Skip to main content

Thank you for visiting nature.com. You are using a browser version with limited support for CSS. To obtain the best experience, we recommend you use a more up to date browser (or turn off compatibility mode in Internet Explorer). In the meantime, to ensure continued support, we are displaying the site without styles and JavaScript.

  • Article
  • Published:

A practical Bayesian method for gravitational-wave ringdown analysis with multiple modes

Abstract

Gravitational-wave (GW) ringdown signals from black holes encode crucial information about the gravitational dynamics in the strong-field regime, which offers unique insights into the properties of black holes. Improving the sensitivity of GW detectors will enable the extraction of several quasi-normal modes from ringdown signals. However, incorporating several modes drastically enlarges the parameter space, posing computational challenges to data analysis. Inspired by the \({\mathcal{F}}\)-statistic method in the continuous GW searches, here we develop an algorithm that enhances the parameter-marginalization scheme, dubbed FIREFLY, which is tailored for accelerating the ringdown signal analysis. FIREFLY analytically marginalizes the amplitude and phase parameters of quasi-normal modes to reduce the computational cost and to speed up the standard Bayesian inference with full parameters from hours to minutes while achieving consistent posterior and evidence. The acceleration becomes more pronounced when more quasi-normal modes are considered. Rigorously based on Bayesian inference and importance sampling, our method is statistically interpretable, flexible in prior choice and compatible with various advanced sampling techniques and, thus, provides a new perspective for accelerating future GW data analysis.

This is a preview of subscription content, access via your institution

Access options

Buy this article

USD 39.95

Prices may be subject to local taxes which are calculated during checkout

Fig. 1: Workflow of FIREFLY.
Fig. 2: Posteriors of the N = 3 scenario in the overtone analysis.
Fig. 3: P-P plots for the overtone analysis.
Fig. 4: Evidences given by FIREFLY and the full-parameter sampling.
Fig. 5: Joint posteriors of the final mass and the final spin with different starting times in the higher-mode analysis.

Similar content being viewed by others

Data availability

The data used in this study can be found in the public SXS Gravitational Waveform Database at https://data.black-holes.org/ (object IDs SXS:BBH:0305 and SXS:BBH:0065). Source data are provided with this paper.

Code availability

The code FIREFLY is publicly available via GitHub at https://github.com/Yiming-astro/Firefly-ringdown. This repository provides all materials needed to reproduce the results of this study.

References

  1. Abbott, B. P. et al. Observation of gravitational waves from a binary black hole merger. Phys. Rev. Lett. 116, 061102 (2016).

    Article  ADS  MathSciNet  Google Scholar 

  2. Abbott, B. P. et al. Tests of general relativity with GW150914. Phys. Rev. Lett. 116, 221101 (2016); erratum 121, 129902 (2018).

    Article  ADS  Google Scholar 

  3. Abbott, R. et al. Tests of general relativity with GWTC-3. Phys. Rev. D 112, 084080 (2025).

    Article  ADS  Google Scholar 

  4. Abbott, B. P. et al. A gravitational-wave standard siren measurement of the Hubble constant. Nature 551, 85–88 (2017).

    Article  ADS  Google Scholar 

  5. Abbott, B. P. et al. GW170817: measurements of neutron star radii and equation of state. Phys. Rev. Lett. 121, 161101 (2018).

    Article  ADS  Google Scholar 

  6. Abbott, R. et al. Population of merging compact binaries inferred using gravitational waves through GWTC-3. Phys. Rev. X 13, 011048 (2023).

    Google Scholar 

  7. Isi, M., Giesler, M., Farr, W. M., Scheel, M. A. & Teukolsky, S. A. Testing the no-hair theorem with GW150914. Phys. Rev. Lett. 123, 111102 (2019).

    Article  ADS  Google Scholar 

  8. Isi, M., Farr, W. M., Giesler, M., Scheel, M. A. & Teukolsky, S. A. Testing the black-hole area law with GW150914. Phys. Rev. Lett. 127, 011103 (2021).

    Article  ADS  Google Scholar 

  9. Cardoso, V., Franzin, E. & Pani, P. Is the gravitational-wave ringdown a probe of the event horizon? Phys. Rev. Lett. 116, 171101 (2016) ; erratum 117, 089902 (2016).

