Melanie Habouzit

TL;DR: In this article, the authors investigate the formation, distribution and growth of BH seeds by using the adaptive mesh refinement code Ramses and find that all high-mass galaxies tend to a host a BH, whereas low-mass counterparts have a lower probability of hosting a H. This probability is modulated by the growth of the galaxy.

TL;DR: In this article, the authors investigate how a typical sub-grid model for AGN feedback affects the evolution of the inner density profiles of massive dark matter haloes and galaxies and find that the integrated inner mass and density slope differences between objects formed in these three simulations significantly evolve with time.

TL;DR: In this article, the authors performed several cosmological hydrodynamical simulations that cover a large range of box sizes and resolutions, thus allowing them to understand the impact of several physical processes on the distribution of direct collapse BHs.

TL;DR: In this paper , a review of the current knowledge in three main source classes for LISA is reviewed; ultracompact stellar-mass binaries, massive black hole binaries, and extreme or intermediate mass ratio inspirals.

TL;DR: The connection between the rapid growth of the first supermassive black holes and the fast chemical evolution of the host galaxy is one of the most puzzling issues for theoretical models as discussed by the authors, with particular emphasis on the conditions that lead to the formation of quasar seeds and their subsequent evolution at z ⩾ 6.