IDCS J1426.5+3508: Cosmological Implications of a Massive, Strong Lensing Cluster at z = 1.75
IDCS J1426.5+3508: Discovery of a Massive, Infrared-selected Galaxy Cluster at z = 1.75
IDCS J1426.5+3508: Sunyaev-Zeldovich Measurement of a Massive Infrared-selected Cluster at z = 1.75
IDCS J1426.5+3508: The Most Massive Galaxy Cluster at z > 1.5
IDCS J1426.5+3508: Weak Lensing Analysis of a Massive Galaxy Cluster at z = 1.75
IDCS J1433.2+3306: An Infrared-selected Galaxy Cluster at z = 1.89
The HST See Change Program. I. Survey Design, Pipeline, and Supernova Discoveries
The impact of satellite trails on Hubble Space Telescope observations
The missing light of the Hubble Ultra Deep Field
Instrument
ACS, ACS/WFC, WFC3, WFC3/IR
Temporal Coverage
2010-11-06T19:38:06Z/2011-09-16T08:25:40Z
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, Stanford comma Spencer Adam, 2012, 'Rest Frame Optical Spectroscopy of Galaxy Clusters at 1.6 < z < 1.9', 1.0, European Space Agency, https://doi.org/10.5270/esa-d0bk85i