446-9494-45bf-911b-284eecf935e9 · outbound

This paper cites Science with the space-based interferometer LISA. V: Extreme mass-ratio inspirals.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals Science with the space-based interferometer LISA. V: Extreme mass-ratio inspirals

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-12T21:08:18.118355Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 99b982f5-b50b-4697-a4d9-7e2fe325f449 · outbound

This paper cites The unique potential of extreme mass-ratio inspirals for gravitational-wave astronomy.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals The unique potential of extreme mass-ratio inspirals for gravitational-wave astronomy

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-12T21:08:18.123443Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 729cf1aa-f2bc-4285-b159-761579342a0a · outbound

This paper cites Newman and R.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals Newman and R

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-12T21:08:18.129537Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bca1009f-2fc6-46a5-95e6-7d5179f0a55d · outbound

This paper cites an unresolved cited work.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals Unresolved cited work

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-12T21:08:18.133710Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 95ab105c-55c3-415a-8357-6768fe87a85d · outbound

This paper cites an unresolved cited work.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals Unresolved cited work

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-12T21:08:18.137801Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1892d8d3-261d-46e3-810d-178d11daead4 · outbound

This paper cites Self-force and radiation reaction in general relativity.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals Self-force and radiation reaction in general relativity

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-12T21:08:18.143705Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5a087cea-fdaf-4662-95fc-b394ec4b0d91 · outbound

This paper cites Pound and B.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals Pound and B

Reference 11

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T21:08:19.103269Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 77d4d564-f33d-4288-8a43-c71132f27f0a · outbound

This paper cites Gravitational wave snapshots of generic extreme mass ratio inspirals.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals Gravitational wave snapshots of generic extreme mass ratio inspirals

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-12T21:08:18.152846Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8a42eb79-da4f-469d-9bad-3987513e2886 · outbound

This paper cites Verifying black hole orbits with gravitational spectroscopy.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals Verifying black hole orbits with gravitational spectroscopy

Reference 13

Resolution: verified exact; local_arxiv, observed 2026-08-12T21:08:18.961703Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 747479e3-1074-473d-bf9d-aaa5113d3228 · outbound

This paper cites An Efficient Numerical Method for Computing Gravitational Waves Induced by a Particle Moving on Eccentric Inclined Orbits around a Kerr Black Hole.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals An Efficient Numerical Method for Computing Gravitational Waves Induced by a Particle Moving on Eccentric Inclined Orbits around a Kerr Black Hole

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-12T21:08:18.163959Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 495e0cf3-a3d5-4820-b277-e4925162c9db · outbound

This paper cites Extreme mass ratio inspirals on the equatorial plane in the adiabatic order.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals Extreme mass ratio inspirals on the equatorial plane in the adiabatic order

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-12T21:08:18.169503Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a4ccac19-c818-4c87-9136-554c72cb2807 · outbound

This paper cites Black Hole Perturbation.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals Black Hole Perturbation

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-12T21:08:18.173731Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4089afe0-b568-4832-adfe-089f7c22efeb · outbound

This paper cites Analytic black hole perturbation approach to gravitational radiation.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals Analytic black hole perturbation approach to gravitational radiation

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-12T21:08:18.178043Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e5adf186-b83c-4ee5-a694-1fcc75007409 · outbound

This paper cites The adiabatic evolution of orbital parameters in the Kerr spacetime.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals The adiabatic evolution of orbital parameters in the Kerr spacetime

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-12T21:08:18.182418Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 77472fa5-5238-48df-93f2-a2eaa55e1c77 · outbound

This paper cites Adiabatic Evolution of three 'Constants' of Motion for Greatly Inclined Orbits in Kerr spacetime.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals Adiabatic Evolution of three 'Constants' of Motion for Greatly Inclined Orbits in Kerr spacetime

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-12T21:08:18.186399Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 39826f4d-a5a5-44b1-817f-6aae343e0ed2 · outbound

