From the 1 of 9 linked papers with an AI index.
1 citations · 1 across the 1 of their papers we have counts for
9 papers
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…
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…
Studying the gravitational-wave population without looking that FAR out
Noah E. Wolfe, Matthew Mould, Jack Heinzel +1
From catalogs of gravitational-wave transients, the population-level properties of their sources and the formation channels of merging compact binaries can be constrained. However,…
When (not) to trust Monte Carlo approximations for hierarchical Bayesian inference
Jack Heinzel, Salvatore Vitale
The coming years of gravitational wave astrophysics promises thousands of new detections, which can unlock fundamental scientific insights if the information in each observation ca…
PixelPop: High Resolution Nonparameteric Inference of Gravitational-Wave Populations in Multiple Dimensions
Jack Heinzel, Matthew Mould, SofÃa Ãlvarez-López +1
The origins of merging compact binaries observed by gravitational-wave detectors remains highly uncertain. Several astrophysical channels may contribute to the overall merger rate,…
Nonparametric analysis of correlations in the binary black hole population with LIGO-Virgo-KAGRA data
Jack Heinzel, Matthew Mould, Salvatore Vitale
Formation channels of merging compact binaries imprint themselves on the distributions and correlations of their source parameters, but current understanding of this population is…