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Tidal Disruption Event Rates across Cosmic Time: Forecasts for LSST, Roman, and JWST and Their Constraints on the Supermassive Black Hole Mass Function

  • Authors: Mitchell Karmen, Suvi Gezari, Colin Norman, Muryel Guolo

Mitchell Karmen et al 2026 The Astrophysical Journal 1006 .

  • Provider: AAS Journals

Caption: Figure 10.

Exponential approximations to the BHMF “slope,” colored by exponent γ (Equation (23)). The semiempirical BHMF (F. Shankar et al. 2009) is well approximated by exponential downsizing with redshift, while the simulated BHMFs behave more stochastically.

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