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Knowledge Discovery workflows for the classification of AGNs in multi-wavelength spaces: the Blazars case

机译:知识发现工作流程为多波长空间中AGN分类:Blazars案例

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The development of new AGNs selection techniques based on the massive multiwavelength datasets that are becoming more and more frequent in astronomy is a crucial task to gather statistically significant samples and shed light on the physical nature of this diverse class of extragalactic sources. Novel characterizations of specific classes of sources from unexplored region of their spectrum and unusual combinations of the observational parameters can translate into new classification criteria. In this innovative data environment, the whole process ranging from the discovery of new patterns to the application of such patters to the selection of new AGNs, has to be tackled using a Knowledge Discovery (KD) workflow. A KD workflows is a combination of different KD methods that automatically extract the more interesting patters from data, reduce the complexity of the dataset and provide astronomers with the simplest possible amount of information to be interpreted. In this talk, I will describe an original KD workflow which, in one of its first applications, has led to the discovery of a previously unknown peculiar pattern followed by blazars in the mid-Infrared color space (the blazars WISE locus), and the development of a new classification criterion based on this pattern and useful to tackle different problems. The comprehensive KD workflow used to derive these results encompasses unsupervised methods for the exploration of the multi-dimensional observable spaces, and supervised method for the training and optimization of classifiers based on the patterns determined in the observable spaces. In particular, I will describe the new methods for the association of unidentified gamma-ray sources and the extraction of candidate blazars from mid-Infrared photometric catalog based on the WISE blazars locus.
机译:基于大量多波长数据集的新AGNS选择技术的开发是在天文学中变得越来越多的频繁的,是在这种多种胶质源的物理性质上收集统计上显着的样本和脱落的关键任务。从未开发的地区的频谱区域和观察参数的不寻常组合的小说特征可以转化为新的分类标准。在这一创新的数据环境中,必须使用知识发现(KD)工作流程来解决新模式的整个过程从发现这种模式的应用到应用新AGN。 KD工作流是不同KD方法的组合,可以自动提取来自数据的更有趣的图案,降低数据集的复杂性,并提供有可能解释的最简单信息量的天文学家。在这次谈话中,我将描述一个原始的KD工作流程,它在其第一个应用程序中,它导致了一个先前未知的特殊模式,然后在中红外颜色空间(Blazars Wise Locus)中的布拉恩,以及基于此模式的新分类标准的开发,并有用可用于解决不同的问题。用于导出这些结果的全面KD工作流包括基于可观察空间中确定的图案的模式探索多维可观察空间的无监督方法,以及对分类器的训练和优化的监督方法。特别是,我将描述未识别的伽马射线源和候选布拉齐的提取的新方法,以及基于明智的布拉齐克轨迹的中红外光度法目录。

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