What key difference in appearance or nature is noted when comparing the structure of the Quipu to the Hercules-Corona Borealis Great Wall (HCBBW)?
The Quipu appears to be a more coherent, filamentary structure.
Both the Quipu and the Hercules-Corona Borealis Great Wall (HCBBW) have been cited as candidates for record-breaking size, with both estimated around 10 billion light-years across. However, when examining the evidence derived from tracing methods—both utilizing Gamma-Ray Bursts—a distinction arises in their perceived physical configuration. The Quipu is characterized as appearing to be a more cohesive and distinctly filamentary structure composed of galaxy filaments and proto-superclusters woven together. In contrast, the HCBBW, while also a massive overdensity traced through specific GRB distributions, may represent a slightly different manifestation of large-scale grouping, suggesting less structural coherence than what is attributed to the Quipu network.

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