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Cited article:

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Formation and evolution of binary black holes in N-body simulations of star clusters with up to two million stars

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Monthly Notices of the Royal Astronomical Society 538 (2) 639 (2025)
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No evidence that the binary black hole mass distribution evolves with redshift

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Pair-instability Gap Black Holes in Population III Star Clusters: Pathways, Dynamics, and Gravitational-wave Implications

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No Need to Know: Toward Astrophysics-free Gravitational-wave Cosmology

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Binary black hole mergers from Population III star clusters

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Astronomy & Astrophysics 690 A106 (2024)
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Exploring Field-evolution and Dynamical-capture Coalescing Binary Black Holes in GWTC-3

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Gravitational waves from mergers of Population III binary black holes: roles played by two evolution channels

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Monthly Notices of the Royal Astronomical Society 534 (3) 1634 (2024)
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