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首页> 外文期刊>The Astrophysical journal >SDSS J115517.35+634622.0: A Newly Discovered Gravitationally Lensed Quasar
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SDSS J115517.35+634622.0: A Newly Discovered Gravitationally Lensed Quasar

机译:SDSS J115517.35 + 634622.0:一种新发现的引力透镜类星体

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摘要

We report the discovery of SDSS J115517.35+634622.0, a previously unknown gravitationally lensed quasar. The lens system exhibits two images of a z = 2.89 quasar, with an image separation of 1832 ± 0007. Near-IR imaging of the system reveals the presence of the lensing galaxy between the two quasar images. Based on absorption features seen in the Sloan Digital Sky Survey (SDSS) spectrum, we determine a lens galaxy redshift of z = 0.1756. The lens is rather unusual in that one of the quasar images is only 022 ± 007 (~0.1 Reff) from the center of the lens galaxy, and photometric modeling indicates that this image is significantly brighter than predicted by a SIS model. This system was discovered in the course of an ongoing search for strongly lensed quasars in the data set from the SDSS.
机译:我们报告了SDSS J115517.35 + 634622.0(以前未知的重力透镜类星体)的发现。镜头系统展示了两个z = 2.89类星体的图像,图像分离度为1832±0007。该系统的近红外成像显示出两个类星体图像之间存在透镜星系。根据斯隆数字天空测量(SDSS)光谱中的吸收特征,我们确定z = 0.1756的镜头星系红移。镜头是非常不寻常的,因为其中一个类星体图像距离镜头星系中心仅022±007(〜0.1 Reff),并且光度学模型表明该图像比SIS模型所预测的要明亮得多。这个系统是在持续搜寻来自SDSS数据集中的强镜头类星体的过程中发现的。
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