    Article  ADS  Google Scholar 

  10. Teukolsky, S. A. Perturbations of a rotating black hole. 1. Fundamental equations for gravitational electromagnetic and neutrino field perturbations. Astrophys. J. 185, 635–647 (1973).

    Article  ADS  Google Scholar 

  11. Berti, E., Cardoso, J., Cardoso, V. & Cavaglia, M. Matched-filtering and parameter estimation of ringdown waveforms. Phys. Rev. D 76, 104044 (2007).

    Article  ADS  Google Scholar 

  12. Dreyer, O. et al. Black hole spectroscopy: testing general relativity through gravitational wave observations. Class. Quantum Grav. 21, 787–804 (2004).

    Article  ADS  Google Scholar 

  13. Christensen, N. & Meyer, R. Markov chain Monte Carlo methods for Bayesian gravitational radiation data analysis. Phys. Rev. D 58, 082001 (1998).

    Article  ADS  Google Scholar 

  14. Sharma, S. Markov chain Monte Carlo methods for Bayesian data analysis in astronomy. Ann. Rev. Astron. Astrophys. 55, 213–259 (2017).

    Article  ADS  Google Scholar 

  15. Skilling, J. Nested sampling. AIP Conf. Proc. 735, 395 (2004).

    Article  ADS  MathSciNet  Google Scholar 

  16. Skilling, J. Nested sampling for general Bayesian computation. Bayesian Anal. 1, 833–859 (2006).

    Article  MathSciNet  Google Scholar 

  17. Abac, A. et al. The science of the Einstein Telescope. Preprint at http://arxiv.org/abs/2503.12263 (2025).

  18. Hu, Q. & Veitch, J. Costs of Bayesian parameter estimation in third-generation gravitational wave detectors: an assessment of current acceleration methods. Phys. Rev. D 112, 084039 (2025).

    Article  ADS  Google Scholar 

  19. Reitze, D. et al. Cosmic Explorer: the U.S. contribution to gravitational-wave astronomy beyond LIGO. Bull. Am. Astron. Soc. 51, 035 (2019).

    Google Scholar 

  20. Reitze, D. et al. The US program in ground-based gravitational wave science: contribution from the LIGO laboratory. Bull. Am. Astron. Soc. 51, 141 (2019).

    Google Scholar 

  21. Punturo, M. et al. The Einstein Telescope: a third-generation gravitational wave observatory. Class. Quantum Grav. 27, 194002 (2010).

    Article  ADS  Google Scholar 

  22. Hild, S. et al. Sensitivity studies for third-generation gravitational wave observatories. Class. Quantum Grav. 28, 094013 (2011).

    Article  ADS  Google Scholar 

  23. Amaro-Seoane, P. et al. Laser interferometer space antenna. Preprint at http://arxiv.org/abs/1702.00786 (2017).

  24. Hu, W.-R. & Wu, Y.-L. The Taiji Program in Space for gravitational wave physics and the nature of gravity. Natl Sci. Rev. 4, 685–686 (2017).

    Article  Google Scholar 

  25. Luo, J. et al. TianQin: a space-borne gravitational wave detector. Class. Quantum Grav. 33, 035010 (2016).

    Article  ADS  Google Scholar 

  26. Bhagwat, S., Pacilio, C., Barausse, E. & Pani, P. Landscape of massive black-hole spectroscopy with LISA and the Einstein Telescope. Phys. Rev. D 105, 124063 (2022).

    Article  ADS  Google Scholar 

  27. Bhagwat, S., Pacilio, C., Pani, P. & Mapelli, M. Landscape of stellar-mass black-hole spectroscopy with third-generation gravitational-wave detectors. Phys. Rev. D 108, 043019 (2023).

    Article  ADS  Google Scholar 

  28. Pitte, C., Baghi, Q., Besançon, M. & Petiteau, A. Exploring tests of the no-hair theorem with LISA. Phys. Rev. D 110, 104003 (2024).

    Article  ADS  MathSciNet  Google Scholar 

  29. Berti, E., Cardoso, V. & Starinets, A. O. Quasinormal modes of black holes and black branes. Class. Quantum Grav. 26, 163001 (2009).

