90 citations · 203 across the 11 of their papers we have counts for
7 papers · 1 filter
Robust Measurement of Stellar Streams Around the Milky Way: Correcting Spatially Variable Observational Selection Effects in Optical Imaging Surveys
K. K. Boone, P. S. Ferguson, M. Tabbutt +47
Observations of density variations in stellar streams are a promising probe of low-mass dark matter substructure in the Milky Way. However, survey systematics such as variations in…
An Assessment of the In-Situ Growth of the Intracluster Light in the High Redshift Galaxy Cluster SpARCS1049+56
Capucine Barfety, Félix-Antoine Valin, Tracy M. A. Webb +11
The formation of the stellar mass within galaxy cluster cores is a poorly understood process. It features the complicated physics of cooling flows, AGN feedback, star formation and…
The Morphology-Density relationship in 1<z<2 clusters
Elizaveta Sazonova, Katherine Alatalo, Jennifer Lotz +8
The morphology-density relationship states that dense cosmic environments such as galaxy clusters have an overabundance of quiescent elliptical galaxies, but it is unclear at which…
See Change: VLT spectroscopy of a sample of high-redshift Type Ia supernova host galaxies
S. C. Williams, I. M. Hook, B. Hayden +9
The Supernova Cosmology Project has conducted the `See Change' programme, aimed at discovering and observing high-redshift (1.13 z 1.75) Type Ia supernovae (SNe Ia).…
The Massive and Distant Clusters of WISE Survey VI: Stellar Mass Fractions of a Sample of High-Redshift Infrared-selected Clusters
Bandon Decker, Mark Brodwin, Zubair Abdulla +17
We present measurements of the stellar mass fractions () for a sample of high-redshift () infrared-selected galaxy clusters from the Massive and Dista…
ALMA Observations of Gas-Rich Galaxies in z~1.6 Galaxy Clusters: Evidence for Higher Gas Fractions in High-Density Environments
A. G. Noble, M. McDonald, A. Muzzin +16
We present ALMA CO (2-1) detections in 11 gas-rich cluster galaxies at z~1.6, constituting the largest sample of molecular gas measurements in z>1.5 clusters to date. The observati…