Enabling New Discoveries with Machine Learning
arXiv:2609.10109 · doi:10.1017/S174392132400317X
Abstract
The next generation of telescopes such as the Square Kilometre Array and the Vera C. Rubin Observatory will produce enormous quantities of data, too large for traditional analysis techniques. Machine learning has proven invaluable in handling massive data volumes and automating tasks traditionally done by human scientists. The question is, can machine learning also automate scientific discovery? Recent advances in the field have made this feasible but only when combined with expert human input through active learning. Astronomaly is a publicly available framework for active anomaly detection in astronomy. It learns to make recommendations of interesting sources to a user, allowing scientists to quickly uncover rare and new classes of objects in large datasets. In this paper, we review some of the discoveries made using Astronomaly, discuss the latest deep learning-based approaches and explore the critical role of the cyber-human interface in unveiling cosmic mysteries hidden in massive astronomical datasets.
arXiv commentProceedings for the IAU General Assembly 2024 (Cape Town): Focus Meeting 7, invited talk. 7 pages, 4 figure
References in corpus (11)
- LSST: from Science Drivers to Reference Design and Anticipated Data Products
- Overview of the DESI Legacy Imaging Surveys
- Galaxy Zoo : Morphologies derived from visual inspection of galaxies from the Sloan Digital Sky Survey
- Galaxy Zoo 1 : Data Release of Morphological Classifications for nearly 900,000 galaxies
- Astronomaly: Personalised Active Anomaly Detection in Astronomical Data
- Unsupervised machine learning for transient discovery in Deeper, Wider, Faster light curves
- A unique, ring-like radio source with quadrilateral structure detected with machine learning
- Real-Time Detection of Anomalies in Large-Scale Transient Surveys
- Astronomaly at scale: searching for anomalies amongst 4 million galaxies
- Enabling Unsupervised Discovery in Astronomical Images through Self-Supervised Representations
- A Classifier-Based Approach to Multi-Class Anomaly Detection for Astronomical Transients