Abstract
We present a Convolutional Neural Network (CNN) for use in the Real-Bogus classification of transient detections made by the Asteroid Terrestrial Impact Last Alert System (ATLAS) and subsequent efforts to improve performance since initial development. In transient detection surveys the number of alerts made outstrips the capacity for human scanning, necessitating the use of machine learning aids to reduce the number of false positives presented to annotators. We take a sample of recently annotated data from each of the three operating ATLAS telescope with ∼340,000 real (known transients) and ∼1,030,000 bogus detections per model. We retrained the CNN architecture with these data specific to each ATLAS unit, achieving a median False Positive Rate (FPR) of 0.72 per cent for a 1.00 per cent missed detection rate. Further investigations indicate if we reduce the input image size it results in increases to the false positive rate. Finally architecture adjustments and comparisons to contemporary CNNs indicate our retrained classifier is providing an optimal FPR. We conclude that the periodic retraining and readjustment of classification models on survey data can yield significant improvements as data drift arising from changes to optical and detector performance can lead to new features in the model and subsequent deteriorations in performance.
| Original language | English |
|---|---|
| Pages (from-to) | 385–399 |
| Number of pages | 15 |
| Journal | RAS Techniques and Instruments |
| Volume | 3 |
| Issue number | 1 |
| DOIs | |
| Publication status | Published - 12 Jul 2024 |
UN SDGs
This output contributes to the following UN Sustainable Development Goals (SDGs)
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SDG 3 Good Health and Well-being
Keywords
- Algorithms
- Classification
- Convolutional Neural Networks
- Data Methods
- Machine Learning
- Supernovae
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