• black hole spectroscopy
• black holes
• gravitational waves
• higher modes
• ringdown

The last phase of black hole binary coalescences is known as the ringdown, in which the newly formed black hole relaxes to its stationary state by emitting gravitational waves. Ringdown studies provides a unique way to study gravity in extreme curvature regime and understand the nature of black holes. The linear theory of black hole perturbations predicts that the ringdown consists of a sum of different modes of vibration, which are exponentially damped harmonics oscillations projected onto spherical harmonics. The excitation of the different modes depends on the specific process that perturbs the black hole, and for quasi-circular binary coalescences the fundamental mode dominates the ringdown emission. Besides, asymmetries in the system can excite higher subdominant modes of vibration. The measurement of the frequencies and damping times of these higher modes allows to test general relativity by comparing the predicted values against the observations.
We describe the first time domain analysis with an effective one-body ringdown model on the third catalog of gravitational waves events GWTC-3, both for parameters estimation and to assess the detectability of higher modes in the events. This work sets the bases towards the positive identification and characterisation of higher modes in the ringdown signals with future, more sensitive gravitational wave detectors, and opens the concrete possibility of conducting multimodal tests of general relativity in the strong field regime.