activity
20092026
most citedThe EAGLE project: Simulating the evolution and assembly of galaxies and their environments

3.7k citations · 7.6k across the 48 of their papers we have counts for

collaborators
Showing 2016Show all

9 papers · 1 filter

astro-ph.GA2016★ 18 cited

Tidal features of classical Milky Way satellites in a CDM universe

M. -Y. Wang, Azadeh Fattahi, Andrew P. Cooper +6

We use the APOSTLE cosmological hydrodynamic simulations to examine the effects of tidal stripping on cold dark matter (CDM) sub haloes that host three of the most luminous Milky W…

astro-ph.GA2016★ 79 cited

Post-Newtonian dynamical modeling of supermassive black holes in galactic-scale simulations

Antti Rantala, Pauli Pihajoki, Peter H. Johansson +3

We present KETJU, a new extension of the widely-used smoothed particle hydrodynamics simulation code GADGET-3. The key feature of the code is the inclusion of algorithmically regul…

astro-ph.GA2016★ 57 cited

Properties of Local Group galaxies in hydrodynamical simulations of sterile neutrino dark matter cosmologies

Mark R. Lovell, Sownak Bose, Alexey Boyarsky +10

We study galaxy formation in sterile neutrino dark matter models that differ signifi- cantly from both cold and from `warm thermal relic' models. We use the EAGLE code to carry out…

astro-ph.GA2016★ 88 cited

The oldest and most metal poor stars in the APOSTLE Local Group simulations

Else Starkenburg, Kyle A. Oman, Julio F. Navarro +5

We examine the spatial distribution of the oldest and most metal poor stellar populations of Milky Way-sized galaxies using the APOSTLE cosmological hydrodynamical simulations of t…

astro-ph.GA2016★ 125 cited

Shaken and Stirred: The Milky Way's Dark Substructures

Till Sawala, Pauli Pihajoki, Peter H. Johansson +4

The predicted abundance and properties of the low-mass substructures embedded inside larger dark matter haloes differ sharply among alternative dark matter models. Too small to hos…

astro-ph.GA2016★ 46 cited

The cold dark matter content of Galactic dwarf spheroidals: no cores, no failures, no problem

Azadeh Fattahi, Julio F. Navarro, Till Sawala +5

We examine the dark matter content of satellite galaxies in Lambda-CDM cosmological hydrodynamical simulations of the Local Group from the APOSTLE project. We find excellent agreem…

astro-ph.GA2016★ 65 cited

Knowing the unknowns: uncertainties in simple estimators of galactic dynamical masses

David J. R. Campbell, Carlos S. Frenk, Adrian Jenkins +7

The observed stellar kinematics of dispersion-supported galaxies are often used to measure dynamical masses. Recently, several analytical relationships between the stellar line-of-…

astro-ph.GA2016★ 92 cited

The low-mass end of the baryonic Tully-Fisher relation

Laura V. Sales, Julio F. Navarro, Kyle Oman +11

The scaling of disk galaxy rotation velocity with baryonic mass (the "Baryonic Tully-Fisher" relation, BTF) has long confounded galaxy formation models. It is steeper than the M ~…

astro-ph.GA2016★ 86 cited

Missing dark matter in dwarf galaxies?

Kyle A. Oman, Julio F. Navarro, Laura V. Sales +5

We use cosmological hydrodynamical simulations of the APOSTLE project along with high-quality rotation curve observations to examine the fraction of baryons in ΛCDM haloes that col…