Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency | Paper Citation Record

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Unresolved cited work

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Unresolved cited work

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Unresolved cited work

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Unresolved cited work

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Unresolved cited work

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This paper cites ˆL· ˆN 1−( ˆL· ˆN)2 # (ˆL× ˆN)· ˆdL d f =.

Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency ˆL· ˆN 1−( ˆL· ˆN)2 # (ˆL× ˆN)· ˆdL d f =

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Observation bdf46c74-0edb-4a7f-9396-c60cecbdcc04 · outbound

This paper cites Abbott, R.

Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Abbott, R

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Unresolved cited work

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Observation f804f28e-6da9-4b73-a099-f7177d82c375 · outbound

This paper cites Acernese, M.

Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Acernese, M

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

Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency org/superevents/public/O4/(2025)

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

Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency GWTC-4.0: Updating the Gravitational-Wave Transient Catalog with Observations from the First Part of the Fourth LIGO-Virgo-KAGRA Observing Run

Reference 12

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This paper cites Somiya, Classical and Quantum Gravity29, 124007 (2012).

Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Somiya, Classical and Quantum Gravity29, 124007 (2012)

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Unresolved cited work

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Akutsu, M

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Maggiore, C

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This paper cites A Horizon Study for Cosmic Explorer: Science, Observatories, and Community.

Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency A Horizon Study for Cosmic Explorer: Science, Observatories, and Community

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This paper cites Current status of space gravitational wave antenna DECIGO and B-DECIGO.

Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Current status of space gravitational wave antenna DECIGO and B-DECIGO

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Laser Interferometer Space Antenna

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This paper cites Hanna, S.

Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Hanna, S

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Messick, K

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This paper cites GstLAL: A software framework for gravitational wave discovery.

Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency GstLAL: A software framework for gravitational wave discovery

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This paper cites Low-latency analysis pipeline for compact binary coalescences in the advanced gravitational wave detector era.

Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Low-latency analysis pipeline for compact binary coalescences in the advanced gravitational wave detector era

Reference 23

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency The MBTA Pipeline for Detecting Compact Binary Coalescences in the Third LIGO-Virgo Observing Run

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Unresolved cited work

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Unresolved cited work

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Klimenko and G

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Klimenko, G

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Unresolved cited work

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Unresolved cited work

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency The population of merging compact binaries inferred using gravitational waves through GWTC-3

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Unresolved cited work

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Unresolved cited work

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Cutler and E

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Unresolved cited work

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Unresolved cited work

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Computationally efficient models for the dominant and sub-dominant harmonic modes of precessing binary black holes

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Ossokine, A

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Varma, S

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Understanding how fast black holes spin by analysing data from the second gravitational-wave catalogue

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Damour, Phys

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Racine, Phys

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Hannam, P

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Observation 1ed050c5-786b-4ace-aacf-bf7a83905681 · outbound

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Schmidt, F

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency A generalized precession parameter $\chi_\mathrm{p}$ to interpret gravitational-wave data

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Gangardt, N

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency When will we observe binary black holes precessing?

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Two-harmonic approximation for gravitational waveforms from precessing binaries

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Rarity of precession and higher-order multipoles in gravitational waves from merging binary black holes

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Lindblom, B

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Planck 2018 results. VI. Cosmological parameters

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Unresolved cited work

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Takahashi and T

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Unresolved cited work

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Poisson and C

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Bildsten and C

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Kesden, D

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Gerosa, M

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Unresolved cited work

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Unresolved cited work

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Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Unresolved cited work

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This paper cites Physics, Astrophysics and Cosmology with Gravitational Waves.

Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Physics, Astrophysics and Cosmology with Gravitational Waves

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Observation 0526dc8b-f06e-4723-9048-d356980ff0bc · outbound

This paper cites Distinguishing black-hole spin-orbit resonances by their gravitational-wave signatures.

Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Distinguishing black-hole spin-orbit resonances by their gravitational-wave signatures

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-04T17:49:18.630456Z

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Observation 83c77a1b-6a6b-48c0-a5c2-77d204600711 · outbound

This paper cites Efficient multi-timescale dynamics of precessing black-hole binaries.

Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Efficient multi-timescale dynamics of precessing black-hole binaries

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-04T17:49:18.634847Z

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Observation a4afdb40-2d75-4cc4-b904-9209c16b32aa · outbound

This paper cites Systematic biases due to waveform mismodeling in parametrized post-Einsteinian tests of general relativity: The impact of neglecting spin precession and higher modes.

Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Systematic biases due to waveform mismodeling in parametrized post-Einsteinian tests of general relativity: The impact of neglecting spin precession and higher modes

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-04T17:49:18.639309Z

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Observation c9bc195b-c72d-4ade-a1d9-5221d1aa9b42 · outbound

This paper cites Singh, M.

Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Singh, M

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-04T17:49:18.643779Z

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Observation 5c3a4e75-5f65-4f66-8a56-267c4b14d7c3 · outbound

This paper cites Relativistic Binaries in Globular Clusters.

Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Relativistic Binaries in Globular Clusters

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-04T17:49:18.648014Z

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Observation 5a577fb9-e84d-4505-928d-6665e292e3b5 · outbound

This paper cites Illuminating Black Hole Binary Formation Channels with Spins in Advanced LIGO.

Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Illuminating Black Hole Binary Formation Channels with Spins in Advanced LIGO

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-04T17:49:18.652579Z

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Observation 6856b327-c4c2-405f-9708-470bf4f84781 · outbound

This paper cites Kalogera, Astrophys.

Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Kalogera, Astrophys

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-04T17:49:18.656953Z

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Observation 3d3be85d-152a-4126-a52d-f12c7d35b00a · outbound

This paper cites The Evolution of Compact Binary Star Systems.

Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency The Evolution of Compact Binary Star Systems

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-04T17:49:18.661024Z

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Observation b7c5dc3e-e960-459d-bdfe-a66a0253ceaa · outbound

This paper cites Hierarchical mergers of stellar-mass black holes and their gravitational-wave signatures.

Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Hierarchical mergers of stellar-mass black holes and their gravitational-wave signatures

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-04T17:49:18.665445Z

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Observation e3b7bff1-bbd8-437d-8759-3d1bca365ffe · outbound

This paper cites Signatures of spin precession and nutation in isolated black-hole binaries.

Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Signatures of spin precession and nutation in isolated black-hole binaries

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-04T17:49:18.669940Z

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Observation 44cf1e74-f6f1-45fb-8a0a-13de1485a99d · outbound

This paper cites Stanzione, B.

Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Stanzione, B

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-04T17:49:18.674422Z

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Observation 7fe49d10-6648-4336-bdb3-59851bb23e88 · outbound

This paper cites Astropy: A Community Python Package for Astronomy.

Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Astropy: A Community Python Package for Astronomy

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-04T17:49:18.678636Z

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Observation cbc5a885-2df4-4351-a2b4-65419106b060 · outbound

This paper cites The Astropy Project: Building an inclusive, open-science project and status of the v2.0 core package.

Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency The Astropy Project: Building an inclusive, open-science project and status of the v2.0 core package

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-04T17:49:18.682796Z

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Observation d71a3181-a48e-487d-b6c5-8de2e04ddab6 · outbound

This paper cites The Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package.

Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency The Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-04T17:49:18.687135Z

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Observation d7920110-4a8f-4484-a4c1-bfa98b369fe7 · outbound

This paper cites an unresolved cited work.

Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Unresolved cited work

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-04T17:49:18.691294Z

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Observation f6861b4f-670d-49cd-a7e1-d789a06e3f13 · outbound

This paper cites an unresolved cited work.

Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Unresolved cited work

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-04T17:49:18.695338Z

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Observation 19527816-1f96-4863-a866-e549bba9dc99 · outbound

This paper cites Virtanen, R.

Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Virtanen, R

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-04T17:49:18.699373Z

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Observation 5b694295-9a81-49ae-b789-73af31c19532 · outbound

This paper cites Gommers, P.

Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Gommers, P

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-04T17:49:18.703488Z

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Observation e8fb9cf9-add6-4910-8c18-9be276603193 · outbound

This paper cites PRECESSION: Dynamics of spinning black-hole binaries with python.

Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency PRECESSION: Dynamics of spinning black-hole binaries with python

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-04T17:49:18.707569Z

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Observation edc218e4-be10-4bc0-9931-82be66534853 · outbound

This paper cites Wagg and F.

Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Wagg and F

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-04T17:49:18.712037Z

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Observation c5c11d5c-9efd-4aab-a1a9-166a5e35033e · outbound

This paper cites an unresolved cited work.

Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Unresolved cited work

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-04T17:49:18.716067Z

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Observation ff029858-44a2-44e1-b4eb-b16bdc9d1454 · outbound

This paper cites an unresolved cited work.

Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Unresolved cited work

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-04T17:49:18.720231Z

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Observation f4e94f97-52f8-408f-9a1a-3bab5b1352e1 · outbound

This paper cites Chatziioannou, A.

Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Chatziioannou, A

Reference 85

Resolution: unresolved; no resolver link, observed 2026-08-04T17:49:18.724264Z

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Observation 48869a9d-190c-4cb9-b0de-107ea38f247a · outbound

This paper cites an unresolved cited work.

Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Unresolved cited work

Reference 86

Resolution: unresolved; no resolver link, observed 2026-08-04T17:49:18.728383Z

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