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Single-epoch supernova classification with deep convolutional neural networks

机译:具有深度卷积神经网络的单纪元超新星分类

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Supernovae Type-Ia (SNela) play a significant role in exploring the history of the expansion of the Universe, since they are the best-known standard candles with which we can accurately measure the distance to the objects. Finding large samples of SNela and investigating their detailed characteristics have become an important issue in cosmology and astronomy. Existing methods relied on a photometric approach that first measures the luminance of supernova candidates precisely and then fits the results to a parametric function of temporal changes in luminance. However, it inevitably requires multi-epoch observations and complex luminance measurements. In this work, we present a novel method for classifying SNela simply from single-epoch observation images without any complex measurements, by effectively integrating the state-of-the-art computer vision methodology into the standard photometric approach. Experimental results show the effectiveness of the proposed method and reveal classification performance comparable to existing photometric methods with multi-epoch observations.
机译:Supernovae Type-IA(Snela)在探索宇宙扩展的历史中起着重要作用,因为它们是最着名的标准蜡烛,我们可以准确地测量与物体的距离。寻找大型Snela并调查他们的详细特征已成为宇宙学和天文学的重要问题。现有方法依赖于光度方法,首先将Supernova候选的亮度精确测量,然后将结果拟合到亮度中的时间变化的参数函数。然而,它不可避免地需要多纪元观察和复杂的亮度测量。在这项工作中,我们通过有效地将最先进的计算机视觉方法与标准光度法相结合,提出了一种简单地从单秒钟观测图像进行分类的新方法,而不是任何复杂的测量。实验结果表明了该方法的有效性,并揭示了与多钟观测的现有光度法相当的分类性能。

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