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A Survey for LargeImage Separation Lensed Quasars

机译:大图像分离镜头类星体的调查

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The statistics of gravitationally lensed quasars with multiple images in the 0".17" range have been measured in various surveys. Little is known, however, about lensed-quasar statistics at larger image separations, which probe masses on the scale of galaxy clusters. We extend the results of the Hubble Space Telescope (HST) Snapshot Survey for Lensed Quasars to the 7"50" range for a subsample of 76 quasars that is free of known selection effects. Using a combination of multicolor photometry and spec- troscopy, we show that none of the point sources in the entire field of view of the HST observations of these quasars are lensed images. Large-separation quasar lensing is therefore not common. We carry out a detailed calculation of the expected statistics of large-separation lensing for this quasar sample, incorp- orating realistic input for the mass profiles and mass function of galaxy clusters.
机译:在各种调查中都已测量了在0“ .17”范围内具有多个图像的重力透镜类星体的统计数据。但是,关于较大图像分离时的透镜类星体统计信息知之甚少,该图像探测星系团规模的质量。对于没有已知选择效应的76个类星体的子样本,我们将哈勃太空望远镜(HST)镜头类星体快照调查的结果扩展到7“ 50”范围。通过将多色光度法和光谱法结合使用,我们发现在这些类星体的HST观测的整个视场中,没有点光源是镜头图像。因此,大间隔的类星体镜头并不常见。我们对该类星体样本进行了大分离透镜预期统计量的详细计算,并结合了星系团质量分布和质量函数的实际输入。

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