Stellar Classification vis-à-vis Convolutional Neural Network

Anurag Dutta, A. S. Antony Raj, A. Ramamoorthy, J. Harshith, Yash Soni, Unnati Sadh
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引用次数: 5

Abstract

As a result of recent advancements in technology, a variety of new computational fields have emerged. Some examples of these fields are machine learning and intelligence, information science, the internet of things, and others. The advancement of humanity will be greatly aided by these fields. The development of Artificial Intelligence led to the creation of a great deal of Neural Networks. Convolutional Neural Networks are one variation of Neural Networks that we are utilizing in this work. These networks are known to perform quite admirably for Image Categorization, which is one of the purposes for which we are utilizing them. The work encompasses Stellar Classification. There are many stellar entities occupying the region known as universal space. Astrophysicists are familiar with a good number of them, but there are still a great many of these types of entities that have not been discovered yet. Because of the great distance that separates our planet from other stellar entities, any attempt to communicate with them through any channel is highly unlikely to be successful. The most information we could possibly acquire is just a guess as to what kind of entity they are. So, if any scientific observatory comes with a nascent search of any distant entity, we could potentially predict which stellar group they belong to. For the purposes of this work, we are only going to focus on two different types of Stella: Stars and Galaxies. For the purpose of training the Convolutional Neural Network, we have used a dataset on Stellar Types with Image Categorization created by the Aryabhata Research Institute of Observational Sciences (ARIES), which is located in Nainital, India. This dataset was made publicly available.
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恒星分类与-à-vis卷积神经网络
由于最近技术的进步,出现了各种新的计算领域。这些领域的一些例子是机器学习和智能、信息科学、物联网等。这些领域将极大地促进人类的进步。人工智能的发展导致了大量神经网络的产生。卷积神经网络是我们在这项工作中使用的神经网络的一种变体。众所周知,这些网络在图像分类方面表现相当出色,这也是我们使用它们的目的之一。这项工作包括恒星分类。有许多恒星实体占据着被称为宇宙空间的区域。天体物理学家对其中的许多都很熟悉,但仍有许多这类实体尚未被发现。由于我们的星球与其他恒星实体之间的距离很远,任何通过任何渠道与它们通信的尝试都不太可能成功。我们可能获得的最多信息只是猜测它们是什么样的实体。因此,如果任何科学天文台对任何遥远的实体进行初步搜索,我们就有可能预测它们属于哪个恒星群。为了这项工作的目的,我们只关注两种不同类型的斯特拉:恒星和星系。为了训练卷积神经网络,我们使用了位于印度奈尼塔尔的Aryabhata观测科学研究所(ARIES)创建的带有图像分类的恒星类型数据集。这个数据集是公开的。
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