An Increase in the Faint Red Galaxy Population in Massive Clusters since z ~ 0.5
Dark Matter in the Galaxy Cluster CL J1226+3332 at z = 0.89
Evolution of the Ultraviolet Upturn at 0.3 < z < 1: Exploring Helium-rich Stellar Populations
Galaxy Populations in Massive z = 0.2-0.9 Clusters. I. Analysis of Spectroscopy
Harnessing the Hubble Space Telescope Archives: A Catalog of 21,926 Interacting Galaxies
Little change in the sizes of the most massive galaxies since z = 1
Stellar Populations and Evolution of Early-type Cluster Galaxies: Constraints from Optical Imaging and Spectroscopy of z = 0.5-0.9 Galaxy Clusters
The colour-magnitude relations of ClJ1226.9+3332, a massive cluster of galaxies at z = 0.89
The Evolution of Bulge-dominated Field Galaxies from z 1 to the Present
The Fundamental Plane for z = 0.8-0.9 Cluster Galaxies
The Gemini/HST Cluster Project: Structural and Photometric Properties of Galaxies in Three z = 0.28-0.89 Clusters
The Gemini/HST Galaxy Cluster Project: Redshift 0.2-1.0 Cluster Sample, X-Ray Data, and Optical Photometry Catalog
The history of mass assembly of faint red galaxies in 28 galaxy clusters since z = 1.3
The impact of satellite trails on Hubble Space Telescope observations
The Influence of Mass and Environment on the Evolution of Early-Type Galaxies
The Type Ia Supernova Rate in Redshift 0.5-0.9 Galaxy Clusters
Instrument
ACS, ACS/HRC, ACS/WFC
Temporal Coverage
2003-04-07T17:14:31Z/2003-04-28T08:10:36Z
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, Ebeling comma Harald, 2004, 'Measuring the mass distribution in the most distant, very X-ray luminous galaxy cluster known', 1.0, European Space Agency, https://doi.org/10.5270/esa-wx1p021
