Cluster galaxies in XMMU J2235-2557: galaxy population properties in most massive environments at z ~ 1.4
Colour gradients in cluster ellipticals at z ~ 1.4: the hidden content of the galaxy central regions
Galaxy kinematics in the XMMU J2235-2557 cluster field at z 1.4
Hubble Space Telescope Weak-lensing Study of the Galaxy Cluster XMMU J2235.3 - 2557 at z ~ 1.4: A Surprisingly Massive Galaxy Cluster When the Universe is One-third of its Current Age
Multi-wavelength study of XMMU J2235.3-2557: the most massive galaxy cluster at z > 1
Sizes, colour gradients and resolved stellar mass distributions for the massive cluster galaxies in XMMUJ2235-2557 at z = 1.39
Substellar and low-mass dwarf identification with near-infrared imaging space observatories
The impact of satellite trails on Hubble Space Telescope observations
The KMOS Cluster Survey (KCS). II. The Effect of Environment on the Structural Properties of Massive Cluster Galaxies at Redshift 1.39 < z < 1.61
The KMOS Cluster Survey (KCS). I. The Fundamental Plane and the Formation Ages of Cluster Galaxies at Redshift 1.4 < z < 1.6
Instrument
ACS, ACS/WFC
Temporal Coverage
2005-06-10T17:22:11Z/2005-06-27T21:10:24Z
Version
1.0
Mission Description
Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
European Space Agency, Ford et al., 2006, 'ACS Imaging of Galaxy Cluster XMMUJ2235.3-2557 at z=1.4', 1.0, European Space Agency, https://doi.org/10.5270/esa-kjl4nb9
