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Identifying the 3FHL Catalog. I. Archival Swift Observations and Source Classification

机译:识别3FHL目录。一,档案快速观测和资料来源分类

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We present the results of an identification campaign of unassociated sources from the Fermi Large Area Telescope 3FHL catalog. Out of 200 unidentified sources, we selected 110 sources for which archival Swift-XRT observations were available, 52 of which were found to have exactly one X-ray counterpart within the 3FHL 95% positional uncertainty. In this work, we report the X-ray, optical, IR, and radio properties of these 52 sources using positional associations with objects in various catalogs. The Wide-field Infrared Survey Explorer color–color plot for sources suggests that most of these belong to the blazar class family. The redshift measurements for these objects range from z?=?0.277 to z?=?2.1. Additionally, under the assumption that the majority of these sources are blazars, three machine-learning algorithms are employed to classify the sample into flat spectrum radio quasars or BL Lacertae objects. These suggest that the majority of the previously unassociated sources are BL Lac objects, in agreement with the fact the BL Lac objects represent by far the most numerous population detected above 10 GeV in 3FHL.
机译:我们展示了费米大面积望远镜3FHL目录中未关联来源的识别运动的结果。在200个未知源中,我们选择了110个可进行档案Swift-XRT观测的源,其中52个在3FHL 95%位置不确定性范围内恰好具有一个X射线对应物。在这项工作中,我们使用与各种目录中的对象的位置关联来报告这52个源的X射线,光学,IR和无线电特性。广源红外勘测浏览器的色-色图表明,其中大多数属于blazar类家族。这些物体的红移测量值的范围为z≥0.277至z≥2.1。另外,假设这些来源中的大多数是爆炸物,则采用三种机器学习算法将样本分类为平面频谱类星体或BL Lacertae对象。这些表明大多数先前未关联的来源是BL Lac对象,这与BL Lac对象代表了迄今为止在3FHL中检测到的10 GeV以上的最多的种群这一事实相一致。

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