This paper cites Calculation of radiation reaction effect on orbital parameters in Kerr spacetime.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals Calculation of radiation reaction effect on orbital parameters in Kerr spacetime

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-12T21:08:18.190503Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1f83a069-46e8-43bf-b362-886e21af7b4a · outbound

This paper cites Gravitational Waves from a Particle in Circular Orbits around a Schwarzschild Black Hole to the 22nd Post-Newtonian Order.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals Gravitational Waves from a Particle in Circular Orbits around a Schwarzschild Black Hole to the 22nd Post-Newtonian Order

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-12T21:08:18.195019Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1be6f980-102c-4122-a44c-c3b807cccd88 · outbound

This paper cites Gravitational Waves from a Particle in Circular Orbits around a Rotating Black Hole to the 11th Post-Newtonian Order.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals Gravitational Waves from a Particle in Circular Orbits around a Rotating Black Hole to the 11th Post-Newtonian Order

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-12T21:08:18.199307Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2eda6ae2-66e2-4e01-9a9e-3227cff3b8f8 · outbound

This paper cites Analytic post-Newtonian expansion of the energy and angular momentum radiated to infinity by eccentric-orbit non-spinning extreme-mass-ratio inspirals to 19PN.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals Analytic post-Newtonian expansion of the energy and angular momentum radiated to infinity by eccentric-orbit non-spinning extreme-mass-ratio inspirals to 19PN

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-12T21:08:18.204299Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 72c24cdc-80b9-49a0-8436-9e99df043b36 · outbound

This paper cites Determination of new coefficients in the angular momentum and energy fluxes at infinity to 9PN for eccentric Schwarzschild extreme-mass-ratio inspirals using mode-by-mode fitting.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals Determination of new coefficients in the angular momentum and energy fluxes at infinity to 9PN for eccentric Schwarzschild extreme-mass-ratio inspirals using mode-by-mode fitting

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-12T21:08:18.208978Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ca9ff800-2260-4907-bf31-e99436259745 · outbound

This paper cites Tidal heating and torquing of the primary black hole in eccentric-orbit, non-spinning extreme-mass-ratio inspirals to 22PN order.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals Tidal heating and torquing of the primary black hole in eccentric-orbit, non-spinning extreme-mass-ratio inspirals to 22PN order

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-12T21:08:18.213623Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 737e136b-9eb6-400c-a5d9-52086b2d4797 · outbound

This paper cites Analytical high-order post-Newtonian expansions for extreme mass ratio binaries.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals Analytical high-order post-Newtonian expansions for extreme mass ratio binaries

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-12T21:08:18.218645Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8a0a713c-1aad-4cd7-8763-5eac80ae4be1 · outbound

This paper cites Analytical high-order post-Newtonian expansions for spinning extreme mass ratio binaries.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals Analytical high-order post-Newtonian expansions for spinning extreme mass ratio binaries

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-12T21:08:18.225810Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b0b80c0d-f231-4b67-a87c-dcfc2b323eee · outbound

This paper cites High-order post-Newtonian expansion of the redshift invariant for eccentric-orbit non-spinning extreme-mass-ratio inspirals.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals High-order post-Newtonian expansion of the redshift invariant for eccentric-orbit non-spinning extreme-mass-ratio inspirals

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-12T21:08:18.231603Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c213eb2a-8814-4774-bfa8-3e192d206300 · outbound

This paper cites High-order post-Newtonian expansion of the generalized redshift invariant for eccentric-orbit, equatorial extreme-mass-ratio inspirals with a spinning primary.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals High-order post-Newtonian expansion of the generalized redshift invariant for eccentric-orbit, equatorial extreme-mass-ratio inspirals with a spinning primary

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-12T21:08:18.236145Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d753f9c4-8b9f-40e3-9492-d6aea52a30cb · outbound

This paper cites Gravitational Waves from a Particle Orbiting Around a Rotating Black Holes: Post-Newtonian Expansion.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals Gravitational Waves from a Particle Orbiting Around a Rotating Black Holes: Post-Newtonian Expansion

