Living on the edge: Testing for compact population features at the edges of parameter space
Asad Hussain, Maximiliano Isi, Aaron Zimmerman

TL;DR
This paper presents a truncated Gaussian mixture model approach to accurately detect population features near parameter boundaries, reducing bias and computational cost in astrophysical data analysis.
Contribution
The authors introduce a novel truncated Gaussian mixture model framework that improves boundary feature inference, demonstrated on gravitational wave data with lower computational costs.
Findings
Accurately estimates zero-spin binary black hole fractions.
Reduces bias in boundary population feature detection.
Achieves similar results to previous methods with less computation.
Abstract
Many astrophysical population studies involve parameters that exist on a bounded domain, such as the dimensionless spins of black holes or the eccentricities of planetary orbits, both of which are confined to . In such scenarios, we often wish to test for distributions clustered near a boundary, e.g., vanishing spin or orbital eccentricity. Conventional approaches -- whether based on Monte Carlo, kernel density estimators, or machine-learning techniques -- often suffer biases at the boundaries. These biases stem from sparse sampling near the edge, kernel-related smoothing, or artifacts introduced by domain transformations. We introduce a truncated Gaussian mixture model framework that substantially mitigates these issues, enabling accurate inference of narrow, edge-dominated population features. While our method has broad applications to many astronomical domains, we consider…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Astrophysical Phenomena and Observations · Astronomy and Astrophysical Research
