From Universe Today, Feb. 3, 2021: Recent published results from the Dark Energy Survey point to intracluster light — feeble light from rogue stars that don’t belong to a galaxy — as a potential pathway to measure dark matter. Fermilab scientist Yuanyuan Zhang contextualizes the findings.
From Super Interessante, Jan. 31, 2021: A team of researchers from Fermilab and the National Observatory in Brazil used the light of solitary stars to calculate the mass of some of the largest structures in the cosmos — galaxy clusters. In addition to taking the most detailed measurement ever published of intracluster light, the team’s new method of measurement can help further investigate dark matter.
From Forbes, Jan. 14, 2021: The Dark Energy Survey recently publicly released an enormous amount of data for anyone to use. This data set contains nearly seven hundred million individual astronomical objects. Fermilab scientist Don Lincoln explains how collaborators on the Dark Energy Survey study the history of the universe and highlights a number of the scientific findings in DES’s rich trove of data.
The international collaboration, including Fermilab, the National Center for Supercomputing Applications, NOIRLab and others, releases a massive, public collection of astronomical data and calibrated images from six years of surveys. This data release is one of the largest astronomical catalogs issued to date.
Scientists on the Dark Energy Survey have used observations of the smallest known galaxies to better understand dark matter, the mysterious substance that makes up 85% of the matter in the universe. The smallest galaxies can contain hundreds to thousands of times more dark matter than normal visible matter, making them ideal laboratories for studying this mysterious substance. By performing a rigorous census of small galaxies surrounding our Milky Way, scientists on the Dark Energy Survey have been able to constrain the fundamental particle physics that governs dark matter.
From Astronomy, March 31, 2020: Astronomers have discovered 139 new minor planets orbiting the Sun beyond Neptune by searching through data from the Dark Energy Survey, which is led by Fermilab. The new method for spotting small worlds is expected to reveal many thousands of distant objects in coming years — meaning these first hundred or so are likely just the tip of the iceberg.
From WDRB, March 29, 2020: A study published earlier this month by astronomers at the University of Pennsylvania distinguished more than 100 new planets in our solar system, but estimates show there could be as many as 70,000. These trans-Neptunian objects were found in the data gathered by the Dark Energy Survey, led by Fermilab.
From EarthSky, March 29, 2020: Astronomers analyzed data from the Dark Energy Survey, led by Fermilab, to find over 100 new little worlds in the cold outer reaches of our solar system. These trans-Neptunian objects orbit in the cold outer reaches of our solar system, out beyond Neptune, taking hundreds of years to orbit the sun once.
From Physics World, March 24, 2020: Scientists using the first year of data from the Dark Energy Survey, which is led by Fermilab, establish that there is a correlation between the positions of gravitational lenses — deduced from the stretching of distant galaxies — and gamma-ray photons. A data comparison from gravitational lensing and gamma-ray observations reveals that regions of the sky with greater concentrations of matter emit more gamma rays.