Supernova Detection Based on Multi-scale Fusion Faster RCNN

Dongjiao Guo, Bo Qiu, Yanping Liu, Guanjie Xiang
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Abstract

Supernovae are of great significance in the study of life evolution and expansion history of the universe. In this paper, multi-scale fusion Faster RCNN model is used to realize automatic detection of supernovae. Firstly, the dataset was synthesized and rotated to enhance supernova features. Secondly, based on the Faster RCNN architecture, the network combined with Resnet50 and PAFPN is used to extract image features, so as to obtain multi-scale feature maps and improve the ability of the network to extract small target features. Finally, OHEM network is introduced into the network to balance the difference between positive and negative sample in number. The prepared dataset was used for the training of the multi-scale fusion Faster RCNN model, and the MACRO-F1 of the test set was up to 96.6%. The method proposed in this paper can realize the detection of supernovae from astronomical imagery with relatively high accuracy.
基于多尺度融合的快速RCNN超新星探测
超新星在研究生命演化和宇宙膨胀史中具有重要意义。本文采用多尺度融合Faster RCNN模型实现了超新星的自动探测。首先,对数据集进行合成和旋转,增强超新星特征;其次,基于Faster RCNN架构,结合Resnet50和PAFPN对图像特征进行提取,获得多尺度特征图,提高网络对小目标特征的提取能力。最后,在网络中引入OHEM网络,平衡正负样本数量的差异。将准备好的数据集用于多尺度融合Faster RCNN模型的训练,测试集的MACRO-F1达到了96.6%。本文提出的方法能够以较高的精度实现天文图像对超新星的探测。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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