2,500 New Active Black Holes Identified, Raising Questions About How They Evolve

Dark Energy Spectroscopic Instrument (DESI) finds actively feeding black holes and a host of other black hole candidates.

By Paul Smaglik
Feb 19, 2025 10:15 PMFeb 19, 2025 10:10 PM
Artist’s illustration of dwarf galaxy with active galactic nucleus (IMAGE)
This artist’s illustration depicts a dwarf galaxy that hosts an active galactic nucleus — an actively feeding black hole. In the background are many other dwarf galaxies hosting active black holes, as well as a variety of other types of galaxies hosting intermediate-mass black holes. (Credit: NOIRLab/NSF/AURA/J. da Silva/M. Zamani)

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Scientists using the Dark Energy Spectroscopic Instrument (DESI) have completed two major tasks. They’ve compiled the largest ever sample of dwarf galaxies (systems contain up to a mere several billion stars, compared to the Milky Way’s estimated 2 billion to 400 billion) that host an actively feeding black hole. They’ve also recorded the largest collection of potential intermediate-mass black holes so far.

Both results are reported in The Astrophysical Journal and provide new insight into the formation and evolution of both galaxies and black holes. They are essentially early returns from DESI’s 5-year run, representing about 20 percent of the first year of data collected by the instrument.

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