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-12T21:08:18.241194Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bc38e6c4-416a-48e5-8c74-8ff26374e451 · outbound

This paper cites an unresolved cited work.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals Unresolved cited work

Reference 31

Resolution: unresolved; raw_fallback, observed 2026-08-12T21:08:19.090784Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation f88a527d-c871-48d5-9e73-040b33f1cb33 · outbound

This paper cites Intermediate and Extreme Mass-Ratio Inspirals -- Astrophysics, Science Applications and Detection using LISA.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals Intermediate and Extreme Mass-Ratio Inspirals -- Astrophysics, Science Applications and Detection using LISA

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-12T21:08:18.252376Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 94f7875c-abfc-47fa-84ba-6399e072c2b7 · outbound

This paper cites Research Update on Extreme-Mass-Ratio Inspirals.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals Research Update on Extreme-Mass-Ratio Inspirals

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-12T21:08:18.257280Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a35897fc-0207-419c-a919-653747ea6a75 · outbound

This paper cites Post-Newtonian expansion of gravitational energy and angular momentum fluxes: inclined spherical orbits about a Kerr black hole.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals Post-Newtonian expansion of gravitational energy and angular momentum fluxes: inclined spherical orbits about a Kerr black hole

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-12T21:08:18.262035Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cc80397a-d23e-46f5-8fd8-ef68043be119 · outbound

This paper cites Self-forced inspirals with spin-orbit precession.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals Self-forced inspirals with spin-orbit precession

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-12T21:08:18.268578Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation df05d248-066f-4a1c-8c46-1dc98afa45c3 · outbound

This paper cites A Comparison of search templates for gravitational waves from binary inspiral.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals A Comparison of search templates for gravitational waves from binary inspiral

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-12T21:08:18.273866Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 462e55a0-711d-4993-a9a7-7c207c2dfdfd · outbound

This paper cites Comparison of post-Newtonian templates for compact binary inspiral signals in gravitational-wave detectors.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals Comparison of post-Newtonian templates for compact binary inspiral signals in gravitational-wave detectors

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-12T21:08:18.278501Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 71378598-d321-4fc7-80d9-af594bdba01b · outbound

This paper cites Comparison of post-Newtonian templates for extreme mass ratio inspirals.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals Comparison of post-Newtonian templates for extreme mass ratio inspirals

Reference 38

Resolution: verified exact; local_arxiv, observed 2026-08-12T21:08:18.640906Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 5a81cbfe-23b4-40d2-b472-401ead6897ff · outbound

This paper cites High-accuracy comparison of numerical relativity simulations with post-Newtonian expansions.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals High-accuracy comparison of numerical relativity simulations with post-Newtonian expansions

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-12T21:08:18.290015Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 31b7fb85-3485-4879-9599-bf7d63610c2d · outbound

This paper cites Ineffectiveness of Pad\'e resummation techniques in post-Newtonian approximations.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals Ineffectiveness of Pad\'e resummation techniques in post-Newtonian approximations

Reference 40

Resolution: verified exact; local_arxiv, observed 2026-08-12T21:08:18.605150Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation cc406892-12ba-4983-943b-ae3ead476e3d · outbound

This paper cites Measuring gravitational waves from binary black hole coalescences: II. the waves' information and its extraction, with and without templates.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals Measuring gravitational waves from binary black hole coalescences: II. the waves' information and its extraction, with and without templates

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-12T21:08:18.301198Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation de89cca9-5254-464d-b062-f40f948eaa76 · outbound

This paper cites Model Waveform Accuracy Standards for Gravitational Wave Data Analysis.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals Model Waveform Accuracy Standards for Gravitational Wave Data Analysis

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-12T21:08:18.305889Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0f077490-8e3a-45b2-91b9-00ef266729de · outbound

This paper cites Extreme mass-ratio inspirals around a spinning horizonless compact object.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals Extreme mass-ratio inspirals around a spinning horizonless compact object

