After mapping millions of galaxies, dark energy survey finishes data collection

After mapping millions of galaxies, dark energy survey finishes data collection
The Dark Energy Survey, an international effort to map millions of galaxies, detect supernovae and find patterns of cosmic structure, finished taking data on Jan. 9, 2019. Credit: Fermilab

For the past six years, Fermi National Accelerator Laboratory has been part of an international effort to create an unprecedented survey of distant galaxies and better understand the nature of dark energy—the mysterious force accelerating the expansion of the universe.

After scanning about a quarter of the southern skies over 800 nights, the Dark Energy Survey finished taking data on Jan. 9. It ends as one of the most sensitive and comprehensive surveys of its kind, recording data from more than 300 million distant galaxies.

Fermilab, an affiliate of the University of Chicago, served as lead laboratory on the survey, which included more than 400 scientists and 26 institutions. The findings created the most accurate dark matter map of the universe ever made, shaping our understanding of the cosmos and its evolution. Other discoveries include the most distant supernova ever detected, a bevy of dwarf satellite galaxies orbiting our Milky Way, and helping to track the first-ever detection of gravitational waves from neutron stars back to its source.

According to Dark Energy Survey Director Rich Kron, a Fermilab scientist and professor at the University of Chicago, those results—and the scientists who made them possible—are where much of the real accomplishment of the Dark Energy Survey lies.

"The first generations of students and postdoctoral researchers on the Dark Energy Survey are now becoming faculty at research institutions and are involved in upcoming sky surveys," Kron said. "The number of publications and people involved are a true testament to this experiment. Helping to launch so many careers has always been part of the plan, and it's been very successful."

Now the job of analyzing that data takes center stage, providing opportunities for new breakthroughs. The survey has already released a full range of papers based on its first year of data, and scientists are now diving into the rich seam of catalogued images from the first several years of data, looking for clues to the nature of dark energy.

The first step in that process, according to Fermilab scientist Josh Frieman, a professor at UChicago and former director of the Dark Energy Survey, is to find the signal in all the noise.

"We're trying to tease out the signal of dark energy against a background of all sorts of non-cosmological stuff that gets imprinted on the data," Frieman said. "It's a massive ongoing effort from many different people around the world."

After mapping millions of galaxies, dark energy survey finishes data collection
The Dark Energy Survey’s primary instrument, the 570-megapixel Dark Energy Camera, is mounted on the Blanco Telescope in Chile. Credit: Fermilab

More comprehensive results on dark energy are expected within the next few years.

The data for the survey was collected using the Dark Energy Camera mounted on the Blanco 4-meter telescope at Cerro Tololo Inter-American Observatory in Chile. The camera, which is one of the most powerful digital imaging devices in existence, was built and tested at Fermilab, America's leading particle physics laboratory located in Batavia, Illinois. Fermilab is named after Nobel laureate Enrico Fermi, a Nobel-winning physicist and member of UChicago's faculty.

The Dark Energy Camera, called DECam, will remain mounted on the Blanco telescope at Cerro Tololo for another five to 10 years and will continue to be a useful instrument for scientific collaborations around the world.

"DECam was needed to carry out the Dark Energy Survey, but it also created a new tool for discovery—from the solar system to the distant universe," said Alistair Walker of the National Optical Astronomy Observatory, a Dark Energy Survey team member and the DECam instrument scientist. "For example, 12 new moons of Jupiter were recently discovered with DECam, and the detection of distant star-forming galaxies in the early universe, when the universe was only a few percent of its present age, has yielded new insights into the end of the cosmic dark ages."

Steve Heathcote, director of the Cerro Tololo Inter-American Observatory, also foresees a bright future for the Dark Energy Camera.

"Although the data taking for the Dark Energy Survey is coming to an end, DECam will continue its exploration of the universe from the Blanco telescope and is expected remain a front-line engine of discovery for many years," Heathcote said.

The generated 50 terabytes (50 million megabytes) of data over its six observation seasons. That data is stored and analyzed at the National Center for Supercomputing Applications at the University of Illinois at Urbana-Champaign.

The DES collaboration will now focus on generating new results from its six years of data, including new insights into dark . With one era at an end, the next era of the Dark Energy Survey is just beginning.


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Dark Energy Survey completes six-year mission

Citation: After mapping millions of galaxies, dark energy survey finishes data collection (2019, January 31) retrieved 16 June 2019 from https://phys.org/news/2019-01-millions-galaxies-dark-energy-survey.html
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Jan 31, 2019
Dark energy is the dark matter outflow associated with our universal black hole.

The energy described in the following article at the scale of our Universe's super-supermassive black hole is dark energy.

'Black holes banish matter into cosmic voids'
http://www.spaced...999.html

> "Some of the matter falling towards the [supermassive black] holes is converted into energy. This energy is delivered to the surrounding gas, and leads to large outflows of matter, which stretch for hundreds of thousands of light years from the black holes, reaching far beyond the extent of their host galaxies."

Our visible universe is in the outflow of a super-supermassive black hole. As ordinary matter falls toward the super-supermassive black hole it evaporates into dark matter. It is the dark matter outflow which pushes the galaxy clusters, causing them to move outward and away from us. The dark matter outflow is dark energy.

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