调谐到空间频率空间

IF 5.4 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
J. P. Carvajal, F. E. Bauer, I. Reyes-Jainaga, F. Förster, A. M. Muñoz Arancibia, M. Catelan, P. Sánchez-Sáez, C. Ricci, A. Bayo
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引用次数: 0

摘要

上下文。瞬态天体物理现象研究的一个重大挑战是伪事件的识别,其中人造地球轨道卫星和碎片仍然是主要污染物。现有的管道可以有效地识别卫星轨迹,但它们往往会错过更复杂的特征,比如卫星闪烁的集合。在鲁宾天文台时代,操作规模将比其前身兹威基瞬变设施(ZTF)增加十倍,需要在分类纯度、信息警报的数据压缩和管道速度方面进行关键改进。我们探索在差分图像上使用二维快速傅里叶变换(FFT)作为改进卫星探测机器学习算法的工具。以事件快速分类的自动学习(ALeRCE)单图章分类器为基准,我们调整了它的架构,除了三个(科学、参考、差分)ZTF图像图章(以下简称图章)外,还接收了差分图像的FFT的一个切出。我们探索了各种图章大小和分辨率,评估了合并FFT图像的好处,特别是当数据压缩由于警报大小限制和管道速度限制而至关重要时(例如,在大规模调查中,如空间和时间的遗留调查)。FFT的加入可以显著提高卫星的探测性能。最显著的改进发生在最小视场模型(16″),在包含完整的63张″差分图像计算的FFT后,其卫星分类精度从(72.0±2.9)%提高到(87.8±1.3)%。这证明了FFT在压缩和提取相关大尺度卫星特征方面的有效性。然而,单独的FFT并不能完全匹配完整的63″,(95.9±1.3)%和多尺度(90.6±0.8)%模型所达到的精度,这突出了上下文空间信息的互补重要性。我们展示了如何利用fft从警报流中剔除卫星和空间碎片特征。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Tuning into the spatial frequency space
Context. A significant challenge in the study of transient astrophysical phenomena is the identification of bogus events, among which human-made Earth-orbiting satellites and debris remain major contaminants. Existing pipelines can effectively identify satellite trails, but they often miss more complex signatures, such as collections of satellite glints. In the Rubin Observatory era, the scale of operations will increase tenfold with respect to its precursor, the Zwicky Transient Facility (ZTF), requiring crucial improvements in classification purity, data compression for informative alerts, and pipeline speed.Aims. We explore the use of a 2D Fast Fourier Transform (FFT) on difference images as a tool to improve satellite-detection machine learning algorithms.Methods. Using the Automatic Learning for the Rapid Classification of Events (ALeRCE) single-stamp classifier as a baseline, we adapted its architecture to receive a cutout of the FFT of the difference image, in addition to the three (science, reference, difference) ZTF image cutouts (hereafter stamps). We explored various stamp sizes and resolutions, assessing the benefits of incorporating FFT images, particularly when data compression is critical due to alert size limitations and pipeline speed constraints (e.g., in large-scale surveys such as the Legacy Survey of Space and Time).Results. The inclusion of the FFT can significantly improve satellite detection performance. The most notable improvement occurred in the smallest field-of-view model (16″), whose satellite classification accuracy increased from (72.0 ± 2.9)% to (87.8 ± 1.3)% after including the FFT, computed from the full 63″ difference images. This demonstrates the effectiveness of FFT in compressing and extracting relevant large-scale satellite features. However, the FFT alone did not fully match the accuracy achieved by the full 63″, (95.9 ± 1.3)% and multiscale (90.6 ± 0.8)% models, highlighting the complementary importance of contextual spatial information.Conclusions. We show how FFTs can be leveraged to cull satellite and space debris signatures from alert streams.
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来源期刊
Astronomy & Astrophysics
Astronomy & Astrophysics 地学天文-天文与天体物理
CiteScore
10.20
自引率
27.70%
发文量
2105
审稿时长
1-2 weeks
期刊介绍: Astronomy & Astrophysics is an international Journal that publishes papers on all aspects of astronomy and astrophysics (theoretical, observational, and instrumental) independently of the techniques used to obtain the results.
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