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From the 1 of 20 linked papers with an AI index.

activity
20242026
most citedEvidence of the pair instability gap from black hole masses

13 citations · 14 across the 4 of their papers we have counts for

collaborators

20 papers

astro-ph.HE20261 cited

Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop

Sofia Alvarez-Lopez, Jack Heinzel, Matthew Mould +1

The paper presents PixelPop, a high‑resolution Bayesian non‑parametric framework that captures multidimensional correlations among masses, spins, and redshifts of binary black hole…

astro-ph.HE2026

Joint population and strong-lensing inference for resolved gravitational-wave events probes the black-hole merger rate beyond the peak of star formation

Matthew Mould

Gravitational waves can be lensed by intervening potentials of various scales. Strong lensing leads to underestimated distances and overestimated masses, biasing astrophysical resu…

gr-qc2026

End-to-End Population Inference from Gravitational-Wave Strain using Transformers

Konstantin Leyde, Stephen R. Green, Maximilian Dax +3

The population of compact binaries encodes information about their astrophysical origins and the expansion of the universe. Hierarchical Bayesian methods infer these properties by…

astro-ph.HE202613 cited

Evidence of the pair instability gap from black hole masses

Hui Tong, Maya Fishbach, Eric Thrane +13

Stellar theory predicts a forbidden range of black-hole masses between -- due to pair-instability supernovae, but evidence for such a gap in the mass distri…

gr-qc2026

Gravitational-wave astronomy requires population-informed parameter estimation

Matthew Mould, Rodrigo Tenorio, Davide Gerosa

Gravitational-wave events are interpreted in terms of Bayesian posteriors for their source properties inferred under unphysical reference priors. Though these parameter estimates a…

astro-ph.HE2026

Measurement prospects for the pair-instability mass cutoff with gravitational waves

Matthew Mould, Jack Heinzel, Sofia Alvarez-Lopez +3

Pair-instability supernovae leave behind no compact remnants, resulting in a predicted gap in the distribution of stellar black-hole masses. Gravitational waves from binary black-h…