| Issue |
A&A
Volume 706, February 2026
|
|
|---|---|---|
| Article Number | A361 | |
| Number of page(s) | 10 | |
| Section | Extragalactic astronomy | |
| DOI | https://doi.org/10.1051/0004-6361/202557376 | |
| Published online | 20 February 2026 | |
Expect the unexpected: Augmented mixture models for black-hole-population studies
Institut für Theoretische Astrophysik, ZAH, Universität Heidelberg Albert-Ueberle-Str. 2 69120 Heidelberg, Germany
★ Corresponding author: This email address is being protected from spambots. You need JavaScript enabled to view it.
Received:
23
September
2025
Accepted:
8
January
2026
Context. Black-hole-population studies are currently performed either using astrophysically motivated models (informed but rigid in their functional forms) or via non-parametric methods (flexible, but not directly interpretable).
Aims. In this paper, we present a statistical framework to complement the predictive power of astrophysically motivated models with the flexibility of non-parametric methods.
Methods. Our method makes use of the Dirichlet distribution to robustly infer the relative weights of different models as well as of the Gibbs sampling approach to efficiently explore the parameter space.
Results. After having validated our approach using simulated data, we applied this method to the binary black-hole mergers observed during the first three observing runs of the LIGO-Virgo-KAGRA collaboration using both phenomenological and astrophysical models as parametric models, finding results in agreement with the currently available literature.
Key words: gravitational waves / methods: statistical / stars: black holes
© The Authors 2026
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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