activity
20032021
most citedAn Orphan in the "Field of Streams"

290 citations · 2.4k across the 28 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

10 papers · 1 filter

astro-ph.GA20216 cited

Chemodynamics of metal-poor wide binaries in the Galactic halo: Association with the Sequoia event

Dongwook Lim, Andreas J. Koch-Hansen, Camilla Juul Hansen +4

Recently, an increasing number of wide binaries has been discovered. Their chemical and dynamical properties are studied through extensive surveys and pointed observations. However…

astro-ph.GA202050 cited

Breaking Beta: A comparison of mass modelling methods for spherical systems

J. I. Read, G. A. Mamon, E. Vasiliev +6

We apply four different mass modelling methods to a suite of publicly available mock data for spherical stellar systems. We focus on the recovery of the density and velocity anisot…

astro-ph.GA2018

Reliable mass calculation in spherical gravitating systems

Foivos I. Diakogiannis, Geraint F. Lewis, Rodrigo A. Ibata +3

We present an innovative approach to the methodology of dynamical modelling, allowing practical reconstruction of the underlying dark matter mass without assuming both the density…

astro-ph.GA2018

Dynamical modelling of dwarf-spheroidal galaxies using Gaussian-process emulation

Amery Gration, Mark I. Wilkinson

We present a novel and efficient method for fitting dynamical models of stellar kinematic data in dwarf spheroidal galaxies (dSph). Our approach is based on Gaussian-process emulat…

astro-ph.GA201719 cited

A novel JEAnS analysis of the Fornax dwarf using evolutionary algorithms: mass follows light with signs of an off-centre merger

Foivos I. Diakogiannis, Geraint F. Lewis, Rodrigo A. Ibata +4

Dwarf galaxies, among the most dark matter dominated structures of our universe, are excellent test-beds for dark matter theories. Unfortunately, mass modelling of these systems su…

astro-ph.GA20172 cited

Too small to succeed: the difficulty of sustaining star formation in low-mass haloes

Claire Cashmore, Mark Wilkinson, Chris Power +1

We present high resolution simulations of an isolated dwarf spheroidal (dSph) galaxy between redshifts and , the epoch when several Milky Way dSph satellites exp…