Star Discrepancy Subset Selection: Problem Formulation and Efficient Approaches for Low Dimensions

François Clèment; Carola Doerr; Luís Paquete

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arXiv · 2101.07881

Star Discrepancy Subset Selection: Problem Formulation and Efficient Approaches for Low Dimensions

François Clèment·Carola Doerr·Luís Paquete

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Abstract

Motivated by applications in instance selection, we introduce the star discrepancy subset selection problem, which consists of finding a subset of m out of n points that minimizes the star discrepancy. First, we show that this problem is NP-hard. Then, we introduce a mixed integer linear formulation (MILP) and a combinatorial branch-and-bound (BB) algorithm for the star discrepancy subset selection problem and we evaluate both approaches against random subset selection and a greedy construction on different use-cases in dimension two and three. Our results show that the MILP and BB are efficient in dimension two for large and small $m/n$ ratio, respectively, and for not too large n. However, the performance of both approaches decays strongly for larger dimensions and set sizes. As a side effect of our empirical comparisons we obtain point sets of discrepancy values that are much smaller than those of common low-discrepancy sequences, random point sets, and of Latin Hypercube Sampling. This suggests that subset selection could be an interesting approach for generating point sets of small discrepancy value.

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BibTeX RIS

François Clèment, Carola Doerr, Luís Paquete. 2022-01-04. Star Discrepancy Subset Selection: Problem Formulation and Efficient Approaches for Low Dimensions. https://arxiv.org/abs/2101.07881

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