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Systematic Biases in Estimating the Properties of Black Holes Due to Inaccurate Gravitational-Wave Models

Arnab Dhani ^1,*, Sebastian H. Völkel ¹, Alessandra Buonanno ^1,2, Hector Estelles ¹, Jonathan Gair ¹, Harald P. Pfeiffer¹, Lorenzo Pompili ¹, and Alexandre Toubiana¹

¹Max Planck Institute for Gravitational Physics (Albert Einstein Institute), Am Mühlenberg 1, Potsdam 14476, Germany
²Department of Physics, University of Maryland, College Park, Maryland 20742, USA

^*Contact author: arnab.dhani@aei.mpg.de

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Articles Citing

Systematic Biases in Estimating the Properties of Black Holes Due to Inaccurate Gravitational-Wave Models

Quasinormal Modes Ratios as Agnostic Test of General Relativity

Adding equatorial-asymmetric effects for spin-precessing binaries into the seobnrv5phm waveform model

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Challenges in the nonlinear evolution of unequal mass binaries in scalar-Gauss-Bonnet gravity

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Accounting for the known unknowns: A parametric framework to incorporate systematic waveform errors in gravitational-wave parameter estimation

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Systematic biases in parameter estimation on LISA binaries: The effect of excluding higher harmonics for non-spinning binaries

Applications of machine learning in gravitational-wave research with current interferometric detectors

GW241011 and GW241110: Exploring Binary Formation and Fundamental Physics with Asymmetric, High-spin Black Hole Coalescences

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