activity
20142018
most citedThe Caterpillar Project: A Large Suite of Milky Way Sized Halos

120 citations · 511 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.GA2018★ 44 cited

The Origin of r-process Enhanced Metal-Poor Halo Stars In Now-Destroyed Ultra-Faint Dwarf Galaxies

Kaley Brauer, Alexander P. Ji, Anna Frebel +3

The highly r-process enhanced (r-II) metal-poor halo stars we observe today could play a key role in understanding early ultra-faint dwarf galaxies, the smallest building blocks of…

astro-ph.GA2018★ 30 cited

CDM Predictions for the Satellite Population of M33

Ekta Patel, Jeffrey L. Carlin, Erik J. Tollerud +2

Triangulum (M33) is the most massive satellite galaxy of Andromeda (M31), with a stellar mass of about . Based on abundance matching techniques, M33's tota…

astro-ph.GA2017★ 12 cited

Selecting ultra-faint dwarf candidate progenitors in cosmological N-body simulations at high redshifts

Mohammadtaher Safarzadeh, Alexander P. Ji, Gregory A. Dooley +4

The smallest satellites of the Milky Way ceased forming stars during the epoch of reionization and thus provide archaeological access to galaxy formation at . Numerical studie…

astro-ph.GA2017★ 84 cited

The predicted luminous satellite populations around SMC and LMC-mass galaxies - A missing satellite problem around the LMC?

Gregory A. Dooley, Annika H. G. Peter, Jeffrey L. Carlin +3

Recent discovery of many dwarf satellite galaxies in the direction of the Small and Large Magellanic Clouds (SMC and LMC) provokes questions of their origins, and what they can rev…

astro-ph.GA2016★ 61 cited

Tracing the first stars and galaxies of the Milky Way

Brendan F. Griffen, Gregory A. Dooley, Alexander P. Ji +3

We use 30 high-resolution dark matter halos of the simulation suite to probe the first stars and galaxies of Milky Way-mass systems. We quantify the environment of th…

astro-ph.GA2016★ 55 cited

An observer's guide to the (Local Group) dwarf galaxies: predictions for their own dwarf satellite populations

Gregory A. Dooley, Annika H. G. Peter, Tianyi Yang +3

A recent surge in the discovery of new ultrafaint dwarf satellites of the Milky Way has inspired the idea of searching for faint satellites, $10^3\, \mathrm{M_{\odot}} < M_* < 10^6…

astro-ph.GA2016★ 78 cited

Enhanced tidal stripping of satellites in the galactic halo from dark matter self-interactions

Gregory A. Dooley, Annika H. G. Peter, Mark Vogelsberger +2

We investigate the effects of self-interacting dark matter (SIDM) on the tidal stripping and evaporation of satellite galaxies in a Milky Way-like host. We use a suite of five zoom…

astro-ph.GA2015★ 120 cited

The Caterpillar Project: A Large Suite of Milky Way Sized Halos

Brendan F. Griffen, Alexander P. Ji, Gregory A. Dooley +4

We present the largest number of Milky Way sized dark matter halos simulated at very high mass ( M/particle) and temporal resolution (5 Myrs/snapshot) don…

astro-ph.CO2014★ 27 cited

The Effects of Varying Cosmological Parameters on Halo Substructure

Gregory A. Dooley, Brendan F. Griffen, Phillip Zukin +4

We investigate how different cosmological parameters, such as those delivered by the WMAP and Planck missions, affect the nature and evolution of dark matter halo substructure. We…