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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
A CALIBRATION OF NICMOS CAMERA 2 FOR LOW COUNT RATES
Red sequence of Abell X-ray underluminous clusters
J. J. Trejo-Alonso, C. A. Caretta, T. F. Laganá, et al. Monthly Notices of the Royal Astronomical Society 441(1) 776 (2014) https://doi.org/10.1093/mnras/stu595
The morphological transformation of red sequence galaxies in the distant cluster XMMU J1229+0151
P. Cerulo, W. J. Couch, C. Lidman, et al. Monthly Notices of the Royal Astronomical Society 439(3) 2790 (2014) https://doi.org/10.1093/mnras/stu135
Larger sizes of massive quiescent early-type galaxies in clusters than in the field at 0.8 < z < 1.5
L. Delaye, M. Huertas-Company, S. Mei, et al. Monthly Notices of the Royal Astronomical Society 441(1) 203 (2014) https://doi.org/10.1093/mnras/stu496
CANDELS OBSERVATIONS OF THE ENVIRONMENTAL DEPENDENCE OF THE COLOR-MASS-MORPHOLOGY RELATION ATz= 1.6
AGN Triggering in the Infall Regions of Distant X-Ray Luminous Galaxy Clusters at0.9
R. Fassbender, R. Šuhada and A. Nastasi Advances in Astronomy 2012 1 (2012) https://doi.org/10.1155/2012/138380
THEHUBBLE SPACE TELESCOPECLUSTER SUPERNOVA SURVEY. V. IMPROVING THE DARK-ENERGY CONSTRAINTS ABOVEz> 1 AND BUILDING AN EARLY-TYPE-HOSTED SUPERNOVA SAMPLE
THEHUBBLE SPACE TELESCOPECLUSTER SUPERNOVA SURVEY. III. CORRELATED PROPERTIES OF TYPE Ia SUPERNOVAE AND THEIR HOSTS AT 0.9
J. Meyers, G. Aldering, K. Barbary, et al. The Astrophysical Journal 750(1) 1 (2012) https://doi.org/10.1088/0004-637X/750/1/1
Observational constraints on the redshift evolution of X-ray scaling relations of galaxy clusters out toz ~ 1.5
The x-ray luminous galaxy cluster population at 0.9
R Fassbender, H Böhringer, A Nastasi, et al. New Journal of Physics 13(12) 125014 (2011) https://doi.org/10.1088/1367-2630/13/12/125014
XMMU J100750.5+125818: a strong lensing cluster atz= 1.082
1 - The HST/ACS colour–magnitude diagram