In their paper, they explained that in order to study the weak lensing signal of the dark matter filaments, they required two sets of data: a catalog of galaxy cluster pairs that were lensed, and a catalog of background source galaxies with accurate distance measurements.
They combined lensing data from a multi-year sky survey at the Canada-France-Hawaii Telescope with information from the Sloan Digital Sky Survey that mapped luminous red galaxies (LRGs), which are massive, distant, and very old galaxies.
“LRGs are very bright galaxies,” Hudson told Seeker via email. “They tend to be more massive than the average galaxy and live in more massive dark matter ‘halos.’ It's reasonable to expect that the filament or bridge between them might also be more massive than the average.”
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Hudson and Epps combined or “stacked” more than 23,000 galaxy pairs, all located about 4.5 billion light-years away. This allowed them to create a composite image or map that shows the presence of dark matter between galaxies. Hudson told Seeker that the filament in their “image” is the average of all 23,000 pairs.
“The primary reason that we used these galaxies is that they had precise distances (as measured by another team),” Hudson explained. “These distance measurements allowed us to distinguish between pairs of galaxies that were actual pairs in 3D (meaning both are at the same distance from us) as opposed to two galaxies that appeared close on the sky but were actually at very different distances.”
3D pairs would be physically close to each other and hence, will have a bridge whereas the second group are not physically close to each other, and so would not have a bridge between them. Hudson and Epps said their results show the dark matter filament bridge is strongest between systems less than 40 million light years apart.
“By using this technique, we’re not only able to see that these dark matter filaments in the universe exist, we’re able to see the extent to which these filaments connect galaxies together,” Epps said in a statement.
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The Big Bang theory predicts that variations in the density of matter in the very first moments of the universe led the bulk of the matter in the cosmos to condense into a web of tangled filaments. To explain this, astronomer Fritz Zwicky first introduced the concept of dark matter in 1933, when his measurements of galaxies moving within a galaxy cluster showed they must have at least ten times more invisible matter than what is visible.
But it wasn’t until the 1970s that dark matter was taken seriously. Vera Rubin and Kent Ford Jr. mapped the motions of stars within galaxies close to our own Milky Way, and they also concluded that each galaxy had to include enormous amounts of unseen matter, far more than all the visible matter. Later, computer simulations confirmed this and suggested the existence of dark matter, structured like a web, with long filaments that connect to each other at the locations of massive galaxy clusters.
In their paper, Hudson and Epps list dozens of previous studies that have attempted to measure and observe the dark matter web, and they say they hope their stacking techniques to measure the filaments between groups and clusters of galaxies can serve as a foundation for future filament studies. They hope upcoming surveys and telescopes will continue to further our understanding of dark matter.
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