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Detection and Classification of Astronomical Targets with Deep Neural Networks in Wide-field Small Aperture Telescopes

  • Authors: Peng Jia, Qiang Liu, and Yongyang Sun

2020 The Astronomical Journal 159 212.

  • Provider: AAS Journals

Caption: Figure 3.

Flow chart of neural network used for the astronomical target detection and classification framework. The framework uses the FPN to extract features from the original image. Then with the RPN and ROI alignment, feature maps of candidate images are transmitted to the classification and regression neural network. Through box regression and classification, the neural network will classify and obtain the position of these targets. In this figure, boxes stand for the manipulation and arrows stand for the data flow.

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