Nearest neighbor models are among the most basic tools in machine learning, and recent work has demonstrated their effectiveness in the field of astronomy. The performance of these models crucially depends on the underlying metric, and in particular on the selection of a meaningful subset of informative features. The feature selection is task-dependent and usually very time-consuming. In this work, we propose an efficient parallel implementation of incremental feature selection for nearest neighbor models utilizing nowadays graphics processing units. Our framework provides significant computational speed-ups over its sequential single-core competitor of up to two orders of magnitude. We demonstrate the applicability of the overall scheme on one of the most challenging tasks in astronomy: redshift estimation for distant galaxies.
SEEK ID: https://publications.h-its.org/publications/446
Research Groups: Astroinformatics
Publication type: InProceedings
Journal: European Symposium on Artificial Neural Networks, Computational Intelligence And Machine Learning
Book Title: 22st European Symposium on Artificial Neural Networks, Computational Intelligence And Machine Learning Bruges April 23-24-25, 2014
Publisher: ESANN
Citation: European Symposium on Artificial Neural Networks, Computational Intelligence and Machine Learning. Bruges (Belgium), 23-25 April 2014
Date Published: 17th Mar 2014
Registered Mode: manually
Views: 6194
Created: 18th Oct 2019 at 09:28
Last updated: 5th Mar 2024 at 21:23
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