ALMA Pinpoints a Strong Overdensity of U/LIRGs in the Massive Cluster XCS J2215 at z = 1.46
Evolutionary Phases of Gas-rich Galaxies in a Galaxy Cluster at z = 1.46
High-resolution ALMA Study of CO J = 2-1 Line and Dust Continuum Emissions in Cluster Galaxies at z = 1.46
Molecular Gas Reservoirs in Cluster Galaxies at z = 1.46
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 Galaxy Clusters Project
The missing light of the Hubble Ultra Deep Field
Instrument
WFC3, WFC3/IR
Temporal Coverage
2015-06-08T19:49:08Z/2015-11-10T06:32:20Z
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, Beifiori comma Alessandra, 2016, 'Unveiling the mass-to-light distribution of high-redshift clusters', 1.0, European Space Agency, https://doi.org/10.5270/esa-1c5q2ne