An article to be published in “The Astrophysical Journal” reports the discovery of about 2,500 new candidate active galactic nuclei in dwarf galaxies and about 300 new candidate intermediate-mass black holes. A team of researchers examined observations conducted with the Dark Energy Spectroscopic Instrument (DESI) on the Nicholas U. Mayall 4-meter Telescope in Arizona to find all these possible black holes.

An article published in the journal Nature Astronomy reports the results of a study of seven galaxy clusters which contain various supermassive black holes that offers evidence that outbursts generated at these black holes help cool the gas they feed on. A team of researchers used observations with multiple instruments to examine seven galaxy clusters. Outbursts in the form of jets from the supermassive black holes in those clusters cool the gas by forming thin filaments. Some of that gas will eventually flow back toward those black holes, triggering more outbursts in a mechanism in which the black holes “cook” their own meals.

Two articles – one published in the journal “Nature Astronomy” and one in “The Astrophysical Journal Letters” – report different aspects of a study of the blazar cataloged as VLASS J041009.05−013919.88, or simply J0410−0139, the most distant found so far. Two teams of researchers used several space and ground-based telescopes and some radio telescopes to obtain detections in various electromagnetic bands.

An article published in the journal “The Astrophysical Journal” reports the results of X-ray observations of the jets emitted by the supermassive black hole at the center of the Centaurus A galaxy. A team of researchers used NASA’s Chandra X-ray Observatory to find a V-shaped structure that indicates that one of the jets hit something whose nature is uncertain. Only Chandra’s X-ray observations revealed that unusual structure, cataloged as C4, while many other instruments, especially radio telescopes, had never shown such anomalies.

An article published in the journal “Nature Astronomy” reports the results of the study of the dwarf galaxy cataloged as LID-568, which has at its center a supermassive black hole that is devouring materials at a rate that is more than 40 times faster than its theoretical limits. A team of researchers led by astronomer Hyewon Suh of the International Gemini Observatory/NSF NOIRLab combined observations conducted with the Chandra and James Webb space telescopes to obtain precise data on this voracious supermassive black hole. We see it as it was about 1.5 billion years after the Big Bang and its discovery indicates a way in which these very extreme objects manage to grow so quickly.