    Article  ADS  MathSciNet  Google Scholar 

  30. Bhagwat, S., Forteza, X. J., Pani, P. & Ferrari, V. Ringdown overtones, black hole spectroscopy, and no-hair theorem tests. Phys. Rev. D 101, 044033 (2020).

    Article  ADS  MathSciNet  Google Scholar 

  31. Jaranowski, P., Krolak, A. & Schutz, B. F. Data analysis of gravitational-wave signals from spinning neutron stars. 1. The signal and its detection. Phys. Rev. D 58, 063001 (1998).

    Article  ADS  Google Scholar 

  32. Wang, H.-T., Yim, G., Chen, X. & Shao, L. Gravitational wave ringdown analysis using the F-statistic. Astrophys. J. 974, 230 (2024).

    Article  ADS  Google Scholar 

  33. Wang, H.-T., Wang, Z., Dong, Y., Yim, G. & Shao, L. Reanalyzing the ringdown signal of GW150914 using the F-statistic method. Phys. Rev. D 111, 064037 (2025).

    Article  ADS  MathSciNet  Google Scholar 

  34. Prix, R. Bayesian QNM search on GW150914. LIGO Document T1500618-v4 (LIGO, 2016); https://dcc.ligo.org/LIGO-T1500618/public

  35. Isi, M. & Farr, W. M. Analyzing black-hole ringdowns. Preprint at http://arxiv.org/abs/2107.05609 (2021).

  36. Prix, R. & Krishnan, B. Targeted search for continuous gravitational waves: Bayesian versus maximum-likelihood statistics. Class. Quantum Grav. 26, 204013 (2009).

    Article  ADS  Google Scholar 

  37. Ashok, A., Covas, P. B., Prix, R. & Papa, M. A. Bayesian F-statistic-based parameter estimation of continuous gravitational waves from known pulsars. Phys. Rev. D 109, 104002 (2024).

    Article  ADS  MathSciNet  Google Scholar 

  38. Gabbard, H., Messenger, C., Heng, I. S., Tonolini, F. & Murray, R. Bayesian parameter estimation using conditional variational autoencoders for gravitational-wave astronomy. Nat. Phys. 18, 112–117 (2022).

    Article  Google Scholar 

  39. Dax, M. et al. Real-time gravitational wave science with neural posterior estimation. Phys. Rev. Lett. 127, 241103 (2021).

    Article  ADS  Google Scholar 

  40. Dax, M. et al. Neural importance sampling for rapid and reliable gravitational-wave inference. Phys. Rev. Lett. 130, 171403 (2023).

    Article  ADS  Google Scholar 

  41. Pacilio, C., Bhagwat, S. & Cotesta, R. Simulation-based inference of black hole ringdowns in the time domain. Phys. Rev. D 110, 083010 (2024).

    Article  ADS  Google Scholar 

  42. Robert, C. P. & Casella, G. Monte Carlo Statistical Methods (Springer, 2004).

  43. Boyle, M. et al. The SXS Collaboration catalog of binary black hole simulations. Class. Quantum Grav. 36, 195006 (2019).

    Article  ADS  Google Scholar 

  44. Higson, E., Handley, W., Hobson, M. & Lasenby, A. Dynamic nested sampling: an improved algorithm for parameter estimation and evidence calculation. Stat. Comput. 29, 891 (2019).

    Article  MathSciNet  Google Scholar 

  45. Ashton, G. et al. Bilby: a user-friendly Bayesian inference library for gravitational-wave astronomy. Astrophys. J. Suppl. Ser. 241, 27 (2019).

    Article  ADS  Google Scholar 

  46. Giesler, M., Isi, M., Scheel, M. A. & Teukolsky, S. Black hole ringdown: the importance of overtones. Phys. Rev. X 9, 041060 (2019).

    Google Scholar 

  47. Peyré, G. & Cuturi, M. Computational optimal transport: with applications to data science. Found. Trends Mach. Learn. 11, 355–607 (2019).

    Article  Google Scholar 

  48. Wang, Y., Shang, Y. & Babak, S. EMRI data analysis with a phenomenological waveform. Phys. Rev. D 86, 104050 (2012).

    Article  ADS  Google Scholar 

  49. Hu, Q. & Veitch, J. Rapid premerger localization of binary neutron stars in third-generation gravitational-wave detectors. Astrophys. J. Lett. 958, L43 (2023).

