activity
20082026
most citedTracing the outer halo in a giant elliptical to 25 Reff

46 citations · 118 across the 12 of their papers we have counts for

collaborators
Showing 2024Show all

6 papers · 1 filter

astro-ph.GA2024

Massive Star Cluster Formation with Binaries. I. Evolution of Binary Populations

Claude Cournoyer-Cloutier, Alison Sills, William E. Harris +7

We study the evolution of populations of binary stars within massive cluster-forming regions. We simulate the formation of young massive star clusters within giant molecular clouds…

astro-ph.GA2024★ 8 cited

Discovery of Two Ultra-Diffuse Galaxies with Unusually Bright Globular Cluster Luminosity Functions via a Mark-Dependently Thinned Point Process (MATHPOP)

Dayi Li, Gwendolyn Eadie, Patrick Brown +8

We present \textsc{Mathpop}, a novel method to infer the globular cluster (GC) counts in ultra-diffuse galaxies (UDGs) and low-surface brightness galaxies (LSBGs). Many known UDGs…

astro-ph.SR2024

The Effect of Age and Stellar Model Choice on Globular Cluster Color-to-Metallicity Conversions

Kate Hartman, William E. Harris

The photometric colors of globular clusters (GCs) act as effective proxies for metallicity, since all normally used optical/IR color indices exhibit a nonlinear but monotonic relat…

astro-ph.IM2024★ 2 cited

Utilizing Voronoi Tessellations to Determine Radial Density Profiles

Veronika Dornan, William E. Harris

We have developed a novel method of determining 2D radial density profiles for astronomical systems of discrete objects using Voronoi tessellations. This Voronoi-based method was t…

astro-ph.IM2024

Photometric Completeness Modelled With Neural Networks

William E. Harris, Joshua S. Speagle

In almost any study involving optical/NIR photometry, understanding the completeness of detection and recovery is an essential part of the work. The recovery fraction is, in genera…

astro-ph.GA2024★ 3 cited

Deep HST/UVIS imaging of the candidate dark galaxy CDG-1

Pieter van Dokkum, Dayi David Li, Roberto Abraham +4

CDG-1 is a tight grouping of four likely globular clusters in the Perseus cluster, and a candidate dark galaxy with little or no diffuse light. Here we provide new constraints on t…