Finite signal-to-noise ratio bias in parameter estimation for damped oscillations: cautionary remark about catalog-level black-hole spectroscopy
Koutarou Kyutoku
gr-qc, astro-ph.HE
Submitted: 2026-07-06
Comments: 7 pages, 2 figures, a Mathematica file attached
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Black Hole Spectroscopy: Testing General Relativity through Gravitational Wave Observations
- Black hole spectroscopy: from theory to experiment
- Quasinormal modes of black holes and black branes
- Tests of general relativity with GW150914
- Tests of General Relativity with Binary Black Holes from the second LIGO-Virgo Gravitational-Wave Transient Catalog
- Tests of General Relativity with GWTC-3
- GWTC-4.0: Tests of General Relativity. III. Tests of the Remnants
- Catalog variance of testing general relativity with gravitational-wave data
- Challenges testing the no-hair theorem with gravitational waves
- Black Hole Spectroscopy: Systematic Errors and Ringdown Energy Estimates
- Analyzing black-hole ringdowns
- Quantifying Systematic Biases in Black Hole Spectroscopy
- Use and Abuse of the Fisher Information Matrix in the Assessment of Gravitational-Wave Parameter-Estimation Prospects
- Gravitational Waves from Mergin Compact Binaries: How Accurately Can One Extract the Binary's Parameters from the Inspiral Waveform?
- Mining information from binary black hole mergers: a comparison of estimation methods for complex exponentials in noise
- On gravitational-wave spectroscopy of massive black holes with the space interferometer LISA
- Ringdown overtones, black hole spectroscopy, and no-hair theorem tests
- Agnostic black hole spectroscopy: Quasinormal mode content of numerical relativity waveforms and limits of validity of linear perturbation theory
- Iterative extraction of overtones from black hole ringdown
- Striking the right tone: toward a self-consistent framework for measuring black hole ringdowns
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