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-12T21:08:18.310609Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 50146948-8125-4164-9e6b-fe6dbe2a4010 · outbound

This paper cites Improved filters for gravitational waves from inspiralling compact binaries.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals Improved filters for gravitational waves from inspiralling compact binaries

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-12T21:08:18.315394Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d0dd51e7-6714-4254-9f2b-88ade230a061 · outbound

This paper cites Improved resummation of post-Newtonian multipolar waveforms from circularized compact binaries.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals Improved resummation of post-Newtonian multipolar waveforms from circularized compact binaries

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-12T21:08:18.320634Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3cc3a6c8-8511-476d-bd9a-0d80eb06ffe2 · outbound

This paper cites The construction and use of LISA sensitivity curves.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals The construction and use of LISA sensitivity curves

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-12T21:08:18.324995Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3ba55963-9977-493d-8a6f-03af585e1565 · outbound

This paper cites Probing horizon scale quantum effects with Love.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals Probing horizon scale quantum effects with Love

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-12T21:08:18.329171Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9180b938-0ce5-4cc8-9710-918844e2f857 · outbound

This paper cites Faithful Effective-One-Body waveforms of small-mass-ratio coalescing black-hole binaries.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals Faithful Effective-One-Body waveforms of small-mass-ratio coalescing black-hole binaries

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-12T21:08:18.333973Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4dae310a-93d7-45d4-ac7b-bafe330749b5 · outbound

This paper cites Comparing Effective-One-Body gravitational waveforms to accurate numerical data.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals Comparing Effective-One-Body gravitational waveforms to accurate numerical data

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-12T21:08:18.338345Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e50fc89b-de62-4847-a930-44692cde7e5b · outbound

This paper cites Post-Newtonian factorized multipolar waveforms for spinning, non-precessing black-hole binaries.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals Post-Newtonian factorized multipolar waveforms for spinning, non-precessing black-hole binaries

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-12T21:08:18.344431Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c63670cf-9a2f-438b-934b-02dafdb516d2 · outbound

This paper cites Impact of the second order self-forces on the dephasing of the gravitational waves from quasi-circular extreme mass-ratio inspirals.

Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals Impact of the second order self-forces on the dephasing of the gravitational waves from quasi-circular extreme mass-ratio inspirals

Reference 51

Resolution: verified exact; local_arxiv, observed 2026-08-12T21:08:18.411400Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Pith citing papers

Observation a5b494ff-aa8b-4075-b9dd-bdc02481ed92 · inbound

Post-Newtonian expansion of gravitational energy and angular momentum fluxes: inclined spherical orbits about a Kerr black hole cites this paper.

Post-Newtonian expansion of gravitational energy and angular momentum fluxes: inclined spherical orbits about a Kerr black hole Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-12T20:28:15.018325Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 287055cf-a023-493b-92a6-b4e3d2fadc7e · 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 Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-03T02:31:00.550181Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d5a95f2e-3342-4e8a-8f4a-2921488d315a · inbound

Efficient and Stable Computation of Gravitational-Wave Fluxes from Generic Kerr Orbits via a Unified HeunC Framework cites this paper.

Efficient and Stable Computation of Gravitational-Wave Fluxes from Generic Kerr Orbits via a Unified HeunC Framework Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals

Reference 76

Resolution: verified exact; arxiv_id, observed 2026-05-12T03:06:19.372922Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 71d556e1-b50e-4e1e-8563-a3ff5fc49cd9 · inbound

Efficient and Stable Computation of Gravitational-Wave Fluxes from Generic Kerr Orbits via a Unified HeunC Framework cites this paper.

Reference 76

Resolution: verified exact; arxiv_id, observed 2026-05-13T07:47:32.613387Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 62e0961f-b4bb-4784-9bbc-68030475b420 · inbound

Efficient and Stable Computation of Gravitational-Wave Fluxes from Generic Kerr Orbits via a Unified HeunC Framework cites this paper.

Reference 76

Resolution: verified exact; arxiv_id, observed 2026-07-01T13:35:45.733406Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.