LGMLSep 17, 2020

LAAT: Locally Aligned Ant Technique for discovering multiple faint low dimensional structures of varying density

arXiv:2009.08326v27 citations
Originality Incremental advance
AI Analysis

This addresses a critical preprocessing challenge for machine learning tasks in domains like astronomy where noise and varying densities impair manifold detection, though it appears incremental as it builds on existing ant colony optimization ideas.

The paper tackles the problem of extracting multiple low-dimensional manifolds with varying densities from noisy data, such as in astronomical datasets, by proposing a biologically inspired ant colony optimization method that captures locally aligned points and reinforces behavior with pheromones, demonstrating improved performance over state-of-the-art approaches on synthetic and real datasets.

Dimensionality reduction and clustering are often used as preliminary steps for many complex machine learning tasks. The presence of noise and outliers can deteriorate the performance of such preprocessing and therefore impair the subsequent analysis tremendously. In manifold learning, several studies indicate solutions for removing background noise or noise close to the structure when the density is substantially higher than that exhibited by the noise. However, in many applications, including astronomical datasets, the density varies alongside manifolds that are buried in a noisy background. We propose a novel method to extract manifolds in the presence of noise based on the idea of Ant colony optimization. In contrast to the existing random walk solutions, our technique captures points that are locally aligned with major directions of the manifold. Moreover, we empirically show that the biologically inspired formulation of ant pheromone reinforces this behavior enabling it to recover multiple manifolds embedded in extremely noisy data clouds. The algorithm performance in comparison to state-of-the-art approaches for noise reduction in manifold detection and clustering is demonstrated, on several synthetic and real datasets, including an N-body simulation of a cosmological volume.

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