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AutoSourceID-Light Fast optical source localization via U-Net and Laplacian of Gaussian

ASTRONOMY & ASTROPHYSICS(2022)

Radboud Univ Nijmegen | Univ Nova Gorica | Univ Iceland | IFIC UV CSIC

Cited 2|Views30
Abstract
Aims. With the ever-increasing survey speed of optical wide-field telescopes and the importance of discovering transients when they are still young, rapid and reliable source localization is paramount. We present AutoSourceID-Light (ASID-L), an innovative framework that uses computer vision techniques that can naturally deal with large amounts of data and rapidly localize sources in optical images. Methods. We show that the ASID-L algorithm based on U-shaped networks and enhanced with a Laplacian of Gaussian filter provides outstanding performance in the localization of sources. A U-Net network discerns the sources in the images from many different artifacts and passes the result to a Laplacian of Gaussian filter that then estimates the exact location. Results. Using ASID-L on the optical images of the MeerLICHT telescope demonstrates the great speed and localization power of the method. We compare the results with SExtractor and show that our method outperforms this more widely used method. ASID-L rapidly detects more sources not only in low- and mid-density fields, but particularly in areas with more than 150 sources per square arcminute. The training set and code used in this paper are publicly available.
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astronomical databases,miscellaneous,methods,data analysis,stars,imaging,techniques,image processing
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要点】:本文提出了一种基于U-Net和Laplacian of Gaussian滤波器的AutoSourceID-Light(ASID-L)框架,能快速且准确地在光学图像中进行光源定位,提高了光学宽视场望远镜暂现源发现的效率。

方法】:采用U-Net网络识别图像中的光源,并利用Laplacian of Gaussian滤波器估计光源的精确位置。

实验】:使用MeerLICHT望远镜的光学图像进行测试,实验结果显示ASID-L方法在速度和定位能力上优于广泛使用的SExtractor方法,特别是在每平方角分超过150个光源的高密度区域。所使用的训练集和代码已公开可用。