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Cosmographic mapping of the Sloan Great Wall reveals the largest known basin of attraction

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[Submitted on 3 Jun 2026]

4d ago· 2 min readenInsight

Summary

This paper presents a cosmographic analysis of the Sloan Great Wall using Hamiltonian Monte Carlo forward reconstruction within a ΛCDM framework. Constrained by the Cosmicflows-4 compendium of galaxy distances and radial velocities, the study reconstructs probabilistic density and velocity fields. By following velocity streamlines to gravitational potential minima, the researchers identify the Sloan basin of attraction as the largest in the study region, spanning ~0.13c (about 560 million light-years) in diameter. The analysis reveals how streamlines converge on the Sloan Great Wall, and examines the relationship with the Ho`oleilana baryon acoustic oscillation feature. The findings are augmented by video and interactive models.

Key quotes

· 4 pulled
The Sloan basin of attraction is by far the largest basin in the study region, extending across a diameter of ~0.13c.
Streamlines of the reconstructed velocity field started from arbitrary points in space can be followed to sinks, i.e. the minima of the gravitational potential, due to the distribution of mass.
It is of interest to see the relationship of the Ho`oleilana baryon acoustic oscillation feature with the Sloan basin of attraction.
The solution can be assigned probabilities, with uncertainties associated with the imperfect data and the random nature of the ΛCDM model.
Snippet from the RSS feed
The Sloan Great Wall is a dominant structure that is relatively nearby. As well as evident in redshift survey maps, its presence is manifested in distortions to cosmic expansion. Here, Hamiltonian Monte Carlo forward reconstruction in a ΛCDM framework giv

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