933 citations · 6.4k across the 103 of their papers we have counts for
105 papers
GOGREEN: a critical assessment of environmental trends in cosmological hydrodynamical simulations at z ~ 1
Egidijus Kukstas, Michael L. Balogh, Ian G. McCarthy +28
Recent observations have shown that the environmental quenching of galaxies at z ~ 1 is qualitatively different to that in the local Universe. However, the physical origin of these…
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…
Ionizing radiation from AGNs at z>3.3 with the Subaru Hyper Suprime-Cam Survey and the CFHT Large Area U-band Deep Survey (CLAUDS)
Ikuru Iwata, Marcin Sawicki, Akio K. Inoue +8
We use deep and wide imaging data from the CFHT Large Area U-band Deep Survey (CLAUDS) and the Hyper Suprime-Cam Subaru Strategic Program (HSC-SSP) to constrain the ionizing radiat…
HST/WFC3 grism observations of clusters: Evidence for rapid outside-in environmental quenching from spatially resolved H maps
Jasleen Matharu, Adam Muzzin, Gabriel B. Brammer +12
We present and publicly release (https://www.gclasshst.com) the first spatially resolved H maps of star-forming cluster galaxies at , made possible with the Wide Field C…
The GOGREEN survey: Transition Galaxies and The Evolution of Environmental Quenching
Karen McNab, Michael L. Balogh, Remco F. J. van der Burg +25
We measure the rate of environmentally-driven star formation quenching in galaxies at , using eleven massive () galaxy clusters…
The GOGREEN survey: Dependence of galaxy properties on halo mass at z > 1 and implications for environmental quenching
Andrew M. M. Reeves, Michael L. Balogh, Remco F. J. van der Burg +18
We use photometric redshifts and statistical background subtraction to measure stellar mass functions in galaxy group-mass () haloes at $1<z<1.…