80 citations · 215 across the 10 of their papers we have counts for
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A Physical Model for the Quasar Luminosity Function Evolution between Cosmic Dawn and High Noon
Keven Ren, Michele Trenti
Modeling the evolution of the number density distribution of quasars through the Quasar Luminosity Function (QLF) is critical to improve our understanding of the connection between…
The Diversity of Environments Around Luminous Quasars at Redshift
Keven Ren, Michele Trenti, Madeline A. Marshall +2
Significant clustering around the rarest luminous quasars is a feature predicted by dark matter theory combined with number density matching arguments. However, this expectation is…
Limits to Rest-Frame Ultraviolet Emission From Far-Infrared-Luminous z~6 Quasar Hosts
Madeline A. Marshall, Mira Mechtley, Rogier A. Windhorst +20
We report on a Hubble Space Telescope search for rest-frame ultraviolet emission from the host galaxies of five far-infrared-luminous quasars and the hot-dust…
Stochastic Processes as the Origin of the Double-Power Law Shape of the Quasar Luminosity Function
Keven Ren, Michele Trenti, Tiziana Di Matteo
The Quasar Luminosity Function (QLF) offers insight into the early co-evolution of black holes and galaxies. It has been characterized observationally up to redshift with…
The Brightest Galaxies at Cosmic Dawn from Scatter in the Galaxy Luminosity versus Halo Mass Relation
Keven Ren, Michele Trenti, Charlotte A. Mason
The Ultraviolet Luminosity Function (UVLF) is a key observable for understanding galaxy formation from cosmic dawn. There has been considerable debate on whether Schechter-like LFs…
The Cosmic Web Around The Brightest Galaxies During The Epoch Of Reionization
Keven Ren, Michele Trenti, Simon J. Mutch
The most luminous galaxies at high-redshift are generally considered to be hosted in massive dark-matter halos of comparable number density, hence residing at the center of overden…