在没有监督的情况下比较分子云的形态

IF 5.4 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
Pablo Richard, Erwan Allys, François Levrier, Antoine Gusdorf, Constant Auclair
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引用次数: 0

摘要

分子云是天体物理对象,其复杂的非线性动力学表现在其复杂的形态特征上。许多研究高阶统计和物理性质之间的桥梁已经强调了非高斯形态特征在捕获物理信息中的价值。然而,由于这种桥梁通常在模拟的监督世界中具有特征,将其转移到观察可能是危险的,特别是当模拟和观察之间的差异仍然未知时。在本文中,我们旨在直接从观测数据中评估一组统计数据的判别能力。为此,我们开发了一个测试,该测试允许我们比较给定未标记数据集的两组汇总统计数据的信息能力。与监督方法相反,该测试不需要了解与数据相关的任何类标签或参数。相反,它基于统计兼容性的概念来评估和比较汇总统计的退化程度。我们将此测试应用于赫歇尔观测到的14个附近分子云的柱密度图,并迭代比较不同的典型汇总统计集。我们表明,这些云的标准高斯描述是高度退化的,但在对地图的对数进行估计时可以大大改进。这说明,如果使用得当,低阶统计仍然是一个非常强大的工具。我们进一步表明,这种描述仍然表现出少量的简并性,其中一些是由简化的小波散射变换提供的高阶统计量提升的。这些简并在密度分子云坍缩的观测结果和最先进的模拟结果之间存在定量差异,并且它们不存在于对数分数布朗运动模型中。最后,我们展示了如何将识别的汇总统计信息协同用于构建形态距离,并对其进行视觉评估并给出令人信服的结果。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Comparing the morphology of molecular clouds without supervision
Molecular clouds are astrophysical objects whose complex nonlinear dynamics are reflected in their complex morphological features. Many studies investigating the bridge between higher-order statistics and physical properties have highlighted the value of non-Gaussian morphological features in capturing physical information. Yet, as this bridge is usually characterized in the supervised world of simulations, transferring it to observations can be hazardous, especially when the discrepancy between simulations and observations remains unknown. In this paper, we aim to evaluate, directly from the observation data, the discriminating ability of a set of statistics. To do so, we developed a test that allowed us to compare the informative power of two sets of summary statistics for a given unlabeled dataset. Contrary to supervised approaches, this test does not require knowledge of any class label or parameter associated with the data. Instead, it evaluates and compares the degeneracy levels of the summary statistics based on a notion of statistical compatibility. We applied this test to column density maps of 14 nearby molecular clouds observed by Herschel and iteratively compared different sets of typical summary statistics. We show that a standard Gaussian description of these clouds is highly degenerate but can be substantially improved when being estimated on the logarithm of the maps. This illustrates that low-order statistics, when properly used, remain a very powerful tool. We further show that such descriptions still exhibit a small quantity of degeneracies, some of which are lifted by the higher-order statistics provided by reduced wavelet scattering transforms. These degeneracies quantitatively differ between observations and state-of-the-art simulations of dense molecular cloud collapse, and they are not present for log-fractional Brownian motion models. Finally, we show how the summary statistics identified can be cooperatively used to build a morphological distance, which is evaluated visually and gives convincing results.
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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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