activity
20152023
most citedDark matter cores all the way down

317 citations · 799 across the 13 of their papers we have counts for

collaborators

14 papers

astro-ph.GA2023

A search for faint resolved galaxies beyond the Milky Way in DES Year 6: A new faint, diffuse dwarf satellite of NGC 55

M. McNanna, K. Bechtol, S. Mau +63

We report results from a systematic wide-area search for faint dwarf galaxies at heliocentric distances from 0.3 to 2 Mpc using the full six years of data from the Dark Energy Surv…

astro-ph.GA2023

The Hubble Space Telescope Survey of M31 Satellite Galaxies II. The Star Formation Histories of Ultra-Faint Dwarf Galaxies

A. Savino, D. R. Weisz, E. D. Skillman +34

We present the lifetime star formation histories (SFHs) for six ultra-faint dwarf (UFD; , ) satellite galaxies of M31 based on…

hep-ex2021★ 1 cited

Updated physics performance of the ESSnuSB experiment

A. Alekou, E. Baussan, N. Blaskovic Kraljevic +48

In this paper, we present the physics performance of the ESSnuSB experiment in the standard three flavor scenario using the updated neutrino flux calculated specifically for the ES…

astro-ph.GA2020★ 11 cited

The Elusive Distance Gradient in the Ultra-Faint Dwarf Galaxy Hercules: A Combined Hubble Space Telescope and Gaia View

Burçin Mutlu-Pakdil, David J. Sand, Denija Crnojević +6

The ultra-faint dwarf galaxy Hercules has an extremely elongated morphology with both photometric overdensities and kinematic members at large radii, suggesting that it may be tida…

astro-ph.GA2019★ 22 cited

Signatures of Tidal Disruption in Ultra-Faint Dwarf Galaxies: A Combined HST, Gaia, and MMT/Hectochelle Study of Leo V

Burçin Mutlu-Pakdil, David J. Sand, Matthew G. Walker +10

The ultra-faint dwarf galaxy Leo V has shown both photometric overdensities and kinematic members at large radii, along with a tentative kinematic gradient, suggesting that it may…

astro-ph.GA2018★ 135 cited

Extending the Globular Cluster System-Halo Mass Relation to the Lowest Galaxy Masses

Duncan A. Forbes, Justin I. Read, Mark Gieles +1

High mass galaxies, with halo masses , reveal a remarkable near-linear relation between their globular cluster (GC) system mass and their host galaxy…