Maximilian Häberle

Sep 17, 2024 | nature.com | Maximilian Häberle |Nadine Neumayer |Anil Seth |Andrea Bellini |Mattia Libralato |Holger Baumgardt | +11 more

Correction to: Nature https://doi.org/10.1038/s41586-024-07511-z Published online 10 July 2024In the version of the article initially published, the third equation in the “The escape velocity provides a minimum black hole mass” section was presented incorrectly; the original and revised equations are shown below. The error was in description, only, and does not impact the results.

Jul 10, 2024 | nature.com | Maximilian Häberle |Nadine Neumayer |Anil Seth |Andrea Bellini |Mattia Libralato |Holger Baumgardt | +11 more

AbstractBlack holes have been found over a wide range of masses, from stellar remnants with masses of 5–150 solar masses (M☉), to those found at the centres of galaxies with M > 105M☉. However, only a few debated candidate black holes exist between 150M☉ and 105M☉. Determining the population of these intermediate-mass black holes is an important step towards understanding supermassive black hole formation in the early universe1,2.