activity
20192021
collaborators

7 papers

astro-ph.GA2021

EDGE: Two routes to dark matter core formation in ultra-faint dwarfs

Matthew D. A. Orkney, Justin I. Read, Martin P. Rey +6

In the standard Lambda cold dark matter paradigm, pure dark matter simulations predict dwarf galaxies should inhabit dark matter haloes with a centrally diverging density `cusp'. T…

hep-ph2020

New Constraints on the Mass of Fermionic Dark Matter from Dwarf Spheroidal Galaxies

James Alvey, Nashwan Sabti, Victoria Tiki +7

Dwarf spheroidal galaxies are excellent systems to probe the nature of fermionic dark matter due to their high observed dark matter phase-space density. In this work, we review, re…

astro-ph.GA2020

EDGE: A new approach to suppressing numerical diffusion in adaptive mesh simulations of galaxy formation

Andrew Pontzen, Martin P. Rey, Corentin Cadiou +4

We introduce a new method to mitigate numerical diffusion in adaptive mesh refinement (AMR) simulations of cosmological galaxy formation, and study its impact on a simulated dwarf…

astro-ph.GA2020

EDGE: From quiescent to gas-rich to star-forming low-mass dwarf galaxies

Martin P. Rey, Andrew Pontzen, Oscar Agertz +3

We study how star formation is regulated in low-mass field dwarf galaxies (), using cosmological high-resolution ($3 \, \text{pc}…

astro-ph.GA2019

EDGE: The origin of scatter in ultra-faint dwarf stellar masses and surface brightnesses

Martin P. Rey, Andrew Pontzen, Oscar Agertz +4

We demonstrate how the least luminous galaxies in the Universe, ultra-faint dwarf galaxies, are sensitive to their dynamical mass at the time of cosmic reionization. We select a lo…

astro-ph.GA2019

Globular clusters as probes of dark matter cusp-core transformations

M. D. A. Orkney, J. I. Read, James A. Petts +1

Bursty star formation in dwarf galaxies can slowly transform a steep dark matter cusp into a constant density core. We explore the possibility that globular clusters (GCs) retain a…