在SCI 126中，鲜红星系群均匀地分布在核心和边缘之间。 在SCI 111中，这些星系群则倾向于聚集成高密度区域。

Within SCl 126, these BRG groups were evenly distributed between the core and the outskirts while in SCl 111, these groups tended to congregate towards the high density regions.

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而这些事情据Kashlinsky和他的同事们推断，可能是由于来自非常非常遥远的星系群的流动，所以，是不能以宇宙物质团块的不均匀分布来解释的。

And these flows that Kashlinsky and his colleagues have inferred of clusters that are very, very far away can't be explained by the lumpy distribution of matter.

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这些编码是四次群最大似然可译分布空时编码，并且功率在中继之间随时间均匀分布。

These codes are four-group ML decodable and have uniform distribution of power among the relays as well as in time.

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