论文标题
HSC成像(Sugohi)中重力透镜对象的调查。 V. HSC-SSP调查中的小组到集群量表镜头搜索
Survey of Gravitationally-lensed Objects in HSC Imaging (SuGOHI). V. Group-to-cluster scale lens search from the HSC-SSP Survey
论文作者
论文摘要
我们报告了HSC成像中属于重力镜头对象调查的最大候选强力镜头样本,以进行组到群集量表(Sugohi-C)系统。这些候选者是根据S18A Subrime-CAM Subaru战略计划(HSC-SSP)调查的S18A数据发布汇编的。我们从视觉上检查$ \ sim39,500 $ Galaxy簇,从几个目录中选择,与宽,深和超过的领域重叠,跨越群集红移范围$ 0.05 <z_ {Cl} <z_ {Cl} <1.38 $。我们发现了641个候选镜头系统,其中536个是新的。从完整的样本中,几乎有47个是真正的镜头,其中181个是高度可能的镜头,413个是可能的镜头系统。此外,我们在检查期间偶尔发现的星系尺度上介绍了131个镜头。我们使用X-Shooter获得了10个候选者的光谱随访。通过此随访,我们将8个系统确认为强力透镜。在其余两个中,其中一个来源太微弱,无法检测到任何发射,另一个来源的暂定红移靠近镜头红移,但是该系统中的其他弧线尚未在光谱上观察到。由于HSC-SSP是一项正在进行的调查,因此我们希望使用此过程找到$ \ sim600 $确定或可能的镜头,甚至与其他镜头查找方法结合使用。
We report the largest sample of candidate strong gravitational lenses belonging to the Survey of Gravitationally-lensed Objects in HSC Imaging for group-to-cluster scale (SuGOHI-c) systems. These candidates are compiled from the S18A data release of the Hyper Suprime-Cam Subaru Strategic Program (HSC-SSP) Survey. We visually inspect $\sim39,500$ galaxy clusters, selected from several catalogs, overlapping with the Wide, Deep, and UltraDeep fields, spanning the cluster redshift range $0.05<z_{cl}<1.38$. We discover 641 candidate lens systems, of which 536 are new. From the full sample, 47 are almost certainly bonafide lenses, 181 of them are highly probable lenses and 413 are possible lens systems. Additionally, we present 131 lens candidates at galaxy-scale serendipitously discovered during the inspection. We obtained spectroscopic follow-up of 10 candidates using the X-shooter. With this follow-up, we confirm 8 systems as strong gravitational lenses. Of the remaining two, one of the sources is too faint to detect any emission, and the other has a tentative redshift close to the lens redshift, but additional arcs in this system are yet to be observed spectroscopically. Since the HSC-SSP is an ongoing survey, we expect to find $\sim600$ definite or probable lenses using this procedure and even more if combined with other lens finding methods.