The Dark Energy Spectroscopic Instrument (DESI) completed its 5 month Survey Validation
in 2021 May. Spectra of stellar and extragalactic targets from Survey Validation constitute …

We present the completed catalog of ultradiffuse galaxy (UDG) candidates (7070 objects)
from our search of the DR9 Legacy Survey images, including distance and total mass …

We study the formation of ultradiffuse galaxies (UDGs) using the cosmological
hydrodynamical simulation TNG50 of the Illustris-TNG suite. We define UDGs as dwarf …

In this work, we extend the catalog of low-surface brightness (LSB) galaxies, including ultra-
diffuse galaxy (UDG) candidates, within≈ 0.4R vir of the Hydra I cluster of galaxies based …

We present a catalog of 5598 ultra-diffuse galaxy (UDG) candidates with effective radius re>
5 farcs 3 distributed throughout the southern portion of the DESI Legacy Imaging Survey …

We use spectral energy distribution (SED) fitting to place constraints on the stellar
population properties of 29 quiescent ultra-diffuse galaxies (UDGs) across different …

We examine ultra-diffuse galaxies (UDGs) and their relation to non-UDGs in mass–radius–
luminosity space. We begin by publishing Keck/KCWI spectroscopy for the Coma cluster …

We use spectral energy distribution fitting to place constraints on the stellar populations of
59 ultra-diffuse galaxies (UDGs) in the low-to-moderate density fields of the MATLAS survey …

The Dark Energy Spectroscopic Instrument (DESI) completed its five-month Survey
Validation in May 2021. Spectra of stellar and extragalactic targets from Survey Validation …

Large diffuse galaxies are hard to find, but understanding the environments where they live,
their numbers, and ultimately their origins, is of intense interest and importance for galaxy …