Supermassive black holes in cosmological simulations I: MBH − M⋆ relation and black hole mass function

@article{Habouzit2021SupermassiveBH,
  title={Supermassive black holes in cosmological simulations I: MBH − M⋆ relation and black hole mass function},
  author={M'elanie Habouzit and Yuan Li and Rachel S Somerville and Shy Genel and Annalisa Pillepich and Marta Volonteri and Romeel A. Dav'e and Yetli Rosas-Guevara and Stuart McAlpine and S{\'e}bastien Peirani and Lars Hernquist and Daniel Angl{\'e}s-Alc{\'a}zar and Amy E. Reines and Richard G. Bower and Yohan Dubois and Dylan Nelson and Christophe Pichon and Mark Vogelsberger},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2021}
}
The past decade has seen significant progress in understanding galaxy formation and evolution using large-scale cosmological simulations. While these simulations produce galaxies in overall good agreement with observations, they employ different sub-grid models for galaxies and supermassive black holes (BHs). We investigate the impact of the sub-grid models on the BH mass properties of the Illustris, TNG100, TNG300, Horizon-AGN, EAGLE, and SIMBA simulations, focusing on the MBH − M⋆ relation… 
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References

SHOWING 1-10 OF 174 REFERENCES
The Mass Relations between Supermassive Black Holes and Their Host Galaxies at 1 < z < 2 with HST-WFC3
Correlations between the mass of a supermassive black hole and the properties of its host galaxy (e.g., total stellar mass (M*), luminosity (Lhost)) suggest an evolutionary connection. A powerful
Black hole mass estimation for active galactic nuclei from a new angle
The scaling relations between supermassive black holes and their host galaxy properties are of fundamental importance in the context black hole-host galaxy co-evolution throughout cosmic time. In
Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies: Supplemental Material
This is the Supplemental Material to Kormendy and Ho 2013, ARAA, 51, 511 (arXiv:1304.7762). Section S1 summarizes indirect methods that are used to estimate black hole (BH) masses for galaxies with
A synthesis model for AGN evolution: supermassive black holes growth and feedback modes
We present a comprehensive synthesis model for the active galactic nuclei (AGN) evolution and the growth of supermassive black hole (SMBH) in the Universe. We assume that black holes accrete in just
Black hole – Galaxy correlations in simba
We examine the co-evolution of galaxies and supermassive black holes in the simba cosmological hydrodynamic simulation. simba grows black holes via gravitational torque-limited accretion from cold
First results from the IllustrisTNG simulations: matter and galaxy clustering
Hydrodynamical simulations of galaxy formation have now reached sufficient volume to make precision predictions for clustering on cosmologically relevant scales. Here we use our new IllustrisTNG
Relations Between Central Black Hole Mass and Total Galaxy Stellar Mass in the Local Universe
Scaling relations between central black hole (BH) mass and host galaxy properties are of fundamental importance to studies of BH and galaxy evolution throughout cosmic time. Here we investigate the
The EAGLE simulations of galaxy formation: calibration of subgrid physics and model variations
We present results from thirteen cosmological simulations that explore the parameter space of the "Evolution and Assembly of GaLaxies and their Environments" (EAGLE) simulation project. Four of the
CONSTRAINTS ON BLACK HOLE GROWTH, QUASAR LIFETIMES, AND EDDINGTON RATIO DISTRIBUTIONS FROM THE SDSS BROAD-LINE QUASAR BLACK HOLE MASS FUNCTION
We present an estimate of the black hole mass function of broad-line quasars (BLQSOs) that self-consistently corrects for incompleteness and the statistical uncertainty in the mass estimates, based
Black holes on FIRE: stellar feedback limits early feeding of galactic nuclei
We introduce massive black holes (BHs) in the Feedback In Realistic Environments (FIRE) project and perform high-resolution cosmological hydrodynamic simulations of quasar-mass haloes [Mhalo(z = 2) ≈
...
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