    Article  ADS  Google Scholar 

  50. Berti, E. & Klein, A. Mixing of spherical and spheroidal modes in perturbed Kerr black holes. Phys. Rev. D 90, 064012 (2014).

    Article  ADS  Google Scholar 

  51. Finn, L. S. Detection, measurement and gravitational radiation. Phys. Rev. D 46, 5236–5249 (1992).

    Article  ADS  Google Scholar 

  52. Loredo, T. J. & Wolpert, R. L. Bayesian inference: more than Bayes’s theorem. Front. Astron. Space Sci. 11, 1326926 (2024).

    Article  ADS  Google Scholar 

  53. Thrane, E. & Talbot, C. An introduction to Bayesian inference in gravitational-wave astronomy: parameter estimation, model selection, and hierarchical models. Publ. Astron. Soc. Aust. 36, e010 (2019); erratum 37, e036 (2020).

    Article  ADS  Google Scholar 

  54. Tokdar, S. T. & Kass, R. E. Importance sampling: a review. Wiley Interdiscip. Rev.: Comput. Stat. 2, 54–60 (2010).

    Article  Google Scholar 

Download references

Acknowledgements

We thank H. W. Lee, H. Nakano and N. Uchikata for comments. This work was supported by the National Natural Science Foundation of China (Grant Nos. 123B2043 and 12573042), the Beijing Natural Science Foundation (1242018), the National SKA Program of China (Grant No. 2020SKA0120300), the Max Planck Partner Group Program funded by the Max Planck Society and the High-performance Computing Platform of Peking University. H.-T.W. and L.S. are supported by the Fundamental Research Funds for the Central Universities at Dalian University of Technology and Peking University, respectively. J.Z. is supported by the National Natural Science Foundation of China (Grant No. 12405052) and the Startup Research Fund of Henan Academy of Sciences (Grant No. 241841220).

Author information

Authors and Affiliations

Authors

Contributions

Y.D. and Z.W. contributed equally to the work, namely to the design and programming of the FIREFLY code and writing the initial draft of the paper. H.-T.W. contributed to the \({\mathcal{F}}\)-statistic-based method and developed preliminary sampling codes for the ringdown analysis. J.Z. contributed to the Bayesian analysis and sampling implementation. L.S. contributed to the design and methodology of FIREFLY and writing the paper and supervised and coordinated the whole project. All co-authors discussed the results and provided input to the data analysis and the content of the paper.

Corresponding author

Correspondence to Lijing Shao.

Ethics declarations

Competing interests

The authors declare no competing interests.

Peer review

Peer review information

Nature Astronomy thanks the anonymous reviewers for their contribution to the peer review of this work.

Additional information

Publisher’s note Springer Nature remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.

Supplementary information

Supplementary Information (download PDF )

Supplementary Figs. 1–9, section (Zero-noise injection) and Table 1.

Supplementary Data 1 (download ZIP )

Source Data for Supplementary Figs. 1–6 and 8–9.

Source data

Source Data Fig. 2 (download XLSX )

Statistical source data for Fig. 2.

Source Data Fig. 3 (download XLSX )

Statistical source data for Fig. 3.

Source Data Fig. 4 (download XLSX )

Statistical source data for Fig. 4.

Source Data Fig. 5 (download XLSX )

Statistical source data for Fig. 5.

Rights and permissions

Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law.

Reprints and permissions

About this article

Check for updates. Verify currency and authenticity via CrossMark

Cite this article

Dong, Y., Wang, Z., Wang, HT. et al. A practical Bayesian method for gravitational-wave ringdown analysis with multiple modes. Nat Astron (2026). https://doi.org/10.1038/s41550-025-02766-6

Download citation

  • Received:

  • Accepted:

  • Published:

  • Version of record:

  • DOI: https://doi.org/10.1038/s41550-025-02766-6

Search

Quick links

Nature Briefing

Sign up for the Nature Briefing newsletter — what matters in science, free to your inbox daily.

Get the most important science stories of the day, free in your inbox. Sign up for Nature Briefing