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Colour matters: the effects of lensing on the positional offsets between optical and submillimetre galaxies in Herschel-ATLAS

机译:颜色问题:镜头对Herschel-ATLAS光学和亚毫米星系之间位置偏移的影响

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摘要

We report an unexpected variation in the positional offset distributions between Herschel-ATLAS sub-millimetre (submm) sources and their optical associations, depend-ing on both 250-μm signal-to-noise ratio and 250/350-μm colour.We show that redderand brighter submm sources have optical associations with a broader distribution ofpositional offsets than would be expected if these offsets were due to random positionalerrors in the source extraction. The observation can be explained by two possible ef-fects: either red submm sources trace a more clustered population than blue ones, andtheir positional errors are increased by confusion; or red submm sources are generallyat high redshifts and are frequently associated with low-redshift lensing structureswhich are identified as false counterparts. We perform various analyses of the data,including the multiplicity of optical associations, the redshift and magnitude distribu-tions in H-ATLAS in comparison to HerMES, and simulations of weak lensing, and weconclude that the effects are most likely to be explained by widespread weak lensing ofHerschel -SPIRE sources by foreground structures. This has important consequencesfor counterpart identification and derived redshift distributions and luminosity func-tions of submm surveys.
机译:我们报告了Herschel-ATLAS亚毫米(submm)光源及其光学关联之间的位置偏移分布出乎意料的变化,这取决于250μm的信噪比和250 /350μm的颜色。较红色和较亮的亚毫米源具有比位置偏移分布更宽的光学关联,如果这些偏移是由于源提取中的随机位置误差而导致的,则这种关联更广泛。观察结果可以用两种可能的效应来解释:要么红色的亚毫米源比蓝色的亚毫米源追踪更多的聚集种群,并且它们的位置误差由于混乱而增加;或红色submm光源通常处于高红移状态,并经常与被标识为假对应物的低红移透镜结构相关联。我们对数据进行了各种分析,包括光学关联的多样性,与HerMES相比H-ATLAS中的红移和幅度分布以及微弱透镜的模拟,我们得出结论认为,这种影响最有可能由广泛的现象来解释。前景结构对Herschel -SPIRE源的弱镜头。这对于亚毫米测量的对应物识别以及派生的红移分布和发光度功能具有重要的意义。

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