340 citations · 4.3k across the 51 of their papers we have counts for
48 papers
The AGN fraction in high-redshift protocluster candidates selected by Planck and Herschel
Caleb Gatica, Ricardo Demarco, Hervé Dole +4
A complete understanding of the mass assembly history of structures in the universe requires the study of the growth of galaxies and their supermassive black holes (SMBHs) as a fun…
The galaxy mass-size relation in CARLA clusters and proto-clusters at 1.4 < z < 2.8: larger cluster galaxy sizes
Anton V. Afanasiev, Simona Mei, Hao Fu +12
(Abridged) We study the galaxy mass-size relation in CARLA spectroscopically confirmed clusters at , which span a total stellar mass $11.3<\mathrm{log}(M^c_*/M_{\odot})<…
Morphology-density Relation, Quenching, and Mergers in CARLA Clusters and Proto-Clusters at
Simona Mei, Nina A. Hatch, Stefania Amodeo +11
(Abridged) To understand if the morphology-density and passive-density relations are already established at z>1.5, we study galaxies in 16 confirmed clusters at from th…
Massive molecular gas reservoir around the central AGN in the CARLA J1103+3449 cluster at z=1.44
Vladan Markov, Simona Mei, Philippe Salomé +14
Passive early-type galaxies dominate cluster cores at z 1.5. At higher redshift, cluster core galaxies are observed to have still on-going star-formation, fuelled by cold…
Spectroscopic Confirmation of a Coma Cluster Progenitor at z ~ 2.2
Behnam Darvish, Nick Z. Scoville, Christopher Martin +17
We report the spectroscopic confirmation of a new protocluster in the COSMOS field at 2.2, COSMOS Cluster 2.2 (CC2.2), originally identified as an overdensity of narrowb…
Spitzer Planck Herschel Infrared Cluster (SPHerIC) survey: Candidate galaxy clusters at 1.3 < z < 3 selected by high star-formation rate
C. Martinache, A. Rettura, H. Dole +17
There is a lack of large samples of spectroscopically confirmed clusters and protoclusters at high redshifts, 1.5. Discovering and characterizing distant (proto-)clusters is im…