activity
20032023
most citedOff the Beaten Path: A New Approach to Realistically Model The Orbital Decay of Supermassive Black Holes in Galaxy Formation Simulations

178 citations · 1.1k across the 18 of their papers we have counts for

collaborators
Showing 2014Show all

5 papers · 1 filter

astro-ph.EP201449 cited

The 3-dimensional architecture of the Upsilon Andromedae planetary system

Russell Deitrick, Rory Barnes, Barbara McArthur +4

The Upsilon Andromedae system is the first exoplanetary system to have the relative inclination of two planets' orbital planes directly measured, and therefore offers our first win…

astro-ph.IM20141 cited

Adaptive Techniques for Clustered N-Body Cosmological Simulations

Harshitha Menon, Lukasz Wesolowski, Gengbin Zheng +4

ChaNGa is an N-body cosmology simulation application implemented using Charm++. In this paper, we present the parallel design of ChaNGa and address many challenges arising due to t…

astro-ph.GA201498 cited

Faint dwarfs as a test of DM models: WDM vs. CDM

Fabio Governato, Daniel Weisz, Andrew Pontzen +12

We use high resolution HydroN-Body cosmological simulations to compare the assembly and evolution of a small field dwarf (stellar mass ~ 10 M, total mass 10$^{10}…

astro-ph.GA201477 cited

Orbital Decay of Supermassive Black Hole Binaries in Clumpy Multiphase Merger Remnants

R. Roškar, L. Mayer, D. Fiacconi +3

We simulate an equal-mass merger of two Milky Way-size galaxy discs with moderate gas fractions at parsec-scale resolution including a new model for radiative cooling and heating i…

astro-ph.EP2014132 cited

Effects of Extreme Obliquity Variations on the Habitability of Exoplanets

J. C. Armstrong, R. Barnes, S. Domagal-Goldman +3

We explore the impact of obliquity variations on planetary habitability in hypothetical systems with high mutual inclination. We show that large amplitude, high frequency obliquity…