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Regional Effect Plots for Machine Learning Model Interpretation

Published online by Cambridge University Press:  05 October 2026

Christos Diou*
Affiliation:
Department of Informatics and Telematics, Harokopio University of Athens, Greece
Vasileios Gkolemis
Affiliation:
Department of Informatics and Telematics, Harokopio University of Athens, Greece ATHENA Research Center, Athens, Greece
Theodoros Dalamagas
Affiliation:
ATHENA Research Center, Athens, Greece
*
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Abstract

Machine learning (ML) is increasingly important in astrophysics, enabling the analysis of large, complex datasets for tasks such as stellar classification and gravitational wave detection. Yet many ML models are highly non-linear, with intricate feature interactions that make them difficult to interpret and often viewed as “black boxes.” Interpretability is therefore essential for ensuring trust, scientific validity, but also for uncovering new scientific insights.

Global feature effect methods address this by quantifying how input features influence model outputs on average. However, such explanations may be misleading when strong interactions cause individual behaviours to deviate from the average. Regional effect plots mitigate this by partitioning the feature space into more homogeneous subspaces, producing more accurate effect estimates.

This talk reviews global feature effect methods, introduces recent advances, and presents Effector, an open-source Python package for efficiently generating accurate global and regional feature effect plots.

Information

Type
Contributed Paper
Creative Commons
Creative Common License - CCCreative Common License - BY
This is an Open Access article, distributed under the terms of the Creative Commons Attribution licence (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted re-use, distribution and reproduction, provided the original article is properly cited.
Copyright
© The Author(s), 2026. Published by Cambridge University Press on behalf of The International Astronomical Union
Figure 0

Figure 1. Figure 1 long description.PDP (blue) and ICE plots (red) illustrating the effect of the “hour” feature on the number of bike rentals. In (a), the whole dataset is used, while in (b) and (c) we observe the PDP for working and non-working days respectively. These subregions (automatically identified using the algorithm proposed in (Gkolemis et al. 2023b)) lead to reduced heterogeneity of the feature effects.

Figure 1

Figure 2. Example comparing (a) ALE (with fixed bin size) with (b) RHALE (with optimal bin size). RHALE finds a variable bin splitting that minimises heterogeneity, leading to improved estimation of the feature effect (top plots)