Analysis of GWTC-3 with multiple quasicircular models
gr-qc, astro-ph.HE
Submitted: 2026-09-14
Updated: 2026-09-14
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Advanced LIGO
- Advanced Virgo: a 2nd generation interferometric gravitational wave detector
- Overview of KAGRA: Detector design and construction history
- Observation of Gravitational Waves from a Binary Black Hole Merger
- Binary Black Hole Mergers in the first Advanced LIGO Observing Run
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- Observation of gravitational waves from two neutron star-black hole coalescences
- GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run
- GWTC-2.1: Deep Extended Catalog of Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run
- GWTC-4.0: Updating the Gravitational-Wave Transient Catalog with Observations from the First Part of the Fourth LIGO-Virgo-KAGRA Observing Run
- GWTC-5.0: Observations from the Second Part of the Fourth LIGO-Virgo-KAGRA Observing Run and Updates to the Gravitational-Wave Transient Catalog
- GWTC-4.0: Methods for Identifying and Characterizing Gravitational-wave Transients
- Expanding RIFT: Improving performance for GW parameter inference
- Enriching the Symphony of Gravitational Waves from Binary Black Holes by Tuning Higher Harmonics
- Multipolar Effective-One-Body Waveforms for Precessing Binary Black Holes: Construction and Validation
- Computationally efficient models for the dominant and sub-dominant harmonic modes of precessing binary black holes
- GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run
- Analysis of GWTC-3 with fully precessing numerical relativity surrogate models
- Systematic challenges for future gravitational wave measurements of precessing binary black holes
- Impact of subdominant modes on the interpretation of gravitational-wave signals from heavy binary black hole systems
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