Hyperion proto-supercluster
The Hyperion proto-supercluster is the largest and earliest known proto-supercluster, 5,000 times the mass of the Milky Way and seen at 20% of the current age of the universe. It was discovered in 2018 by analysing the redshifts of 10,000 objects observed with the Very Large Telescope in Chile.
Discovery
The discovery was announced in late 2018.The discovery team led by Olga Cucciati used computational astrophysics methods and astroinformatics; statistical techniques were applied to large datasets of galaxy redshifts, using a two-dimensional Voronoi tessellation to correlate gravitational interaction of visible structures. The existence of non-visible structures was inferred.
Correlation was based on redshift data captured in a sky survey called VIMOS-VLT Deep Survey, using the Visible Multi Object Spectrograph instrument of the Very Large Telescope in Chile, and other surveys to a lesser extent. Spectroscopic redshift data for 3,822 objects was selected.
The discovery was published in Astronomy & Astrophysics in September 2018.