Reconstructing parametric gravitational-wave population fits from non-parametric results without refitting the data
Cecilia Maria Fabbri, Davide Gerosa, Alessandro Santini, Matthew Mould, Alexandre Toubiana, Jonathan Gair

TL;DR
This paper introduces a method to reconstruct different population models from existing non-parametric gravitational-wave data fits, streamlining analysis and avoiding repeated data processing.
Contribution
It provides a practical recipe to derive parametric population distributions from non-parametric fits without re-accessing raw data or refitting, enhancing efficiency and interpretability.
Findings
Successfully applied to black-hole binary mass distributions
Enables comparison of multiple models using a goodness-of-fit metric
Reduces computational effort by avoiding repeated data refitting
Abstract
Combining multiple events into population analyses is a cornerstone of gravitational-wave astronomy. A critical component of such studies is the assumed population model, which can range from astrophysically motivated functional forms to non-parametric treatments that are flexible but difficult to interpret. In practice, the current approach is to fit the data multiple times with different population models to identify robust features. We propose an alternative strategy: assuming the data have already been fit with a flexible model, we present a practical recipe to reconstruct the population distribution of a different model. As our procedure postprocesses existing results, it avoids the need to access the underlying gravitational-wave data again and handle selection effects. Additionally, our reconstruction metric provides a goodness-of-fit measure to compare multiple models. We apply…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Atomic and Subatomic Physics Research · Geophysics and Gravity Measurements
