Through the observation of which energetic celestial events was the massive distribution pattern constituting the Quipu structure primarily mapped?
Gamma-Ray Bursts (GRBs)
The capability to map a structure as immense as the Quipu stems from utilizing extremely luminous astronomical markers rather than relying solely on the visible light from average galaxies, which are too faint or too distant to survey effectively at these cosmological scales. The key to tracing the Quipu was the study of Gamma-Ray Bursts (GRBs). GRBs are recognized as the most luminous electromagnetic events known in the universe, typically signaling the catastrophic collapse of massive stars into black holes or the merger of neutron stars. Because they shine so intensely, they can be detected across cosmological distances, acting as bright beacons. Astronomers found that the locations of these GRBs clustered along the filaments and walls that define the Quipu, thereby revealing the underlying scaffolding of matter.

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