The host galaxies of z=7 quasars: predictions from the BLUETIDES simulation
Madeline A Marshall, Yueying Ni, Tiziana Di Matteo, J Stuart B Wyithe, Stephen Wilkins, Rupert AC Croft, Jussi K Kuusisto
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | OXFORD UNIV PRESS | Published : 2020
We examine the properties of the host galaxies of z=7 quasars using the large volume, cosmological hydrodynamical simulation BLUETIDES. We find that the 10 most massive black holes and the 191 quasars in the simulation (with MUV,AGN106.5M⊙ black hole, indicating that minor mergers play at least some role in growing black holes in the early Universe.
Awarded by Australian Research Council Centre of Excellence
Awarded by NSF
Awarded by NASA
We thank the referee for valuable and constructive comments that helped to improve the quality of this paper. We also thank Bram Venemans for a useful discussion on the measurement of star formation rates from sub-mm observations. This research was supported by the Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), through project number CE170100013. The BLUETIDES simulation was run on the BlueWaters facility at the National Center for Supercomputing Applications. Part of this work was performed on the OzSTAR national facility at Swinburne University of Technology, which is funded by Swinburne University of Technology and the National Collaborative Research Infrastructure Strategy (NCRIS). MAM acknowledges the support of an Australian Government Research Training Program (RTP) Scholarship, and a Postgraduate Writing-Up Award sponsored by the Albert Shimmins Fund. TDM acknowledges funding from NSF ACI-1614853, NSF AST-1517593, NSF AST-1616168, and NASA ATP 19-ATP19-0084. TDM and RAC also acknowledge ATP 80NSSC18K101 and NASA ATP 17-0123. This paper makes use of version 17.00 of CLOUDY, last described by Ferland et al. (2017).