论文标题

使用SWIFT和WISE数据将3FGL非相关目录中的Blazar候选者分类为BL LAC和FSRQ

Classifying blazar candidates from the 3FGL unassociated catalog into BL Lacs and FSRQs using Swift and WISE data

论文作者

Kaur, Amanpreet, Falcone, Abraham D., Stroh, Michael C.

论文摘要

我们利用机器学习方法将Bl lacertae对象(BL LAC)与可能的X射线Blazar对应物与Fermi 3FGL非相关伽马射线源的样本中的平坦光谱无线电类星体(FSRQ)区分开。从我们以前的工作中,我们提取了84个来源,这些资源被归类为$ \ geq $ 99%的likley,以成为Blazars。然后,我们一起利用Swift $ - $ XRT,FERMI和WISE(广阔的红外调查探索器)数据来区分Blazar,FSRQ或BL lac的特定类型。可以使用各种X射线和伽马射线参数来区分这些子类。这些也已知这些颜色颜色图上占据了不同的参数空间。一起使用所有这些数据将为分类来源提供更强大的结果。我们利用一个随机的森林分类器来计算每个Blazar与BL LAC或FSRQ相关的概率。基于p $ _ {bll} $,这是每个源是BL LAC的概率,我们根据以下值将源放在五个不同的类别中; P$_{bll}$ $\geq$ 99%: highly likely BL Lac, P$_{bll}$ $\geq$ 90%: likely BL Lac, P$_{bll}$ $\leq$ 1%: highly likely FSRQ, P$_{bll}$ $\leq$ 10%: likely FSRQ, and 90% $<$ p $ _ {bll} $ $ <$ <$ 10%:模棱两可。我们的结果将84个Blazar候选人分类为50个可能的BL LAC,其余34个则模棱两可。这些来源的一小部分已被列为最新的Fermi目录4FGL中的相关来源,在这些情况下,我们的结果一致。

We utilize machine learning methods to distinguish BL Lacertae objects (BL Lac) from Flat Spectrum Radio Quasars (FSRQ) within a sample of likely X-ray blazar counterparts to Fermi 3FGL unassociated gamma-ray sources. From our previous work, we have extracted 84 sources that were classified as $\geq$ 99% likley to be blazars. We then utilize Swift$-$XRT, Fermi, and WISE (The Wide-field Infrared Survey Explorer) data together to distinguish the specific type of blazar, FSRQs or BL Lacs. Various X-ray and Gamma-ray parameters can be used to differentiate between these subclasses. These are also known to occupy different parameter space on the WISE color-color diagram. Using all these data together would provide more robust results for the classified sources. We utilized a Random Forest Classifier to calculate the probability for each blazar to be associated with a BL Lac or an FSRQ. Based on P$_{bll}$, which is the probability for each source to be a BL Lac, we placed our sources into five different categories based on this value as follows; P$_{bll}$ $\geq$ 99%: highly likely BL Lac, P$_{bll}$ $\geq$ 90%: likely BL Lac, P$_{bll}$ $\leq$ 1%: highly likely FSRQ, P$_{bll}$ $\leq$ 10%: likely FSRQ, and 90% $<$ P$_{bll}$ $<$ 10%: ambiguous. Our results categorize the 84 blazar candidates as 50 likely BL Lacs and the rest 34 being ambiguous. A small subset of these sources have been listed as associated sources in the most recent Fermi catalog, 4FGL, and in these cases our results are in agreement on the classification.

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