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A 100 Mpc2 Structure Traced by Hyperluminous Galaxies around a Massive z = 2.85 Protocluster
George C.P. Wang, Scott C. Chapman, Nikolaus Sulzenauer, Frank Bertoldi, Christopher C. Hayward, Ryley Hill, Satoshi Kikuta, Yuichi Matsuda, Douglas Rennehan, Douglas Scott, Ian Smail and Charles C. Steidel The Astrophysical Journal 983(1) 69 (2025) https://doi.org/10.3847/1538-4357/adb834
The quiescent population at 0.5 ≤ z ≤ 0.9: Environmental impact on the mass–size relation
M. Figueira, M. Siudek, A. Pollo, J. Krywult, D. Vergani, M. Bolzonella, O. Cucciati and A. Iovino Astronomy & Astrophysics 687 A117 (2024) https://doi.org/10.1051/0004-6361/202347774
The Kormendy relation of early-type galaxies as a function of wavelength in Abell S1063, MACS J0416.1-2403, and MACS J1149.5+2223
The Fundamental Plane of cluster spheroidal galaxies at z ∼ 1.3: evidence for mass-dependent evolution
P Saracco, A Gargiulo, F La Barbera, M Annunziatella and D Marchesini Monthly Notices of the Royal Astronomical Society 491(2) 1777 (2020) https://doi.org/10.1093/mnras/stz3109
The VIMOS Public Extragalactic Redshift Survey (VIPERS)
The Gemini/HST Galaxy Cluster Project: Environment Effects on the Stellar Populations in the Lynx Clusters at z = 1.27
Inger Jørgensen, Laura C. Hunter, Conor R. O’Neill, Kristin Chiboucas, Ryan K. Cole, Sune Toft and Ricardo P. Schiavon The Astrophysical Journal 881(1) 42 (2019) https://doi.org/10.3847/1538-4357/ab2d9d
The Kormendy relation of galaxies in the Frontier Fields clusters: Abell S1063 and MACS J1149.5+2223
Luca Tortorelli, Amata Mercurio, Maurizio Paolillo, et al. Monthly Notices of the Royal Astronomical Society 477(1) 648 (2018) https://doi.org/10.1093/mnras/sty617
The Gemini/Hubble Space Telescope Galaxy Cluster Project: Stellar Populations in the Low-redshift Reference Cluster Galaxies
Constraints on Quenching of Z ≲ 2 Massive Galaxies from the Evolution of the Average Sizes of Star-forming and Quenched Populations in COSMOS
A. L. Faisst, C. M. Carollo, P. L. Capak, S. Tacchella, A. Renzini, O. Ilbert, H. J. McCracken and N. Z. Scoville The Astrophysical Journal 839(2) 71 (2017) https://doi.org/10.3847/1538-4357/aa697a
The KMOS Cluster Survey (KCS). I. The Fundamental Plane and the Formation Ages of Cluster Galaxies at Redshift 1.4 < Z < 1.6*
Alessandra Beifiori, J. Trevor Mendel, Jeffrey C. C. Chan, Roberto P. Saglia, Ralf Bender, Michele Cappellari, Roger L. Davies, Audrey Galametz, Ryan C. W. Houghton, Laura J. Prichard, Russell Smith, John P. Stott, David J. Wilman, Ian J. Lewis, Ray Sharples and Michael Wegner The Astrophysical Journal 846(2) 120 (2017) https://doi.org/10.3847/1538-4357/aa8368
TheChandraDeep Field South as a test case for Global Multi Conjugate Adaptive Optics
E. Portaluri, V. Viotto, R. Ragazzoni, et al. Monthly Notices of the Royal Astronomical Society 466(3) 3569 (2017) https://doi.org/10.1093/mnras/stw3214
The most massive galaxies in clusters are already fully grown atz ∼ 0.5
L. J. Oldham, R. C. W. Houghton and Roger L. Davies Monthly Notices of the Royal Astronomical Society 465(2) 2101 (2017) https://doi.org/10.1093/mnras/stw2791
The abundance and colours of galaxies in high-redshift clusters in the cold dark matter cosmology
Alexander I. Merson, Carlton M. Baugh, Violeta Gonzalez-Perez, et al. Monthly Notices of the Royal Astronomical Society 456(2) 1681 (2016) https://doi.org/10.1093/mnras/stv2706
Morphological evolution of cluster red sequence galaxies in the past 9 Gyr
Roberto De Propris, Malcolm N. Bremer and Steven Phillipps Monthly Notices of the Royal Astronomical Society 461(4) 4517 (2016) https://doi.org/10.1093/mnras/stw1521
Ultramassive dense early-type galaxies: Velocity dispersions and number density evolution sincez= 1.6
Galaxy sizes as a function of environment at intermediate redshift from the ESO Distant Cluster Survey
Kshitija Kelkar, Alfonso Aragón-Salamanca, Meghan E. Gray, et al. Monthly Notices of the Royal Astronomical Society 450(2) 1246 (2015) https://doi.org/10.1093/mnras/stv670
RX J0848.6+4453: THE EVOLUTION OF GALAXY SIZES AND STELLAR POPULATIONS IN Az= 1.27 CLUSTER