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First lensed quasar systems from the VST-ATLAS survey : one quad, two doubles, and two pairs of lensless twins.

机译:VST-ATLAS调查中的第一个带透镜的类星体系统:一个四边形,两个双透镜和两对无透镜双胞胎。

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摘要

We have analyzed images from the VST-ATLAS survey to identify candidate gravitationally lensed quasar systems in a sample of WISE sources with $W1-W2gt 0.7$. Results from follow-up spectroscopy with the Baade 6.5 m telescope are presented for eight systems. One of them is a quadruply lensed quasar, and two are doubly lensed systems. Two are projected superpositions of two quasars at different redshifts. In one system, two quasars, although at the same redshift, have very different emission line profiles and constitute a physical binary. In two systems, the component spectra are consistent with the lensing hypothesis, after allowing for microlensing. However, as no lensing galaxy is detected in these two systems, we classify them as lensless twins. More extensive observations are needed to establish whether they are in fact lensed quasars or physical binaries.
机译:我们分析了来自VST-ATLAS调查的图像,以识别W1-W2 > 0.7 $的WISE光源样本中的重力透镜类星体系统。介绍了使用Baade 6.5 m望远镜进行的后续光谱学分析的结果,涉及了8个系统。其中之一是四透镜类星体,两个是双透镜系统。两个投影在不同的红移下是两个类星体的投影叠加。在一个系统中,两个类星体尽管具有相同的红移,但它们的发射谱线轮廓却大不相同,并且构成了一个物理双星。在两个系统中,允许微透镜化之后,成分光谱与透镜化假设一致。但是,由于在这两个系统中均未检测到透镜星系,因此我们将其分类为无透镜双胞胎。需要更广泛的观察来确定它们实际上是透镜类星体还是物理双星。

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