# Optical Transient Object Classification in Wide Field Small Aperture   Telescopes with Neural Networks

**Authors:** Peng Jia, Yifei Zhao, Gang Xue, Dongmei Cai

arXiv: 1904.12987 · 2019-07-17

## TL;DR

This paper introduces neural network-based methods for classifying transient images in wide field small aperture telescopes, achieving over 97% accuracy through ensemble learning, thereby enhancing transient discovery efficiency.

## Contribution

It presents two novel neural network approaches for transient image classification and demonstrates their effectiveness with real data, improving accuracy with ensemble methods.

## Key findings

- Both methods achieve over 94% accuracy.
- Ensemble learning boosts accuracy to over 97%.
- Different models have complementary classification properties.

## Abstract

Wide field small aperture telescopes are working horses for fast sky surveying. Transient discovery is one of their main tasks. Classification of candidate transient images between real sources and artifacts with high accuracy is an important step for transient discovery. In this paper, we propose two transient classification methods based on neural networks. The first method uses the convolutional neural network without pooling layers to classify transient images with low sampling rate. The second method assumes transient images as one dimensional signals and is based on recurrent neural networks with long short term memory and leaky ReLu activation function in each detection layer. Testing with real observation data, we find that although these two methods can both achieve more than 94% classification accuracy, they have different classification properties for different targets. Based on this result, we propose to use the ensemble learning method to further increase the classification accuracy to more than 97%.

## Full text

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## Figures

10 figures with captions in the complete paper: https://tomesphere.com/paper/1904.12987/full.md

## References

61 references — full list in the complete paper: https://tomesphere.com/paper/1904.12987/full.md

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Source: https://tomesphere.com/paper/1904.12987